Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2023-05-10 08:00:12-08:47:30
Coordination with SST and IRIS - Dynamics of flux cancellation in neutral lines
Dynamics of flux cancellation in neutral lines
x,y:574",225"
Max FOV:25"x81"
Target:Active Region
Nearby Events
6302A Continuum Intensity25"x81"1191 spectra
6302A Longitudinal Flux Density25"x81"1191 spectra
6302A Transverse Flux Density25"x81"1191 spectra
6302A Velocity 6301.5A25"x81"1191 spectra
Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 10 MB
SP Movies (Javascript)
SP Movies (MP4)
SOTSP: Coordination with SST and IRIS - Dynamics of flux cancellation in neutral lines
2023-05-10T08:00:12 to 2023-05-10T08:47:30
Science Goal: Dynamics of flux cancellation in neutral lines
Program: Very Fast Map, 23x82", 1-side, repeat
Target: Active Region
xcen=574 ycen=225
Instrument: SOTSP
HOP/JOP: 401
Description: abstract of observational proposal Scientific Justification: The investigation focuses on the physics of flux cancellation in neutral lines. Reconnection events along neutral lines form the photosphere to higher heights in the atmosphere are believed to be behind the formation of filament channels, the seeds of CMEs. A large number of cancellation events in coordination with SST (Halpha - looking for heating events such as Ellerman bombs) is needed to elucidate the physical processes behind the creation of filament channels. request to SOT Similar to HOP330 on 2017 April 22 at 14UT, but twice as wide (i.e. 20").

abstract of observational proposal Scientific Justification: The investigation focuses on the physics of flux cancellation in neutral lines. Reconnection events along neutral lines form the photosphere to higher heights in the atmosphere are believed to be behind the formation of filament channels, the seeds of CMEs. A large number of cancellation events in coordination with SST (Halpha - looking for heating events such as Ellerman bombs) is needed to elucidate the physical processes behind the creation of filament channels. request to SOT Similar to HOP330 on 2017 April 22 at 14UT, but twice as wide (i.e. 20").

Annotations:
Hits: 83
Chief Observer
Cruz (RCO)
Related Links
Cites: Coordination with SST and IRIS - Dynamics of flux cancellation in neutral lines     
Timeline: gif use
See also
Datasets
Order AIA Data Cutout
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0.01 min fov: 25,81 images: 1191 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0.01 min fov: 25,81 images: 1191 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0.01 min fov: 25,81 images: 1191 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0.01 min fov: 25,81 images: 1191 JavaScript Landing Page
Time Series (SP Datacubes)
JavaScript MP4
VOEvent XML Planning Event