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SUNSAT Telemetry
- Subject: [amsat-bb] SUNSAT Telemetry
- From: Bob Bruninga <bruninga@xxxxxxxxxxxxx>
- Date: Tue, 10 Oct 2000 17:01:09 -0400 (EDT)
Here is how to interpret SUNSAT APRS Status and Telemetry packets:
>OBC1v8: up=20/01:49:17, rst=wdog, Tue Oct 10 11:18:06 UTC 2000
FIELD1: On Board Computer software version
FIELD2: Up time in Days, Hours, Minutes and Seconds
FIELD3: Reason for the last RESET ( POWER-ON, TELECOMMAND, or WATCHDOG)
FIELD4: Onboard Clock Time
The SUNSAT APRS telemetry is sampled once every 4 minutes. Thus, in 24
samples, you get a full 98 minutes of data which constitues one orbit.
To give whole orbit data, the 24 sample telemetry buffer is transmitted
one packet every 9.6 seconds so that a complete set can be received in
just 4 minutes. THus the 000 packet is the current value and each
subsequent one is the previous 4 minute one:
SUNSAT-3>APRS:T#000,098,133,140,041,046,11100000
SUNSAT-3>APRS:T#001,099,138,110,041,038,11111111
SUNSAT-3>APRS:T#002,099,140,191,042,040,11111100... etc
Telemetry data is identified by a T# header , then a serial number, then
5 analog telemetry channels, and then 8 Binary Bits.
SERIAL#: Whole Orbit buffer pointer (0 in the first example above),
CHANNEL1: Battery state of charge percent (98 %)
CHANNEL2: Battery voltage in 10ths of a volt (13.3 V)
CHANNEL3: Battery charge current -128 in 10's of Milliamps
(140 - 128)*10 = 120 ma
CHANNEL4: Battery temperature in degrees C (41 øC),
CHANNEL5: Top plate sun sensor reading (46, an uncalibrated value).
BINARY BITS: The last field indicates the state of the 8 solar panels
(0: sourcing the power bus, 1: shunted, dumping energy).
The above telemetry was when SUNSAT was over Arkansas and it was just sunrise in
Maryland. Thus SUNSAT was in daylight even though Arkansas was in dark.
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