Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2007-11-05 10:34:30-11:49:30
HOP44
SUMER campaign - Multi-wavelength observations of coronal hole plumes at solar minimum
x,y:-26",952"
Max FOV:55"x162"
Target:Coronal Hole, North pole
Nearby Events
6302A Continuum Intensity55"x162"344 spectra
6302A Longitudinal Flux Density55"x162"344 spectra
6302A Transverse Flux Density55"x162"344 spectra
6302A Velocity 6301.5A55"x162"344 spectra

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Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 11 MB
SOTSP: HOP44
2007-11-05T10:34:30 to 2007-11-05T11:49:30
Science Goal: SUMER campaign - Multi-wavelength observations of coronal hole plumes at solar minimum
Program: Very Deep Mode 100x164" no repeat
Target: Coronal Hole, North pole
xcen=-26 ycen=952
Instrument: SOTSP
HOP/JOP: 44
Description: The photospheric magnetic fields as they evolve during the formation of plumes are essential to understand the role of magnetic reconnection in heting these structures.

The photospheric magnetic fields as they evolve during the formation of plumes are essential to understand the role of magnetic reconnection in heting these structures.

Annotations:
Hits: 43
Chief Observer
Observer:
Related Links
Cites: HOP44     
Timeline: gif use
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Datasets
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saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: -1 min fov: 55,162 images: 344 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: -1 min fov: 55,162 images: 344 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: -1 min fov: 55,162 images: 344 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: -1 min fov: 55,162 images: 344 JavaScript Landing Page
Time Series (SP Datacubes)