Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2008-01-17 12:00:46-13:01:54
HOP 62 quiet sun
CORE: Thermal distributions and evolutions of coronal structures
x,y:-117",6"
Max FOV:111"x122"
Target:Quiet Sun
Nearby Events
6302A Continuum Intensity111"x122"713 spectra
6302A Longitudinal Flux Density111"x122"713 spectra
6302A Transverse Flux Density111"x122"713 spectra
6302A Velocity 6301.5A111"x122"713 spectra
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Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SOTSP: HOP 62 quiet sun
2008-01-17T12:00:46 to 2008-01-17T13:01:54
Science Goal: CORE: Thermal distributions and evolutions of coronal structures
Program: Normal map 120x120"
Target: Quiet Sun
xcen=-117 ycen=6
Instrument: SOTSP
HOP/JOP: 62
Description: No specific request to SOT. Quiet Sun dynamics study run. Scientific Objectives: XRT has the capability for thermal studies using multi-filter observation sequences. Some multi-filter observations have been performed to-date, but the XRT Team would like to perform some coordinated observations with EIS and SOT. The primary science objective is study the thermal distribution and evolution of loop structures in active regions as well as XBPs, and cooler coronal structures, as seen by XRT and EIS rasters. (For example, some initial results by Reeves et al. directly show the spatial and thermal distribution of cooling plasma throughout coherent post-flare loop structures.)

No specific request to SOT. Quiet Sun dynamics study run. Scientific Objectives: XRT has the capability for thermal studies using multi-filter observation sequences. Some multi-filter observations have been performed to-date, but the XRT Team would like to perform some coordinated observations with EIS and SOT. The primary science objective is study the thermal distribution and evolution of loop structures in active regions as well as XBPs, and cooler coronal structures, as seen by XRT and EIS rasters. (For example, some initial results by Reeves et al. directly show the spatial and thermal distribution of cooling plasma throughout coherent post-flare loop structures.)

Annotations:
Hits: 41
Chief Observer
Magara
Related Links
Cites: HOP 62 quiet sun     
Timeline: gif use
See also
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wavelength: 6302A Continuum Intensity cadence: -1 min fov: 111,122 images: 713 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: -1 min fov: 111,122 images: 713 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: -1 min fov: 111,122 images: 713 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: -1 min fov: 111,122 images: 713 JavaScript Landing Page
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