| Overview | Where | Groups: Mode, FOV, # spectra in map | Data Links |
|---|
2019-09-28 09:25:04-10:12:28
 |
HOP 373 filament in North Formation and destabilisation of filaments |
|
|
| 6302A Continuum Intensity | 236"x162" | 749 spectra | | 6302A Longitudinal Flux Density | 236"x162" | 749 spectra | | 6302A Transverse Flux Density | 236"x162" | 749 spectra | | 6302A Velocity 6301.5A | 236"x162" | 749 spectra |
|
Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 12 MB |
SOTSP: HOP 373 filament in North
2019-09-28T09:25:04 to 2019-09-28T10:12:28
Science Goal: Formation and destabilisation of filaments
Program: Fast map, 230"x164", Q65, 1-side CCD
Target: Filament
xcen=379 ycen=574
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.
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: 35
Chief Observer
Tiwari and DeRosa (RCO) -> Hasegawa
See also
Get All Data
saaIntervals
hiIntervals
Time Series (SP Datacubes)
wavelength: 6302A Continuum Intensity cadence: 0 min fov: 236,162 images: 749 JavaScript Landing Page
