2024-09-24T22:21:46.000Z 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 Arai Matsumoto Cruz (RCO) --> Okamoto 0 HOP 386 DL-NIRSP Coord AR12891 Active Region SS SS 12891 8 20211105_190005 573 601 581 8 88 400 6 1 1 1 0 21 2012 399 0.9975 675.419 215.718 63.242 101.44 2021-11-05T19:00:05.000Z 2021-11-05T19:34:02.000Z 675.419 215.718 DL-NIRSP (DKIST) First Light Normal map 60"x101", Q65Q75, 1-side request to SOT Only SOT/SP is required for this coordination. SP should be operated in a mode so that there is no pixel summation to achieve the highest spatial resolution, using a raster step that is equal to the slit width, and data from the full slit is saved. Because this coordination will likely occur during Hinode's eclipse season, short, non-continuous rasters are acceptable. Rasters of pores should include the entire pore. Rasters of a sunspot do not need to cover the entire sunspot, but should include regions of umbra, penumbra, and granulation. Rasters of plage or quiet-sun should be focused on magnetic elements and should be at least 10" wide. Short rasters should be repeated during a 3 hour observing window. The best time for observations will likely be 18-21 UT for seeing and weather.;;request to SOT Only SOT/SP is required for this coordination. SP should be operated in a mode so that there is no pixel summation to achieve the highest spatial resolution, using a raster step that is equal to the slit width, and data from the full slit is saved. Because this coordination will likely occur during Hinode's eclipse season, short, non-continuous rasters are acceptable. Rasters of pores should include the entire pore. Rasters of a sunspot do not need to cover the entire sunspot, but should include regions of umbra, penumbra, and granulation. Rasters of plage or quiet-sun should be focused on magnetic elements and should be at least 10" wide. Short rasters should be repeated during a 3 hour observing window. The best time for observations will likely be 18-21 UT for seeing and weather. ivo://sot.lmsal.com/VOEvent#2021-11-05T19:00:00Z