Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2012-11-06 14:19:26-14:43:41
Understanding the Driving Mechanisms and Properties of RBEs Using IBIS and Hinode
Understanding the Driving Mechanisms and Properties of RBEs Using IBIS and Hinode
x,y:-227",68"
Max FOV:121"x122"
Target:Active Region
Nearby Events
6302A Continuum Intensity121"x122"384 spectra
6302A Longitudinal Flux Density121"x122"384 spectra
6302A Transverse Flux Density121"x122"384 spectra
6302A Velocity 6301.5A121"x122"384 spectra
Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 4 MB
SOTSP: Understanding the Driving Mechanisms and Properties of RBEs Using IBIS and Hinode
2012-11-06T14:19:26 to 2012-11-06T14:43:41
Science Goal: Understanding the Driving Mechanisms and Properties of RBEs Using IBIS and Hinode
Program: Fast map, 123"x123", 1-side CCD
Target: Active Region
xcen=-227 ycen=68
Instrument: SOTSP
HOP/JOP: 203
Description: Request to SOT HOP Number 0203 ~1590Mbits/day Combination of SP and NFI observation. The observing procedure is the same for every day during the coordinated observing run. Only the target will change. SP: ~400Mbits/hr, 1200Mbits/day repeat SP IQUV scans (fast map, FOV 110" x 123", 0.32" slit, 20 min cadence) during the coordinated observation. The gaps between SP scans due to the SAA periods are accepted. FG: ~130Mbits/hr, 390Mbits/day NFI Na I D 5896 longitudinal magnetograms (MG 4 V/I), cadence 64 sec, in the observing period. Similar to the SP FOV. 2x2 summing.

Request to SOT HOP Number 0203 ~1590Mbits/day Combination of SP and NFI observation. The observing procedure is the same for every day during the coordinated observing run. Only the target will change. SP: ~400Mbits/hr, 1200Mbits/day repeat SP IQUV scans (fast map, FOV 110" x 123", 0.32" slit, 20 min cadence) during the coordinated observation. The gaps between SP scans due to the SAA periods are accepted. FG: ~130Mbits/hr, 390Mbits/day NFI Na I D 5896 longitudinal magnetograms (MG 4 V/I), cadence 64 sec, in the observing period. Similar to the SP FOV. 2x2 summing.

Annotations:
Hits: 54
Chief Observer
Cruz (RCO)
Related Links
Cites: Understanding the Driving Mechanisms and Properties of RBEs Using IBIS and Hinode     
Timeline: gif use
See also
Datasets
Order AIA Data Cutout
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 121,122 images: 384 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 121,122 images: 384 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 121,122 images: 384 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 121,122 images: 384 JavaScript Landing Page
Time Series (SP Datacubes)
VOEvent XML Planning Event