Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2024-01-04 14:50:06-17:43:39
HOP 81 (North)
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.
x,y:-21",868"
Max FOV:322"x162"
Target:N Pole
Nearby Events
6302A Continuum Intensity322"x162"1022 spectra
6302A Longitudinal Flux Density322"x162"1022 spectra
6302A Transverse Flux Density322"x162"1022 spectra
6302A Velocity 6301.5A322"x162"1022 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 17 MB
SOTSP: HOP 81 (North)
2024-01-04T14:50:06 to 2024-01-04T17:43:39
Science Goal: 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.
Program: Fast deep mode, 2048 slit position, LIMB ONLY
Target: N Pole
xcen=-21 ycen=868
Instrument: SOTSP
HOP/JOP: 81
Description: CORE (HOP0002) Polar Monitoring Campaign during the Solar Cycle

Annotations:
Hits: 4
Chief Observer
Nitta (RCO) -> Yamasaki
Related Links
Cites: HOP 81 (North)     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 322,162 images: 1022 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 322,162 images: 1022 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 322,162 images: 1022 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 322,162 images: 1022 JavaScript Landing Page
Time Series (SP Datacubes)