Observation

Observation Details

Overview

Where

Groups: Mode, FOV, # spectra in map

Data Links

2007-08-18 10:32:39-10:51:36

EIS+ SOT+XRT Physical mechanisms driving solar microflares and supergranular network dynamics - relevance for coronal heating

x,y:	-5",7"
Max FOV:	95"x162"
Target:	Disk Center
Nearby Events

6302A Continuum Intensity	95"x162"	300 spectra
6302A Longitudinal Flux Density	95"x162"	300 spectra
6302A Transverse Flux Density	95"x162"	300 spectra
6302A Velocity 6301.5A	95"x162"	300 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 5 MB

SOTSP: EIS+ SOT+XRT Physical mechanisms driving solar microflares and supergranular network dynamics - relevance for coronal heating

2007-08-18T10:32:39 to 2007-08-18T10:51:36

Science Goal: EIS+ SOT+XRT Physical mechanisms driving solar microflares and supergranular network dynamics - relevance for coronal heating

Program: Fast map 100 arcsec repeat

Target: Disk Center

xcen=-5 ycen=7

Instrument: SOTSP

HOP/JOP: 20

Description: Daily Note and User Entry: Co-alignment offset pointing (TBD) HOP29, filament, prominence, cavities (18 -22 UT). HOP12 (22 - 3 UT, can be extended to 6 UT if no conflict). HOP20, microflares (7:00 - 13:30 UT) XRT: CCD Bakeout plus test X-ray images
Request to SOT: SOT: We plan (if possible) to run in time a sequence of 3exposures:2using the BFI imager and 1 using the NBIimager.The reason is to cover evolution of the photosphere with its magnetic concentration signatures (G-band), evolution of the longitudinal component of the magnetic field vector inthe photosphere, and evolution of chromosphere (CaIIH)witha reasonable temporal resolution (???`10s per image,???@???`30s???@per???@sequence???@of 3 selected channels).???@ ???@and
#8226
BFI: G-band and CaIIH channels, ???@
FOV:109???hx109???h(1k x1kmode, binning 2 x 2 pxs),

3bit JPEG compression, cadence:???`10s per filtergram,

telemetry needed: 300kbps, nocompensation of the solar rotation
and
#8226
NFI: FeI630.25nm longitudinal magnetograms,other parameters as in

case of BFI
and
#8226
SP:none
Scientific Objectives: This proposal merges together attempts to observe two kinds of solarstructures and
#8211
solar micro flares and super granular network and
#8211
which are planned tobe investigated toaddress common openquestions on the irrelevance for the heating and dynamics of the solar corona.
Other Instruments: DOT SoHO/CDS/MDI/EIT JOP 189: 3-17 Aug 2007 7:00 - 13:30 UT TRACE RHESSI

Annotations:

Chief Observer

Zoe

Timeline: gif use