Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2019-09-24 10:34:31-11:06:51
HOP 373 Filament
Formation and destabilisation of filaments
x,y:331",-419"
Max FOV:161"x162"
Target:Filament
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 373 Filament
2019-09-24T10:34:31 to 2019-09-24T11:06:51
Science Goal: Formation and destabilisation of filaments
Program: Fast map, 164x164", 1-side, Q65, no repeat
Target: Filament
xcen=331 ycen=-419
Instrument: SOTSP
HOP/JOP: 373
Description: Main Objective: SOT/SP would measure the parasitic polarities in the barbs of filaments. Scientific Justification: Filaments are formed with shear flows in channel. It will be interesting to detect the footpoints of filament and mass motions inside the barbs and along the filaments. Spectroscopic observations on the disk in chromosphere lines (Mg II h and k, Halpha) and photosphere lines are required to show the dynamics of the filament by counter-streaming or by turbulence. HMI continua and magnetogram will provide data to follow the large scale evolution of the channel. With HMI surface velocities by using CST (LCT) methods will be determined leading to an estimate of the shear at large scale of the filament and Hinode/SOT will locate the parasitic polarities where the filament has its footpoints.

Annotations:
Hits: 27
Chief Observer
Tiwari and DeRosa (RCO)
Related Links
Cites: HOP 373 Filament     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals
Time Series (SP Datacubes)