RS-39 (Chibis-M) Deploys

RS-39 Chibis-M

RS-39 Chibis-M

RS-39 has CW beacons on 435.315 and 435.215 MHz that can be received directly by schools and colleges for educational outreach purposes. It deployed from Progress M-13M into a 500 km orbit on January 24 at approximately 23:18:30 UT.

On November 2, 2011 cargo ship “Progress M-13M”, which also delivered microsatellite “Chibis-M”, was docked with ISS. The main purpose of “Chibis-M” is the study of physical processes in the vicinity of the lightning, during which the Terrestrial Gamma Ray Flashes (TGFs) are generated. TGFs are likely produced by beams of very energetic electrons, which are accelerated in the intense electric fields generated by large thunderstorm systems.

The deployment of “Chibis-M” in a circular orbit of 500 km will take place during the final phase of “Progress M-13M” operation. According to the plan of the Russian Space Control Centre, undocking of “Progress M-13M” will occur at January 24, 01:59 msk and after two corrections it will be positioned at 500 km orbit. At January 25, 03:14 msk “Chibis-M” will separate. Beside scientific data “Chibis-M” will transmit service telemetry (the housekeeping parameters) in the beacon format on 435.315 or 435.215 MHz CW (Doppler shift +/- 10 kHz) and has the designation of RS-39. The format of data is typical for RS satellites and can be downloaded here.

The telemetry of RS-39 can be easily received directly by schools and colleges for educational outreach purposes. This telemetry will give details of the spacecraft’s health – battery voltages and temperatures of critical units. In combination with orbital data such information will be useful as the curriculum for student lessons.

The team of RS-39 will very much appreciate any reception reports of “Chibis-M”. Special attention is requested for the first orbits as these are outside of control stations for “Chibis-M”. Each report will be confirmed by special QSL card. The email address is amateur-rs39@chibis.cosmos.ru

The RS-39 Chibis-M website managed the by Space Research Institute of the Russian Academy of Sciences (RAS) can be seen in Russian at http://chibis.cosmos.ru/ or in Google English at http://tinyurl.com/RS-39-Chibis-M

As well as measuring electromagnetic parameters of “space weather” in the spectrum 0.1 – 40 kHz the satellite also carries a receiver for the analysis of radio frequency signals in a frequency band of 26-48 MHz. http://www.energia.ru/en/iss/researches/geophis/19.html

RS-39 Morse Code telemetry format http://tinyurl.com/RS-39-Morse-Code-Telemetry

RS-39 Telemetry Decoder http://www.uk.amsat.org/4029

RS-39 Real Time Tracking Map http://chibis.cosmos.ru/cyclogr/prepare1/google/index.html
For Keps click on two gear wheels in top left-hand corner then click on Satellites.

It may be worth checking the AMSAT Bulletin Board (AMSAT-BB) for the very latest news. The 48-hour archive of the AMSAT-BB is at http://www.amsat.org/amsat/archive/amsat-bb/48hour/threads.html or you can join the bulletin board at http://www.amsat.org/amsat-new/tools/maillist/maillist.php

Building a Distributed Satellite Ground Station Network

There was a presentation on building a distributed satellite ground station network at the Chaos Communication Congress held December 27-30 and the video is now available.

The AMSAT-UK FUNcube Dongle VHF/UHF Software Defined Radio gets a brief mention at 39:26 into the video.

The video kicks off with an appearance by Nick Farr then the presentation by Gregor Jehle (Hadez), Armin Bauer and Andreas Hornig gets underway.

Watch 28C3: Building a Distributed Satellite Ground Station Network – A Call To Arms (en)

Hackers Plan Space Satellites http://www.uk.amsat.org/3172 

Hackerspace Global Grid http://shackspace.de/wiki/doku.php?id=project:hgg

London Hackspace Project: Hoxton Space Centre http://wiki.london.hackspace.org.uk/view/Project:Hoxton_Space_Centre

London Hackspace work on HackSat1 http://www.uk.amsat.org/2482

The DIY Magic of Amateur Radio video http://www.uk.amsat.org/3158

ITF-1 CubeSat – Imagine The Future

University of Tsukuba ITF-1 (YUI) CubeSat

University of Tsukuba ITF-1 (YUI) CubeSat

Students at the University of Tsukuba are working on the ITF-1 (YUI) CubeSat project that is planned to be launched on a H-IIA rocket in the fiscal year 2013. The orbit will be 400 by 350km with an inclination of 65 degrees.

The formal name ITF-1 comes from the initial letter of the university slogan “Imagine The Future”.  The satellite also has a popular name YUI which means “bond” in Japanese, it came from the project’s concept‚ “Creating the Worldwide Human Community”.

The 435MHz satellite beacon will send telemetry by a Morse Code audio tone on an FM transmitter running 300 milliwats output. It should be possible to receive it using simple equipment such as a handheld transceiver or scanner. Telemetry information will be first compressed into binary data  and then cut into 5 bits and converted into 10 – 15 Morse codes.

Ayano Okamura ITF-1 Project Manager

Reception reports will be acknowledged with a certificate and the telemetry will be made available on the web.

The UTF-1 Project Manager is Ayano Okamura and you can read her blog at http://tinyurl.com/ITF-1-ProjectManagerBlog

The Chief Tech blog by Asai Eisuke is at http://tinyurl.com/ITF-1-TechBlog

ITF-1 (YUI) on the IARU Amateur Satellite Frequency Coordination pages http://www.amsatuk.me.uk/iaru/formal_detail.php?serialnum=226

ITF-1 website in Google English http://tinyurl.com/CubeSat-ITF-1

QRP APRS Packet Radio to the ISS

International Space Station

International Space Station

Doug Cook KD5PDN’s article about contacting the International Space Station with a few watts and a shoestring budget antenna is now available.

The article “QRP to the ISS” appeared in the February, 2012 issue of QST magazine and, with permission from the ARRL, can be downloaded from Clint Bradford K6LCS’s website.

Doug walks the reader through building a simple tape measure beam, and how to successfully work the ISS with it and a handheld radio.

Read the article at http://www.work-sat.com/Work-Sat/Misc_files/QRP-ISS.pdf

A video by author Doug Cook KD5PDN shows the tape rule antenna and how to set up a Yaesu VX-8R for ISS APRS packet data sending and receiving and other aspects to make a digital contact with the International Space Station. You can also learn how to interpret the audio prompts when packet data is being received.

Watch ISS APRS Contact with a Yaesu VX-8R WB5BSA

There is lots of other information on the Work Satellites website at http://www.work-sat.com/

Student D-STAR Satellite to Launch in 2012

Students at workStudents at the University of Liege are hoping their D-Star GMSK satellite OUFTI-1 will be launched towards the end of this year.

An update on the satellite is published in the January 2012  issue of the OUFTI-1 newsletter at
http://www.leodium.ulg.ac.be/cmsms/uploads/OUFTI-1%20Newsletter%204.pdf

The satellite will have uplinks in the 145 MHz band and downlinks on 435.015 and 435.045 MHz.

OUFTI-1 http://www.leodium.ulg.ac.be/cmsms/

Professor Jacques Verly ON9CWD (Montefiore Institute) and Amandine Denis ON4EYA, Head of Project OUFTI (LTAS) with the flight model (structure) of OUFTI-1 - Image credit ESA

Professor Jacques Verly ON9CWD (Montefiore Institute) and Amandine Denis ON4EYA, Head of Project OUFTI (LTAS) with the flight model (structure) of OUFTI-1 – Image credit ESA

Student Software Defined Radio CubeSat

Students at the University of Vigo have built Xatcobeo a CubeSat that carries a Software Defined Radio (SDR) and a solar panel deployment mechanism.  A launch on an ESA Vega rocket in February is planned.

The IARU Amateur Satellite Coordination Panel pages report that it carries three payloads:

SRAD: a Software Defined Radio. The aim is to test under space conditions a reconfigurable radio. Different modulation schemes will be selected depending on the link conditions.

RDS: an ionizing radiation dosimeter. This dosimeter will take measures of ionizing radiation in a typical LEO orbit for amateur satellites, thus increasing our knwoledge about radiation conditions in this environment.

PDM: a solar panel deployment mechanism to be tested in-flight.

It is planning to use FFSK with AX.25 on UHF. These frequencies have been coordinated – Simplex 437.365MHz and SSR downlink on 145.940MHz.

Further info available at http://www.xatcobeo.com/