Heliophysics Events Knowledgebase Coverage Registry (HCR)
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Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2017-02-15 15:05:45-16:29:58
HOP 332 AR 12635 w/IRIS and EIS
Active region jet studies with Hinode and IRIS
x,y:815",252"
Max FOV:18"x61"
Target:Active Region
Nearby Events
6302A Continuum Intensity18"x61"1494 spectra
6302A Longitudinal Flux Density18"x61"1494 spectra
6302A Transverse Flux Density18"x61"1494 spectra
6302A Velocity 6301.5A18"x61"1494 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 19 MB
SP Movies (Javascript)
SP Movies (MP4)
SOTSP: HOP 332 AR 12635 w/IRIS and EIS
2017-02-15T15:05:45 to 2017-02-15T16:29:58
Science Goal: Active region jet studies with Hinode and IRIS
Program: Faster Full-Res, 16x61", ROI 2, repeat, w/context
Target: Active Region
xcen=815 ycen=252
Instrument: SOTSP
HOP/JOP: 79
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.

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: 44
Chief Observer
Cruz (RCO)
Related Links
Cites: HOP 332 AR 12635 w/IRIS and EIS     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 18,61 images: 1494 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 18,61 images: 1494 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 18,61 images: 1494 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 18,61 images: 1494 JavaScript Landing Page
Time Series (SP Datacubes)
JavaScript MP4