Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2017-02-17 06:35:34-07:07:55
Active region jet studies with Hinode and IRIS
Active region jet studies with Hinode and IRIS
x,y:-624",254"
Max FOV:162"x162"
Target:Active Region Sunspot
Nearby Events
6302A Continuum Intensity162"x162"512 spectra
6302A Longitudinal Flux Density162"x162"512 spectra
6302A Transverse Flux Density162"x162"512 spectra
6302A Velocity 6301.5A162"x162"512 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SOTSP: Active region jet studies with Hinode and IRIS
2017-02-17T06:35:34 to 2017-02-17T07:07:55
Science Goal: Active region jet studies with Hinode and IRIS
Program: Fast map, 164x164", 1-side, Q75, no repeat
Target: Active Region Sunspot
xcen=-624 ycen=254
Instrument: SOTSP
HOP/JOP: 332
Description: Request to SOT HOP Number 0332 SOT participation is optional, but two possibilities are the following: 1) If a well-developed sunspot penumbra is included in the IRIS and
EIS rasters, run a repeated dynamics mode raster (full resolution, no summing, 2.4 sec integration), with FOV approx. 20 x 60 or 20 x 80 arcseconds, wide enough to cover all of the inner penumbra and most of the outer penumbra on one side of the spot. An East-West ROI offset may be used to place the SP raster as desired on the penumbra. This should run at least 2 hours, telemetry permitting. 2) Run repeated fast maps covering the central portion of the IRIS and
EIS rasters, with cadence of 10-20 minutes, similar to HOP 306.

Request to SOT HOP Number 0332 SOT participation is optional, but two possibilities are the following: 1) If a well-developed sunspot penumbra is included in the IRIS and
EIS rasters, run a repeated dynamics mode raster (full resolution, no summing, 2.4 sec integration), with FOV approx. 20 x 60 or 20 x 80 arcseconds, wide enough to cover all of the inner penumbra and most of the outer penumbra on one side of the spot. An East-West ROI offset may be used to place the SP raster as desired on the penumbra. This should run at least 2 hours, telemetry permitting. 2) Run repeated fast maps covering the central portion of the IRIS and
EIS rasters, with cadence of 10-20 minutes, similar to HOP 306.

Annotations:
Hits: 45
Chief Observer
Cruz (RCO) --> Bamba
Related Links
Cites: Active region jet studies with Hinode and IRIS     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 162,162 images: 512 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 162,162 images: 512 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 162,162 images: 512 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 162,162 images: 512 JavaScript Landing Page