2024-09-24T22:21:28.000Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin Advanced Tech Center, 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA 94304 null null HINODE SOTSP Sakao Sterling Shine 0 Bart's Waves disk center, Quiet Sun Bart's Waves DC, QS, WAV 2 20070220_102501 50 76 75 2 68 14 2 2 1 1 0 21 2048 1301 92.92857142857143 121.824 6.911 2.241 40.576 2007-02-20T10:25:01.000Z 2007-02-20T11:09:34.000Z 121.824 6.911 Bart's Waves Dynamic Mode, 16 slits, 30 sec cadence, no repeat a) Ca + 15 seconds of NGI magnetogram with large FOV at 60 sec cadence for 3 hours or b) "Bart's Waves" with 3 hours of Ca + blue continuum at 20 seconds cadence with magnetogram context every half-hour Typical day will see a few different pointings (2 or 3) and for each pointing EIS will probably run both the above programmes, so 6 hours per pointing is best. N.B. EIS requests to perform these observations OUTSIDE the timerange 0800 - 1100 UT. SOT observes the H-alpha filament just west of central meridian (256.5, -31.5), following rotation from 2007/02/19 10:40 to 18:04 Then quiet disk center (following rotation) starting at (-26,0) from 2/19 18:14 to 2/20 11:10.;;a) Ca + 15 seconds of NGI magnetogram with large FOV at 60 sec cadence for 3 hours or b) "Bart's Waves" with 3 hours of Ca + blue continuum at 20 seconds cadence with magnetogram context every half-hour Typical day will see a few different pointings (2 or 3) and for each pointing EIS will probably run both the above programmes, so 6 hours per pointing is best. N.B. EIS requests to perform these observations OUTSIDE the timerange 0800 - 1100 UT. SOT observes the H-alpha filament just west of central meridian (256.5, -31.5), following rotation from 2007/02/19 10:40 to 18:04 Then quiet disk center (following rotation) starting at (-26,0) from 2/19 18:14 to 2/20 11:10. ivo://sot.lmsal.com/VOEvent#2007-02-20T09:40:00Z