http://ovsa.njit.edu//wiki/index.php?action=history&feed=atom&title=2023_January2023 January - Revision history2026-04-17T04:59:38ZRevision history for this page on the wikiMediaWiki 1.38.1http://ovsa.njit.edu//wiki/index.php?title=2023_January&diff=7032&oldid=prevDgary: Created page with "[http://www.ovsa.njit.edu/wiki/index.php/Expanded_Owens_Valley_Solar_Array#Observing_Log Back to Observing Log] == January 10 == EOVSA suffered a major mishap in which all of the feeds were burned due to an undetected BRIGHTSCRAM condition. No observations are available until February 20, after which we were observing only with 8 antennas. Ants 1, 2, 3, 4, 5, and 7 are more or less normal, while Ants 6 and 8 have much reduced sensitivity and hence are not calibrated a..."2023-05-28T15:28:03Z<p>Created page with "[http://www.ovsa.njit.edu/wiki/index.php/Expanded_Owens_Valley_Solar_Array#Observing_Log Back to Observing Log] == January 10 == EOVSA suffered a major mishap in which all of the feeds were burned due to an undetected BRIGHTSCRAM condition. No observations are available until February 20, after which we were observing only with 8 antennas. Ants 1, 2, 3, 4, 5, and 7 are more or less normal, while Ants 6 and 8 have much reduced sensitivity and hence are not calibrated a..."</p>
<p><b>New page</b></p><div>[http://www.ovsa.njit.edu/wiki/index.php/Expanded_Owens_Valley_Solar_Array#Observing_Log Back to Observing Log]<br />
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== January 10 ==<br />
EOVSA suffered a major mishap in which all of the feeds were burned due to an undetected BRIGHTSCRAM condition. No observations are available until February 20, after which we were observing only with 8 antennas. Ants 1, 2, 3, 4, 5, and 7 are more or less normal, while Ants 6 and 8 have much reduced sensitivity and hence are not calibrated above about 10 GHz.</div>Dgary