Friday, June 6, 2014
Ham Radio assisted in Reactivating Three Decade Old NASA Satellite
The U-K newspaper the Daily Mail says that several radio amateurs were involved with Project Reboot in regaining control on May 29th of the 35 year old abandoned International Sun-Earth Explorer 3 spacecraft. Hams named in the article include Dennis Wingo, KD4ETA; Achim Vollhardt, DH2VA, and Mario Lorenz DL5MLO.
The International Sun-Earth Explorer was launched in 1978 to study Earth’s magnetosphere. It carries thirteen scientific instruments to measure plasmas, energetic particles, waves, and fields. As of this past May, all but one is thought to be functional. An on-board data handling system gathers the scientific and engineering information from all systems in the spacecraft. It then formats this information into a serial stream for transmission back to Earth by an on-board 5 watt transmitter.
After completing its main mission, the satellite was repurposed in 1983 to study two comets. At that time it was renamed the International Cometary Explorer and has been in a heliocentric orbit since then, traveling just slightly faster than Earth. It’s finally catching up to our planet from behind, and will be closest to Earth this August.
Now, KD4ETA has released an update on the attempts by the projects volunteers, including the radio amateurs, to gain control of the spacecraft. According to Wingo, the probe has been successfully commanded into engineering telemetry mode. He noted the job done by DH2VA and also Phil Karn, KA9Q, to make this happen. Karn is well known in the amateur radio community for his work on the KA9Q Network Operating System, the early 9600 bit FSK radio modems, and more recently, the introduction of forward error correction into the Amateur Satellite Service.
As we go to air, Project Reboot members are working on deadline. If they get the spacecraft to change its orbit quickly, it can use the Moon's gravity to get back into a useful halo orbit. If not, the fear is that for all practical purposes the International Sun-Earth Explorer 3 could be lost. We will keep you posted.
For the Amateur Radio Newsline, I’m Heather Embee, KB3TZD, in Berwick, Pennsylvania.
--
The actual first command to the revived International Sun-Earth Explorer 3 spacecraft was successfully sent from the Arecibo Radio Observatory in Puerto Rico using the facilities 305 meter dish. This after the volunteer team installed the needed modulator, demodulator and power amplifier to make contact and control of the satellite possible. More is on the web at tinyurl.com/reboot-project (AMSAT-UK, Daily Mail, Southgate)
Thursday, June 5, 2014
Artsat One Invader Reports Needed
According to Sanada, the satellite does not reply to commands from the control station and those involved in the project are trying to find out why in hope of finding a fix or work-around. The downlink frequency for Artsat One Invader is 437.325MHz. If you hear the bird please send that information via a form on the web at api.artsat.jp/report
Thursday, March 6, 2014
OSCAR-11 / UOSAT-2 Celebrates 30 Years in Orbit
OSCAR-11, also known as UOSAT-2, was designed and built by a team of engineers at the University of Surrey in Guildford, Surrey, UK as the successor to OSCAR-9 / UOSAT-1 (see Hobby Electronics August 1981).
It was launched from the Western Test Range at Vandenberg Air Base, in Lompoc, California along with LANDSAT-5 on a Delta 3920 rocket on March 1, 1984.
OSCAR-11 was the most rapidly designed OSCAR, going from inception to launch in only five months. It was also the first amateur satellite to carry a digital communications package into Earth orbit, and the first to be controlled by a CPU running software written in the high-level programming language “Forth”.
OSCAR-11 carries beacons in three amateur radio bands.
The 145.826 MHz beacon transmits FM Audio Frequency Shift Keying (AFSK) 1200 bps ASCII data. It the early years it also transmitted a voice message from the digitalker experiment.
The 435.025 MHz beacon transmitted either 1200 bps FM AFSK or 4800 bps PSK data. This beacon was used to downlink information from the Digital Store and Readout (DSR) Experiment, which includes CCD Earth image data, results from the Particle Wave Experiment, and engineering data from the RCA COSMAC 1802 CPU.
The 2401.5 MHz beacon transmitted FM and PSK signals. Antenna polarization for all three beacon transmitters is left-hand circular (LHCP). Only the 145.826 MHz beacon is now operational.
Addition OSCAR-11 information
http://www.g3cwv.co.uk/oscar11.htm
OSCAR-11 page on the DK3WN satellite blog at
http://www.dk3wn.info/p/?cat=47
SSTL Blog – Happy 30th Birthday to UOSAT-2
http://www.sstl.co.uk/Blog/March-201...ay-to-UoSAT-2-
OSCAR-9 and OSCAR-11 TV News Reports
http://amsat-uk.org/2011/10/30/oscar...-news-reports/
BBC Micro ASTRID UoSAT receiver and AMSAT-UK Software Library
http://amsat-uk.org/2011/12/11/
bbc-micro-and-amsat-uk-software-library/
http://www.southgatearc.org/news/201...s_in_orbit.htm
Tuesday, March 4, 2014
Launch of Two Hundred 437MHz Satellites
They will be deployed into a 325×315 km 51.5 degree inclination orbit. You should be able to watch the launch live on NASA TV at http://www.nasa.gov/multimedia/nasatv
A Sprite is a tiny, 3.5 by 3.5 cm, single-board spacecraft that was developed by Zac Manchester KD2BHC. It has a microcontroller, radio, and solar cells and is capable of carrying single-chip sensors, such as thermometers, magnetometers, gyroscopes, and accelerometers.
The 200 Sprites are carried in a 3U CubeSat called KickSat. They are stacked atop a spring-loaded pusher and secured by a nichrome burn wire system.
On reaching orbit KickSat will perform a de-tumble maneuver and establish communication with Cornell University’s ground station. After check-out, the spacecraft will be put in a sun-pointing attitude and spun up to maintain that attitude.
A command signal from the ground station will then trigger the deployment and the Sprites will be released as free-flying spacecraft. After deployment, telemetry and sensor measurements from the individual Sprites will be received through Cornell’s ground station in Ithaca, NY, as well as several other amateur ground stations around the world.
Due to the low orbit Sprites will have a short lifetime before they re-enter the atmosphere and burn up. In the best-case scenario the orbital lifetime could be six weeks but realistically it may be considerably shorter depending on atmospheric conditions.
All Sprites operate on a single frequency of 437.240 MHz and use Code Division Multiple Access (CDMA). The transmitter runs 10 mW output of Minimum Shift Keying (MSK) modulated binary data with each data bit modulated as a 511 bit Pseudo-Random Number (PRN) sequence. The ITU emission designator is 50K0G1D.
The KickSat CubeSat has downlinks on 437.505 MHz and 2401-2436.2 MHz.
KickSat Sprite Ground Station by Andy Thomas G0SFJ http://kicksat.wordpress.com/support...round-station/
British Interplanetary Society: Sprite Technical Summary http://www.bis-space.com/2013/03/09/...hnical-summary
KickSat project information http://zacinaction.github.io/kicksat/
KickSat on KickStarter https://www.kickstarter.com/projects/zacinaction/
kicksat-your-personal-spacecraft-in-space/
Check this site for the latest CRS 3 launch date http://spaceflightnow.com/tracking/
http://www.southgatearc.org/news/201...satellites.htm
Friday, February 21, 2014
Cubesats Deployed from International Space Station
In addition to the 28 Planet Labs micro-birds, there are also four amateur radio CubeSats waiting to be placed on-orbit. These are LituanicaSat-1, LitSat-1, ArduSat-2 and UAPSat-1 as well as a 915 MHz CubeSat SkyCube. All are planned to be deployed in the coming weeks.
Wednesday, February 19, 2014
Cape II Amateur Radio Satellite Cube OSCAR 75 or LO-75
The CAPE II ham satellite operates on 145.825 MHz FM with a CW beacon signing the call W5UL. The bird also includes a digipeaters, text to speech operation, a simplex repeater, e-mail and tweet functions. The ground station software can be downloaded at www.ulcape.org
Wednesday, February 12, 2014
Going to Space: Send Your Name to the Asteroid Bennu
The "Messages to Bennu" microchip will travel to the asteroid aboard the Origins Spectral Interpretation Resource Identification Security Regolith Explorer spacecraft. The robotic mission will spend more than two years at the asteroid, which has a width of only about 1,760 feet. The spacecraft will collect a sample of Bennu's surface and then return it to Earth .
The deadline to submit your name online is Sept. 30, 2014. Participants who submit their names to the "Messages to Bennu" campaign will be able to print a certificate of appreciation to document their involvement. To submit your name for inclusion on this mission please take your web browser to planetary.org/bennu. While there are no instructions as to how to how to include your callsign, we found it simple to just put it right after your last name. (ANS, NASA)
Thursday, November 21, 2013
ISS Celebrated its 15th Birthday
The International Space Station began construction with the arrival on-orbit of the Russian built Zarya Module. This lead to the ongoing international mission to build the orbital outpost one piece at a time.
Today, the ISS is about the size of a football field with roughly the same amount of livable space as a six-bedroom house. Amateur Radio became a part of the Space Station two weeks after the first two licensed ham radio operators took up residence in it on Expedition One. Since then hams have taken part in all 38 expeditions to this point.
Five different space agencies representing fifteen countries have contributed to construction of the $100 billion orbital outpost.
Monday, October 7, 2013
LADEE Spacecraft goes into Lunar Orbit
Saturday, March 2, 2013
LES 1
Phil Williams, G3YPQ, is an Amateur Radio Astronomer in
North Cornwall in the U.K.. According to reports he
accidentally picked up the signal and after cross checking
with various lists, he identified it as LES 1.
LES 1 was built by the Massachusetts Institute of Technology
and launched in 1965. The satellite failed to reach its
intended orbit owing to a wiring error and has been drifting
out of control ever since.
Williams ran across it while monitoring near 237 MHz when he
noticed a signal with a peculiar signal drift caused by the
bird tumbling end over end every 4 seconds as the solar
panels became shadowed by the satellites engine. Williams
said that gives the signal a particularly ghostly sound as
the voltage from the solar panels fluctuates.
The LES 1 satellite is about the size of a small car and is
not likely to re-enter the atmosphere for a long time as the
orbit is still relatively high. It poses no threat other
than that caused by the thousands of other pieces of space
junk currently in orbit. By now its likely that the on
board batteries have now disintegrated so its likely that
some other component failure has caused the transmitter to
start up when its in sunlight bringing the ghost satellite
back to life.
Tuesday, February 19, 2013
Smartphone-Sat- STRAND-1
The BBC says that the world’s first 'smartphone-sat' project called STRAND-1 will be ready to launch at the end of February. The STRAND-1 CubeSat will carry a Google Nexus One Android smartphone into space to demonstrate the feasibility of using cheap smartphone’s electronics to control a spacecraft.
Also included will be a software-based speech synthesizer to commemorate the U-O-SAT family of amateur radio satellites that were launched in the 1980′s. There will also be an amateur radio AX.25 packet radio downlink on 437.575 MHz.
The STRAND-1 satellite was built in Guildford in the United Kingdom by volunteers from the Surrey Space Centre and Surrey Satellite Technology Limited in their spare time. It is planned to be launched on February 25th into a 785 km orbit by the Indian Space Research Organization rocket. More is on-line at www.amsat-uk.org and we will have more ham radio space related news later on in this weeks Amateur Radio Newsline report. (AMSAT-UK)
Monday, February 18, 2013
ARISS has switched after experiencing issues w/Kenwood D700
Frank Bauer, KA3HDO, is AMSAT's Vice President for Human Spaceflight Programs. He says that for some reason signals from the Service Module Kenwood D700 radio are much diminished. He notes that a recent contact with Israel had low audio levels. Another contact with the Hospital for Sick Children was even worse. Only one student was able to talk to Chris Hadfield before signals on the ground were lost even though the crew reports hearing the ground station well.
It should be noted that both these contacts were with made using telebridge stations which have above average gear. Also astro-ham Hadfield used the space stations IP Phone, immediately after the hospital radio contact and answered all the student's questions so that all was not lost. A later contact with a school in Japan using the Columbus Module Ericsson radio proved very successful. (ANS, ARISS)
Monday, July 2, 2012
SimpleSat Look Down from W9KE
SimpleSat
A: If you do not have internet access the program will work but the tracking map will not
be displayed.
A: Still need internet access to authenticate my Bing Maps license number.
Friday, May 25, 2012
HORYU-2 Satellite
Wednesday, April 25, 2012
Japan will be Launching 16 Educational Ham-Sats
The first of the new birds to be launched will be the amateur radio satellite HORYU-2 built by students at the Kyushu Institute of Technology. Its mission is to take pictures of the Earth using a small C-MOS camera called SCAMP that was developed by the University of Surrey in the UK. The SCAMP camera takes a 640x480 pixel picture in the popular JPEG format. That means from 700 km altitude, one pixel corresponds to 1.6 km. HORYU-2 will be followed in July by the transport of several items to the International Space Station. This mission will deliver the Japanese Experiment Module Small Satellite Orbital Deployer or JEM along with the Japanese CubeSats WE- WISH, FITSAT-1 and RAIKO. These CubeSats should be deployed from the ISS in September using the JEM and robot arm. FITSAT-1 may be the most interesting of these. It will use a neodymium magnet for attitude control. It will also have multiple downlinks. These include CW on 437.250 MHz, AX.25 on 437.445 MHz and a 4 watt high speed data transmitter on 5840 MHz. The latter is capable of sending a 640 by 480 VGA JPEG image in 6 seconds. In addition to its other experiments, FITSAT-1 will also carry a set of high power LED's that will be driven with 100W pulses to produce extremely bright flashes. It is hoped, will be observable by the unaided eye or with small binoculars from the ground. Both the 5840 MHz and optical downlinks have a high power consumption so it may be that they are only activated only over Japan. In December the TSUBAME satellite is planned to be launched on a Japanese H-IIA booster. It will carry a CW beacon on 437.250 MHz and AX.25 packet at 1200 and 9600 bit per second telemetry on 437.505 MHz. The remaining satellites will be placed into orbit on subsequent flights.
Saturday, March 10, 2012
Next-Gen Weather Satellites to Improve Tornado Warnings
Feb 29, 2012: When you read the following paragraph, consider the following: Tornado season hasn't even started yet. On Jan. 22 and 23, 2012, more than 37 tornadoes struck the southern USA. Ten of them tore across the Lower Mississippi Valley into Alabama. Worst hit were St. Clair and Jefferson County, Ala., where 2 people were killed, about 100 others injured, and at least $30 million in damage was done. It was a chilling reminder of the April 2011 onslaught of deadly tornadoes that took a staggering toll across southern and Midwestern states.
In southern parts of the USA, tornado season tends to peak in springtime. Yet January 2012 produced 73 winter tornadoes -- third most of any January in recorded history. Most of them struck southern states. And since over a quarter of the incredible 1,688 twisters confirmed across the US in 2011 occurred in the four-state region of Alabama, Georgia, Mississippi and Tennessee, residents there are becoming ever more wary of darkening skies.
"Even with our advances in science and communications, we can still be surprised by the deadliest storms," says NOAA scientist Steve Goodman. "But NOAA is working with NASA and university researchers to give more lead time in tornado warnings."
Southern tornadoes are especially insidious and challenging to track. The hilly, forested terrain in southern states makes an approaching twister harder to spot than in the flat Midwest. In the south you might not see the first evidence of an approaching tornado until it's almost in your back yard.
An Alabama resident describes the scene just before one of the April 2011 twisters struck near his home: "Suddenly, all the trees in my back yard corkscrewed violently, in unison, toward the northwest." Moments later, the storm was there.
Rain wrapped tornadoes are especially hard to see, as are night-time tornadoes. And records indicate that southern tornadoes often strike at night.
To reduce the surprise, NOAA and NASA2 are developing the Geostationary Operational Environmental Satellite-R, or "GOES-R series," with the first expected to launch in late 2015. These next-generation weather satellites bristle with state-of-the-art instruments for improved scouting of these killer storms, even at night.
Tornadoes are, by their very nature, difficult to pin down. The Advanced Baseline Imager (ABI) on GOES-R will improve meteorologists' ability to assess conditions that spawn twisters. Compared to current GOES imagers, the ABI provides twice the spatial resolution, three times as many channels of information, and more than five times the update rate.
"ABI will give us a much clearer picture of the clouds – where and how tall they are, how much and what kind of moisture they hold, and how they are moving and intensifying," says NOAA research meteorologist Tim Schmit.
Most importantly, ABI can better detect the super-cold "overshooting tops" that mean severe weather is imminent. "Overshooting tops portend huge energy inside the cloud – it takes tremendous energy and upward velocity to poke through the lid of the tropopause," explains Schmit.
"During episodes of severe weather, ABI can show conditions every 30 to 60 seconds. The system in use now only shows them every 7.5 minutes. And in normal mode, ABI will send readings over the continental U.S. every 5 minutes as opposed to every 15-30 minutes."
Lightning is another key to tornadoes.
"Studies show that sudden changes in the total lightning correlate with [the onset of] tornadoes," says Goodman.
Detecting lightning is a new specialty of GOES-R.
"GOES-R's Geostationary Lightning Mapper, or GLM, will see all the lightning: cloud-to-ground, cloud-to-cloud, and inside each cloud. And since this is the first time we'll have lightning detection from geostationary orbit, it means GOES-R will constantly monitor and map the lightning across the western hemisphere."
The GLM is expected to give 7 more minutes of lead time in tornado warnings. Average lead time now is 13 minutes.
"With GOES-R you'll have upwards of 20 minutes to get to a safe haven."
That sure beats standing in your back yard, in the dark, waiting for the trees to twist.
Friday, February 3, 2012
RS-39 Now in Orbit.; Reception Reports Needed
RS-39 also carries CW beacons on 435.215 and 435.315 MHz. Hams hearing these signals are being asked to submit reception reports via e-mail to the Space Research Institute of the Russian Academy of Sciences at amateur-rs39 (at) chibis (dot) cosmos (dot) ru. Each report will be acknowledged with a special QSL card.
We will have more ham radio space related news later on in this week’s Amateur Radio Newsline report.
Monday, August 1, 2011
ARISSat-1/KEDR
HOUSTON --
Two cosmonauts will conduct a six-hour spacewalk on Wednesday, Aug. 3, to continue outfitting the Russian segment of the International Space Station. NASA Television will broadcast the spacewalk beginning at 9 a.m. CDT.
Expedition 28 Russian Flight Engineers Sergei Volkov and Alexander Samokutyaev will install laser communications equipment and replace experiments on the Zvezda service module. They also will retrieve a rendezvous antenna, relocate a boom structure to aid future spacewalks and deploy a small satellite equipped with an amateur radio transmitter and a student-built experiment.
The duo will wear Russian Orlan spacesuits and will emerge from the Pirs docking compartment airlock at about 9:30 a.m. The spacewalk will be the third for Volkov, who performed two spacewalks as Expedition 17 commander in 2008. This will be the first spacewalk for Samokutyaev.
For NASA TV downlink, schedule and streaming video information, visit:
For information about the International Space Station, visit:
Wednesday, January 19, 2011
NASA needs Amateur Radio Operators
I think this is really cool.
------------------------------------------------
HUNTSVILLE, Ala. -- Wednesday, Jan. 19 at 11:30 a.m. EST, engineers at Marshall Space Flight Center in Huntsville, Ala., confirmed that the NanoSail-D nanosatellite ejected from Fast Affordable Scientific and Technology Satellite, FASTSAT. The ejection event occurred spontaneously and was identified this morning when engineers at the center analyzed on board FASTSAT telemetry. The ejection of NanoSail-D also has been confirmed by ground-based satellite tracking assets.
Amateur ham operators are asked to listen for the signal to verify NanoSail-D is operating. This information should be sent to the NanoSail-D dashboard at: http://nanosaild.engr.scu.edu/dashboard.htm. The NanoSail-D beacon signal can be found at 437.270 MHz.
Further Reading; click here
Follow the NanoSail-D mission operation on Twitter at:
For additional information on the time line of the NanoSail-D deployment visit:
To learn more about FASTSAT and the NanoSail-D missions visit:
Tuesday, December 21, 2010
SO-67 FM Suspended
Got this in the E-Mail box this morning
Johann Lochner, ZR1CBC, reports that the FM Amateur Radio transponder on SO-67 is being temporarily suspended due to a probable radiation event.
On the AMSAT bulletin board he writes:
Last week the flash boot memory of a CAN controller on Sumbandila was corrupted by a probable radiation event. It does not affect satellite health but prevents activation of the amateur radio repeater, as the particular script detects an anomaly and aborts.
The same problem also occurred in October of 2009 and was corrected. However, the fix requires time consuming effort, which cannot be exerted immediately.
SO-67 repeater activations are therefore suspended. We apologize for any disappointment and hope to return to normal operations somewhere in January.
73 de ZR1CBC, Johann.
AMSAT Bulletin Board AMSAT-BB
http://www.amsat.org/amsat-new/tools/maillist/
Southern African Amateur Radio Satellite Association (SA AMSAT)
http://www.amsatsa.org.za/
HOW TO READ PROPAGATION NUMBERS
The A index [ LOW is GOOD ]
- 1 to 6 is BEST
- 7 to 9 is OK
- 11 or more is BAD
Represents the overall geomagnetic condition of the ionosphere ("Ap" if averaged from the Kp-Index) (an average of the eight 3-hour K-Indices) ('A' referring to amplitude) over a given 24 hour period, ranging (linearly) typically from 1-100 but theoretically up to 400.
A lower A-Index generally suggests better propagation on the 10, 12, 15, 17, & 20 Meter Bands; a low & steady Ap-Index generally suggest good propagation on the 30, 40, 60, 80, & 160 Meter Bands.
SFI index [ HIGH is GOOD ]
- 70 NOT GOOD
- 80 GOOD
- 90 BETTER
- 100+ BEST
The measure of total radio emissions from the sun at 10.7cm (2800 MHz), on a scale of 60 (no sunspots) to 300, generally corresponding to the sunspot level, but being too low in energy to cause ionization, not related to the ionization level of the Ionosphere.
Higher Solar Flux generally suggests better propagation on the 10, 12, 15, 17, & 20 Meter Bands; Solar Flux rarely affects the 30, 40, 60, 80, & 160 Meter Bands.
K index [ LOW is GOOD ]
- 0 or 1 is BEST
- 2 is OK
- 3 or more is BAD
- 5 is VERY VERY BAD
The overall geomagnetic condition of the ionosphere ("Kp" if averaged over the planet) over the past 3 hours, measured by 13 magnetometers between 46 & 63 degrees of latitude, and ranging quasi-logarithmically from 0-9. Designed to detect solar particle radiation by its magnetic effect. A higher K-index generally means worse HF conditions.
A lower K-Index generally suggests better propagation on the 10, 12, 15, 17, & 20 Meter Bands; a low & steady Kp-Index generally suggest good propagation on the 30, 40, 60, 80, & 160 Meter Bands.
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