Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
SOTSP: Understanding the Driving Mechanisms and Properties of RBEs Using IBIS and Hinode
2012-11-06T16:54:00 to 2012-11-06T17:43:05
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=-228 ycen=61
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.

Annotations:
Hits: 22
Chief Observer
Cruz (RCO)
Related Links
Cited By: Get Data
Timeline: gif use
See also
Datasets
saaIntervals hiIntervals
contextwavelength: null cadence: fov: null,null images: null