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 Arikawa Sterling Cruz 31 HOP31 CH boundary Coronal Hole SUMER campaign- Coronal holes boundaries evolution CH 11 20071114_091905 84 106 106 11 86 600 2 2 1 2 0 22 2032 300 1 331.171 -152.102 95.1 162.304 2007-11-14T09:19:05.000Z 2007-11-14T09:38:01.000Z 331.171 -152.102 SUMER campaign- Coronal holes boundaries evolution Fast map 100 arcsec --SUMER Campaign--- HOP31: Coronal Hole Boundaries Evolution (WED 11/14: 0016 ?? 0613, then 0630 ?? 1111) HOP31 CH boundary 2007/11/14 00:16:00 - 2007/11/14 06:13:35 pointing: (254,-160) FG05 (0x0173) Na IV,Ca,BC 2kx2k 2x2 (3min) SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec 2007/11/14 06:30:00 - 2007/11/14 11:02:00 pointing: (309,-159) FG05 (0x0173) Na IV,Ca,BC 2kx2k 2x2 (3min) SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec Request to SOT HOP Number 0031 SOT - Ca H and G band, SP fast maps, magnetic field, Halpha. POC: TBD With this present study, we want to observe equatorial coronal hole boundaries in order to find spectroscopic signatures of the physical processes which take place using simultaneously SUMER/EIS observations which will permit observations in spectral lines covering a large temperature range (from 40 000 K to a few million degrees).;;--SUMER Campaign--- HOP31: Coronal Hole Boundaries Evolution (WED 11/14: 0016 ??? 0613, then 0630 ??? 1111) HOP31 CH boundary 2007/11/14 00:16:00 - 2007/11/14 06:13:35 pointing: (254,-160) FG05 (0x0173) Na IV,Ca,BC 2kx2k 2x2 (3min) SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec 2007/11/14 06:30:00 - 2007/11/14 11:02:00 pointing: (309,-159) FG05 (0x0173) Na IV,Ca,BC 2kx2k 2x2 (3min) SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec SP11 (0x0054) Fast map 100 arcsec Request to SOT HOP Number 0031 SOT - Ca H and G band, SP fast maps, magnetic field, Halpha. POC: TBD With this present study, we want to observe equatorial coronal hole boundaries in order to find spectroscopic signatures of the physical processes which take place using simultaneously SUMER/EIS observations which will permit observations in spectral lines covering a large temperature range (from 40 000 K to a few million degrees). ivo://sot.lmsal.com/VOEvent#2007-11-14T09:19:00Z