Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2010-11-28 09:18:17-11:45:13
HOP176 Disk Center Fixed
High Resolution Multi-Wavelength Study of Small-Scale Jets on Solar Disk
x,y:-11",-8"
Max FOV:33"x122"
Target:disk center, Spicule and Jets
Nearby Events
6302A Continuum Intensity33"x122"2189 spectra
6302A Longitudinal Flux Density33"x122"2189 spectra
6302A Transverse Flux Density33"x122"2189 spectra
6302A Velocity 6301.5A33"x122"2189 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 28 MB
SP Movies (Javascript)
SP Movies (MP4)
SOTSP: HOP176 Disk Center Fixed
2010-11-28T09:18:17 to 2010-11-28T11:45:13
Science Goal: High Resolution Multi-Wavelength Study of Small-Scale Jets on Solar Disk
Program: Fast map 32x122", 1-side, Q75, repeat
Target: disk center, Spicule and Jets
xcen=-11 ycen=-8
Instrument: SOTSP
HOP/JOP: 176
Description: High Resolution Multi-Wavelength Study of Small-Scale Jets on Solar Disk Combination of SP and FG observation with SP as first priority. The observing procedure is the same for every day during the coordinatedobserving run. Only the target will change (4 days active region, 3 days each for quiet Sun observations within and outside of a coronal hole as close to disk center as possible). SP: ~400 Mbits/hr, 1200 Mbits/day Context SP IQUV scan (fast map, for 64" x 123", 0.32" slit, 14 min) at the beginning and end of the coordinated high cadence observing run. Continuous high cadence SP IQUV scans (fast 32" x 123", 0.32" slit, 7 min cadence) during the coordinated observation. FG: ~170 Mbits/hr, 510 Mbits/day Ca II H and G-band image sequence during coordinated observation (2-minute cadence, 111" x 111" FOV, 2 x 2 pixel binning).

High Resolution Multi-Wavelength Study of Small-Scale Jets on Solar Disk Combination of SP and FG observation with SP as first priority. The observing procedure is the same for every day during the coordinatedobserving run. Only the target will change (4 days active region, 3 days each for quiet Sun observations within and outside of a coronal hole as close to disk center as possible). SP: ~400 Mbits/hr, 1200 Mbits/day Context SP IQUV scan (fast map, for 64" x 123", 0.32" slit, 14 min) at the beginning and end of the coordinated high cadence observing run. Continuous high cadence SP IQUV scans (fast 32" x 123", 0.32" slit, 7 min cadence) during the coordinated observation. FG: ~170 Mbits/hr, 510 Mbits/day Ca II H and G-band image sequence during coordinated observation (2-minute cadence, 111" x 111" FOV, 2 x 2 pixel binning).

Annotations:
Hits: 46
Chief Observer
Shimizu
Related Links
Cites: HOP176 Disk Center Fixed     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 33,122 images: 2189 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 33,122 images: 2189 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 33,122 images: 2189 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 33,122 images: 2189 JavaScript Landing Page
Time Series (SP Datacubes)
JavaScript MP4