Observation

Observation Details

Overview

Where

Groups: Mode, FOV, # spectra in map

Data Links

2007-11-14 04:48:16-05:05:56

HOP31 CH boundary

SUMER campaign- Coronal holes boundaries evolution

x,y:	288",-153"
Max FOV:	89"x162"
Target:	Coronal Hole
Nearby Events

6302A Continuum Intensity	89"x162"	280 spectra
6302A Longitudinal Flux Density	89"x162"	280 spectra
6302A Transverse Flux Density	89"x162"	280 spectra
6302A Velocity 6301.5A	89"x162"	280 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 4 MB

SOTSP: HOP31 CH boundary

2007-11-14T04:48:16 to 2007-11-14T05:05:56

Science Goal: SUMER campaign- Coronal holes boundaries evolution

Program: Fast map 100 arcsec

Target: Coronal Hole

xcen=288 ycen=-153

Instrument: SOTSP

HOP/JOP: 31

Description: --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).

Annotations:

Chief Observer

Cruz