Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2021-08-24 02:13:04-02:45:26
HOP 362 Plage in AR 12858
The role of chromospheric jets for the heating of plages
x,y:844",128"
Max FOV:161"x162"
Target:Active Region
Nearby Events
6302A Continuum Intensity161"x162"509 spectra
6302A Longitudinal Flux Density161"x162"509 spectra
6302A Transverse Flux Density161"x162"509 spectra
6302A Velocity 6301.5A161"x162"509 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 8 MB
SOTSP: HOP 362 Plage in AR 12858
2021-08-24T02:13:04 to 2021-08-24T02:45:26
Science Goal: The role of chromospheric jets for the heating of plages
Program: Fast map, 164x164", 1-side, Q75, no repeat
Target: Active Region
xcen=844 ycen=128
Instrument: SOTSP
HOP/JOP: 362
Description: Main Objective: Chromospheric jets and photospheric magnetic fields in plage regions Scientific Justification: The main purpose is spectroscopically revealing the role of chromospheric jets for the heating of plages by investigating time variation of chromospheric absorption lines around fine structures in plages. Chromospheric lines (CaII, MgII, H-alpha) are observed with spectroscopes of IRIS and Hida/DST. The chromospheric temperature will be derived from CaII and MgII, and velocity field will be derived from H-alpha. On the other hand, photospheric magnetic fields under jets are observed with HINODE/SOT.

Main Objective: Chromospheric jets and photospheric magnetic fields in plage regions Scientific Justification: The main purpose is spectroscopically revealing the role of chromospheric jets for the heating of plages by investigating time variation of chromospheric absorption lines around fine structures in plages. Chromospheric lines (CaII, MgII, H-alpha) are observed with spectroscopes of IRIS and Hida/DST. The chromospheric temperature will be derived from CaII and MgII, and velocity field will be derived from H-alpha. On the other hand, photospheric magnetic fields under jets are observed with HINODE/SOT.

Annotations:
Hits: 106
Chief Observer
Tiwari (RCO)
Related Links
Cites: HOP 362 Plage in AR 12858     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 161,162 images: 509 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 161,162 images: 509 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 161,162 images: 509 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 161,162 images: 509 JavaScript Landing Page
Time Series (SP Datacubes)