Friday, May 29, 2009

New Solar Cycle 24 Prediction

Courtesy of NASA Science News, Author: Dr. Tony Phillips | Credit: Science@NASA

An international panel of experts led by NOAA and sponsored by NASA has released a new prediction for the next solar cycle. Solar Cycle 24 will peak, they say, in May 2013 with a below-average number of sunspots.

"If our prediction is correct, Solar Cycle 24 will have a peak sunspot number of 90, the lowest of any cycle since 1928 when Solar Cycle 16 peaked at 78," says panel chairman Doug Biesecker of the NOAA Space Weather Prediction Center.

It is tempting to describe such a cycle as "weak" or "mild," but that could give the wrong impression.

"Even a below-average cycle is capable of producing severe space weather," points out Biesecker. "The great geomagnetic storm of 1859, for instance, occurred during a solar cycle of about the same size we’re predicting for 2013."

The 1859 storm--known as the "Carrington Event" after astronomer Richard Carrington who witnessed the instigating solar flare--electrified transmission cables, set fires in telegraph offices, and produced Northern Lights so bright that people could read newspapers by their red and green glow. A recent report by the National Academy of Sciences found that if a similar storm occurred today, it could cause $1 to 2 trillion in damages to society's high-tech infrastructure and require four to ten years for complete recovery. For comparison, Hurricane Katrina caused "only" $80 to 125 billion in damage.



Above: This plot of sunspot numbers shows the measured peak of the last solar cycle in blue and the predicted peak of the next solar cycle in red. Credit: NOAA/Space Weather Prediction Center.

The latest forecast revises an earlier prediction issued in 2007. At that time, a sharply divided panel believed solar minimum would come in March 2008 followed by either a strong solar maximum in 2011 or a weak solar maximum in 2012. Competing models gave different answers, and researchers were eager for the sun to reveal which was correct.

"It turns out that none of our models were totally correct," says Dean Pesnell of the Goddard Space Flight Center, NASA's lead representative on the panel. "The sun is behaving in an unexpected and very interesting way."

Researchers have known about the solar cycle since the mid-1800s. Graphs of sunspot numbers resemble a roller coaster, going up and down with an approximately 11-year period. At first glance, it looks like a regular pattern, but predicting the peaks and valleys has proven troublesome. Cycles vary in length from about 9 to 14 years. Some peaks are high, others low. The valleys are usually brief, lasting only a couple of years, but sometimes they stretch out much longer. In the 17th century the sun plunged into a 70-year period of spotlessness known as the Maunder Minimum that still baffles scientists.



Above: Yearly-averaged sunspot numbers from 1610 to 2008. Researchers believe upcoming Solar Cycle 24 will be similar to the cycle that peaked in 1928, marked by a red arrow. Credit: NASA/MSFC

Right now, the solar cycle is in a valley--the deepest of the past century. In 2008 and 2009, the sun set Space Age records for low sunspot counts, weak solar wind, and low solar irradiance. The sun has gone more than two years without a significant solar flare.

"In our professional careers, we've never seen anything quite like it," says Pesnell. "Solar minimum has lasted far beyond the date we predicted in 2007."

In recent months, however, the sun has begun to show timorous signs of life. Small sunspots and "proto-sunspots" are popping up with increasing frequency. Enormous currents of plasma on the sun’s surface ("zonal flows") are gaining strength and slowly drifting toward the sun’s equator. Radio astronomers have detected a tiny but significant uptick in solar radio emissions. All these things are precursors of an awakening Solar Cycle 24 and form the basis for the panel's new, almost unanimous forecast.

According to the forecast, the sun should remain generally calm for at least another year. From a research point of view, that's good news because solar minimum has proven to be more interesting than anyone imagined. Low solar activity has a profound effect on Earth’s atmosphere, allowing it to cool and contract. Space junk accumulates in Earth orbit because there is less aerodynamic drag. The becalmed solar wind whips up fewer magnetic storms around Earth's poles. Cosmic rays that are normally pushed back by solar wind instead intrude on the near-Earth environment. There are other side-effects, too, that can be studied only so long as the sun remains quiet.

Meanwhile, the sun pays little heed to human committees. There could be more surprises, panelists acknowledge, and more revisions to the forecast.

"Go ahead and mark your calendar for May 2013," says Pesnell. "But use a pencil."

Wednesday, May 27, 2009

HOT SPOT DXING- Monitoring North and South Korea on shortwave radio

North Korea has responded to international condemnation of its nuclear test and a threat of new U.N. sanctions by saying it is no longer bound by an armistice signed with South Korea at the end of the 1950-53 Korean War, in essence, we are now back at a state of war with North Korea.

For complete Shortwave Broadcast schedules for both North and South Korea, see our Shortwave Central Blog at http://mt-shortwave.blogspot.com/2009/05/hot-spot-dxing-monitoring-north-and.html

See the Reuters story at
http://in.reuters.com/article/worldNews/idINIndia-39913120090527

North Korea Threatens Armed Strike, End to Armistice, see Bloomberg story at
http://www.bloomberg.com/apps/news?pid=20601087&sid=awBTCPe7S2gw&refer=worldwide

NKorea threatens to attack US, SKorean warships, see AP story athtp://apnews.myway.com/article/20090527/D98EKAHG0.html

Tuesday, May 26, 2009

Very Rare VHF/UHF Grid to Activate in South Louisiana -- EL58


Courtesy of the Ohio/Penn DX Bulletin #907.

K5, UNITED STATES (6m/Grid/LH/USI Op). Members of the "EL58 Grid ActivationGroup" will be active as K5N between May 29-31st (1700-1700z). Activitywill be from the sandy beach facing the Gulf of Mexico in Grid SquareEL58hx, ARLHS USA 1101 under the "Visual Site Rule" and a New USI Island(USI LA105S - Burwood Island, LA) (South West Pass). The operation will be6 meters ONLY, consist of 2 stations with both SSB/CW, and M/S capability,two 6M5 antennas, and 6 operators. Power out will be approximately 200W.Operating frequencies are: 50.100/CW, 50.150/SSB and 50.315 Meteor Scatter.QSL via: Joey Fierro II, 1054 Cajun Ln, Magnolia, MS 39652. Operatorsmentioned are: Al/WA4EWV, Bill/K5YG, Bob/WN2E, Bruce/N5SIX, Daniel/KE5KDMand Danny/N5OMG.

Visit their Web pages at: http://www.kcvhfgridbandits.com/kc_vhf_grid_bandits_018.htmhttp://w4abc.com/K5N.html

And this note from Danny N5OMG, one of the gang heading to south Louisiana:

It is less than a week till our operation in EL58 and we have updated our website with some interesting items. Our video from the scouting trip and the info regarding the lighthouse and island we will be activating on HF has been updated. It should be very lively down there.

At this time, all transportation has been finalized, our group members are consolidating the items for departure, and our last few conference calls will be later this week to tie up any loose ends. Our internet should be ready when we get there, so we will be monitoring both pingjockey and packetcluster nodes.

Although our main focus, and reason for being there, will be 6 meters, look for K5N on the HF IOTA freqs.. and maybe guest appearances elsewhere??

For those who haven't yet seen the website: http://www.kcvhfgridbandits.com/kc_vhf_grid_bandits_018.htm

With our special thanks to JD-N0IRS for the work he put in to this project. Thanks to JD, our logo has been finalized as well, it is too cool...

If you haven't yet made a schedule for Meteor Scatter, please email Bruce for a time slot. Check the slots available at: http://www.ykc.com/wa5ufh/EL58/EL58hx.htm and send your requests to Bruce: n5six@bellsouth.net

If you have any questions or need info, our email address: k5n@bellsouth.net

73, and hope to work everyone from EL58

Danny-N5OMG

Amateur Radio Museum Ships Event This Next Weekend

Courtesy of Howard Bingham, KE5APJ

Mark your calendars, Jun6 - 7, 2009 Battleship New Jersey Amateur Radio Station will conduct an event involving amateur radio operators at over 50 "Museum Ships", this will include both SSB & CW operations from in many cases on-board the 50 museum ships that may include operation of original ship radios over long wire antennas.

Details are at: http://www.nj2bb.org/museums/index.html

In Texas there will be the Battleship Texas, Submarine Cavalla, Destroyer Escort Stewart, Aircraft Carrier Lexington.

The Brazos Valley Amateur Radio Club (http://www.bvarc.org/) is sponsoring operation from Galveston Seawolf Park using long wire antennas aboard the USS Cavala and the Destroyer Escort USS Stewart on several bands & will include PSK31 from the radio room of the USS Cavalla. Club call "KK5W" will be used from Galveston, operators will work 40, 20, 10 and 6 meters from the site, as well as a few other frequencies. (See the listing of suggested frequencies at the Battleship New Jersey site.).

Documented contacts with call KK5W will count as 2 ships contacted, if 15 or more ships are contacted, logs submitted with 15 different ships will get you a colorful "Marine Ships 2009" 8.5 x 11 certificate in addition to QSL cards.

http://www.nj2.org/museum/index.html

These are fun events and I have a lot of neat QSLs from these floating museums. Hope to see you in the pilups this weekend.

Sunday, May 24, 2009

Report: Faulty Communications Imperil President

As reported in an online Wired article by Kim Zetter, the U.S. Secret Service is asking for $34 million to help upgrade its communication system, and says that without the money the president’s life could be in danger, according to a news report.

More on this story at http://www.wired.com/threatlevel/2009/05/secretservice/.

Saturday, May 16, 2009

NHC's WX4NHC Sets On-The-Air Station Test



Courtesy of the The ARRL Letter Vol. 28, No. 19 May 15, 2009

The annual WX4NHC On-the-Air Station Test from the National Hurricane Center (NHC) in Miami will take place Saturday, May 30, from 1300-2100 UTC. "The purpose of this annual Station Test is to test all of our radio equipment, computers and antennas using as many modes and frequencies as possible. This is not a contest or simulated hurricane exercise. New equipment and software will be tested, and we will also conduct some operator training," said WX4NHC Assistant Amateur Radio Volunteer Coordinator Julio Ripoll, WD4R.

Ripoll said that WX4NHC also will be testing new computers and software, as well as conducting operator training. "NHC Director Bill Read, KB5FYA, will be at WX4NHC, making contacts," he said. WX4NHC will be on the air on HF, VHF and UHF, plus 2 and 30 meter APRS. Suggested SSB frequencies are 3.950, 7.268, 14.325, 21.325 and 28.525 MHz, +/-QRM; WX4NHC reports that they will mostly be on 14.325 MHz and will make announcements when they change frequencies. WX4NHC also will be on the VoIP Hurricane Net 1700-1900 UTC (IRLP node 9219/EchoLink WX-TALK Conference) and on South Florida area VHF/UHF repeaters and simplex; APRS and e-mail will also be monitored.

Stations working WX4NHC exchange call sign, signal report, location and name plus a brief weather report, such as "sunny," "rain" or "cloudy." Non-hams may submit their actual weather using the On-Line Hurricane Report Form. QSL to WD4R and include a self-addressed, stamped envelope. Do not send cards to the NHC. Due to security measures, no visitors will be allowed at NHC during the test.

Scientists Predict Solar Cycle 24 to Peak in 2013

Courtesy of the The ARRL Letter Vol. 28, No. 19 May 15, 2009

At the annual Space Weather Workshop held in Boulder, Colorado last month <http://www.swpc.noaa.gov/sww/index.html>, an international panel of experts led by NOAA's Space Weather Prediction Center (SWPC) predicted that Solar Cycle 24 will peak in May 2013 with 90 sunspots per day on average. If the prediction proves true, Solar Cycle 24 will be the weakest cycle since Solar Cycle 16, which peaked with 78 daily sunspots in 1928, and ninth weakest since the 1750s, when numbered cycles began.

The panel predicted that the lowest sunspot number between cycles -- the solar minimum -- occurred in December 2008, marking the end of Solar Cycle 23 and the start of Solar Cycle 24. If December's prediction holds up <http://www.arrl.org/news/stories/2008/01/07/100/>, at 12 years and seven months Solar Cycle 23 will be the longest since 1823 and the third longest since 1755. Solar cycles span 11 years on average, from minimum to minimum.

An unusually long, deep lull in sunspots led the panel to revise its 2007 prediction that the next cycle of solar storms would start in March 2008 and peak in late 2011 or mid-2012. The persistence of a quiet sun also led the panel to a consensus that Solar Cycle 24 will be what they called "moderately weak."

Although the peak is still four years away, a new active period of Earth-threatening solar storms will be the weakest since 1928. Despite the prediction, the scientists said that Earth is still vulnerable to a severe solar storm. Solar storms are eruptions of energy and matter that escape from the Sun and may head toward Earth, where even a weak storm can damage satellites and power grids, disrupting communications, the electric power supply and GPS. A single strong blast of "solar wind" can threaten national security, transportation, financial services and otheressential functions.

The most common measure of a solar cycle's intensity is the number of sunspots -- Earth-sized blotches on the sun marking areas of heightened magnetic activity. The more sunspots there are, the more likely it is that solar storms will occur, but a major storm can occur at any time.
"As with hurricanes, whether a cycle is active or weak refers to the number of storms, but everyone needs to remember it only takes one powerful storm to cause huge problems," said NOAA scientist Doug Biesecker, who chaired the panel. "The strongest solar storm on record occurred in 1859 during another below-average cycle." The 1859 storm shorted out telegraph wires, causing fires in North America and Europe and sent readings of Earth's magnetic field soaring. It also producednorthern lights so bright that people read newspapers by their light, he said.

Biesecker cited a recent report by the National Academy of Sciences that found if a storm that severe occurred today, it could cause $1-2 trillion in damages the first year and require four to 10 years for recovery, compared to the $80-125 billion of damage that resulted from Hurricane Katrina<http://www.nap.edu/nap-cgi/report.cgi?record_id=12507&type=pdfxsum>.

The Space Weather Prediction Center is part of the National Weather Service and is one of the nine National Centers for Environmental Prediction. It is the nation's official source of space weather alerts, watches and warnings. SWPC provides real-time monitoring and forecasting of solar and geophysical events that impact satellites, power grids, communications, navigation and many other technological systems.

Friday, May 15, 2009

Shuttle snapped up against sun


Interesting story of the space shuttle captured by an amateur astronomer transiting in front of the Sun. The complete story at http://www.thesun.co.uk/sol/homepage/news/article2431157.ece

*FLASH FLASH FLASH*

From Lars Kalland/SM6NM

The *planned* transmission with the Alexanderson alternator on 17.2 kHz at
Grimeton Radio/SAQ at Tuesday 19 May is *moved to Wednesday 20 May* at the
same times, 07:00 UTC and 07:30 UTC.

Saturday, May 09, 2009

Grimeton Radio/SAQ Planned Transmissions - 2009

Courtesy of Lars Kalland SM6NM, via Ary Boender and the UDXF gang (thanks):-

There will hopefully be transmissions with the Alexanderson alternator on 17.2 kHz, CW (A1A) at the following dates and times during 2009:

1) Tuesday, May 19 2009 at 07:00 and 07:30 UTC.

There will be a transmission to celebrate the Japanese VLF-station Josami Radio/JND when it will be nominated to Institute of Electrical and Electronics Engineers (IEEE) Milestone and also celebrate its start 80 years ago. The radio station is now a museum. No reports required and no QSL-cards are given.

2) Sunday, May 24 2009 at 10:55 UTC.

A transmission will take place to celebrate the First Swedish Coast Radio Station and 100 years of Karlskrona Radio/SAA. The station is still working on military frequencies. No reports required and no QSL-cards are given.

3) Sunday, June 28 at 09:00 and 12:00 UTC.

The annual transmission on "Alexander Day". The station is open to visitors. We are glad to receive reports and will exchange QSL-cards.

4) Saturday, October 24 at 09:00 UTC.

As last year we will transmit on United Nations Day. No reports required and no QSL-cards are given.

5) Thursday, December 24, Christmas Eve at 08:00 UTC.

The Christmas transmission as before. The stations is open to visitors. We are glad to receive reports and will exchange QSL-cards.

We will start tuning up some 30 minutes before message. Also read our web site: http://www.alexander.n.se.

QSL-reports are, when indicated, kindly received via:

- E-mail to: info@alexander.n.se
- or fax to: +46-340-674195
- or via: SM bureau
- or direct by mail to: Alexander - Grimeton Veteranradios Vaenner,Radiostationen, Grimeton 72 S-430 16 ROLFSTORP SWEDEN

Yours,

Lars Kalland SM6NM

Wednesday, May 06, 2009

Rocket set for launch on Virginia Eastern Shore

A U.S. military satellite designed to detect hidden enemy weapons and quickly inform U.S. troops of their location is set for launch from Virginia's Eastern Shore tomorrow evening from 2000-2300 EDT. The Air Force TacSet-3 satellite and two other payloads is set to blast off on a 69-foot-high Minotaur 1 rocket from NASA's Wallops Flight Facility and the Mid-Atlantic Regional Spaceport.

TacSat-3 features three revolutionary trials: the Raytheon Company-built Advanced Responsive Tactically Effective Military Imaging Spectrometer hyperspectral imager, the Office of Naval Research's Satellite Communications Package, and the Air Force Research Laboratory's Space Avionics Experiment. This trio of payloads will offer real-time imagery (within 10 minutes of collection), sea-based information transmitted from ocean buoys and plug-and-play avionics to assist the warfighter in keeping one step ahead of the adversary.

Scientists say the 880-pound satellite atop the $60 million spacecraft will offer hyperspectral images and deliver them in 10 minutes. Officials say it is especially suited to battle conditions in the rugged, mountainous terrain of Afghanistan.

Military officials say it the satellite is successful, it could be ready for actual battlefield use in a year or two.

Two of the Tactical Satellite-3's trio of payloads may be called secondary, but their importance to the success of the spacecraft's year-long mission is primary.

Employing plug-and-play technology, the Space Avionics Experiment will provide backup downlink capability for TacSat-3's main experiment, the Advanced Responsive Tactically-Effective Military Imaging Spectrometer, and the Satellite Communications Package will transmit sea-based and space-generated data to ground stations.

Once launched, it will serve as the inaugural demonstration of plug- and-play avionics operating in the cosmos environment. The AFRL-funded SAE payload features plug-and-play components similar to desktop computer Universal Serial Bus components, which, if required due to a system failure, will perform data transfer to enable downlink of ARTEMIS sensor data, as well as will provide TacSat-3 with global positioning system information.

"The purpose of the technology is to significantly reduce spacecraft development time from years to months to weeks, as well as to lower production costs," said Maurice Martin, responsive systems group lead, the AFRL's Space Vehicles Directorate. "Our plan during TacSat-3's flight is to evaluate the Space Avionics Experiment on an occasional basis to ensure the components' reliability in case they are called upon to function in full operational mode."

Managed by the Office of Naval Research, the Satellite Communications Package will collect data from ocean buoys and then TacSat-3's onboard processor will download the details to a ground station. In addition, the U.S. Army Space and Missile Defense Command/Army Forces Strategic Command will utilize the SCP experiment's ultra high frequency radio link known as the Army Tactical Data Link.

"USASMDC/ARSTRAT is going to use the Satellite Communications Package payload's ATDL to provide a direct tactical downlink of onboard processed information from the ARTEMIS to the joint force commander. The JFC will have direct access to task the spacecraft as it appears over the horizon, while the satellite is still in view, the requested information will then be transmitted back to the JFC," said Allen Kirkham, Army Space and Missile Defense Command Battle Lab technical lead for the TacSat-3 Joint Military Assessment, Peterson AFB, Colo. "We will coordinate with the TacSat-3 program team to utilize the SCP's ATDL for a few two-week periods during the spacecraft's 12-month mission. We also intend to use the SCP's ATDL during a major exercise to allow us to collect data and perform a Joint Military Utility Assessment of the satellite and sensor's capabilities to support the joint force commander in the field."

As a significant team member in the program, the Space and Missile Systems Center's Space Development and Test Wing, also situated at Kirtland AFB, is providing the Orbital Sciences Corp.'s Minotaur I launch vehicle. The four-stage rocket consists of two structures taken from retired Minuteman intercontinental ballistic missiles, and another two stages from Orbital's Pegasus booster. In addition, the Dept. of Defense's Operationally Responsive Space office is underwriting the launch and will be heading the Military Utility assessment to determine the operational value of the low-cost satellite and its three payloads. SMC's Space Development and Test Wing will also assist mission operations during TacSat-3's flight in Low Earth Orbit at approximately 425 kilometers (264 miles) altitude.

The downlink frequencies for this spacecraft have not been determined. We believe there will be a UHF military downlink from this satelite. Any reports on the freqs to be used by this bird or any post launch intercepts would be appreciated.

Three cubesats will be launched as secondary payloads on the TacSat-3 mission. The satellites, which contain their own power and data systems, are four-inch cubes that weigh 2.2 pounds each. The cubesats are being provided by California Polytechnic State University, San Luis Obispo; The Aerospace Corporation, El Segundo, Calif. and the Hawk Institute for Space Sciences, Pocomoke City, Md.

These three cubesats are named PharmaSat-1, HawkSat-1 and PolySat CP6. The three satellites are placed in a Poly Picosatellite Orbital Deployer (P-POD), the standard deployment system for cubesats. The P-POD was developed by the Aerospace Engineering Department at Cal Poly. During the rocket’s ascent, each cubesat will be deployed separately from the P-POD into space.

The PharmaSat experiment, developed by NASA’s Ames Research Center and will measure the influence of microgravity upon yeast resistance to an antifungal agent. PharmaSat focuses on questions key to countermeasure development for long-term space travel and habitation.

PharmaSat-1 will be in a low earth orbit at 40 degrees inclination. This submission is for a beacon on board PharmaSat. The orbit should be nearly circular with an altitude of 390 Km at the start of the mission, degrading to 200km after approx 250 to 300 days, at which time it would de-orbit. There will be a 150mW UHF beacon operating with 1200baud AX25 packet for 1/2 sec every 5 secs. Command and control will use an experimental licence in the 2.4 GHz ISM band. The satellite will be a triple cubesat with a mass of approx 4 kg. The co-ordinated downlink frequency is 437.465 MHz. See http://www.inwspace.org/genesatbeacon_fig1.htm for more info.

Hawksat-1 is a demonstrator cubesat mission. Payload consists of multiple COTS and custom products. The co-ordinated downlink frequency is 437.345 MHz. Views can be found at http://www.hawkspace.org/hawksat.htm

The experiment Polysat CP6 will measure plasma fields, using three tape measures that extend out about a meter, charging them up to 400 volts, and looking at the electrons flowing around the spacecraft in the plasma. The co-ordinated downlink frequency is 437.365 MHz (1200 bps AX.25). See http://polysat.calpoly.edu/index.php

Tuesday, May 05, 2009

New Uniden Scanners Announced

Uniden has made the following announcement regarding two new scanners that are perfect for Milcom monitoring.

Today Uniden is announcing two new scanner models: The BCD996XT and BCT15X base / mobile scanners bring the latest improvements to Uniden's core scanner platform to the mobile scanner audience.

Complete details about these scanners will soon be available covered in our main Scanner Manuals site, but here are some of the features added to the new models:

More memory

BCD996XT: 25,000 channels
BCT15X: 9,000 channels

Fully automatic P25 decoding (BCD996XT only)

Enhanced GPS compatibility -- controls the scanning of groups of channels within systems.

More channels per system -- up to 500 channels per trunked system.

Channel Number Tagging -- lets you quickly select a channel for monitoring.

Fire Tone-Out Search -- helps to identify the tones used on fire paging dispatch channels.

Band Scope -- provides a visual representation of activity within a selected frequency range to help quickly identify active frequencies or sources of interference.

Multi-Color Display Backlight (BCD996XT only) -- lets you have the scanner alert you to particular channel activity using specific colors.

NAC Decoding -- lets you lelect specific NAC codes to limit reception to only the desired agency. (BCD996XT only)

Individual Channel Volume Offset -- helps to compensate for agencies that over- or under-modulate consistently.

Priority ID scan for trunked systems -- assigns preference to priority channels when evaluating incoming channel grants.

Preemptive Priority for Motorola Systems -- jumps to a priority channel even if the scanner is on a differerent voice communication on the system (requires compatible system-side priority assignments).

And more...

Availability for both models is expected late Summer, 2009.

In a week or so we'll have all the details for all the new features as well as in-depth instructions posted at Scanner Manuals.

Thursday, April 30, 2009

STEREO Reveals the Anatomy of a Solar Storm in 3D


By Donna McKinney, Naval Research Laboratory, Public Affairs

WASHINGTON (NNS) -- Observations from NASA's twin Solar Terrestrial Relations Observatory (STEREO) spacecraft have allowed scientists to reveal for the first time the speed, trajectory, and 3-D shape of solar explosions known as coronal mass ejections, or CMEs.

CMEs are powerful eruptions of plasma and magnetic energy from the sun's outer atmosphere, or corona. When these sudden outbursts are directed toward Earth, they can have both breathtakingly beautiful and potentially damaging effects.

"We can now see a CME from the time it leaves the solar surface until it reaches Earth, and we can reconstruct the event in 3-D directly from the images," said Angelos Vourlidas, a solar physicist at the Naval Research Laboratory (NRL) and project scientist for the NRL-led Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) aboard STEREO.

The NRL team has always been a leader in CME research, beginning with the initial discovery by an NRL-built telescope in 1971 (OSO-7). The CME phenomenon was explored in more detail by another NRL-led experiment (P78-1/Solwind) in the 1980s, resulting in the discovery of the characteristic signature (a halo) of Earth-directed CMEs, as well as the association to interplanetary shocks. Then in 1995, the NRL-led LASCO experiment was launched, with greatly increased sensitivity enabling routine observations of Earth-directed CMEs, firmly establishing the solar origin of space weather events.

"The evolution in imaging capability since the discovery in 1971 to now is just astounding. It took 44 minutes to read out the 256x256 pixel image (worse than most cell phone images), whereas now it takes a few seconds to read out the current 2048x2048 pixel image," said Russ Howard, a solar physicist at NRL and principal investigator of the LASCO and SECCHI experiments.

Until now, CMEs were observed near the sun but the next measurements had to wait until the CME arrived at Earth three to seven days later. STEREO's ability to continuously image a CME from its explosive birth to arrival at Earth is the first time this has been achieved and represents a significant advance. Three-dimensional tracking of an evolving CME is critical to determining its structure and predicting if and how it will affect Earth.

STEREO consists of two nearly identical observatories that make simultaneous observations of CMEs from two different vantage points. One observatory "leads" Earth in its orbit around the sun, while the other observatory "trails" the planet.

"The larger the separation between the spacecraft, the larger the structures we can examine," said Vourlidas.

Using the SECCHI telescopes, solar physicists can examine a CME's structure, velocity, mass, and direction in the corona and track it through interplanetary space. Such measurements can help determine when a CME will reach Earth, at what speed and how much energy it will deliver to Earth's magnetosphere.

CMEs carry billions of tons of plasma into space at thousands of miles per hour. This plasma — which carries some of the magnetic field from the corona with it — can create a large, moving disturbance in space that also produces a shock wave. The shock can accelerate some of the surrounding particles to high energies, a form of "solar cosmic rays" that can be hazardous to spacecraft and astronauts. The shock and CME material, which arrive days later, can produce disruptive space weather during and following their interaction with Earth's magnetosphere and upper atmosphere.

The seriousness of the effects depends on the size and speed of the CME when it arrives at Earth. These sun storms can interfere with communications between ground controllers and satellites, pilots flying near Earth's poles and astronauts on the International Space Station. Radio noise from the storm can also disrupt cell phone service. Disturbances in the ionosphere related to CMEs can affect Global Positioning System navigation and, in extreme cases, induced currents in long cables and transformers on the ground can cause power outages.

The STEREO mission employs two nearly identical observatories to provide 3-D measurements of the sun to study the nature of coronal mass ejections. STEREO is the third mission in NASA's Solar Terrestrial Probes program.

Story at
http://www.navy.mil/search/display.asp?story_id=44798

NASA story at
http://www.nasa.gov/mission_pages/stereo/news/solarstorm3D.html

NASA Gives a Go for for Hubble Service Mission

To help you monitor this Space Shuttle mission and other NASA communications you can download our exclusive Monitoring NASA and Space Shuttle Communications document at http://www.monitoringtimes.com/Monitoring%20NASA%20and%20Space%20Communications.pdf.

NASA managers completed a review Thursday of space shuttle Atlantis’ readiness for flight and selected an official launch date for the STS-125 mission to upgrade the Hubble Space Telescope. Commander Scott Altman and his six crewmates are scheduled to lift off at 2:01 p.m. EDT (1801 UTC), May 11, from NASA’s Kennedy Space Center in Florida.

Atlantis’ launch date was announced following Thursday’s Flight Readiness Review. During the meeting, top NASA and contractor managers assessed the risks associated with the mission and determined the shuttle’s equipment, support systems and procedures are ready for flight.

Atlantis’ 11-day mission will include five spacewalks to refurbish Hubble with state-of-the-art science instruments. After the astronauts’ visit, the telescope’s capabilities will be expanded and its lifetime extended through at least 2014.

Commander Altman will be joined on the mission by Pilot Gregory C. Johnson and Mission Specialists Andrew Feustel, Michael Good, John Grunsfeld, Megan McArthur and Mike Massimino. The spacewalkers are Feustel, Good, Grunsfeld and Massimino. McArthur is the flight engineer and lead for robotic arm operations.

For more information about the STS-125 crew and its mission, visit: http://www.nasa.gov/shuttle

For more information about the Hubble Space Telescope, visit:
http://www.nasa.gov/hubble

Monday, April 27, 2009

2009 Hurricane Op Plan Available

You can get the official Department of Commerce/NOAA National Hurricane Operations Plan for 2009 at http://www.ofcm.gov/nhop/09/pdf/2009%20NHOP%20entire%20document.pdf

As always, as the season progresses and the need arises, this blog and it's sister blog the Milcom Monitoring Post at http://mt-milcom.blogspot.com/ will carry the latest frequency information as it relates to each storm. Don't reply on old outdated list and frequencies that are no longer valid, get the best right here at the BTown Monitoring Post.


It is a prank only -- CA County Opposes Ham Radio

There is a big time rumor circulating on the Internet via email and newsgroups that the San Luis Obispo county supervisors had passed an ordinance banning ham radio.

According to the ARRL newsletter:

"The California county of San Luis Obispo was notified by the Federal Communications Commission Wednesday, April 8 of a rumor on an Internet group site stating that the San Luis Obispo County Board of Supervisors passed an ordinance on March 31 which would ban Amateur Radio operators -- commonly known as ham radio operators -- from operating their transmitting stations. The rumor is posted as an alleged news story from a non-existent Los Angeles news publisher. The story alleges that the purpose of this false action by the Board was due to supposed interference caused by ham radio transmitters, among other reasons. The article has an online posting date of April 1, 2009."

I will not reprint the article here on this blog so that it can be further distributed on the net and promoting this myth but the whole story is a myth and has been fabricated by a prankster as an April Fool joke. Literally within 10 seconds of reading the email I received I had Googled the truth. Please do not pass this one around. At best it is spam and I consider such messages like a virus that is passed one computer to another.

The truth can be found at http://www.slocounty.ca.gov/AssetFactory.aspx?did=19840 or at http://www.arrl.org/news/stories/2009/04/09/10763/.

Saturday, April 25, 2009

Capitol radio system could cost $100M

Surprise, surprise. Just another example of how this U.S. government has gone nuts with spending. There are simplier solutions, but then again this is the imperial U.S. government and when you have an endless trough of money to spend . . .

http://thehill.com/leading-the-news/capitol-radio-system-could-cost-100m-2009-04-22.html

I love Peter S' comment on this and he hits the nail directly on the head.

"crashes sometimes - has dead spots - can be monitored by store bought scanners after they spend $100M same ole same ole, Note - Capitol PD uses 166 Mhz now - DCPD use UHF TRS - FD uses 800Mhz TRS - maybe if they throw up a couple of BDAs they can use theDCFD TRS for free - hey, I just saved $100M - just give me 10% of it."

How how about you feds ponying up and buying some radios and use the DCPD TRS system. Then you might get some interoperability! In fact, maybe i can get DHS to send over some of their interoperability coloring books to the Capitol Hill PD and then we can all learn to work together.

You bunch of big dummies. Another fleecing of the US taxpayers.

Sunday, April 19, 2009

Tyco Electronics Sells Its Wireless Systems Business to Harris Corporation

Tyco Electronics Ltd. today (April 16) announced that the company has entered into a definitive agreement to sell its Wireless Systems business to Harris Corporation for $675 million in cash, subject to final working capital adjustments. Wireless Systems is a leader in the development of large-scale critical communications systems based on Internet Protocol (IP) technology for customers in the public safety, utility, transit and public service industries. The business generated sales of $461 million in fiscal 2008.

According to Tyco Electronics Chief Executive Officer Tom Lynch, "The sale of the Wireless Systems business will increase our focus on our core connectivity business and substantially completes the streamlining of our portfolio that we began two years ago. Wireless Systems is an ideal fit for Harris, whose size, resources and experience in the communications industry should help position the business for accelerated growth."

The transaction is subject to customary regulatory approvals and is expected to close in the summer of 2009. Tyco Electronics will report the results of the Wireless Systems business as a discontinued operation beginning with its fiscal third quarter, ending June 26, 2009.

And from Harris:

Harris Corporation (NYSE:HRS), an international communications and information technology company, has signed a definitive agreement to acquire the Tyco Electronics Wireless Systems business (formerly known as M/A-COM), an established provider of mission-critical wireless communications systems for law enforcement, fire and rescue, and public service organizations.

Tyco Electronics Wireless Systems, a business segment of Tyco Electronics Ltd. (NYSE:TEL; BSX:TEL), was formed in 1999 and grew through the acquisition of ComNet Ericsson in 2001 to create Tyco Electronics Wireless Systems ("Wireless Systems"). Wireless Systems will be combined with the Harris RF Communications business segment, creating a dynamic new organization that will provide end-to-end wireless network solutions to the growing $9 billion global land mobile radio systems market.

"The combination of RF Communications and Wireless Systems creates a powerful supplier in the global land mobile radio systems market," said Howard L. Lance, chairman, president and CEO of Harris. "With an 80-year heritage in providing communications for the public safety market, Wireless Systems has established a large installed customer base, extensive domain knowledge, and well-developed sales channels, which serve the federal, state, and local public safety markets. Wireless Systems provides complete end-to-end infrastructure solutions, including IP-based voice and data networks, which support multiple platforms and provide interoperability among disparate systems. Harris RF Communications offers industry-leading radio technology, including the latest in software-defined multiband radios for interoperability and upgradeability, high-level encryption capable of supporting top secret communications, and digital waveform technology. In addition, Harris brings to the new partnership access to well-established business channels for the Department of Defense, U.S. federal agencies, and international customers."

Under the definitive agreement, Harris will purchase the Wireless Systems assets of Tyco Electronics for $675 million in cash, subject to post-closing adjustments. The goodwill arising on completion of the acquisition will be an allowable tax expense with an estimated net present value of $60 million, resulting in an effective purchase price of $615 million. The transaction excludes the State of New York wireless network contract awarded to Wireless Systems in December 2004. Wireless Systems' revenue for the fiscal year ending September 26, 2008, was $463 million, and earnings before interest, taxes, depreciation and amortization (EBITDA) was $86 million. The acquisition is expected to be slightly accretive to Harris earnings in fiscal 2010, excluding acquisition-related charges, and a significant contributor to earnings in fiscal 2011 and fiscal 2012. Morgan Stanley acted as the financial advisor to Harris, while Jones Day provided legal advice.

Wireless Systems is headquartered in Lowell, Massachusetts, with product development and manufacturing facilities in Lynchburg, Virginia, and has approximately 1,150 employees, including 500 engineers and scientists. Principal end-markets for the business include public safety and public service, federal government, transit and transportation, and utilities. End-to-end solutions include network systems and software solutions; mobile and portable radio equipment; broadband WiMAX products for high speed-data applications; and operations, service and maintenance. The business is a key player in the wireless communications standards process, successfully driving its products to open standards in both U.S. and international markets, including the next-generation digital APCO P25 standard.

Wireless Systems will operate as a business unit under the Harris RF Communications segment, headquartered in Rochester, New York. Chuck Dougherty will continue to serve as president of Wireless Systems and will report to Dana Mehnert, president of RF Communications.

"This acquisition greatly accelerates our entry into the land mobile radio systems market and creates a significant opportunity for growth in both North American and international markets," said Mehnert. "Complementary distribution channels will provide Harris with immediate access to state and local government markets for our new UnityT family of multiband radios and will expand the reach for Wireless Systems infrastructure and single-band radios to the Department of Defense, U.S. federal agencies, and international customers. We look forward to delivering a new level of capability and value and bringing industry-leading customer service and support to this market by leveraging the nationwide Harris IT Services workforce."

"Reliable, secure voice and data communications are essential to first responders and government agencies entrusted with ensuring the public's health and safety," said Dougherty. "We have successfully deployed over 500 systems worldwide. Integrating our products, systems, technologies and market channels with Harris will allow our combined businesses to bridge the interoperability gap and unite public safety responders at all levels of state, local and federal government."

Thursday, April 09, 2009

NDB Decommissioned

For my NDB monitoring friends:

CWI - MHW NDB Clinton IA on 377 kHz has been decommissioned as of 4/1/2009.
BPW - MHW NDB Osceola AR on 239 kHz has been decommissioned as of 4/3/2009.

Wednesday, April 08, 2009

CONUS ARINC VHF Radio Network

I have had several request by monitors regarding the frequencies used by the ARINC VHF Radio Network. So the map below which you can download has all the freqs used nationwide. I always have the freqs in my area programmed in my scanner and have some very interesting comms from time to time.

Saturday, March 28, 2009

NASA's Orion Capsule Built and Tested at NSWC Carderock

WEST BETHESDA, Md. (NNS) -- Naval Surface Warfare Center (NSWC) Carderock Division engineers, along with a NASA test and evaluation team are conducting initial Post-Landing Orion Recovery Test(PORT) operations, March 23-27.

The team will test a full-scale model of NASA's Orion space capsule at Carderock's pentagon-shaped test pond.

The model, measuring 16.5 feet in diameter and weighing 18,000 pounds, was built by NSWC Carderock in its model fabrication facility. The area is primarily used for Navy ship and submarine model design, fabrication, mission test support, and specialized manufacturing services using computer aided numerically controlled machines, programming, stereolithography, manufacturing, wood and composite material fabrication.

NSWC Carderock, a field activity of Naval Sea Systems Command, also uses its model fabrication facility to design ships and systems that are both "state of the art" and easily upgradable.

The PORT objective is to determine what the environment will be like for the astronaut and recovery crews at landing, and incorporate those lessons into the spacecraft design.

The Carderock test pond provides a controlled environment for NASA space crew recovery personnel and 920th Air Wing's Para Rescue Divers for familiarization diving before testing procedures in the uncontrolled waters of the Atlantic Ocean during the week of Apr. 6.

"Divers were in the water March 25, practicing attaching flotation collars," said Richard Banko, Carderock lead engineer and principle Navy-NASA test coordinator. "We're currently testing opening and closing the hatch with the flotation collars in place and then we're going to do night testing, and conduct these evolutions all over again without natural lighting, using only the diver's lighting."

After completing diver familiarization, the crew module will be transported to the National Mall in Washington for display at the National Air and Space Museum.

Alan Rhodes, NASA's Constellation Program Test and Verification officer, had high praise for the quality of work NSWC Carderock personnel provided for their Orion project.

"The Carderock team has gone far above and beyond our expectations in support of this project that I'm almost at a loss for words of praise," said Rhodes. "When you look at where we started planning a year and a half ago, and look at the finished crew model, and its water testing, it's truly amazing how well this model was built, how well it fits within the tolerances we've asked for it."

Carderock engineers and researchers will also participate in the testing when the model is transported to sea and launched by NASA's space shuttle solid rocket booster recovery ship. The team will quantify the seakeeping characteristics of the mock-up.

"It's a test model we will use for years to come, and we have the right team from Carderock to thank for it," said Rhodes.

Tuesday, March 10, 2009

Mothballed NASA Satellite Awaits New Life

BY STEPHEN CLARK, SPACEFLIGHT NOW

The long-grounded Deep Space Climate Observatory may be revived for an assignment very different from the controversial mission that was cancelled for its infamous mix of politics and science.

NASA, NOAA and the U.S. Air Force completed a comprehensive study last month to determine the feasibility of finally launching the refrigerator-sized satellite, which has been confined to a lonely corner of a Maryland warehouse for seven years.

The agencies are discussing adapting the DSCOVR spacecraft for a new mission to monitor solar wind and space weather from the L1 libration point, a site 1 million miles away where the pull of gravity from the sun and Earth is equal.

You can see the rest of the story at
http://spaceflightnow.com/news/n0903/01dscovr/

Elk City NDB Decommissioned

According to the FAA the Elk City, Oklahoma non-directional beacon (NDB), ID-EZY on 241.0 kHz has been decommissioned.

Friday, March 06, 2009

The Spaceflight Website to Host Shuttle Launch Video Coverage

Spaceflight Now will be joining forces with veteran space broadcasters Miles O'Brien and David Waters to provide video coverage of space shuttle Discovery's next mission, scheduled for launch on Wednesday, March 11.

More details are available at http://spaceflightnow.com/shuttle/sts119/090305broadcast/

You can get more details on the mission at http://spaceflightnow.com/shuttle/sts119/090304date/

Thursday, March 05, 2009

Julius Genachowski Nominated as Next FCC Chairman

From the ARRL

ARLB014 Julius Genachowski Nominated as Next FCC Chairman

On Tuesday, March 3, President Barack Obama nominated Julius Genachowski as FCC Chairman. Genachowski, 46, is a technology executive and a former classmate of Obama's from Harvard Law School. Upon Senate confirmation, Genachowski will replace Acting FCC Chairman Michael Copps; Copps took over the Commission on January 22, 2009, two days after then-Chairman Kevin Martin resigned. Genachowski has been widely praised by industry executives and consumer-activist groups -- two groups often at odds -- for his wide-ranging experience and intimate knowledge of technology issues.

"I can think of no one better than Julius Genachowski to serve as chairman of the Federal Communications Commission," said President Obama. "He will bring to the job diverse and unparalleled experience in communications and technology, with two decades of accomplishment in the private sector and public service. I know him as the son of immigrants who carries a deep appreciation for this country and the American dream; and as the proud father of three children working with his wife Rachel to be responsible parents in this digital age."

According to the Wall Street Journal, speculation has been rife as to why President Obama had not put forth Genachowski's name before now, saying that "his nomination has centered on the administration's efforts to find at least one more nominee -- more likely two -- to fill other open spots on the FCC's five-person board. Agency nominations tend to move through the Senate more quickly if a Democratic nominee is paired with a Republican nominee."

The Wall Street Journal said that a number of Republicans -- including FCC Deputy General Counsel Ajit Pai -- have been mentioned as a possible replacement for the seat left vacant by Republican Deborah Taylor Tate when she left the Commission in January. "On the Democratic side, speculation is growing that FCC Commissioner Jonathan Adelstein may not be renominated for the seat he currently holds. South Carolina public utilities commission official Mignon Clyburn (daughter of [Democrat Representative] Jim Clyburn) has been most often mentioned by people close to the Obama team as a candidate for that seat," the Journal reported. "Adelstein could be up for a job elsewhere in the Obama administration, insiders say, possibly at the Agriculture Department."

Acting Chairman Copps said President Obama "made an excellent choice in announcing his intent to nominate Julius Genachowski to be the next Chairman of the FCC. Julius has the knowledge, experience and dedication to lead this Agency forward as we tackle the many challenges confronting the country -- and the Commission. I look forward to the prospect of working with him on a communications agenda focused on serving consumers and the public interest. He will find here a talented and energized team of public servants committed to precisely this goal. I wish him a successful Senate confirmation."

Commissioner Adelstein also added his congratulations: "I warmly congratulate my friend Julius Genachowski on his nomination by President Barack Obama to be Chairman of the Federal Communications Commission. He is the right person at the right time for the job. His leadership, experience and intelligence will serve him and the American people well as he takes the helm of the FCC during this pivotal time for our country and the agency. By designating a Chairman with such a strong strategic vision, striking talents, wealth of experience inside and outside the Commission, and practical understanding of technology, President Obama once again demonstrates his commitment to the transformational power of communications technology and innovation."

Commissioner Robert McDowell congratulated Genachowski on his nomination, saying he "will bring a valuable perspective to the Commission with his experience not only in government, but in the private sector. I look forward to working closely with Mr. Genachowski on the many important communications challenges that lie ahead for the American people."

Additional information -- including Genachowski's background -- can be found on the web at, http://www.arrl.org/news/stories/2009/03/03/10684/?nc=1

Thursday, February 05, 2009

NDB Update - 2/4/2009

WARREN, AR NDB - MHW 226.000 REN N33°32.82' W92°05.76' 180/1°17.9'E
This beacon will decommission effective 12 March 2009

Saturday, January 24, 2009

NASA Sees the 'Dark Side' of the Sun


An artist's concept of one of the STEREO spacecraft.

Note for my readers who have X-band capability, you can participate in monitoring these spacecraft. More in the storey below-N5FPW

January 23, 2009: Today, NASA researchers announced an event that will transform our view of the Sun and, in the process, super-charge the field of solar physics for many years to come.

"On February 6, 2011," says Chris St. Cyr of the Goddard Space Flight Center, "Super Bowl XLV will be played in Arlington, Texas."

Wait … that's not it.

And on the same day," he adds, "NASA's two STEREO spacecraft will be 180 degrees apart and will image the entire Sun for the first time in history."

STEREO's deployment on opposite sides of the Sun solves a problem that has vexed astronomers for centuries: At any given moment they can see only half of the stellar surface. The Sun spins on its axis once every 25 days, so over the course of a month the whole Sun does turn to face Earth, but a month is not nearly fast enough to keep track of events. Sunspots can materialize, explode, and regroup in a matter of days; coronal holes open and close; magnetic filaments stretch tight and—snap!—they explode, hurling clouds of hot gas into the solar system. Fully half of this action is hidden from view, a fact which places space weather forecasters in an awkward position. How can you anticipate storms when you can't see them coming? Likewise researchers cannot track the long-term evolution of sunspots or the dynamics of magnetic filaments because they keep ducking over the horizon at inconvenient times. STEREO's global view will put an end to these difficulties.

The global view is still two years away. Already, however, the two spacecraft are beaming back over-the-horizon images that have researchers and forecasters glued to their monitors.

"This is a perspective we've never had before," says STEREO mission scientist Lika Guhathakurta of NASA headquarters. "We're now monitoring more than 270 degrees of solar longitude—that's 3/4ths of the star."

"After all these years," she laughs, "we're finally getting to see the dark side of the Sun."

(Editor's note: The Sun has no dark side. That was a solar physics joke.)

STEREO's journey to the "dark side" began on Oct. 25, 2006, when the twin probes left Earth together onboard a Delta II rocket. High above the atmosphere, they separated and headed for the Moon. What happened next was a first in space navigation. The Moon acted as a gravitational slingshot, flinging the two probes in opposite directions—STEREO-A ahead of Earth and STEREO-B behind. They've been spreading apart ever since.

Because of the way the Sun spins (counterclockwise in the diagram above), STEREO-B gets a sneak preview of sunspots and coronal holes before they turn to face Earth—a boon for forecasters.

"I know forecasters at NOAA's Space Weather Prediction Center monitor STEREO-B very closely," says St Cyr. "It lets them know what's coming."

At the moment, STEREO-B enjoys a 3-day look-ahead advantage over Earth-based observatories. This has allowed researchers to predict geomagnetic storms as much as 72 hours earlier than ever before. On several occasions in late 2008, STEREO-B spotted a coronal hole spewing solar wind before any other spacecraft did.

St. Cyr notes that experienced ham radio operators can participate in this historic mission by helping NASA capture STEREO's images. The busy Deep Space Network downloads data from STEREO only three hours a day. That's plenty of time to capture all of the previous day's data, but NASA would like to monitor the transmissions around the clock.

"So we're putting together a 'mini-Deep Space Network' to stay in constant contact with STEREO," says Bill Thompson, director of the STEREO Science Center at Goddard.

The two spacecraft beam their data back to Earth via an X-band radio beacon. Anyone with a 10-meter dish antenna and a suitable receiver can pick up the signals. The data rate is low, 500 bits per second, and it takes 3 to 5 minutes to download a complete image.

So far, the mini-Network includes stations in the United Kingdom, France and Japan—and Thompson is looking for more: "NASA encourages people with X-band antennas to contact the STEREO team. We would gladly work with them and figure out how they can join our network."

The two STEREO spacecraft rank among most sophisticated solar observatories launched by NASA to date. They are equipped with sensors that measure the speed, direction and composition of the solar wind; receivers that pick up radio emissions from explosions and shock waves in the sun's atmosphere; telescopes that image the solar surface and all the tempests that rage there; and coronagraphs to monitor events in the sun's outer atmosphere.

"So, really," says Guhathakurta, "we're not only seeing the sun's dark side, we're feeling, tasting and listening to it as well."

Super Bowl Sunday may never be the same….

Graphics with this story at:
http://science.nasa.gov/headlines/y2009/23jan_darkside.htm?list1066509

Thursday, January 22, 2009

Severe Space Weather


Auroras over Blair, Nebraska, during a geomagnetic storm in May 2005. Photo credit: Mike Hollingshead/Spaceweather.com

That's the surprising conclusion of a NASA-funded study by the National Academy of Sciences entitled Severe Space Weather Events—Understanding Societal and Economic Impacts. In the 132-page report, experts detailed what might happen to our modern, high-tech society in the event of a "super solar flare" followed by an extreme geomagnetic storm. They found that almost nothing is immune from space weather—not even the water in your bathroom.

The problem begins with the electric power grid. "Electric power is modern society's cornerstone technology on which virtually all other infrastructures and services depend," the report notes. Yet it is particularly vulnerable to bad space weather. Ground currents induced during geomagnetic storms can actually melt the copper windings of transformers at the heart of many power distribution systems. Sprawling power lines act like antennas, picking up the currents and spreading the problem over a wide area. The most famous geomagnetic power outage happened during a space storm in March 1989 when six million people in Quebec lost power for 9 hours: image.

According to the report, power grids may be more vulnerable than ever. The problem is interconnectedness. In recent years, utilities have joined grids together to allow long-distance transmission of low-cost power to areas of sudden demand. On a hot summer day in California, for instance, people in Los Angeles might be running their air conditioners on power routed from Oregon. It makes economic sense—but not necessarily geomagnetic sense. Interconnectedness makes the system susceptible to wide-ranging "cascade failures."

To estimate the scale of such a failure, report co-author John Kappenmann of the Metatech Corporation looked at the great geomagnetic storm of May 1921, which produced ground currents as much as ten times stronger than the 1989 Quebec storm, and modeled its effect on the modern power grid. He found more than 350 transformers at risk of permanent damage and 130 million people without power. The loss of electricity would ripple across the social infrastructure with "water distribution affected within several hours; perishable foods and medications lost in 12-24 hours; loss of heating/air conditioning, sewage disposal, phone service, fuel re-supply and so on."

"The concept of interdependency," the report notes, "is evident in the unavailability of water due to long-term outage of electric power--and the inability to restart an electric generator without water on site."

The strongest geomagnetic storm on record is the Carrington Event of August-September 1859, named after British astronomer Richard Carrington who witnessed the instigating solar flare with his unaided eye while he was projecting an image of the sun on a white screen. Geomagnetic activity triggered by the explosion electrified telegraph lines, shocking technicians and setting their telegraph papers on fire; Northern Lights spread as far south as Cuba and Hawaii; auroras over the Rocky Mountains were so bright, the glow woke campers who began preparing breakfast because they thought it was morning. Best estimates rank the Carrington Event as 50% or more stronger than the superstorm of May 1921.

"A contemporary repetition of the Carrington Event would cause … extensive social and economic disruptions," the report warns. Power outages would be accompanied by radio blackouts and satellite malfunctions; telecommunications, GPS navigation, banking and finance, and transportation would all be affected. Some problems would correct themselves with the fading of the storm: radio and GPS transmissions could come back online fairly quickly. Other problems would be lasting: a burnt-out multi-ton transformer, for instance, can take weeks or months to repair. The total economic impact in the first year alone could reach $2 trillion, some 20 times greater than the costs of a Hurricane Katrina or, to use a timelier example, a few TARPs.

What's the solution? The report ends with a call for infrastructure designed to better withstand geomagnetic disturbances, improved GPS codes and frequencies, and improvements in space weather forecasting. Reliable forecasting is key. If utility and satellite operators know a storm is coming, they can take measures to reduce damage—e.g., disconnecting wires, shielding vulnerable electronics, powering down critical hardware. A few hours without power is better than a few weeks.

NASA has deployed a fleet of spacecraft to study the sun and its eruptions. The Solar and Heliospheric Observatory (SOHO), the twin STEREO probes, ACE, Wind and others are on duty 24/7. NASA physicists use data from these missions to understand the underlying physics of flares and geomagnetic storms; personnel at NOAA's Space Weather Prediction Center use the findings, in turn, to hone their forecasts.

At the moment, no one knows when the next super solar storm will erupt. It could be 100 years away or just 100 days. It's something to think about the next time you flush.

Sunday, January 18, 2009

Naval Observatory Soon Will Track Time to 100 Trillionths of Second

By John Ohab, Special to American Forces Press Service

The ultra-precise timing technology that enables NAVSTAR Global Positioning Systems and high-speed Internet communication soon may resolve the measure of time to 100 trillionths of a second, according to the world's authority in time-keeping and celestial observation.

"To know when an event occurred, you need a clock. We are that clock," said Geoff Chester, public affairs officer at the U.S. Naval Observatory, the majority contributor to the international determination of time. He explained the development of this new timing technology during yesterday's premier of the Defense Department's "Armed with Science" radio program on BlogTalkRadio.com.

For centuries, clocks have measured seconds through regular, rhythmic oscillations of a pendulum, a swinging weight susceptible to influence by factors such as gravity, temperature, and air viscosity. In the 1950s, scientists began investigating the oscillations of particular atoms as a more precise way to define the second.

"Atomic time is independent of what Earth does," Chester said. "Atomic clocks define time scales in terms of a certain number of oscillations of a certain type of atom that take place in the course of one second. The master clock at the Naval Observatory is an ensemble of dozens of these devices, and we take a weighted average of all of them to determine our base-reference time scale."

Standard atomic clocks measure microwave signals emitted from atoms as they change energy levels. Since 1967, the one-second time interval has been defined as the duration of 9,192,631,770 cycles of radiation corresponding to the transition between two energy levels of the cesium-133 atom.

"We guarantee that no two seconds that come out of here over the course of a year will differ by more than one billionth of a second," Chester said. "Our clock is so precise that it will not gain or lose one second on the order of 3 million years."

To meet the demands of technology and the needs of society, researchers at the U.S. Naval Observatory continue to develop more precise time-keeping systems. By 2010, they hope to release an operational version of their newest clock, known as a "fountain clock," which uses laser beams to induce oscillations of the rubidium atom. This rubidium fountain clock will provide a measure of time accurate to 100 trillionths of a second, about 10 to 100 times more precise than the current master clock.

"Rubidium atoms are smaller and easier to manipulate," Chester explained. "They allow us to keep a much better timescale than what we keep today."

The U.S. Naval Observatory, one of about 50 scientific laboratories concerned with time-keeping, maintains one-third of the operational atomic clocks currently deployed around the world.

In addition to its role in defining and maintaining universal time, the Naval Observatory also acts as a reference point for navigation and communications technologies that affect people's everyday lives. For instance, its ultra-precise time-keeping systems enable computer networks to rapidly and accurately transmit information, and the constellation of satellites used in GPS relies on the master clock to calculate locations on the Earth's surface.

"People ask what time is about," Chester said. "Timing is everything."

NASA debuts Global Hawk autonomous aircraft for Earth science

One of two Global Hawk aircraft that were transferred from the Air Force to NASA in December 2007 will begin missions to support NASA's Science Mission Directorate and the Earth science community. The aircraft, located at the Dryden Flight Research Center at Edwards, Calif., brings a new capability to the science community for measuring, monitoring and observing remote locations of the Earth. The two Global Hawks were the first and sixth aircraft built for the Air Force under the original development program. (NASA photo/Tony Landis)

NASA and the Northrop Grumman Corp. of Los Angeles have unveiled the first Global Hawk aircraft system to be used for environmental science research, heralding a new application for the world's first fully autonomous high-altitude, long-endurance aircraft. The debut took place Jan. 15 at NASA's Dryden Flight Research Center in Edwards, Calif.

NASA and Northrop Grumman are returning NASA's two Global Hawk aircraft to flight this year under a space act agreement signed in May 2008. NASA plans to use the aircraft for missions to support its Science Mission Directorate and the Earth science community that require high-altitude, long-distance airborne capability.

"Today marks the debut of NASA's newest airborne science capability," said Kevin L. Petersen, director of Dryden. "These Global Hawks represent the first non-military use of this remarkable robotic aircraft system. NASA's partnership with Northrop Grumman has made this possible."

The Air Force transferred the Global Hawks to NASA in December 2007. They are among the first seven built in the original Advanced Concept Technology Demonstration program, which the Defense Advanced Research Projects Agency sponsored. Northrop Grumman specialists will share in the use of the aircraft to conduct their own flight demonstrations for expanded markets, missions and airborne capabilities, including integration of autonomous aircraft systems into the national airspace.

Global Hawk can fly at altitudes up to 65,000 feet for more than 31 hours at a time. To date, the aircraft have flown more than 28,000 hours.

The National Oceanic and Atmospheric Administration, or NOAA, also is partnering with NASA to develop this new airborne research tool. NOAA officials are participating in the project management and piloting of the NASA Global Hawks and the development of scientific instruments and future Earth science research campaigns.

"The Global Hawks will provide superb new measurement possibilities for our climate science and applications programs," said Michael Freilich, director of NASA's Earth Science Division in Washington.

"This collaboration is a model for NASA's wide-ranging Earth-observation activities to advance our understanding of Earth as an integrated system, which are critical to developing responses to environmental change here and around the world," he said.

NASA's initial use of the aircraft to support Earth science will be the Global Hawk Pacific 2009 program. This campaign will consist of six long-duration missions over the Pacific and Arctic regions in the late spring and early summer of 2009. Twelve scientific instruments integrated into one of the NASA Global Hawk aircraft will collect atmospheric data while flying high through Earth's atmosphere in the upper troposphere and lower stratosphere.

Global Hawk has many potential applications for the advancement of science, improvement of hurricane monitoring techniques, development of disaster support capabilities, and development of advanced autonomous aircraft system technologies. For example, Global Hawks were used to help monitor wildfires in Southern California in 2007 and 2008.

NASA's Dryden Flight Research Center, located on Edwards Air Force Base in the Mojave Desert of Southern California, is NASA's primary installation for atmospheric flight research. It has supported NASA's technology development efforts in aeronautics, environmental science, space exploration and space operations for more than 60 years.

Powerful Solar Storm Could Shut Down U.S. for Months



A new study from the National Academy of Sciences outlines grim possibilities on Earth for a worst-case scenario solar storm.

Damage to power grids and other communications systems could be catastrophic, the scientists conclude, with effects leading to a potential loss of governmental control of the situation.

The prediction is based in part on a major solar storm in 1859 that caused telegraph wires to short out in the United States and Europe, igniting widespread fires.

See the rest of this copyrighted article on the FoxNews website at

http://www.foxnews.com/story/0,2933,478024,00.html

Saturday, January 17, 2009

Btown Blog Logs - 1/17/2009



Here are the latest active civilian aero freqs intercepted this morning here in Btown.

**Need some help from my readers. Does anyone have any additional information on ATL ARTCC freq 125.825 (RCAG, Sector, etc)?

124.325 ATL ARTCC Hampton GA Ultra High Altitude FL330 and above Sector 23 Clark Hill Sector

124.875 ATL ARTCC Chattanooga TN High Altitude Sector 36 Alatoona Sector

125.025 ATL ARTCC Jonesville SC High Altitude FL330 and above Sector 26 High Rock Sector

125.575 ATL ARTCC Columbus GA High Altitude Sector 10 LaGrange Sector

125.625 ATL ARTCC Owning (Greenville) SC High Altitude Sector 32 Spartanburg Sector

**125.825 ATL ARTCC Unknown RCAG Atlanta ARTCC Discrete: Ultra High Altitude

125.925 ATL ARTCC Crossville (Hinch Mountain) TN High Altitude Sector 39 Burne Sector

128.000 ATL Approach Control - Erlin 5 STAR Arrival/Herko 2 STAR Arrival

128.725 ATL ARTCC Birmingham AL High Altitude Sector 03 Gadsden Sector

132.050 ATL ARTCC Chattanooga TN Low Altitude Discrete: Approach/Departure services for various small airports via this RCAG Sector 05 Dallas Sector

132.975 ATL ARTCC Hickory NC Ultra High Altitude FL330 and above Sector 43 Pulaski Sector

134.075 ATL ARTCC Newport TN Ultra High Altitude FL330 and above Sector 40 Blue Ridge Sector

Congress unprepared for Jan. 20 emergency

By Jordy Yager
http://thehill.com/leading-the-news/unprepared-for-emergency-2009-01-15.html

Many lawmakers do not know how to use a critical communications system in the event of an emergency during President-elect Obama’s Inauguration.

Despite months of security planning for the Inauguration by various government agencies, a White House-directed phone service that is supposed to be given to every lawmaker for emergency use remains a mystery to many members of Congress.

The chairman of the House Administration Committee, which oversees the security of all House members and staff, has never seen or heard of the tool. “I don’t know anything about it,” said Rep. Robert Brady (D-Pa.). “I’m definitely going to find out, though.”

Brady is far from alone. Eight lawmakers The Hill spoke to on Wednesday said they either were not sure of or did not have the Government Emergency Telecommunications Service (GETS) card, which gives users priority telephone access during emergencies, when traditional phone lines may be disconnected or flooded with calls.

“I don’t know anything about that,” said Rep. Barney Frank (D-Mass.), a committee chairman who has served in the House for nearly 30 years.

Five other members said they had and were familiar with the card, but some of them were unsure how to use it.

The GETS card is one of several emergency preparedness measures taken by the House and Senate sergeants at arms and the House Chief Administrative Office (CAO) to ensure the safety of lawmakers. Lawmakers also are given a card giving them instructions on how to evacuate the Capitol in the event of an emergency.

Lawmakers seem more familiar with that card, as several who were unfamiliar with the GETS knew about the evacuation card.

Still, knowledge of the GETS card could be particularly important on Jan. 20, when most representatives of all three branches of government attend the first black president’s Inauguration.

Without the card, lawmakers might be unable to communicate with emergency personnel to ensure their own safety and the safety of their staffs and any visitors to the Inauguration who are under their care.

They might also be unable to take part in any response to a terrorist attack because of the likelihood that traditional communications lines would be overloaded.

In the event of an emergency, phone service is apt to be interrupted or even inaccessible because of the high volume of people trying to call friends, family and emergency personnel. The GETS system allows for users to supersede this congestion by using an elevated communication highway of sorts.

“GETS is necessary because of the increasing reliance on telecommunications … Recent events have shown that natural disasters, power outages, fiber cable cuts and software problems can cripple the telephone services of entire regions,” reads the GETS website.

On Sept. 11, 2001, lawmakers had major difficulties making calls to their district offices, and then-Rep. Porter Goss (R-Fla.), the chairman of the House Intelligence Committee at the time, had trouble communicating with CIA officials. In the following years, requests for GETS cards surged.

The fact that many lawmakers are unfamiliar with the system isn’t new. A year after the Sept. 11 attacks, then-House Chief Administrative Officer James Eagen testified to Congress that GETS cards had been delivered to all members. But despite that assertion, The Hill in 2006 found that dozens — if not hundreds — of legislators did not have GETS cards in their wallets.

In 2006, then-Sen. Obama told The Hill he did not have a GETS card and asked one of his aides to secure one for him.

The office of the Senate sergeant at arms said it ensures that lawmakers know about the GETS cards.

“We instruct them on what it’s used for, which is for a means of communication if the regular phone system is not available, and whether they choose to use that as their primary [emergency measure] or not is up to them,” said Kimball Winn, the chief information officer for the Senate sergeant at arms.

The CAO declined to comment for this story, and the office of the House sergeant at arms did not return calls.

Still, many lawmakers seem unaware of the cards. Of five members The Hill spoke with who had a GETS card, none could find it in their wallets, and several did not know how to use it, though they said they received instructions at one point.

Surprisingly, members who have been on Capitol Hill for more than 10 years, like Frank and former presidential candidate Rep. Ron Paul (R-Texas), were most unsure of the GETS system.

“I don’t know anything about it,” said Paul at first. “Oh, they might have sent it to me and if they did, I didn’t pay any attention to it.”

Freshman members like Rep. Glenn Nye (D-Va.) and more junior members like Rep. Charlie Dent (R-Pa.), by contrast, said they have been instructed on how to use the calling service and been issued cards with the number.

“I have the card and have had it ever since I was elected,” Dent said. “I keep it in my wallet but I’ve never had to use it.”

With some officials estimating more than 4 million people will attend the Inauguration — the first presidential transfer of power since the United States has been at war and the first since the 2001 terrorist attacks — security officials have taken above-normal measures to ensure the safety of the public and politicians. This transition is likely to leave the country and D.C. more prone to an attack than usual, according to a private report obtained by The Hill last week.

Rep. Michael Capuano (D-Mass.), who chairs the Capitol Security subcommittee, said he had the card but did not know anything about it.

“I was [instructed how to use it] but I don’t remember what it was because I’ve got a cell phone,” said Capuano, who added that he is not very concerned about what he would do in the event of an emergency.

“I’m one member of Congress, so guess what? The world will go on without me.”

Thursday, January 15, 2009

President Announces Declaration For The District Of Columbia

WASHINGTON, D.C. -- The President today declared an emergency exists in the District of Columbia and ordered federal aid to supplement the District's response efforts in support of the 56th Presidential Inauguration. The declaration makes available funding and support for the purposes of ensuring the District of Columbia and the federal government are optimally prepared and postured to respond to the 56th Presidential Inauguration, beginning on January 17 through January 21.

The President's action authorizes the Department of Homeland Security, Federal Emergency Management Agency (FEMA), to provide appropriate assistance for certain emergency protective measures, authorized under Title V of the Stafford Act. FEMA will also be authorized and prepared to coordinate any necessary response efforts, should an emergency arise. Specifically, assistance is available to the District for emergency protective measures that are undertaken to save lives and protect public health and safety. Direct Federal assistance, at 100 percent federal funding will be provided during the period of January 17-21, 2009, and reimbursement of emergency protective measures (Category B), under the Public Assistance program, at 100 percent federal funding for work performed on January 20, 2009. FEMA will reimburse for eligible emergency protective measures performed on January 20, 2009, only if the District has expended on the Presidential Inauguration during the period of January 17-21, 2009, the $15 million appropriated to it for "Emergency Planning and Security Costs" by the Continuing Appropriations Resolution 2009, P.L. 110-329.

FEMA Administrator David Paulison named Donald L. Keldsen the federal coordinating officer for federal coordination operations in the District of Columbia.

The Presidential Inauguration has been designated as a National Security Special Event (NSSE) by the Department of Homeland Security. FEMA's role is to be prepared to respond to a natural disaster, acts of terrorism and other man-made disasters.

FEMA is also taking the following actions to support the 56th Presidential Inauguration.

* FEMA has activated its National Response Coordination Center and Regional Response Coordination Center for FEMA Region III ;
* FEMA's National Incident Management Assistance Team - East has been activated; and
* More than 200 highly trained FEMA employees are supporting the Inauguration at multiple designated locations.

FEMA coordinates the federal government's role in preparing for, preventing, mitigating the effects of, responding to, and recovering from all domestic disasters, whether natural or man-made, including acts of terror.

Sunday, January 11, 2009

CHM Scanning the 56th Presidential Inauguration



If you plan on attending the Prez Inaug next week (personally I wouldn't be within 500 miles of that mess), here is an online PDF guide for scanner radio hobbyist courtesy of the Capitol Hill Monitor group that you might want to bring along.

http://henney.com/chm/0109/chm0109.pdf

Saturday, January 10, 2009

Solar Weather Threat To Wired Earth


U.S.-commissioned report sees possibility of 'space weather [hurricane] Katrina' that could cost up to $2 trillion. See full story http://www.aviationweek.com/avnow/news/channel_space_story.jsp?id=news/SOL010709.xml\

NY State Said to Be Close to Dropping Police Radio Project

By KEN BELSON and AL BAKER

State officials are close to canceling a $2 billion contract to build a statewide wireless network for emergency agencies after critical tests on the network failed late last year, according to state officials briefed on the results.

Lawyers for the vendor, M/A-COM, a subsidiary of Tyco Electronics, sent the state a letter on Friday threatening to sue if officials follow through on their plan to shut down the project, which was intended to improve radio communications throughout the state, but particularly in remote areas where police agencies have trouble talking to one another.

State officials, though, were said to be determined to shut down the project because it was unclear, after a pilot program in two counties and nearly $52 million in expenditures, that M/A-COM's system would ever work as expected. A major problem has been the difficulty and unanticipated cost of installing radio towers in remote, mountainous areas, according to the officials and technical experts, who spoke
anonymously because the contract dispute is at a delicate juncture.

To finish the project, state officials decided that considerably more money would have to be spent at a time when the state is expected to have large budget deficits. At the same time, the state cannot embark on a new network project, no matter what the cost, until it untangles itself from its current contract, one state official said.

"The state is reviewing the letter from the attorneys for M/A-COM," said Morgan Hook, a spokesman for Gov. David A. Paterson. "We anticipate making a decision in short order that will be based on our factual analysis of the system's performance."

Lawyers from Weil, Gotshal & Manges, the firm representing M/A-COM, said in their letter that it was "patently obvious" that the state was determined to cancel the contract because of political and financial pressure and was using technical issues as a pretext for the cancellation.

The State Office for Technology, which has overseen the network's construction since 2005, "has acted in bad faith throughout the past year" and has made "defamatory and untrue statements regarding M/A-COM's performance under the contract," the letter said.

The largest technology contract in state history, the network has had problems from the start, according to state officials. In August, the state sent a default letter to M/A-COM ordering it to fix deficiencies or face cancellation. A decision to cancel the project has seemed imminent since then, and some state officials, and lawyers for the contractor, have spoken of it as a fait accompli.

The original plan, conceived after the attacks of Sept. 11, 2001, was designed to link emergency agencies from the tip of Long Island to Niagara Falls via a series of radio towers. The network was meant to cover 95 percent of New York's area and 97 percent of its roadways, including some of the most remote parts of the state.

The Office for Technology is looking at other methods, including Internet-based communications and cellphone technology, that are said to be more cost-effective and could provide more reliable and cheaper service than the radio technology called for in the original contract.

Daniel M. De Federicis, the president of the Police Benevolent Association of the New York State Troopers, said that until a statewide radio network has been built, his organization would push for improvements in the present patchwork of networks.

"The lack of an operating statewide wireless network is beyond frustrating," Mr. De Federicis said in a statement. "The P.B.A. cannot stress enough that this creates life-and-death situations for police officers, and we are running out of synonyms for `ineptness' to describe the situation."

The project, which is now two years behind schedule, has faced questions from the outset. Critics questioned the Pataki administration's decision to award the contract to M/A-COM, whose bid was $1 billion less than its closest major competitor, Motorola.

The radio system was supposed to be working in Erie County and neighboring Chautauqua County by June 2007, but repeated problems caused the City of Buffalo to quit the statewide system in December 2007.

M/A-COM missed other operational deadlines, finally prompting the Office for Technology to declare in August that the company was in default. The office gave the company 45 days to fix 19 deficiencies.

In their letter Friday, lawyers for the company said that all technological issues had been addressed and that any delays were the fault of the state.

During an 11-day test period in July, the network was found to be inoperable for nearly 44 hours, far more than the 53 minutes of downtime per year authorized by the state.

Since the state default letter was issued in August, some workers hired to build the network have been laid off, and several subcontractors have stopped work on the network.

In late August, the state comptroller, Thomas P. DiNapoli, issued a report criticizing the plan. The report noted that the "network testing was not properly planned or implemented, and the needs of the public safety user agencies were not fully taken into account during the network design and development process."

Separately, M/A-COM agreed to pay the state $4 million after auditors found that the company had billed for services that had not been provided and charged for some equipment that had already been paid for.

A spokesman for M/A-COM, Steven A. Greenberg, said on Friday, "We remain ready to hear from the state, as we have since testing concluded last fall."