Courtesy of AGI's Launch Notification e-mails. AGI's E-mails are sent after every launch and include key spacecraft information such as: the date, time, launch site, launcher, international number, name, and owner. Get more information on thousands of satellites and other vehicles by viewing STK models, animations, and our encyclopedic "Spacecraft Digest" database at www.agi.com/scdigest.
New Launch: 2010 October 19, 1711 UTC
Site: Baikonur Cosmodrome, Kazakhstan
Launcher: Soyuz 2
International Designator(s): 2010-054A, 2010-054B, 2010-054C, 2010-054D, 2010-054E, 2010-054F
SSC Name Owner
37188 GLOBALSTAR M079 GLOB
37189 GLOBALSTAR M074 GLOB
37190 GLOBALSTAR M076 GLOB
37191 GLOBALSTAR M077 GLOB
37192 GLOBALSTAR M075 GLOB
37193 GLOBALSTAR M073 GLOB
"Globalstar's fleet of orbiting communications satellites received reinforcements Tuesday, when a commercial Soyuz rocket launched from Kazakhstan and deployed six advanced spacecraft to restore the company's diminished two-way voice and data services.
"Built by Thales Alenia Space, the satellites are also the cornerstone of a rejuvenated Globalstar constellation Three more Soyuz launches are planned through the summer of 2011, bringing the company's fleet of second-generation satellites to 24 platforms.
"Globalstar officials say the transition to the new satellite fleet will be seamless for the company's 400,000 subscribers, except for a marked improvement in mobile two-way communications service.
"S-band antenna degradation on Globalstar's existing satellites has limited voice and duplex data communications since 2007. The problem has not affected Globalstar's simplex data relay and asset tracking product, according to the company.
"Globalstar subscribers use the satellite network to make mobile phone calls and data transmissions, especially in rural zones where terrestrial coverage is spotty or non-existent.
"By the middle of 2011, Globalstar officials say customers can expect a return to reliable voice and data transmissions. Until then, subscribers can use an application on the company's website to plug in their location and determine what hours satellite coverage is available."
"A Soyuz rocket launched at 1710:59 GMT (1:10:59 p.m. EDT) from the Baikonur Cosmodrome in Kazakhstan. Soaring into a partly cloudy night sky, the Soyuz 2-1a booster and Fregat upper stage accelerated to orbital velocity a few minutes after liftoff.
"After coasting around the world for more than an hour, the Fregat upper stage ignited again to reach the planned separation orbit. The rocket was targeting a circular orbit 572 miles [921 km] high with an inclination of 52 degrees
"Mounted on a specially-built satellite dispenser during launch, the Globalstar spacecraft were released in a choreographed sequence to avoid collisions. Two satellites bolted to the top of the cone-shaped adapter separated first, then four craft on the lower portion of the structure deployed 96 seconds later.
"The satellites' first radio signals were received by ground stations moments after spacecraft separation, according to Jean-Yves Le Gall, chairman and CEO of Arianespace, which oversees commercial Soyuz launches through its Starsem subsidiary."
"In a phone interview from Baikonur on the eve of launch, Navarra said two of the satellites launched Tuesday will enter service in about one month. It will take up to four months for the other four craft to drift to their prescribed orbital locations."
"The new satellites weigh 1,543 pounds [700 kg] at launch and are supposed to operate for 15 years, extending Globalstar's constellation life through at least 2025
"When the Globalstar launch campaign ends next year, the company's fleet will include 24 second-generation spacecraft and eight leftover first-generation satellites built as spares and launched in 2007."
Source: Spaceflight Now, "Six improved Globalstar craft orbited by Soyuz rocket"
Thursday, October 28, 2010
Thursday, October 07, 2010
Launch Notification: SHIJIAN-6G and SHIJIAN-6H
Courtesy of AGI's Launch Notification e-mails. AGI's E-mails are sent after every launch and include key spacecraft information such as: the date, time, launch site, launcher, international number, name, and owner. Get more information on thousands of satellites and other vehicles by viewing STK models, animations, and our encyclopedic "Spacecraft Digest" database at www.agi.com/scdigest.
New Launch: 2010 October 6, 0049 UTC
Site: Taiyuan Space Center, PRC
Launcher: Long March 4B (Chang Zheng 4B)
International Designator(s): 2010-051A, 2010-051B
SSC Name Owner
37179 SJ-6G
(SHIJIAN-6G) PRC
37180 SJ-6H
(SHIJIAN-6H) PRC
"Two research satellites flew into a nearly 400-mile-high [644-km-high] orbit early Wednesday on a Long March rocket, continuing a pace of nearly one Chinese launch a week since the end of July.
"A Long March 4B rocket lifted off at 0049 GMT Wednesday (8:49 p.m. EDT Tuesday) from the Taiyuan space center in northern China. The launch occurred a few hours before the Chang'e 2 lunar orbiter arrived at the moon after a five-day journey from Earth.
"According to the state-run Xinhua news agency, the 15-story rocket carried two Shijian 6 satellites. U.S. military tracking data show the spacecraft orbiting about 375 miles [603 km] above Earth with an inclination of about 98 degrees to the equator.
"It was the 11th space launch of the year for China Seven of those missions have been since the end of July, a span of less than 10 weeks.
"The payloads are the fourth pair of Shijian 6 satellites. The spacecraft, dubbed Shijian 6G and Shijian 6H, will probe the space environment, according to Xinhua.
"No other details of their mission were released.
"Shijian satellites are believed to test technology demonstration and space research experiments. Shijian means "practice" in Chinese.
"The last set of Shijian 6 satellites launched in October 2008. One of the craft, Shijian 6F, became the target of an orbital rendezvous demonstration in August.
"A newly-launched satellite named Shijian 12 approached within 200 meters, or 656 feet, of Shijian 6F in mid-August, according to amateur satellite observations and U.S. Air Force data."
Source: Spaceflight Now, "Pair of research satellites launched by China"
New Launch: 2010 October 6, 0049 UTC
Site: Taiyuan Space Center, PRC
Launcher: Long March 4B (Chang Zheng 4B)
International Designator(s): 2010-051A, 2010-051B
SSC Name Owner
37179 SJ-6G
(SHIJIAN-6G) PRC
37180 SJ-6H
(SHIJIAN-6H) PRC
"Two research satellites flew into a nearly 400-mile-high [644-km-high] orbit early Wednesday on a Long March rocket, continuing a pace of nearly one Chinese launch a week since the end of July.
"A Long March 4B rocket lifted off at 0049 GMT Wednesday (8:49 p.m. EDT Tuesday) from the Taiyuan space center in northern China. The launch occurred a few hours before the Chang'e 2 lunar orbiter arrived at the moon after a five-day journey from Earth.
"According to the state-run Xinhua news agency, the 15-story rocket carried two Shijian 6 satellites. U.S. military tracking data show the spacecraft orbiting about 375 miles [603 km] above Earth with an inclination of about 98 degrees to the equator.
"It was the 11th space launch of the year for China Seven of those missions have been since the end of July, a span of less than 10 weeks.
"The payloads are the fourth pair of Shijian 6 satellites. The spacecraft, dubbed Shijian 6G and Shijian 6H, will probe the space environment, according to Xinhua.
"No other details of their mission were released.
"Shijian satellites are believed to test technology demonstration and space research experiments. Shijian means "practice" in Chinese.
"The last set of Shijian 6 satellites launched in October 2008. One of the craft, Shijian 6F, became the target of an orbital rendezvous demonstration in August.
"A newly-launched satellite named Shijian 12 approached within 200 meters, or 656 feet, of Shijian 6F in mid-August, according to amateur satellite observations and U.S. Air Force data."
Source: Spaceflight Now, "Pair of research satellites launched by China"
Friday, October 01, 2010
Launch Notification: Cosmos 2469
Courtesy of AGI's Launch Notification e-mails. AGI's E-mails are sent after every launch and include key spacecraft information such as: the date, time, launch site, launcher, international number, name, and owner. Get more information on thousands of satellites and other vehicles by viewing STK models, animations, and our encyclopedic "Spacecraft Digest" database at www.agi.com/scdigest.
New Launch: 2010 September 30, 1701 UTC
Site: Plesetsk Missile and Space Complex, Russia
Launcher: Molniya-M
International Designator(s): 2010-049A
SSC Name Owner
37170 COSMOS 2469 CIS
"A Molniya-M carrier rocket successfully released a Kosmos satellite into orbit on Thursday, a spokeman from the Russian Defense Ministry said.
"The rocket blasted off from the Pletesk space center in northern Russia at 21.01 Moscow time (17.01 GMT).
"The satellite will be used by the Russian Defense Ministry for military purposes."
Source: RIA Novosti, "Russia successfully sends Kosmos satellite into orbit"
New Launch: 2010 September 30, 1701 UTC
Site: Plesetsk Missile and Space Complex, Russia
Launcher: Molniya-M
International Designator(s): 2010-049A
SSC Name Owner
37170 COSMOS 2469 CIS
"A Molniya-M carrier rocket successfully released a Kosmos satellite into orbit on Thursday, a spokeman from the Russian Defense Ministry said.
"The rocket blasted off from the Pletesk space center in northern Russia at 21.01 Moscow time (17.01 GMT).
"The satellite will be used by the Russian Defense Ministry for military purposes."
Source: RIA Novosti, "Russia successfully sends Kosmos satellite into orbit"
Thursday, September 23, 2010
Launch Notification: YAOGAN 11, ZHEDA PIXING 1B, ZHEDA PIXING 1C
Courtesy of AGI's Launch Notification e-mails. AGI's E-mails are sent after every launch and include key spacecraft information such as: the date, time, launch site, launcher, international number, name, and owner. Get more information on thousands of satellites and other vehicles by viewing STK models, animations, and our encyclopedic "Spacecraft Digest" database at www.agi.com/scdigest.
New Launch: 2010 September 22, 0242 UTC
Site: Jiuquan Space Center, PRC
Launcher: Long March 2D (Chang Zheng 2D)
International Designator(s): 2010-047A, 2010-047B, 2010-047C
SSC Name Owner
37165 YAOGAN 11 PRC
37166 ZHEDA PIXING 1B PRC
37167 ZHEDA PIXING 1C PRC
"A secret military payload successfully launched aboard a Long March rocket early Wednesday, continuing a feverish pace of Chinese space activity that includes a mysterious orbital rendezvous, an upcoming lunar probe and preps for continued human missions.
"It was the fifth launch in barely 50 days for China, and the second mission in that period lofting a clandestine Yaogan reconnaissance satellite.
"Wednesday's launch began with the blastoff of a Long March 2D rocket at 0242 GMT (10:42 p.m. EDT Tuesday) from the Jiuquan space center in the desert of northwestern China, according to the state-run Xinhua news agency.
"It was 10:42 a.m. Beijing time.
"The 135-foot-tall [41-m-tall] launch vehicle placed Yaogan 11 and two smaller satellites on a path nearly 400 miles [644 km] above Earth.
"The Yaogan 11 payload orbited Wednesday will conduct scientific experiments, survey land resources, estimate crop yields and contribute to natural disaster response efforts, Xinhua reported.
"But the Yaogan satellite series are believed to provide the Chinese military with high-resolution reconnaissance imagery through electro-optical cameras and night-vision radar systems."
Source: Spaceflight Now, "China orbits spy satellite amid uptick in space activity"
New Launch: 2010 September 22, 0242 UTC
Site: Jiuquan Space Center, PRC
Launcher: Long March 2D (Chang Zheng 2D)
International Designator(s): 2010-047A, 2010-047B, 2010-047C
SSC Name Owner
37165 YAOGAN 11 PRC
37166 ZHEDA PIXING 1B PRC
37167 ZHEDA PIXING 1C PRC
"A secret military payload successfully launched aboard a Long March rocket early Wednesday, continuing a feverish pace of Chinese space activity that includes a mysterious orbital rendezvous, an upcoming lunar probe and preps for continued human missions.
"It was the fifth launch in barely 50 days for China, and the second mission in that period lofting a clandestine Yaogan reconnaissance satellite.
"Wednesday's launch began with the blastoff of a Long March 2D rocket at 0242 GMT (10:42 p.m. EDT Tuesday) from the Jiuquan space center in the desert of northwestern China, according to the state-run Xinhua news agency.
"It was 10:42 a.m. Beijing time.
"The 135-foot-tall [41-m-tall] launch vehicle placed Yaogan 11 and two smaller satellites on a path nearly 400 miles [644 km] above Earth.
"The Yaogan 11 payload orbited Wednesday will conduct scientific experiments, survey land resources, estimate crop yields and contribute to natural disaster response efforts, Xinhua reported.
"But the Yaogan satellite series are believed to provide the Chinese military with high-resolution reconnaissance imagery through electro-optical cameras and night-vision radar systems."
Source: Spaceflight Now, "China orbits spy satellite amid uptick in space activity"
Sunday, September 12, 2010
Nine years later: Towers of Babble
From the The Virginian-Pilot, September 11, 2010
http://hamptonroads.com/2010/09/nine-years-later-towers-babble
A network that allows public safety agencies to communicate with each other remains one of the most elusive and pressing recommendations from the 9/11 Commission. Nine years after America was attacked, there's no guarantee that such a system will ever come into existence.
As The New York Times reported this week, squabbling over who will control a prime slice of broadband spectrum has left plans for a nationwide system literally up in the air.
The Federal Communications Commission has been pushing an approach that would have commercial companies buy and control the airwaves and build fourth-generation wireless networks on it. During emergencies, police and fire and emergency personnel would get control of the network, effectively taking over the airwaves to coordinate interagency communication.
Those public safety groups, however, insist such a network is unlikely to have the capacity needed during an emergency, meaning it could fail under heavy use and put lives at risk. They want exclusive control of the entire section of the spectrum, and they're lobbying Congress for it.
It has been six years since the 9/11 Commission issued its massive report, which included recommendations to improve the response to catastrophes on the scale of the terrorist attacks of Sept. 11, 2001.
That makes the prolonged delay over divvying up broadband spectrum and developing a nationwide interoperable communication system all the more frustrating, particularly for commission members. Two years ago, after an FCC auction failed to draw sufficient commercial bids, the commission's vice chairman told The Washington Post: "I've lost patience... The slowness of this just indicates a lack of urgency and a lack of concern about human survival and human life if a disaster strikes."
The unhurried pace is indeed disappointing, especially given the urgency of the problem. During the attacks on the World Trade Center in New York nine years ago, first responders found themselves - for a variety of reasons - unable to communicate with each other. People died as a result.
There has been some progress that will help in future emergencies.
Today, many police and fire departments, including those in South Hampton Roads, use plain English on their radios instead of arbitrary, agency-specific codes.
They have developed interoperable regional systems and standard operating procedures to communicate during emergencies, and they've held joint training to prepare for hurricanes, plane crashes and other disasters.
Such changes have helped communities become better prepared, but each would be more valuable if they were part of a system that permits local, state and federal agencies from Virginia to Oregon to communicate and coordinate in a large-scale emergency.
Officials have said construction of the network could take as much as a decade. That means if Congress has any intention of seeing the system in place before the 20th anniversary of 9/11, it must act now to settle the debate over access to the broadband spectrum.
http://hamptonroads.com/2010/09/nine-years-later-towers-babble
A network that allows public safety agencies to communicate with each other remains one of the most elusive and pressing recommendations from the 9/11 Commission. Nine years after America was attacked, there's no guarantee that such a system will ever come into existence.
As The New York Times reported this week, squabbling over who will control a prime slice of broadband spectrum has left plans for a nationwide system literally up in the air.
The Federal Communications Commission has been pushing an approach that would have commercial companies buy and control the airwaves and build fourth-generation wireless networks on it. During emergencies, police and fire and emergency personnel would get control of the network, effectively taking over the airwaves to coordinate interagency communication.
Those public safety groups, however, insist such a network is unlikely to have the capacity needed during an emergency, meaning it could fail under heavy use and put lives at risk. They want exclusive control of the entire section of the spectrum, and they're lobbying Congress for it.
It has been six years since the 9/11 Commission issued its massive report, which included recommendations to improve the response to catastrophes on the scale of the terrorist attacks of Sept. 11, 2001.
That makes the prolonged delay over divvying up broadband spectrum and developing a nationwide interoperable communication system all the more frustrating, particularly for commission members. Two years ago, after an FCC auction failed to draw sufficient commercial bids, the commission's vice chairman told The Washington Post: "I've lost patience... The slowness of this just indicates a lack of urgency and a lack of concern about human survival and human life if a disaster strikes."
The unhurried pace is indeed disappointing, especially given the urgency of the problem. During the attacks on the World Trade Center in New York nine years ago, first responders found themselves - for a variety of reasons - unable to communicate with each other. People died as a result.
There has been some progress that will help in future emergencies.
Today, many police and fire departments, including those in South Hampton Roads, use plain English on their radios instead of arbitrary, agency-specific codes.
They have developed interoperable regional systems and standard operating procedures to communicate during emergencies, and they've held joint training to prepare for hurricanes, plane crashes and other disasters.
Such changes have helped communities become better prepared, but each would be more valuable if they were part of a system that permits local, state and federal agencies from Virginia to Oregon to communicate and coordinate in a large-scale emergency.
Officials have said construction of the network could take as much as a decade. That means if Congress has any intention of seeing the system in place before the 20th anniversary of 9/11, it must act now to settle the debate over access to the broadband spectrum.
QZS-1 (MICHIBIKI)
Courtesy of AGI's Launch Notification e-mails. AGI's E-mails are sent after every launch and include key spacecraft information such as: the date, time, launch site, launcher, international number, name, and owner. Get more information on thousands of satellites and other vehicles by viewing STK models, animations, and our encyclopedic "Spacecraft Digest" database at www.agi.com/scdigest.
New Launch: 2010 September 11, 1117 UTC
Site: Tanegashima Space Center, Japan
Launcher: H-2A
International Designator(s): 2010-045A
SSC Name Owner
37158 QZS-1 (MICHIBIKI) JPN
"An H-2A rocket flew to space Saturday with a Japanese satellite to meet a pressing need for improved navigation services amid the country's numerous mountains and high-rise buildings.
"The rocket's payload is the first of three planned satellites to fill coverage gaps from U.S. Global Positioning System satellites caused by signal blockage from mountains and skyscrapers.
"Developed by the Japan Aerospace Exploration Agency and four government ministries, the Quasi-Zenith Satellite System is aimed at overcoming ground interference by launching more navigation satellites strategically positioned high in the sky above Asia.
"The line-of-sight navigation signals from GPS satellites can be interrupted in rural hamlets and skyscraper-filled cities like Tokyo, where users occasionally lack sufficient data to determine their position, elevation and time.
"JAXA says a constellation of three QZSS spacecraft would make three-dimensional navigation coverage available 99.8 percent of the time, an improvement over the estimated 90 percent availability with GPS satellites today.
"Four GPS satellites must appear in the sky at one time to triangulate a user's 3D position and time, but buildings and mountains can block signals from spacecraft close to the horizon.
"The first QZSS navigation craft launched Saturday on an H-2A rocket. Its nickname is Michibiki, which means "guiding" or "showing the way" in Japanese.
"Michibiki is demonstrating the system's navigation instruments and proving the satellite works before Japan commits to launching the other two spacecraft.
"The 17-story launcher lifted off at 1117 GMT (7:17 a.m. EDT) from Launch Pad No. 1 at the Yoshinobu launch complex, a shoreline facility at the Tanegashima Space Center off the coast of Kyushu, the southernmost of Japan's main islands."
"JAXA says Michibiki will reach its final orbit in about two weeks. It will be three months before the satellite finishes commissioning tests and can begin its navigation demos.
"Michibiki will circle the Earth at a 45-degree angle to the equator. Its orbital high point will be more than 24,000 miles [38,600 km] over the northern hemisphere and its lowest altitude will be 20,500 miles [33,000 km], according to JAXA.
"Projected against Earth's surface, Michibiki's ground track will chart an asymmetric figure-eight pattern stretching from Japan to Australia as it alternates north and south of the equator.
"Michibiki will be near-zenith, or almost straight up, in the Japanese sky for about eight hours each day. If launched, the two follow-on satellites would permit continuous coverage of Japan."
Source: Spaceflight Now, "Navigation satellite launched to show the way in Japan"
New Launch: 2010 September 11, 1117 UTC
Site: Tanegashima Space Center, Japan
Launcher: H-2A
International Designator(s): 2010-045A
SSC Name Owner
37158 QZS-1 (MICHIBIKI) JPN
"An H-2A rocket flew to space Saturday with a Japanese satellite to meet a pressing need for improved navigation services amid the country's numerous mountains and high-rise buildings.
"The rocket's payload is the first of three planned satellites to fill coverage gaps from U.S. Global Positioning System satellites caused by signal blockage from mountains and skyscrapers.
"Developed by the Japan Aerospace Exploration Agency and four government ministries, the Quasi-Zenith Satellite System is aimed at overcoming ground interference by launching more navigation satellites strategically positioned high in the sky above Asia.
"The line-of-sight navigation signals from GPS satellites can be interrupted in rural hamlets and skyscraper-filled cities like Tokyo, where users occasionally lack sufficient data to determine their position, elevation and time.
"JAXA says a constellation of three QZSS spacecraft would make three-dimensional navigation coverage available 99.8 percent of the time, an improvement over the estimated 90 percent availability with GPS satellites today.
"Four GPS satellites must appear in the sky at one time to triangulate a user's 3D position and time, but buildings and mountains can block signals from spacecraft close to the horizon.
"The first QZSS navigation craft launched Saturday on an H-2A rocket. Its nickname is Michibiki, which means "guiding" or "showing the way" in Japanese.
"Michibiki is demonstrating the system's navigation instruments and proving the satellite works before Japan commits to launching the other two spacecraft.
"The 17-story launcher lifted off at 1117 GMT (7:17 a.m. EDT) from Launch Pad No. 1 at the Yoshinobu launch complex, a shoreline facility at the Tanegashima Space Center off the coast of Kyushu, the southernmost of Japan's main islands."
"JAXA says Michibiki will reach its final orbit in about two weeks. It will be three months before the satellite finishes commissioning tests and can begin its navigation demos.
"Michibiki will circle the Earth at a 45-degree angle to the equator. Its orbital high point will be more than 24,000 miles [38,600 km] over the northern hemisphere and its lowest altitude will be 20,500 miles [33,000 km], according to JAXA.
"Projected against Earth's surface, Michibiki's ground track will chart an asymmetric figure-eight pattern stretching from Japan to Australia as it alternates north and south of the equator.
"Michibiki will be near-zenith, or almost straight up, in the Japanese sky for about eight hours each day. If launched, the two follow-on satellites would permit continuous coverage of Japan."
Source: Spaceflight Now, "Navigation satellite launched to show the way in Japan"
Friday, September 03, 2010
Launch Notification: Cosmos 2464/2465/2466
Courtesy of AGI's Launch Notification e-mails. AGI's E-mails are sent after every launch and include key spacecraft information such as: the date, time, launch site, launcher, international number, name, and owner. Get more information on thousands of satellites and other vehicles by viewing STK models, animations, and our encyclopedic "Spacecraft Digest" database at www.agi.com/scdigest.
New Launch: 2010 September 2, 0053 UTC
Site: Baikonur Cosmodrome, Kazakhstan
Launcher: Proton-M
International Designator(s): 2010-041A, 2010-041B, 2010-041C
SSC Name Owner
37137 COSMOS 2464 CIS
37138 COSMOS 2465 CIS
37139 COSMOS 2466 CIS
"A Proton rocket blasted off overnight Wednesday with three spacecraft to help expand Russia's satellite navigation system to provide positioning services around the world.
"The Proton rocket launched at 0053 GMT Thursday (8:53 p.m. EDT Wednesday) from [P]ad 81 at the Baikonur Cosmodrome in Kazakhstan, where the first pink hues of sunrise splashed the dawn sky.
"With six main engines burning, the Proton soared into mostly clear skies and jettisoned its first stage two minutes after liftoff. The three-stage rocket deployed a Block DM upper stage and the three Glonass payloads in space less than 10 minutes into the mission.
"The Block DM was expected to fire twice to place the Glonass satellites in a circular orbit 12,000 miles [19,000 km] above Earth with an inclination of 64.8 degrees.
"Spacecraft separation occurred at 0426 GMT (12:26 a.m. EDT) in the targeted orbit, according to the Russian Space Agency.
"The satellites are the second group of Glonass platforms launched this year. Three other spacecraft were orbited by a Proton rocket March 1.
"Each satellite weighs about 3,000 pounds [1,360 kg] at launch, including maneuvering fuel to maintan the craft's orientation in space. The modernized Glonass M spacecraft are designed to operate for seven years in orbit, according to their manufacturer, Information Satellite Systems Reshetnev Co.
"Glonass satellites broadcast navigation signals to military and civilian users from their orbital perch, reaching ground receivers across a swath of Earth nearly stretching from pole to pole.
"According to a Russian Space Agency website, 21 Glonass satellites are currently operational. Two more spacecraft are considered spares.
"Glonass satellites are scattered in three orbital groups, each designed for eight spacecraft to achieve global navigation coverage with a total of 24 operating satellites.
"Three more Glonass M satellites are scheduled for launch in November."
[Note: Identifications were made using current orbital motion toward designated orbital slots reported by the Russian Space Agency.]
Source: Spaceflight Now, "Group of navigation satellites launched by Proton rocket"
New Launch: 2010 September 2, 0053 UTC
Site: Baikonur Cosmodrome, Kazakhstan
Launcher: Proton-M
International Designator(s): 2010-041A, 2010-041B, 2010-041C
SSC Name Owner
37137 COSMOS 2464 CIS
37138 COSMOS 2465 CIS
37139 COSMOS 2466 CIS
"A Proton rocket blasted off overnight Wednesday with three spacecraft to help expand Russia's satellite navigation system to provide positioning services around the world.
"The Proton rocket launched at 0053 GMT Thursday (8:53 p.m. EDT Wednesday) from [P]ad 81 at the Baikonur Cosmodrome in Kazakhstan, where the first pink hues of sunrise splashed the dawn sky.
"With six main engines burning, the Proton soared into mostly clear skies and jettisoned its first stage two minutes after liftoff. The three-stage rocket deployed a Block DM upper stage and the three Glonass payloads in space less than 10 minutes into the mission.
"The Block DM was expected to fire twice to place the Glonass satellites in a circular orbit 12,000 miles [19,000 km] above Earth with an inclination of 64.8 degrees.
"Spacecraft separation occurred at 0426 GMT (12:26 a.m. EDT) in the targeted orbit, according to the Russian Space Agency.
"The satellites are the second group of Glonass platforms launched this year. Three other spacecraft were orbited by a Proton rocket March 1.
"Each satellite weighs about 3,000 pounds [1,360 kg] at launch, including maneuvering fuel to maintan the craft's orientation in space. The modernized Glonass M spacecraft are designed to operate for seven years in orbit, according to their manufacturer, Information Satellite Systems Reshetnev Co.
"Glonass satellites broadcast navigation signals to military and civilian users from their orbital perch, reaching ground receivers across a swath of Earth nearly stretching from pole to pole.
"According to a Russian Space Agency website, 21 Glonass satellites are currently operational. Two more spacecraft are considered spares.
"Glonass satellites are scattered in three orbital groups, each designed for eight spacecraft to achieve global navigation coverage with a total of 24 operating satellites.
"Three more Glonass M satellites are scheduled for launch in November."
[Note: Identifications were made using current orbital motion toward designated orbital slots reported by the Russian Space Agency.]
Source: Spaceflight Now, "Group of navigation satellites launched by Proton rocket"
Wednesday, September 01, 2010
Blog Disclosure Statement
This policy is valid from 1 September 2010
This blog is a sponsored blog created or supported by a company. For questions about this blog, please contact teakpub at brmemc dot com.
This blog does not accept any form of advertising, sponsorship, or paid insertions. We write for our own purposes. However, we may be influenced by our background, occupation, religion, political affiliation or experience.
The owner(s) of this blog do not receive any direct compensation in any way from this blog.
The owner(s) of this blog is not compensated to provide opinion on products, services, websites and various other topics. The views and opinions expressed on this blog are purely the blog owners. If we claim or appear to be experts on a certain topic or product or service area, we will only endorse products or services that we believe, based on our expertise, are worthy of such endorsement. Any product claim, statistic, quote or other representation about a product or service should be verified with the manufacturer or provider.
This blog does contain content which might present a conflict of interest. This content may not always be identified. We are employed by or consult with:- Grove Enterprises and Monitoring Times magazine. We have a financial interest in the following that are relevant to our blogging:- Teak Publishing.
To get your own policy, go to http://www.disclosurepolicy.org
This blog is a sponsored blog created or supported by a company. For questions about this blog, please contact teakpub at brmemc dot com.
This blog does not accept any form of advertising, sponsorship, or paid insertions. We write for our own purposes. However, we may be influenced by our background, occupation, religion, political affiliation or experience.
The owner(s) of this blog do not receive any direct compensation in any way from this blog.
The owner(s) of this blog is not compensated to provide opinion on products, services, websites and various other topics. The views and opinions expressed on this blog are purely the blog owners. If we claim or appear to be experts on a certain topic or product or service area, we will only endorse products or services that we believe, based on our expertise, are worthy of such endorsement. Any product claim, statistic, quote or other representation about a product or service should be verified with the manufacturer or provider.
This blog does contain content which might present a conflict of interest. This content may not always be identified. We are employed by or consult with:- Grove Enterprises and Monitoring Times magazine. We have a financial interest in the following that are relevant to our blogging:- Teak Publishing.
To get your own policy, go to http://www.disclosurepolicy.org
Thursday, August 26, 2010
Mysterious Russian 'buzzer' (Enigma S28) radio broadcast changes
From our sister blog, Shortwave Central,(http://mt-shortwave.blogspot.com/) the following posted on the increase in Enigma S28 Russian Buzzer station activity:
The output of Russian number station UVB-76 has increased dramatically over the past week or so. The station, which broadcasts from near Povarovo [on 4625 kHz AM with suppressed lower sideband], is known as “The Buzzer” by its listeners because of the short, monotonous buzz tone that it normally plays 21 to 34 times per minute. It’s only deviated from that signal three times previously - briefly in 1997, 2002 and 2006.
In early August, a garbled recording of a voice speaking Russian was heard by listeners. A few days later, on 23 August at 13:35 UTC, a clearer voice read out the following message twice: “UVB-76, UVB-76 — 93 882 naimina 74 14 35 74 — 9 3 8 8 2 nikolai, anna, ivan, michail, ivan, nikolai, anna, 7, 4, 1, 4, 3, 5, 7, 4″, before returning to its normal broadcasting.
Since then, a number of other distorted voices have appeared over the normal buzzing transmission, as well as knocks and shuffles, as if someone were moving things around inside the broadcasting room. It’s believed that the transmission site has an open microphone, which occasionally picks up sounds from technicians working within the broadcast site.
Additional story at: http://www.wired.co.uk/news/archive/2010-08/25/russian-numbers-station-broadcast-changes (R Netherlands Media Network Weblog)
And from the SCAN-DC newsgroup:
UVB-76 is the callsign of a shortwave radio station that usually broadcasts on the frequency 4625 kHz (AM suppressed lower sideband). It is known among radio listeners by the nickname The Buzzer. It features a short, monotonous buzz tone, repeating at a rate of approximately 25 tones per minute, for 24 hours per day. The station has been observed since around 1982. On rare occasions, the buzzer signal is interrupted and a voice transmission in Russian takes place. Only four to five such events have been noted. Despite much speculation, the actual purpose of this station remains unknown to the public, but is probably used for relaying military orders. There has been a spike in activity as of late August, 2010. More details on the spike below:
http://en.wikipedia.org/wiki/UVB-76#August_2010
Here is the latest intercepts from the Wikipeda link above:
August 2010
There has been a spike in activity on UVB-76 in August 2010. Following messages have been detected by listeners:
On August 20, 2010 at 05:11 UTC, a garbled voice speaking Russian, was detected by amateur listeners. It made a short message with 56° 5'8.23"N little interference and then repeated itself with noticeably more static. This followed recent activity on the station tha little interference and then repeated itself with noticeably more static. This followed recent activity on the station that included more static than usual and several instances of objects being moved/dropped. All of this was detected by amateur listeners and is unconfirmed at the moment.
On August 23, 2010 at 13:35 UTC, a voice speaking in Russian was detected. The voice read out a single, short transmission several times before the line went dead, then returned to its normal broadcast. As the message was transmitted on upper side-band, reception with ordinary AM receivers was weak and distorted.
The message, repeated twice, was: UVB-76, UVB-76 — 93 882 naimina 74 14 35 74 — 9 3 8 8 2 nikolai, anna, ivan, michail, ivan, nikolai, anna, 7, 4, 1, 4, 3, 5, 7, 4[11] (recording of the August 23 2010 voice transmission)
On August 24, 2010 at approximately 04:00 UTC, a heavily distorted voice was heard by amateur listeners.
On August 24, 2010 at 13:25 UTC, another heavily distorted voice was detected by several amateur listeners.
On August 24, 2010 at 17:43 UTC, Hard to hear voices were heard over the transmission.
On August 24, 2010 at around 03:30 UTC, distorted voices in addition to fast beeps and pulses were heard.
On August 25, 2010 around 06:13 UTC, Random knocks or shuffles as if someone is in the room, changes in tone randomly.
On August 25, 2010 at 11:53 GMT the following message was detected: "August 3 5 2 7 Accretion 3 6 0 9 5 6 7 3". A recording is available here mirror Said message is a Google Translate of 3 8 5 2 7 ???????? 3 6 0 9 5 6 7 3. This is identical to the August 25, 2010 06:54 UTC message mentioned below.
On August 25, 2010 at 06:45 UTC, A grumble or garbled sound appeared out of nowhere for 389 ms.
On August 25, 2010 at 06:54 UTC, Another transmission occurred. (Recording of the fifth voice transmission) A new sequence/pattern with a chirping/crank noise occured on top of the previous buzzer. At times this new noise made the old buzzing noise barely audible.The message content was: "UVB-76. UVB-76. 38, 527. ????????. 36, 09, 55, 73.".
On August 25, 2010 at 18:07 UTC, Morse code could be heard behind the buzzer signal. It lasted until approximately 18:20 UTC. At approximately 18:08 UTC A tone was heard in the background followed by a short message.
There is a lot of very interesting additional details at the Wikipedia website above.
Also courtesy of the Spooks list and Jakon Hays, the following associated links:
Saw a post on MeFi this morning about it.
http://www.metafilter.com/95091/4625-kHz
Which cites this site.
http://uvb-76.blogspot.com/2010/08/august-23-2010-935am-pst-voice.html
The wiki page has been updated quite a bit though the day.
http://en.wikipedia.org/wiki/UVB-76
And there is a live stream here.
http://www.justin.tv/rampageturke#/w/340896016/4
The output of Russian number station UVB-76 has increased dramatically over the past week or so. The station, which broadcasts from near Povarovo [on 4625 kHz AM with suppressed lower sideband], is known as “The Buzzer” by its listeners because of the short, monotonous buzz tone that it normally plays 21 to 34 times per minute. It’s only deviated from that signal three times previously - briefly in 1997, 2002 and 2006.
In early August, a garbled recording of a voice speaking Russian was heard by listeners. A few days later, on 23 August at 13:35 UTC, a clearer voice read out the following message twice: “UVB-76, UVB-76 — 93 882 naimina 74 14 35 74 — 9 3 8 8 2 nikolai, anna, ivan, michail, ivan, nikolai, anna, 7, 4, 1, 4, 3, 5, 7, 4″, before returning to its normal broadcasting.
Since then, a number of other distorted voices have appeared over the normal buzzing transmission, as well as knocks and shuffles, as if someone were moving things around inside the broadcasting room. It’s believed that the transmission site has an open microphone, which occasionally picks up sounds from technicians working within the broadcast site.
Additional story at: http://www.wired.co.uk/news/archive/2010-08/25/russian-numbers-station-broadcast-changes (R Netherlands Media Network Weblog)
And from the SCAN-DC newsgroup:
UVB-76 is the callsign of a shortwave radio station that usually broadcasts on the frequency 4625 kHz (AM suppressed lower sideband). It is known among radio listeners by the nickname The Buzzer. It features a short, monotonous buzz tone, repeating at a rate of approximately 25 tones per minute, for 24 hours per day. The station has been observed since around 1982. On rare occasions, the buzzer signal is interrupted and a voice transmission in Russian takes place. Only four to five such events have been noted. Despite much speculation, the actual purpose of this station remains unknown to the public, but is probably used for relaying military orders. There has been a spike in activity as of late August, 2010. More details on the spike below:
http://en.wikipedia.org/wiki/UVB-76#August_2010
Here is the latest intercepts from the Wikipeda link above:
August 2010
There has been a spike in activity on UVB-76 in August 2010. Following messages have been detected by listeners:
On August 20, 2010 at 05:11 UTC, a garbled voice speaking Russian, was detected by amateur listeners. It made a short message with 56° 5'8.23"N little interference and then repeated itself with noticeably more static. This followed recent activity on the station tha little interference and then repeated itself with noticeably more static. This followed recent activity on the station that included more static than usual and several instances of objects being moved/dropped. All of this was detected by amateur listeners and is unconfirmed at the moment.
On August 23, 2010 at 13:35 UTC, a voice speaking in Russian was detected. The voice read out a single, short transmission several times before the line went dead, then returned to its normal broadcast. As the message was transmitted on upper side-band, reception with ordinary AM receivers was weak and distorted.
The message, repeated twice, was: UVB-76, UVB-76 — 93 882 naimina 74 14 35 74 — 9 3 8 8 2 nikolai, anna, ivan, michail, ivan, nikolai, anna, 7, 4, 1, 4, 3, 5, 7, 4[11] (recording of the August 23 2010 voice transmission)
On August 24, 2010 at approximately 04:00 UTC, a heavily distorted voice was heard by amateur listeners.
On August 24, 2010 at 13:25 UTC, another heavily distorted voice was detected by several amateur listeners.
On August 24, 2010 at 17:43 UTC, Hard to hear voices were heard over the transmission.
On August 24, 2010 at around 03:30 UTC, distorted voices in addition to fast beeps and pulses were heard.
On August 25, 2010 around 06:13 UTC, Random knocks or shuffles as if someone is in the room, changes in tone randomly.
On August 25, 2010 at 11:53 GMT the following message was detected: "August 3 5 2 7 Accretion 3 6 0 9 5 6 7 3". A recording is available here mirror Said message is a Google Translate of 3 8 5 2 7 ???????? 3 6 0 9 5 6 7 3. This is identical to the August 25, 2010 06:54 UTC message mentioned below.
On August 25, 2010 at 06:45 UTC, A grumble or garbled sound appeared out of nowhere for 389 ms.
On August 25, 2010 at 06:54 UTC, Another transmission occurred. (Recording of the fifth voice transmission) A new sequence/pattern with a chirping/crank noise occured on top of the previous buzzer. At times this new noise made the old buzzing noise barely audible.The message content was: "UVB-76. UVB-76. 38, 527. ????????. 36, 09, 55, 73.".
On August 25, 2010 at 18:07 UTC, Morse code could be heard behind the buzzer signal. It lasted until approximately 18:20 UTC. At approximately 18:08 UTC A tone was heard in the background followed by a short message.
There is a lot of very interesting additional details at the Wikipedia website above.
Also courtesy of the Spooks list and Jakon Hays, the following associated links:
Saw a post on MeFi this morning about it.
http://www.metafilter.com/95091/4625-kHz
Which cites this site.
http://uvb-76.blogspot.com/2010/08/august-23-2010-935am-pst-voice.html
The wiki page has been updated quite a bit though the day.
http://en.wikipedia.org/wiki/UVB-76
And there is a live stream here.
http://www.justin.tv/rampageturke#/w/340896016/4
Saturday, August 14, 2010
Current status of the ROS digital mode use in the US
Earlier this year there was quite a bit of buzz on the amateur radio newsgroups about a new digital mode known as ROS developed by a non-ham, José Alberto Nieto Ros.
The new mode uses spread spectrum technology at 1 or 16 Baud signalling rates, and is designed to cope with disturbances, low level signals, meteor scatter and moon bounce says José. José claims that receiving signals down to -35 dB (!) with 1 Bd signalling rate and -30 dB (!) with 16 Bd are possible.
But we have a problem here in the US. ROS is a spread spectrum mode and US hams are not allowed to use SS modes below 222 MHz by FCC regulation. Another problem is that hams in other portions of the world are using this 2.2 kHz bandwidth mode in the portion of the ham bands reserved for narrowband comms. Again not a good thing.
On March 4, 2010 the following was posted to the ARRL website:
In mid-February, European amateurs first used a new, experimental digital mode known as ROS. On February 23, 2010 -- after FCC review of the original documents provided from the developer's Web site -- the FCC made the following statements on ROS:
"Section 97.305 is the rule that specifies where different emission types are allowed to be transmitted on different bands. 'ROS' is viewed as 'spread spectrum,' and the creator of the system describes it as that. We assume that he knows what he created. [Section] 97.305 authorizes spread spectrum emission types (defined in Section 97.3) to be transmitted by FCC licensed amateur stations at places we regulate communications only on 222-225 MHz and higher frequency amateur bands. European telecommunication regulatory authorities may authorize amateur stations in Europe to use SS on the HF bands, but this is of no concern to us. The Commission does not determine if a particular mode 'truly' represents spread spectrum as it is defined in the rules. The licensee of the station transmitting the emission is responsible for determining that the operation of the station complies with the rules. This would include determining the type of emission the station is transmitting and that the frequencies being used are authorized for that type of emission."
Since that initial FCC review, several Internet sites have reported a claim -- attributed to the FCC -- that the original statements made had been reconsidered and that the FCC view was now that "ROS cannot be viewed as Spread Spectrum and it would be encompassed within Section 97.309 (RTTY and data emissions codes)."
When queried about this new statement, the FCC's Consumer Assistance Office stated that "[T]he information contained on the ROS Web site was not provided by the FCC." They then reaffirmed the original statements that originated from the FCC's Wireless Bureau, which handles Amateur Radio rules for the US.
The ARRL supports -- as one of the basic purposes of Amateur Radio -- the experimentation and advancing the technical skills of operators. The development and use of any new mode is exciting to many amateurs, and the League encourage amateurs to experiment within the parameters of the rules; however, the ARRL also reminds US licensees that according to Section 97.307, spread spectrum communications are only permissible in the US on frequencies above 222 MHz.
Of course, the debate raged on the various newsgroups about the pros and cons, but soon the conversation slowly died off, until this week. Earlier in the week the conversation cranked up in earnest again about the legally of using ROS in the US on the 30MDG newsgroup. This was due to this post by José on his ROS website:
http://rosmodem.wordpress.com/2010/08/13/the-fcc-allows-ros-to-be-used-in-the-usa/
Instead of investigating the details of the post, a flame war erupted, and is still raging strong even this morning. So now I'm now waiting for the aluminum foil hats (or hard kats with rubber ducks in the middle) to come out and aliens to land in BTown.
Yes, José's choice of a headline was poor "The FCC allows ROS to be used in the USA," since it makes it sound like the FCC has cleared and approved the mode for general hams ops in the US. But the details are in the body of the post:
”The FCC allows ROS to be used in the USA” (only for WE9XLQ)
Instead of taking a pause and looking into the callsign on the FCC website which would have been the prudent thing to do, some gents blew up the situation into a full blown flame war. Theese folks should have their keyboards disabled and given a time out in one corner of their shacks. ;-)))
Now the real truth, WE8XLQ is a newly issued FCC experimental license issued to Reindert A Smit in Alta Loma, CA, to test the ROS mode in the HF spectrum. The license is valid from 8/1/2010 to 1/31/2011.
In the "Explanation" section of the license it states:
Like to use ROS Modem digital mode in Amateur Radio Service. Questions exist about the legality of this mode on frequencies below 225 MHz.
In the "Purpose of Operation" section of the license it states:
Experiment with this mode and research capabilities of this mode under weak signal conditions and make comparisons against other digital modes such as WSJT and PSK31
Complete details are available at the link below: https://fjallfoss.fcc.gov/oetcf/els/reports/STA_Print.cfm?mode=initial&application_seq=45235
So it will be interesting to see how all of this washes out. Personally other than the wideband nature of ROS being used in the narrowband section of the various bands, I don't see why the ARRL and FCC should have opposed the mode in the first place. There is a mode called Chip64/128 which is also described as spread spectrum (full details at http://xoomer.virgilio.it/aporcino/Chip64/index.htm) being used in the HF spectrum. I haven't seen anything being done to ban this mode on the HF spectrum by the FCC. It has been around since 2007.
Not sure why all the fuss over ROS and not CHIP64/128 by the FCC. I look forward to seeing the test results of the ROS mode from WE9XLQ early next year.
In the meantime, here is your caveat. Using the ROS mode on HF by US hams other than Reindert A Smit, WE9XLQ, is illegal. If you use it, you may lose it (your license that is).
The new mode uses spread spectrum technology at 1 or 16 Baud signalling rates, and is designed to cope with disturbances, low level signals, meteor scatter and moon bounce says José. José claims that receiving signals down to -35 dB (!) with 1 Bd signalling rate and -30 dB (!) with 16 Bd are possible.
But we have a problem here in the US. ROS is a spread spectrum mode and US hams are not allowed to use SS modes below 222 MHz by FCC regulation. Another problem is that hams in other portions of the world are using this 2.2 kHz bandwidth mode in the portion of the ham bands reserved for narrowband comms. Again not a good thing.
On March 4, 2010 the following was posted to the ARRL website:
In mid-February, European amateurs first used a new, experimental digital mode known as ROS. On February 23, 2010 -- after FCC review of the original documents provided from the developer's Web site -- the FCC made the following statements on ROS:
"Section 97.305 is the rule that specifies where different emission types are allowed to be transmitted on different bands. 'ROS' is viewed as 'spread spectrum,' and the creator of the system describes it as that. We assume that he knows what he created. [Section] 97.305 authorizes spread spectrum emission types (defined in Section 97.3) to be transmitted by FCC licensed amateur stations at places we regulate communications only on 222-225 MHz and higher frequency amateur bands. European telecommunication regulatory authorities may authorize amateur stations in Europe to use SS on the HF bands, but this is of no concern to us. The Commission does not determine if a particular mode 'truly' represents spread spectrum as it is defined in the rules. The licensee of the station transmitting the emission is responsible for determining that the operation of the station complies with the rules. This would include determining the type of emission the station is transmitting and that the frequencies being used are authorized for that type of emission."
Since that initial FCC review, several Internet sites have reported a claim -- attributed to the FCC -- that the original statements made had been reconsidered and that the FCC view was now that "ROS cannot be viewed as Spread Spectrum and it would be encompassed within Section 97.309 (RTTY and data emissions codes)."
When queried about this new statement, the FCC's Consumer Assistance Office stated that "[T]he information contained on the ROS Web site was not provided by the FCC." They then reaffirmed the original statements that originated from the FCC's Wireless Bureau, which handles Amateur Radio rules for the US.
The ARRL supports -- as one of the basic purposes of Amateur Radio -- the experimentation and advancing the technical skills of operators. The development and use of any new mode is exciting to many amateurs, and the League encourage amateurs to experiment within the parameters of the rules; however, the ARRL also reminds US licensees that according to Section 97.307, spread spectrum communications are only permissible in the US on frequencies above 222 MHz.
Of course, the debate raged on the various newsgroups about the pros and cons, but soon the conversation slowly died off, until this week. Earlier in the week the conversation cranked up in earnest again about the legally of using ROS in the US on the 30MDG newsgroup. This was due to this post by José on his ROS website:
http://rosmodem.wordpress.com/2010/08/13/the-fcc-allows-ros-to-be-used-in-the-usa/
Instead of investigating the details of the post, a flame war erupted, and is still raging strong even this morning. So now I'm now waiting for the aluminum foil hats (or hard kats with rubber ducks in the middle) to come out and aliens to land in BTown.
Yes, José's choice of a headline was poor "The FCC allows ROS to be used in the USA," since it makes it sound like the FCC has cleared and approved the mode for general hams ops in the US. But the details are in the body of the post:
Instead of taking a pause and looking into the callsign on the FCC website which would have been the prudent thing to do, some gents blew up the situation into a full blown flame war. Theese folks should have their keyboards disabled and given a time out in one corner of their shacks. ;-)))
Now the real truth, WE8XLQ is a newly issued FCC experimental license issued to Reindert A Smit in Alta Loma, CA, to test the ROS mode in the HF spectrum. The license is valid from 8/1/2010 to 1/31/2011.
In the "Explanation" section of the license it states:
Like to use ROS Modem digital mode in Amateur Radio Service. Questions exist about the legality of this mode on frequencies below 225 MHz.
In the "Purpose of Operation" section of the license it states:
Experiment with this mode and research capabilities of this mode under weak signal conditions and make comparisons against other digital modes such as WSJT and PSK31
Complete details are available at the link below: https://fjallfoss.fcc.gov/oetcf/els/reports/STA_Print.cfm?mode=initial&application_seq=45235
So it will be interesting to see how all of this washes out. Personally other than the wideband nature of ROS being used in the narrowband section of the various bands, I don't see why the ARRL and FCC should have opposed the mode in the first place. There is a mode called Chip64/128 which is also described as spread spectrum (full details at http://xoomer.virgilio.it/aporcino/Chip64/index.htm) being used in the HF spectrum. I haven't seen anything being done to ban this mode on the HF spectrum by the FCC. It has been around since 2007.
Not sure why all the fuss over ROS and not CHIP64/128 by the FCC. I look forward to seeing the test results of the ROS mode from WE9XLQ early next year.
In the meantime, here is your caveat. Using the ROS mode on HF by US hams other than Reindert A Smit, WE9XLQ, is illegal. If you use it, you may lose it (your license that is).
Thursday, August 12, 2010
Perseid Meteor Shower
The annual Perseid meteor shower is underway. Earth is passing through a wide stream of debris from Comet Swift-Tuttle, and each time a fleck of comet dust hits Earth's atmosphere--flash!--there is a meteor. Forecasters say the shower will peak on Thursday, August 12th, and Friday, August 13th. You can see Perseids flitting across the sky at any time between about 10 pm on Thursday evening and sunrise on Friday morning. Observers who get away from city lights can expect to count dozens of meteors per hour, especially during the dark hours before dawn. http://spaceweather.com
Time to dust off my meteor scatter software and head up to 6 meters for some ping time from EM85.
Time to dust off my meteor scatter software and head up to 6 meters for some ping time from EM85.
Tuesday, August 03, 2010
Solar Tsunami to Strike Earth
NASA's Solar Dynamics Observatory snapped this X-ray photo of the Sun early in the morning of Sunday, August 1st. The dark arc near the top right edge of the image is a filament of plasma blasting off the surface -- part of the coronal mass ejection. The bright region is an unassociated solar flare. NASAFrom FoxNews:
Earth is bracing for a cosmic tsunami Tuesday night as tons of plasma from a massive solar flare head directly toward the planet.
The Sun's surface erupted early Sunday morning, shooting a wall of ionized atoms directly at Earth, scientists say. It is expected to create a geomagnetic storm and a spectacular light show -- and it could pose a threat to satellites in orbit, as well.
"This eruption is directed right at us and is expected to get here early in the day on Aug. 4," said Leon Golub of the Harvard-Smithsonian Center for Astrophysics. "It's the first major Earth-directed eruption in quite some time."
The solar eruption, called a coronal mass ejection, was spotted by NASA's Solar Dynamics Observatory, which captures high-definition views of the sun at a variety of wavelengths. SDO was launched in February and peers deep into the layers of the sun, investigating the mysteries of its inner workings.
"We got a beautiful view of this eruption," Golub said. "And there might be more beautiful views to come if it triggers aurorae."
Views of aurorae are usually associated with Canada and Alaska, but even skywatchers in the northern U.S. mainland are being told they can look toward the north Tuesday and Wednesday evenings for rippling "curtains" of green and red light.
When a coronal mass ejection reaches Earth, solar particles stream down our planet's magnetic field lines toward the poles. In the process, the particles collide with atoms of nitrogen and oxygen in the Earth's atmosphere, which then glow, creating an effect similar to miniature neon signs.
The interaction of the solar particles with our planet's magnetic field has the potential to create geomagnetic storms, or disturbances, in Earth's magnetosphere. And while aurorae are normally visible only at high latitudes, they can light up the sky even at lower latitudes during a geomagnetic storm.
Fortunately for Earth-bound observers, the atmosphere filters out nearly all of the radiation from the solar blast. The flare shouldn't pose a health hazard, Golub told FoxNews.com.
"It's because of our atmosphere," he explained, "which absorbs the radiation, as well as the magnetic field of the Earth, which deflects any magnetic particles produced."
The radiation "almost never" makes it to ground, he noted, though pilots and passengers in airplanes may experience increased radiation levels akin to getting an X-ray.
The solar particles also could affect satellites, though scientists think that possibility is remote. Orbital Sciences Corp. believe a similar blast may have knocked its Galaxy 15 satellite permanently out of action this year.
This type of solar event has both government officials and satellite manufacturers worrying.
NASA scientists warned recently that high-energy electric pulses from the sun could cripple our electrical grid for years, causing billions in damages. In fact, the House is so concerned that the Energy and Commerce committee voted unanimously to approve a bill allocating $100 million to protect the energy grid from this rare but potentially devastating occurrence.
The sun's activity usually ebbs and flows on a fairly predictable cycle. Typically, a cycle lasts about 11 years, taking roughly 5.5 years to move from a solar minimum, a period of time when there are few sunspots, to peak at the solar maximum, during which sunspot activity is amplified.
The last solar maximum occurred in 2001. The latest minimum was particularly weak and long- lasting.
The most recent solar eruption is one of the first signs that the sun is waking up -- and heading toward another maximum.
Space.com contributed to this report.
Propagation Alert: Will it hit Earth?
On August 1, 2010, the Solar Dynamics Observatory (SDO) observed a beautiful prominence eruption that may hit Earth and cause a geomagnetic storm. As the solar cycle progresses and the Sun becomes more active there will be many more opportunities to observe the causes of space weather. Want to see what happens? Follow the event at spaceweather.com.
And from the Spaceweather website:
On August 1st, the entire Earth-facing side of the sun erupted in a tumult of activity. There was a C3-class solar flare, a solar tsunami, multiple filaments of magnetism lifting off the stellar surface, large-scale shaking of the solar corona, radio bursts, a coronal mass ejection and more.
High-latitude sky watchers should be alert for auroras tonight. One and possibly two coronal mass ejections (CMEs) are heading toward Earth, propelled by the solar eruptions of August 1st (see below). NOAA forecasters estimate a 10% chance of major geomagnetic storms and a 45% chance of at least some geomagnetic activity when the clouds arrive on August 3rd and 4th.
And finally this report from our good friend Tomas Hood
At approximately 0855 UTC on August 1, 2010, a C3.2 magnitude soft X-ray flare erupted from NOAA Active Sunspot Region 11092 (1092).
At nearly the same time, a massive filament eruption occurred. Prior to the filament's eruption, NASA's Solar Dynamics Observatory (SDO) Atmospheric Imaging Assembly (AIA) instruments revealed an enormous plasma filament stretching across the sun's northern hemisphere. When the solar shock wave triggered by the C3.2-class X-ray explosion plowed through this filament, it appears to have caused the filament to erupt, sending out a huge plasma cloud (a coronal mass ejection, or CME).
A shock wave can be seen emerging from the origin of the X-ray flare and sweeping across the sun's northern hemisphere into the filament field. The impact of this shock wave may well have propelled the filament into space. The movies (see links, below) seem to support the conclusion that both eruptions, occurring together, are linked, despite the approximately 400,000 kilometer distance between the flare and the filament eruption. How can this be? While we cannot always see the magnetic field lines between solar features (magnetic field lines are not visible unless there is plasma trapped along these field lines), we can assume from this event
that huge connecting field lines existed between the sunspot region and the filament in the sun's northern hemisphere.
This is an amazing event. A complex series of eruptions involving most of the visible surface of the sun has occurred, ejecting plasma toward the Earth. This coronal mass ejection (CME) rides the solar wind. Depending on the speed of the solar wind and the ejected plasma, this cloud will reach Earth's magnetosphere sometime between August 3 and August 5. High-latitude sky watchers should be alert for auroras. Radio communications by way of the ionosphere may become degraded soon after the CME arrives, and the degraded conditions may last for up to three days.
First view at the 304-Angstrom wavelength by SDO/AIA:
http://www.youtube.com/watch?v=VyaqxKkSCpU
Second view at the 171-Angstrom wavelength by SDO/AIA:
http://www.youtube.com/watch?v=HW_-yQY6YlA
Source: SDO/AIA
73 de NW7US, Tomas David Hood ( http://tomas-david-hood.com/ )
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Monday, August 02, 2010
Complex Eruption on the Sun
Space Weather News for August 1, 2010
http://spaceweather.com
GLOBAL ERUPTION: During the early hours of August 1st, NASA's Solar Dynamics Observatory recorded a complex global disturbance on the Earth-facing side of the sun. Most of the sun's northern hemisphere was involved in the event, which included a long-duration C3-class solar flare, a "solar tsunami," and a massive filament eruption. As a result of these blasts, a coronal mass ejection (CME) is heading toward Earth. High-latitude geomagnetic storms and auroras are possible when the cloud arrives a few days hence.
On August 1st around 0855 UT, Earth orbiting satellites detected a C3-class solar flare. The origin of the blast was sunspot 1092. At about the same time, an enormous magnetic filament stretching across the sun's northern hemisphere erupted. NASA's Solar Dynamics Observatory recorded the action.
The timing of these events suggest they are connected, and a review of SDO movies strengthens that conclusion. Despite the ~400,000 km distance between them, the sunspot and filament seem to erupt together; they are probably connected by long-range magnetic fields.
In short, we have just witnessed a complex global eruption involving almost the entire Earth-facing side of the sun.
A coronal mass ejection (CME) produced by the event is heading directly for Earth. High-latitude sky watchers should be alert for auroras when it arrives on or about August 3rd. See forecast below.
3-day Solar-Geophysical Forecast issued Aug 01 22:00 UTC
Solar Activity Forecast: Solar activity is expected to be very low. However, there is a chance for an isolated C-class flare from Region 1092.
Geophysical Activity Forecast: Geomagnetic field activity is expected to be at quiet levels during most of day 1 (02 August). An increase to unsettled to active levels is expected late on day 1 due to the arrival of the full-halo CME observed on 01 August. Activity is expected to increase to unsettled to active levels with a chance for minor storm levels on day 2 (03 August) as CME effects persist. Activity is expected to decrease to quiet to unsettled levels with a chance for active levels on day 3 (04 August) as CME effects subside.
http://spaceweather.com
GLOBAL ERUPTION: During the early hours of August 1st, NASA's Solar Dynamics Observatory recorded a complex global disturbance on the Earth-facing side of the sun. Most of the sun's northern hemisphere was involved in the event, which included a long-duration C3-class solar flare, a "solar tsunami," and a massive filament eruption. As a result of these blasts, a coronal mass ejection (CME) is heading toward Earth. High-latitude geomagnetic storms and auroras are possible when the cloud arrives a few days hence.
On August 1st around 0855 UT, Earth orbiting satellites detected a C3-class solar flare. The origin of the blast was sunspot 1092. At about the same time, an enormous magnetic filament stretching across the sun's northern hemisphere erupted. NASA's Solar Dynamics Observatory recorded the action.
The timing of these events suggest they are connected, and a review of SDO movies strengthens that conclusion. Despite the ~400,000 km distance between them, the sunspot and filament seem to erupt together; they are probably connected by long-range magnetic fields.
In short, we have just witnessed a complex global eruption involving almost the entire Earth-facing side of the sun.
A coronal mass ejection (CME) produced by the event is heading directly for Earth. High-latitude sky watchers should be alert for auroras when it arrives on or about August 3rd. See forecast below.
3-day Solar-Geophysical Forecast issued Aug 01 22:00 UTC
Solar Activity Forecast: Solar activity is expected to be very low. However, there is a chance for an isolated C-class flare from Region 1092.
Geophysical Activity Forecast: Geomagnetic field activity is expected to be at quiet levels during most of day 1 (02 August). An increase to unsettled to active levels is expected late on day 1 due to the arrival of the full-halo CME observed on 01 August. Activity is expected to increase to unsettled to active levels with a chance for minor storm levels on day 2 (03 August) as CME effects persist. Activity is expected to decrease to quiet to unsettled levels with a chance for active levels on day 3 (04 August) as CME effects subside.
Monday, July 19, 2010
HomePatrol-1 - What can it monitor?
I have had several questions regarding what HomePatrol will and will not monitor from the Radioref database. Paul Opitz from Uniden recently wrote the following:
HomePatrol-1 includes all systems and channels in Radio Reference database with the following exceptions:
-- Channels function tagged as Data
-- Channels that are not function tagged
-- Channels function tagged as Deprecated
-- Channels with a mode of "E" (encrypted)
-- Digital channels on system types that cannot be monitored (i.e. ProVoice)
-- Channels in deprecated systems
-- Unmonitorable Systems (i.e. OpenSky / Nextel / etc)
HomePatrol-1 can automatically select for scanning any channel that is properly geotagged. Channels not geotagged can be manually selected (easiest by using the included Sentinel PC software). The geographic selection process is unique to Uniden (and patented, to boot).
At some point, Joes (scanner geeks), will have the ability through the Uniden software to program the HomePatrol-1 with their own frequency list, but this won't happen with the initial release of the unit.
HomePatrol-1 includes all systems and channels in Radio Reference database with the following exceptions:
-- Channels function tagged as Data
-- Channels that are not function tagged
-- Channels function tagged as Deprecated
-- Channels with a mode of "E" (encrypted)
-- Digital channels on system types that cannot be monitored (i.e. ProVoice)
-- Channels in deprecated systems
-- Unmonitorable Systems (i.e. OpenSky / Nextel / etc)
HomePatrol-1 can automatically select for scanning any channel that is properly geotagged. Channels not geotagged can be manually selected (easiest by using the included Sentinel PC software). The geographic selection process is unique to Uniden (and patented, to boot).
At some point, Joes (scanner geeks), will have the ability through the Uniden software to program the HomePatrol-1 with their own frequency list, but this won't happen with the initial release of the unit.
Sunday, July 18, 2010
Uniden HomePatrol Update
Recently some question on the Scan-DC newsgroup came up on the new Uniden HomePatrol scanner. here is a portion of my comments regarding this new scanner.
My initial testing of the unit is pretty cool. The manuals aren't done yet, but if you have every programmed any scanner you don't need one, it is that simple. So folks who do not want to become radio engineers (Uniden calls them Bob and Mabel) will want to purchase this scanner. There will be additional features for advanced users that will be activated in the near future so that power users (Uniden calls them Joe) will have some interesting features they will like in HomePatrol. On the Friday before the Uniden Open House during our formal intro of the product, I had the scanner in my hands about one hour and during that time I master the basica operations and menuing system (actually it took about 20 minutes).
Saturday during the Uniden Open House in Dallas, an 8 year old grandson of one of the hobbyists at my table (I was a table host), programmed the HP scanner for DFW in literally seconds. Yes, Bob and Mabel, it is really that easy.
You can read some of my additional thoughts on my personal blog at
http://monitor-post.blogspot.com/2010/06/revolution-in-scanning-is-coming.html
You can get my exclusive HP spec sheet (based on the testing of the unit we
have in hand) on the Grove Ent website at http://www.grove-ent.com/homepatrol.html
More to come including a full review in Monitoring Times magazine soon.
My initial testing of the unit is pretty cool. The manuals aren't done yet, but if you have every programmed any scanner you don't need one, it is that simple. So folks who do not want to become radio engineers (Uniden calls them Bob and Mabel) will want to purchase this scanner. There will be additional features for advanced users that will be activated in the near future so that power users (Uniden calls them Joe) will have some interesting features they will like in HomePatrol. On the Friday before the Uniden Open House during our formal intro of the product, I had the scanner in my hands about one hour and during that time I master the basica operations and menuing system (actually it took about 20 minutes).
Saturday during the Uniden Open House in Dallas, an 8 year old grandson of one of the hobbyists at my table (I was a table host), programmed the HP scanner for DFW in literally seconds. Yes, Bob and Mabel, it is really that easy.
You can read some of my additional thoughts on my personal blog at
http://monitor-post.blogspot.com/2010/06/revolution-in-scanning-is-coming.html
You can get my exclusive HP spec sheet (based on the testing of the unit we
have in hand) on the Grove Ent website at http://www.grove-ent.com/homepatrol.html
More to come including a full review in Monitoring Times magazine soon.
Saturday, July 17, 2010
This Week on the Radio July 15, 2010
From the ARRL : This week, the North American QSO Party (RTTY), the DMC RTTY Contest and the CQ Worldwide VHF Contest are July 17-18. The Run for the Bacon QRP Contest is July 19. Next week, there is another running of the NCCC Sprint Ladder on July 23. The RSGB Islands on the Air (IOTA) Contest is July 24-25 and the SKCC Sprint July 28. All dates, unless otherwise stated, are UTC. See the ARRL Contest Branch page, the ARRL Contest Update and the WA7BNM Contest Calendar for more info. Looking for a Special Event station? Be sure to check out the ARRL Special Events Station Web page.
Thursday, July 15, 2010
SSTV from ISS on 145.800 MHz FM during July 15-16
ISS Amateur Radio Status: July 13, 2010
SpaceCam planed for July 15-16 By Miles Mann WF1F
MAREX-MG News www.marexmg.org
Manned Amateur Radio Experiment
Notes from the Ariss blog http://ariss-sstv.blogspot.com/
SpaceCam planed for July 15-16 By Miles Mann WF1F
MAREX-MG News www.marexmg.org
Manned Amateur Radio Experiment
Notes from the Ariss blog http://ariss-sstv.blogspot.com/
MAI-75 activation planned for July 15-16 (updated)
An activity to support SSTV activation (MAI-75) has been schedule on July 15 and 16. Times fall between 12:00-15:00 UTC on the 15th and 10:00-12:00 UTC on the 16th . The system will be operating space cam in slide show mode and is expected to use the Martin 1 format. The times are just over 1 orbit each day (two passes over Moscow) so opportunities will be very limited.
Tips for Working Slow Scan TV:
Tips for Working Slow Scan TV:
Will I be able to receive images from SpaceCam1?
Yes! SpaceCam1 will transmit and receive images on amateur radio frequencies, using standard SSTV formats. Although SpaceCam1 is capable of operating in several modes, the recommended format while in Slide Show mode is Robot 36. This format offers the best standard compromise between image quality and transmission time and heat stress.
In addition to two-way "interactive" operation, SpaceCam1 provides the following fully automatic functions:
-- Transmission from a live camera or disk at specified intervals
-- “Slide Show" operation from a set of images stored on the system
-- SSTV Repeater
What equipment will I need to receive the images?
Radio receiver with an outdoor antenna. The radio receive will need to be able to receive FM signals on 145.800 MHz radio band. A PC with SSTV software or a dedicated SSTV scan converter.
For information on how to receive SSTV images from the International Space station, check out the MAREX link: http://www.marexmg.org/fileshtml/howtouseiss.html
Over the next few weeks we maybe receiving images from the International Space station via Slow Scan TV (SSTV). The MAREX team will be collecting these images from the amateur Radio and SWL community and we will post the best.
We would like to collect all images received. However in order to properly catalog the images we request you use the following image naming format. After you receive you images; please rename the images using the following format, All Lower case letters
Year 06, Month 07, Day 31, (UTC time), Call sign, Short text description, .JPG
Example:
New format: 0607311905wf1f.jpg
I removed the first two numbers of the year and the “Z” for UTC time. All dates are assumed to be in UTC dates. The images coming down from ISS will also have a time stamp embedded into the image. You can also use these numbers to generate you file names. If you are a Short Wave listener and do not have a call sign, just place your Initials after the time (0607311905abc.jpg)
If we break this down
Year =06
Month = 07
Day = 31
Time = 1905 UTC
Call sign = wf1f
Description (optional) = Windows shot
Image format = jpg
Image Quality
Please do not put any text over lays on the images, Example, do not put web page or advertisements in the image. Your own call sign and date are acceptable.
Send all images directly to MAREX at Marexmg@comcast.net
We would also like to know the following information in your email.
Name or Call sign
Country / State
Receiver
Software decoding tool
Elevation or range of ISS when you decoded the image.
Slide Show Mode:
The MAREX SpaceCam1 software contains a feature called “Slide Show” mode. It allows the crew to preload a directory full of images that will be automatically transmitted to Earth. The crew will not need to keep pushing a button to send images. In theory the system can run for weeks at a time without crew involvement. The SpaceCam project will be able to transmit over 200 SSTV images per day (Robot 36 format).
Ariss has not announced any plans for a SSTV Uplink frequency.
SSTV Decoding Software http://www.barberdsp.com/
There are many choices in SSTV software, some Free, others with more features cost a few bucks. http://www.marexmg.org/fileshtml/sstvlinkpage.html
So have fun, find your best setup and start practicing (on Earth) how to decode SSTV on 2-meters.
Marexmg Web page
http://www.marexmg.org/
ARISS Web page and other great Space projects
http://www.rac.ca/ariss/
73 Miles WF1F MAREX-MG
Yes! SpaceCam1 will transmit and receive images on amateur radio frequencies, using standard SSTV formats. Although SpaceCam1 is capable of operating in several modes, the recommended format while in Slide Show mode is Robot 36. This format offers the best standard compromise between image quality and transmission time and heat stress.
In addition to two-way "interactive" operation, SpaceCam1 provides the following fully automatic functions:
-- Transmission from a live camera or disk at specified intervals
-- “Slide Show" operation from a set of images stored on the system
-- SSTV Repeater
What equipment will I need to receive the images?
Radio receiver with an outdoor antenna. The radio receive will need to be able to receive FM signals on 145.800 MHz radio band. A PC with SSTV software or a dedicated SSTV scan converter.
For information on how to receive SSTV images from the International Space station, check out the MAREX link: http://www.marexmg.org/fileshtml/howtouseiss.html
Over the next few weeks we maybe receiving images from the International Space station via Slow Scan TV (SSTV). The MAREX team will be collecting these images from the amateur Radio and SWL community and we will post the best.
We would like to collect all images received. However in order to properly catalog the images we request you use the following image naming format. After you receive you images; please rename the images using the following format, All Lower case letters
Year 06, Month 07, Day 31, (UTC time), Call sign, Short text description, .JPG
Example:
New format: 0607311905wf1f.jpg
I removed the first two numbers of the year and the “Z” for UTC time. All dates are assumed to be in UTC dates. The images coming down from ISS will also have a time stamp embedded into the image. You can also use these numbers to generate you file names. If you are a Short Wave listener and do not have a call sign, just place your Initials after the time (0607311905abc.jpg)
If we break this down
Year =06
Month = 07
Day = 31
Time = 1905 UTC
Call sign = wf1f
Description (optional) = Windows shot
Image format = jpg
Image Quality
Please do not put any text over lays on the images, Example, do not put web page or advertisements in the image. Your own call sign and date are acceptable.
Send all images directly to MAREX at Marexmg@comcast.net
We would also like to know the following information in your email.
Name or Call sign
Country / State
Receiver
Software decoding tool
Elevation or range of ISS when you decoded the image.
Slide Show Mode:
The MAREX SpaceCam1 software contains a feature called “Slide Show” mode. It allows the crew to preload a directory full of images that will be automatically transmitted to Earth. The crew will not need to keep pushing a button to send images. In theory the system can run for weeks at a time without crew involvement. The SpaceCam project will be able to transmit over 200 SSTV images per day (Robot 36 format).
Ariss has not announced any plans for a SSTV Uplink frequency.
SSTV Decoding Software http://www.barberdsp.com/
There are many choices in SSTV software, some Free, others with more features cost a few bucks. http://www.marexmg.org/fileshtml/sstvlinkpage.html
So have fun, find your best setup and start practicing (on Earth) how to decode SSTV on 2-meters.
Marexmg Web page
http://www.marexmg.org/
ARISS Web page and other great Space projects
http://www.rac.ca/ariss/
73 Miles WF1F MAREX-MG
Amateur satellite to investigate power line interference
Hans van de Groenendaal ZS6AKV will be giving a presentation on South Africa's first CubeSat at the AMSAT-UK Colloquium in Guildford, England, July 31- Aug 1
The world has experienced a long solar minimum which means that ionospheric communication had been very limited and for a few years was almost exclusively the domain of the commercial broadcasters running Megawatts.
HF radio communication is very susceptible to noise levels that are created by power lines, electrical installations and overhead lines used by trains and busses and power line telecommunication systems. If fact today there are many installation that do not necessarily comply with internationally agreed emission standards. With increasing solar activity interference signals are propagated over large areas and will interfere with HF communication.
The important mission of the SA AMSAT CubeSat is to measure the High Frequency noise levels over South Africa and report these measurement back to a ground station for analysis and action to reduce these unwanted signals. The information from the tiny satellite will identify the areas where the HF frequency polluters are situated and will help in reducing or eliminating the source.
It is also hoped to include a 30 kHz linear transponder and an Automatic Packet Reporting System (APRS) in the CubeSat.
I want one. After the South Africans have done their mapping maybe they can swing it up here to help locate our local power line interference.
The world has experienced a long solar minimum which means that ionospheric communication had been very limited and for a few years was almost exclusively the domain of the commercial broadcasters running Megawatts.
HF radio communication is very susceptible to noise levels that are created by power lines, electrical installations and overhead lines used by trains and busses and power line telecommunication systems. If fact today there are many installation that do not necessarily comply with internationally agreed emission standards. With increasing solar activity interference signals are propagated over large areas and will interfere with HF communication.
The important mission of the SA AMSAT CubeSat is to measure the High Frequency noise levels over South Africa and report these measurement back to a ground station for analysis and action to reduce these unwanted signals. The information from the tiny satellite will identify the areas where the HF frequency polluters are situated and will help in reducing or eliminating the source.
It is also hoped to include a 30 kHz linear transponder and an Automatic Packet Reporting System (APRS) in the CubeSat.
I want one. After the South Africans have done their mapping maybe they can swing it up here to help locate our local power line interference.
Thursday, July 08, 2010
Mississippi Deploys Wireless Radio System To Aid Oil Spill Cleanup
From the Gov Monitor website:
Governor Haley Barbour announced today the distribution of more than 200 radios capable of operating through the Mississippi Wireless Integrated Network to help in the oil spill cleanup along Mississippi’s shoreline and barrier islands.
The MSWIN system, which provides interoperable communication for emergency responders, was created under the direction of Governor Barbour after Hurricane Katrina exposed a critical need.
“Immediately after the storm, we were unable to exchange critical information between various law enforcement agencies and other emergency personnel,” Governor Barbour said. “The ability to communicate can make a huge difference in our ability to fight the oil from the Deepwater Horizon oil spill now, and in the future, it could mean the difference in our ability to save lives in an emergency.”
The MSWIN system allows users to speak through a secure digital radio system operating under the Mississippi Wireless Communications Commission. The Mississippi National Guard, United States Coast Guard and the Mississippi Emergency Management Agency will use the hand-held radios to guide cleanup vessels to oil in the water sighted by aircraft.
“This will help streamline response time to any reports of oil from Mississippi National Guard air operations,” said MEMA Director and WCC Vice Chairman Mike Womack. “The vessels assigned to a particular area will now have the capability to communicate directly with the resources in the air.”
“Interoperability is about breaking down communication barriers,” said WCC Chairman Chris Epps. “This is what the system is designed for, and we are proud that we can assist with and improve the response efforts in the oil disaster.”
The MSWIN system was established with $157 million in federal funds and $57 million in state bond funds. The MSWIN system is currently fully operational in the southern third of the state and is scheduled to be complete throughout the entire state of Mississippi by December of 2011.
Governor Barbour has asked for nearly $84 million more in federal funding to expand the MSWIN system’s broadband capacity beyond voice-only communications. The upgraded system could include photo and ambulance-to-hospital data transmission abilities.
Col. Lee Smithson, who oversees the Mississippi National Guard’s response to the oil spill as commander of Task Force Vigilant Horizon, said the radios will enable National Guard personnel to guide crews to the oil and allow ground crews to document the sightings.
“The radios enable us to fully leverage the capabilities of all supporting agencies. We tie in air, marine and shore activities using one system. It is a game changer in our favor.”
Governor Haley Barbour announced today the distribution of more than 200 radios capable of operating through the Mississippi Wireless Integrated Network to help in the oil spill cleanup along Mississippi’s shoreline and barrier islands.
The MSWIN system, which provides interoperable communication for emergency responders, was created under the direction of Governor Barbour after Hurricane Katrina exposed a critical need.
“Immediately after the storm, we were unable to exchange critical information between various law enforcement agencies and other emergency personnel,” Governor Barbour said. “The ability to communicate can make a huge difference in our ability to fight the oil from the Deepwater Horizon oil spill now, and in the future, it could mean the difference in our ability to save lives in an emergency.”
The MSWIN system allows users to speak through a secure digital radio system operating under the Mississippi Wireless Communications Commission. The Mississippi National Guard, United States Coast Guard and the Mississippi Emergency Management Agency will use the hand-held radios to guide cleanup vessels to oil in the water sighted by aircraft.
“This will help streamline response time to any reports of oil from Mississippi National Guard air operations,” said MEMA Director and WCC Vice Chairman Mike Womack. “The vessels assigned to a particular area will now have the capability to communicate directly with the resources in the air.”
“Interoperability is about breaking down communication barriers,” said WCC Chairman Chris Epps. “This is what the system is designed for, and we are proud that we can assist with and improve the response efforts in the oil disaster.”
The MSWIN system was established with $157 million in federal funds and $57 million in state bond funds. The MSWIN system is currently fully operational in the southern third of the state and is scheduled to be complete throughout the entire state of Mississippi by December of 2011.
Governor Barbour has asked for nearly $84 million more in federal funding to expand the MSWIN system’s broadband capacity beyond voice-only communications. The upgraded system could include photo and ambulance-to-hospital data transmission abilities.
Col. Lee Smithson, who oversees the Mississippi National Guard’s response to the oil spill as commander of Task Force Vigilant Horizon, said the radios will enable National Guard personnel to guide crews to the oil and allow ground crews to document the sightings.
“The radios enable us to fully leverage the capabilities of all supporting agencies. We tie in air, marine and shore activities using one system. It is a game changer in our favor.”
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