2019-10-08T16:21:38.000Z
http://sot.lmsal.com
Paul Bryans
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
paul.bryans@nasa.gov
IRIS
IRIS
null
Paul Bryans
Paul Bryans
3620254071
3620254071
null
HOP 377: magnetic flux emergence during penumbra formation
HOP 377: magnetic flux emergence during penumbra formation
AR
601
-229
0
67.3
59.6
2019-10-09T16:59:28.000Z 2019-10-09T22:05:49.000Z
601 -229
Medium dense 192-step raster 63.1x60 192s Deep x 2 FUV spectrally rebinned x 2
HOP 377: magnetic flux emergence during penumbra formation
HOP 377: magnetic flux emergence during penumbra formation
29 repeats of OBSID 3620254071 - Medium dense 192-step raster 63.1x60 192s Deep x 2 FUV spectrally rebinned x 2
IRIS roll: 0.0 degrees
IRIS planner pointing: (601.0 arcsec, -229.0 arcsec)
OBS duration: 18381.4 seconds = 29 repeats x 633.8 seconds/repeat
OBS data volume: 2320.6 megabytes = 18565.2 megabits = 18381.4 seconds * 1.0 megabits/second