Vintage Spacelab 2 video featuring Amateur Radio

W0ORE STS-51-F QSL Card - Image Credit John Magliacane KD2BD

The second ham radio transmissions by an amateur radio operator in space were made by Tony England W0ORE during the Challenger shuttle mission STS 51-F in 1985.

He achieved the first ever two-way Slow Scan TV (SSTV) space contact during the flight when he contacted GB3RS the headquaters station of the Radio Society of Great Britain (RSGB).

Tony W0ORE was running a Motorola model MX-340 handheld 2-meter transceiver and a Robot Research model 1200C slow-scan television scan converter with an antenna fitted on the inside of one of Challengers windows.

Narrated by the Commander and crew, these videos contains footage selected by the astronauts, as well as their comments on the mission. Footage includes launch, onboard crew activities, and landing. The Shuttle Amateur Radio Experiment (SAREX) is mentioned 11:40 into the video.

Space Shuttle STS-51-F Challenger Spacelab 2 Post Flight Press Conference Film 1985 Part 1 of 2

Part 2 of 2

The ITN TV news report ‘Space Radio Hams’ on the two-way SSTV contact between GB3RS at RSGB HQ and Tony England W0ORE (believed to have been on 145.550 MHz) can be seen at
http://www.itnsource.com/shotlist//ITN/1985/08/04/AS040885006/

Videos taken by a local TV station, of a contact between a school in Staten Island, NY and Tony England W0ORE on STS-51F can be seen at http://www.southgatearc.org/news/january2009/historic_shuttle_videos.htm

John Magliacane KD2BD was one of the amateurs who had a contact with Tony England, see his website at http://www.qsl.net/kd2bd/kd2bd.html

STS-51-F (also known as Spacelab 2) was the nineteenth flight of NASA’s Space Shuttle program, and the eighth flight of Space Shuttle Challenger. It launched from Kennedy Space Center, Florida, on 29 July 1985, and landed at Edwards Air Force Base, California, just under eight days later on 6 August 1985, at 12:45:26 pm PDT.

Shuttle Mission STS-51-F http://en.wikipedia.org/wiki/STS-51-F

Vintage Videos of STS-9 Columbia Mission and Spacelab http://www.uk.amsat.org/7265

AMSAT-LU Balloon Launch May 19

LU7AA brings news that on Saturday May 19 from 11hs-LU on (GMT-3), a free Balloon UV Repeater will fly from the city of General Pico (Airport), Province of La Pampa, Argentina, 571 Km west of Buenos Aires City. See details and photos http://www.amsat.org.ar/globo19.htm

Given administrations requests by Amsat Argentina, launch is authorized and appropiate NOTAM (NOTification to AirMen) had been issued and granted by National Civil Aviation Administration.

Contest & Prices: first 10 station making the most distance & contacts will receive special certificate, top winner will receive a UHF/VHF handy.

Payload will operate as an UHF to VHF crossband repeater, with CW tlm, APRS location and SSTV emissions in local and space frequencies.

According estimates Balloon could reach 100,000 feet height, traveling from 50 to 100 miles towards east.

Thus allowing contacts between stations located in provinces of Buenos Aires, Santa Fe, Entre Rios, Cordoba, Catamarca, Santiago del Estero, La Pampa, San Luis, Mendoza, San Juan, Rio Negro, Neuquen, Uruguay & Chile. (Launch is from Argentina Geo-Center to permit higher participation). See coverage map on
http://www.amsat.org.ar/picocubr.jpg and estimated trajectory in
http://www.amsat.org.ar/pico120519.jpg .

For these experiences, Amsat-LU works with and it is thankful to hams of Radio Clubs of Gral.Pico, QRM Belgrano, APRS Group and amsat-LU members development team as well as those who have actively participated and sent their reports in previous events.

More information at
http://www.amsat.org.ar/lu4aao/experimento_globo_y_parapente.htm.

Several flown experiments have been successfully operated during 2011/12 in manned-gliders, airplanes, captive and free Balloons allowing operational & practice for hams contributing to platform validaton of LUSEX satellite (LU Satellite EXperiment) on development by Amsat Argentina. More on http://lusex.org.ar

In order to monitor the payload (if you are within 400 miles of launch area) you need just an FM receiver either handy or base, in 145.950 for repeater and/or 144.930 for APRS. The repeater, that is activated via 123 Hertz subtone, operates receiving voice FM in 435.950 kHz (-112dbm, 0,56 uV) and emits with 2W the received audio live on 145.950 kHz.

Simultaneously APRS data will be sent in Packet at 1200 bauds in 144.930, and also in 145.950.

The DTI APRS symbol would change from a Balloon (/O) during the ascent to a glider (/g) during parachute descent.

Payload would operate as voice repeater activated by 123 Hz subtone during 1 minute, a warning bip at 40 seconds will indicate telemetry is coming, which is emitted if the repeater is not in use, if in 20 seconds more voice repeater still in use a two bips will be heard signaling that short APRS packages will begin in the different frequencies, also every 5 minutes CW (telegraphy with tones of audio) with CQ + callsign (LU7AA), sequence#, ext. and int. centigrade temperatures and voltage of batteries, after which the cycle will repeat.

Experiment will also emit SSTV pictures in ROBOT-36 (36 seconds) in real time, showing what glider/Balloon sees. Every 5 minutes during ascent/descent and more spaced at high altitudes. (It can be received among others with MIXW, MMSTV & RX-SSTV ).

To study propagation and allow DX station to listen, balloon will also carry a 150 mW CW 7021 Khz transmitter, emiting callsign, sequence, external and internal temperatures and battery voltage.

Payload would also carry on board two TV cameras (one towards earth and another towards horizon) recording video and sound during the flight. These captured videos could be recovered when payload is recovered.

APRS trajectory could be seen every minute, including speed, height, external and internal temperatures and 7.2v battery voltage using UI-View (download from the UI-View official site on http://www.ui-view.org/) and/or to see/follow from Internet connecting to http://aprs.fi/?call=lu7aa-11 or locally via Packet at specified frequencies.

There are georeferenced Maps for UI-View in
http://www.amsat.org.ar/pico.jpg, http://www.amsat.org.ar/pico.txt.
Download and place them in directory Program Files/Peak Systems/UI-View32/MAPS and rename .txt file to .inf.

The experiment in 435.950 KHz besides voice, receives and accepts DTMF sequences commands on demand, I.E. sending B* (DTMF with handy keyboard on UHF) will return S5 … ….. in 145,950 VHF CW, reporting in CW signal strength received from your station, if S9+10 will returns P10.

There are also DTMF commands qualifying emission of CW tlm or APRS beacon or SSTV emission, commands that allows remote release of payload, mode changes, timers control, energy, power, etc.

Frequencies for previous coordination, announcements and flights will be 7090 Khz LSB +/-10 Khz and local repeaters.

During the flights will remain active wide coverage AMSAT-LU APRS Igate LU7AA-10 on 144.930 and 430.930 KHz, operating from the Constituyentes Investigation Center transferring whatever is received towards Internet.

For being an experiment oriented to a next satellite, the contacts made between stations via this payload will be considered valid for the recently announced permanent, gratuitous and applicable Satellite Certificate that AMSAT-LU and RClub QRM Belgrano grants, more info on http://www.amsat.org.ar/certsat.html.

During the Balloon flight, amateur groups will chase the payload, aiming to locate and recover. Trapping ventures holds on this activity, as in the case of the Pampero 15 Balloon sent from San Miguel del Monte which landed in the middle of the Magdalena’s state prison … See http://www.lu5egy.com/Proyecto_pampero/vuelo_15/n_1esk.htm

All reports welcome. If you wish or can organize or want be part of control, or like to pursuit and recovery, or like operating and capturing data as an independent station, and/or wishes to join us personally in this adventure from the launching places email us to parapente at amsat.org.ar.

We appreciate reading of this information and thankful if distribution possible.

73, LU7AA, Amsat-LU, aiming at the future by making the present funny.
Web: http://www.amsat.org.ar/
Email: info at amsat.org.ar

16 Japanese Educational Satellites to be Launched

Kibo Robot Arm CubeSat Deployment

Kibo Robot Arm CubeSat Deployment

Sixteen educational satellites are under construction in Japan. The first should be launched in May 2012 followed by the others over the next two years.

Horyu-2 Structural Thermal Model

HORYU-2 Structural Thermal Model

The first to launch is the amateur radio satellite HORYU-2 built by students at the Kyushu Institute of Technology (KIT). The launch is on a Japanese H-IIA rocket planned for May 17 at 1639-1642 UT.

The mission aims to take pictures of the Earth using a small CMOS camera SCAMP (Surrey Camera Payload) developed by the University of Surrey, a sister university of KIT. SCAMP takes a 640×480 pixel picture in a JPEG format. From 700 km altitude, one pixel corresponds to 1.6 km.

HORYU-2 will be followed in July by the launch of the HTV3 to the International Space Station (ISS). This will deliver the JEM-Small Satellite Orbital Deployer (J-SSOD) along with the Japanese CubeSats WE-WISH, FITSAT-1 and RAIKO. These CubeSats should be deployed from the ISS in September using the Japanese Experiment Module (JEM) robot arm.

Takushi Tanaka JA6AVG and FITSAT

Takushi Tanaka JA6AVG and FITSAT

FITSAT-1, also known as NIWAKA, will use a neodymium magnet for attitude control. It has multiple downlinks, CW on 437.250 MHz, AX.25 on 437.445 MHz and a 4 watt high speed data transmitter on 5840 MHz capable of sending a 640 by 480 VGA JPEG image in 6 seconds.

In addition it carries high power LEDs that will be driven with 100W pulses to produce extremely bright flashes. These, it is hoped, will be observable by the unaided eye or with small binoculars. Both the 5840 MHz and optical downlinks have a high power consumption so it may be that they are only activated over Japan.

In December TSUBAME is planned to be launched on a H-IIA. It aims to have a CW beacon on 437.250 MHz and AX.25 1200/9600bps telemetry on 437.505 MHz.

The satellite blog run by Mineo Wakita JE9PEL is a good source of information on Japanese satellites, see http://tinyurl.com/JE9PEL-Satellite-Blog

The satellite blog of Nader Omer ST2NH contains a summary of Mineo’s information which is reproduced here:

Horyu-2
http://kitsat.ele.kyutech.ac.jp/what_horyu2_2.html
437.375MHz 1200bps FSK CW
——————————————————————————-

RAIKO
http://www.astro.mech.tohoku.ac.jp/RAIKO/
2U (10 cm by 10 cm by 20 cm)
——————————————————————————-

FITSAT-1
http://www.fit.ac.jp/~tanaka/fitsat.shtml
437.250MHz CW, 437.445MHz FM, 5840.00MHz High speed data
——————————————————————————

WE WISH
http://www.meisei.co.jp/news/2011/0617_622.html
IR pictures of the earth surface with 320×256 pixels
that will be downlinked in approx 110 secs using SSTV.
437.505MHz SSTV, Telemetry, CW

http://www.meisei.co.jp/english/news/2011/0617_636.html (English Version)

—————————————————————————–

STARS-II
http://stars1.eng.kagawa-u.ac.jp/
437.245MHz CW (mother), 437.255MHz CW (daughter)
437.405MHz FM (mother), 437.425MHz FM (daughter)
—————————————————————————-

TeikyoSat
http://sites.google.com/site/spacesystemteikyo/Home/teikyo-sat
—————————————————————————-

Komolebi
http://www.nano-sat.org/shinshu/files/2010shinshu/09_okamoto.pdf
—————————————————————————-

KSAT2
http://leo.sci.kagoshima-u.ac.jp/~n-lab/KSAT-HP/Ksat2.html
—————————————————————————-

INVADER
http://artsat.jp/
—————————————————————————-

OPUSAT
http://www.sssrc.aero.osakafu-u.ac.jp/OPUSAT_home.html
—————————————————————————-

ITF-1
http://yui.kz.tsukuba.ac.jp/
Mission 1 Establish human network by amateur satellite
Mission 2 Prove the ability of the micro engineered 1/20 wavelength small antenna
Mission 3 Prove the stable operation of FRAM based microcontroller and
other microcontroller in space environment
437.425 MHz
—————————————————————————-

RISING-2
http://www.astro.mech.tohoku.ac.jp/RISING-2/
—————————————————————————-

SPROUT
http://sat.aero.cst.nihon-u.ac.jp/sprout/
—————————————————————————-

UNIFORM-1
http://www.wakayama-u.ac.jp/ifes/news/20120328.html
—————————————————————————-
SOCRATES
http://www.aes.co.jp/company/
—————————————————————————-

TSUBAME
http://lss.mes.titech.ac.jp/ssp/tsubame/
437.505MHz AX.25/SRLL, 9600bps GMSK, 1200bps AFSK
437.250MHz CW
—————————————————————————-

AMSAT-LU SSTV and Crossband Repeater on Glider and Balloon

AMSAT-LU SSTV and GPS Payload

View of communications experiment: Below is the plate of the repeater. Top left is the SSTV camera and top right is the GPS receiver module. Image credit LU7AA

An SSTV and crossband repeater payload developed by AMSAT-LU will be flown on a Glider and a High Altitude Balloon on March 3 and 17.

AMSAT-LU LU7AA report:

We are pleased to inform next Saturday March-3 2012 (if weather permits) from 12hs (GMT-3), Amsat-LU and friends will be flying from Zarate (Route 193, km 19 from Buenos Aires) an UV repeater including APRS + SSTV + CW + DTMF thru several flights aboard manned glider, as test for LUSEX (LU Satellite Experiment), being developed by AMSAT-LU.

Afterwards on Saturday March-17 from 12hs-LU on (GMT-3), a free Balloon will fly same payload from the city of Junin (Club of Gliders, Lagoon of Gomez), 250Km west of Buenos Aires City.

Payload will operate as an UHF to VHF crossband repeater, with CW tlm, APRS location and SSTV emissions in local and space frequencies.

According to estimates Balloon could reach 100,000 feet (30 km) in height, travelling from 50 to 100 miles towards east.

Thus allowing contacts between stations located in provinces of Buenos Aires, Santa Fe, Entre Rios, Cordoba, La Pampa, San Luis and Uruguay.  See coverage map on http://www.amsat.org.ar/junincubr.jpg and possible trajectory in http://www.amsat.org.ar/junin120215.jpg .

For these experiences, Amsat-LU works with and it is thankful to hams of Radio Clubs of Junin, QRM Belgrano, APRS Group, Don Bosco Ramos Mejia School, gliders Clubs of Zarate, Junin and Cañuelas, and the twelve Amsat-LU members development team as well as those who have actively participated and sent their reports in previous experiences.

More information at http://www.amsat.org.ar/lu4aao/experimento_globo_y_parapente.htm

AMSAT-LU Glider

Glider

Several flown experiments have been successfully operated during 2011 in manned-gliders, airplanes, captive and free Balloons allowing operational & practice for hams contributing to platform validaton of LUSEX satellite (LU Satellite EXperiment) on development by Amsat Argentina. More on http://lusex.org.ar

In order to monitor the payload (if you are within 400 miles of launch area) you need just an FM receiver either handy or base, in 145.950 for repeater and/or 144.930 for APRS. The repeater, that is activated via 123 Hertz subtone, operates receiving voice FM in 435.950 Khz (-112dbm, 0,56 uV) and emits with 2W the received audio live on 145.950 Khz.

Simultaneously APRS data will be sent in Packet at 1200 bauds in 144.930, and also in 145.950.

The DTI APRS symbol would change from a Balloon (/O) during the ascent to a glider (/g) during parachute descent.

Payload would operate as voice repeater activated by 123 Hz subtone during 1 minute, a warning bip at 40 seconds will indicate telemetry is coming, which is emitted if the repeater is not in use, if in 20 seconds more voice repeater still in use a two bips will be heard signaling that short APRS packages will begin in the different frequencies, also every 5 minutes CW (telegraphy with tones of audio) with CQ + callsign (LU7AA), sequence#, ext. and int. centigrade temperatures and voltage of batteries, after which the cycle will repeat.

AMSAT-LU RF Module

The system board containing RF transmitter module, receiver module, level adjustments, duplexer and antenna connector. Image credit LU7AA

Experiment for the first time in these flights will emit SSTV pictures in ROBOT-36 (36 seconds) in real time, showing what glider/Balloon sees. Every 5 minutes during ascent/descent and more spaced at high altitudes. (It can be received among others with MIXW, MMSTV & RX-SSTV ).

Payload would also carry on board two TV cameras (one towards earth and another towards horizon) recording video and sound during the flight. These captured videos could be recovered when payload is recovered.

APRS trajectory could be seen every minute, including speed, height, external and internal temperatures and 7.2v battery voltage using UI-View ( download from the UI-View official site on http://www.ui-view.org/ ) and/or to see/follow from Internet connecting to http://aprs.fi/?call=lu7aa-11 or locally via Packet at specified frequencies.

There are georeferenced Maps for UI-View in http://www.amsat.org.ar/junin.jpg, http://www.amsat.org.ar/junin.txt, http://www.amsat.org.ar/zarate.jpg, http://www.amsat.org.ar/zarate.txt, http://www.amsat.org.ar/lachoza.jpg and http://www.amsat.org.ar/lachoza.txt . Download and place them in directory Program Files/Peak Systems/UI-View32/MAPS and rename files .txt to .inf.

The experiment in 435.950 KHz besides voice, receives and accepts DTMF sequences commands on demand, I.E. sending B* (DTMF with handy keyboard on UHF) will return S5 … ….. in 145,950 VHF CW, reporting in CW signal strength received from your station, if S9+10 will returns P10.

There are also DTMF commands qualifying emission of CW tlm or APRS beacon or SSTV emission, commands that allows remote release of payload, mode changes, timers control, energy, power, etc.

Frequencies for previous coordination, announcements and flights will be 7090 Khz LSB +/-10 Khz and local repeaters.

During the flights will remain active wide coverage AMSAT-LU APRS Igate LU7AA-10 on 144.930 and 430.930 KHz, operating from the Constituyentes Investigation Center transferring whatever is received towards Internet.

For being an experiment oriented to a next satellite, the contacts made between stations via this payload will be considered valid for the recently announced permanent, gratuitous and applicable Satellite Certificate that AMSAT-LU and RClub QRM Belgrano grants, more info on http://www.amsat.org.ar/certsat.html

During the Balloon flight, amateur groups will chase the payload, aiming to locate and recover. Trapping ventures holds on this activity, as in the case of the Pampero 15 Balloon sent from San Miguel del Monte which landed in the middle of the Magdalena’s state prison … See http://www.lu5egy.com/Proyecto_pampero/vuelo_15/n_1esk.htm

All reports welcome. If you wish or can organize or want be part of control, or like to pursuit and recovery, or like operating and capturing data as an independent station, and/or wishes to join us personally in this adventure from the launching places email us to parapente at amsat.org.ar.

We appreciate reading of this information and thankful if distribution possible.

73, LU7AA, Amsat-LU, aiming at the future by making the present funny.
http://www.amsat.org.ar/
info at amsat.org.ar

FrequencyCast ARISSat-1 Video

The UK Tech Podcast, FrequencyCast, has released a short video showing reception in Essex of FM voice and an SSTV image from the amateur radio satellite ARISSat-1.

The 145.950 MHz FM signal was recorded at 1055 UT on November 14, 2011 and was uploaded to support the feature at http://www.essexham.co.uk/arissat

Watch ARISSat-1 Amateur Radio Satellite Pass 14 Nov 2011

Catch the Last ARISSat-1 Telemetry Competition
http://www.uk.amsat.org/2011/11/09/catch-the-last-arissat-1-telemetry/

ARISSat-1 Re-entry Date January ? http://www.uk.amsat.org/2011/12/01/arissat-1-re-entry-date/

Essex Ham http://www.essexham.co.uk/

FrequencyCast – The UK’s TV and Tech Podcast http://www.frequencycast.co.uk/

RSGB-Shuttle SSTV Contact on TV News

A vintage TV news report first broadcast Aug 4, 1985 shows a contact between RSGB HQ in Potters Bar and Astronaut Tony England W0ORE in the Challenger shuttle on mission STS 51-F.

Tony W0ORE was running a Motorola model MX-340 handheld 2-meter transceiver and a Robot Research model 1200C slow-scan television scan converter with an antenna fitted on the inside of one of Challengers windows.

RSGB General Manager David Evans G3OUF was among those at the Society’s station GB3RS.

It is believed the voice contact was carried out on 145.550 MHz FM and the RSGB HQ team acheived a first with a two-way exchange of Slow Scan TV (SSTV) pictures.

Watch the ITN TV news report ‘Space Radio Hams’ at
http://www.itnsource.com/shotlist//ITN/1985/08/04/AS040885006/