Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2008-01-05 11:07:05-12:10:18
HOP62 thermal structure of corona
CORE: Thermal distributions and evolutions of coronal structures
x,y:-438",-63"
Max FOV:317"x162"
Target:Active Region
Nearby Events
6302A Continuum Intensity317"x162"1000 spectra
6302A Longitudinal Flux Density317"x162"1000 spectra
6302A Transverse Flux Density317"x162"1000 spectra
6302A Velocity 6301.5A317"x162"1000 spectra
Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 17 MB
SOTSP: HOP62 thermal structure of corona
2008-01-05T11:07:05 to 2008-01-05T12:10:18
Science Goal: CORE: Thermal distributions and evolutions of coronal structures
Program: Fast Map, Full FOV
Target: Active Region
xcen=-438 ycen=-63
Instrument: SOTSP
HOP/JOP: 62
Description: No specific request for SOT. 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 for SOT. 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: 56
Chief Observer
Katsukawa
Related Links
Cites: HOP62 thermal structure of corona     
Timeline: gif use
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Datasets
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wavelength: 6302A Continuum Intensity cadence: 0 min fov: 317,162 images: 1000 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 317,162 images: 1000 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 317,162 images: 1000 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 317,162 images: 1000 JavaScript Landing Page
Time Series (SP Datacubes)
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