PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT INTERCHANGE_FORMAT = ASCII PUBLICATION_DATE = 1997-07-09 NOTE = "Internal memo describing system temperature determinations using data acquired during the Clementine bistatic radar experiment at DSS 43. Since DSS 43 data are not included in this archive, the results are not directly applicable." END_OBJECT = TEXT END Amplitude Calibration from 41000626 data ======================================== Ambient load temperature was reported as Tamb = 20.5C = 293.5K (1) Channel 1 (RCP) --------------- After correction for Channel 1 (RCP) attenuator changes, compare power levels with ambient load connected (23658-23768 secs and 23789-23940 secs) to power levels with antenna pointed to sky (23183-23573 secs). Ambient load raises noise power by 11.9 dB -- a factor of 15.488 -- the "Y-factor". If noise power generated in front end of receiver (e.g., maser and DSN antenna itself) is Trcvr and cosmic noise is Tsky, then for RCP Trcvr + Tamb ------------ = 15.488 (2) Trcvr + Tsky The quantity we are interested in is Trcvr + Tsky, since this is the source of noise power coming from the receiver in the absence of spacecraft signal, microwave thermal emission from the lunar surface, or radio echo. We can rearrange terms in (2) to give Trcvr + Tsky = (Tamb - Tsky)/14.488 (3) At microwave frequencies, the sky typically has a temperature on the order of 3K, so Tsky << Tamb. In fact, we can make a small table to see the effects: Tsky Trcvr + Tsky ---- ------------ 0K 20.26K 1K 20.19K 3K 20.05K 5K 19.91K Since the Tamb report may easily be in error by 1C and the Y-factor may easily be in error by 0.1 dB (2%), we take our estimate of system temperature on Channel 1 to be Trcvr + Tsky = 20.0 +/- 0.5K (4) Channel 3 (LCP) --------------- After correction for Channel 3 (LCP) attenuator changes, compare power levels with ambient load connected (23770-23787 secs and 23942-24142 secs) to power levels with antenna pointed to sky (23183-23436 secs). Ambient load raises noise power by 11.6 dB -- a factor of 14.454 -- the "Y-factor". Following the same steps as for Channel 1, we arrive at Trcvr + Tsky = (Tamb - Tsky)/13.454 (3) A similar table shows: Tsky Trcvr + Tsky ---- ------------ 0K 21.82K 1K 21.74K 3K 21.59K 5K 21.44K We take our estimate of system temperature on Channel 3 to be Trcvr + Tsky = 21.6 +/- 0.5K (4) Relative Amplitudes ------------------- Execution of PREPPOWER on the first 100 sec of samples for each polarization yields relative power measurements of 610 for RCP and 662 for LCP. Over this time interval, the attenuators on both channels were set to 33. The ratio of these powers is indistinguishable from the ratio of the two system temperatures. We can adopt attenuator settings of 33 dB as our reference level (GAIN = 1.0) on each channel.