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CHARACTERISTICS of OSCAR-11 (U-O-11) (UoSAT-2)
This gravity gradient stabilized satellite was designed and built by the
University of Surrey AMSAT Group and launched from the USA into a circular
700 Km high Quasi-Polar 98 minute period orbit.
OSCAR-11 has no transponders, but transmits valuable scientific
telemetry including 'WOD' (Whole Orbit Data) of many of it's channels.
These include numerous temperatures, magnetometer readings, radiation and
micro-meteorite impact data. It also transmits regular bulletins of general
amateur radio and space interest. It has played a useful function in
providing tracking data and Doppler positioning to numerous scientific
expeditions inluding the joint Canadian Russian trans-polar ski-trek. A
voice encoder also provides spoken telemetry and uplinked messages.
The transmissions are easily received using a simple crossed dipole
(turnstile) or a small preferably circularly polarized Yagi to any
conventional 2m FM receiver without modification. A CCD Camera provides
earth pictures
Demodulators and computer Programs are available from AMSAT-UK for
directly translating the telemetry, WOD, pictures, bulletins etc. directly
from the audio socket of the receiver or via taped recordings to a
computer.
FREQUENCIES for UoSAT-OSCAR-11
Beacon 145.826 MHz (AFSK/FM)
Beacon 435.025 MHz (AFSK/FM)
Beacon 2401.500 MHz (AFSK/FM)
QTH for AMSAT-UK: Ron Broadbent, G3AAJ,
Secretary AMSAT-UK,
94 Herongate Road,
Wanstead Park,
London
E12 5EQ
United Kingdom.
Reports of OSCAR-11 and it's educational use deployment are welcomed by:
UoSAT Spacecraft Laboratory,
School of Electronic and Electrical Engineering,
University of Surrey,
Guildford,
Surrey,
GU12 5XH
United Kingdom.
Pat Gowen, G3IOR @ GB7VLS
21578.SAT
Characteristics of SARA NASA Cat.No. 21578
SARA is an acronym of 'Satellite Amateur de Radio-Astronomie' (Amateur
Radio Astronomy Satellite), a very small 19 Kg satellite constructed by
radio amateur engineers of ESIEESPACE near Paris. SARA was launched by
ARIANE with OSCAR-22 from ESA in Kourou into a solar-synchronous 100 minute
period orbit that passes over earth locations between 1000 and 1400 UTC and
again between 2200 and 0200 UTC local time. SARA's callsign is transmitted
in ASCII in the first line as FX0SAT, as is the full QTH of ESIEESPACE.
SARA's function is the study of eight channels of radio emissions of
the planet Jupiter between 2 and 15 MHz, which are unable to penetrate
earth's ionosphere. It transmits the data as 300 bauds digital temetry on
145.955 MHz FM +/- 5 KHz deviation, which is receivable on any 2m FM
receiver, preferably with a pre-amplifier and good cross polarized azimuth-
elevation trained Yagi, as the signal is not very strong.
A 500 Hz sub-carrier contains the battery voltage information, defined
by V (in Volts) = 0.0148 x F, where F is the tone frequency received. A 220
Hz sub-carrier gives the structure temperature by T (in Deg.C) = 0.714 x (F
- 164.2) where F is the tone frequency received. The 50 Hz bandwidth audio
filter circuit below from Hilburn and Johnson's Manual of Active Filter
Design will function between the receiver audio output and a frequency
meter with R2 set at 2K for 210 HZ and at 350 Ohms for 500 Hz
! ! C1 .03uF
,------! !-------------------------,
! ! ! !
! R3 !
! 330K !
! ,--------/\/\/\/--------o
! C2 ! !
! .03uF ! o +V !
! ! ! ! 2 ,\ ! !
IN o--/\/\/\/-----o---! !----o---!- \ ! 7 !
R1 16K ! ! ! ! \! !
! ! \ !
\ ! 741 >----------o----> OUT
/ R2 ! / 6
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* Origin: The CatWalk BBS Davie, Fl 305-370-3528 USR V.EveryThing
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