Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2017-08-10 10:56:06-11:43:30
CH observations w/IRIS
Coronal hole observations with IRIS
x,y:-17",-394"
Max FOV:225"x162"
Target:Coronal Hole
Nearby Events
6302A Continuum Intensity225"x162"727 spectra
6302A Longitudinal Flux Density225"x162"727 spectra
6302A Transverse Flux Density225"x162"727 spectra
6302A Velocity 6301.5A225"x162"727 spectra
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SP Cubes 12 MB
SOTSP: CH observations w/IRIS
2017-08-10T10:56:06 to 2017-08-10T11:43:30
Science Goal: Coronal hole observations with IRIS
Program: Fast map, 230"x164", Q65, 1-side CCD
Target: Coronal Hole
xcen=-17 ycen=-394
Instrument: SOTSP
HOP/JOP: 0
Description: Objectives: 1: To observe the evolution of the magnetic field distribution around the poles during the solar cycle. 2: To understand the relationship between photospheric magnetic field and the coronal structures (include the solar wind) around the poles.

Annotations:
Hits: 115
Chief Observer
DeRosa (RCO) -> Nitta (RCO)
Related Links
Cites: CH observations w/IRIS     
Timeline: gif use
See also
Datasets
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wavelength: 6302A Continuum Intensity cadence: 0 min fov: 225,162 images: 727 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 225,162 images: 727 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 225,162 images: 727 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 225,162 images: 727 JavaScript Landing Page
Time Series (SP Datacubes)
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