Differences
This shows you the differences between two versions of the page.
projects:jupiter:intercont-2023-12-27 [2024/01/10 15:43] wucknitz |
projects:jupiter:intercont-2023-12-27 [2024/03/05 13:57] (current) wucknitz |
||
---|---|---|---|
Line 1: | Line 1: | ||
====== Observations 2023-12-27 20:30-22:30 UTC ====== | ====== Observations 2023-12-27 20:30-22:30 UTC ====== | ||
- | This time was chosen because of a good chance to see DAM signals from both hemispheres of Jupiter, so that that could be calibration relative to each other. We observed with NenuFAR, the LWA (LWA1, LWA-SV), KAIRA, GLOW, and other international LOFAR stations (FIXME). It is very sad that our Ukrainian friends cannot participate with UTR2 anymore. | + | This time was chosen because of a good chance to see DAM signals from both hemispheres of Jupiter, so that they can be calibrated relative to each other. We observed with NenuFAR, the LWA (LWA1, LWA-SV), KAIRA, and a number of LOFAR stations (all six of GLOW, PL612, IE613, LV614). It is very sad that our Ukrainian friends cannot participate with UTR2 anymore. |
All LOFAR(-like) stations observed in RCU mode 3 (band 10_90) with 8-bit recording of 244 subbands (40-283, 8-55 MHz). Beamforming was done in direction ''0.5826639,0.2118205,J2000'' or ''0,0,JUPITER''. | All LOFAR(-like) stations observed in RCU mode 3 (band 10_90) with 8-bit recording of 244 subbands (40-283, 8-55 MHz). Beamforming was done in direction ''0.5826639,0.2118205,J2000'' or ''0,0,JUPITER''. | ||
Line 55: | Line 55: | ||
**People involved: Olaf Wucknitz, Francesco Angelo Iraci, Sai Chaitanya Susarla, Krishnakumar Moochickal Ambalappat** | **People involved: Olaf Wucknitz, Francesco Angelo Iraci, Sai Chaitanya Susarla, Krishnakumar Moochickal Ambalappat** | ||
+ | |||
+ | |||
+ | ==== PL610 ==== | ||
+ | |||
+ | **People involved: Mariusz Pożoga** | ||