Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
SOTSP: HOP 95 NBPs
2009-02-07T10:11:00 to 2009-02-07T11:57:00
Science Goal: A statistical analysis of the Magnetic fields of the Network Bright Points (NBP) with the BFI and NFI at the boundaries of supergranules
Program: Fast map, 220"x123", Q75, 1-side CCD
Target: Disk Center, Network bright points
xcen=-48 ycen=0
Instrument: SOTSP
HOP/JOP: 95
Description: The BFI will provide images in the G band. On such images, NBPs appear as proxies of intense magnetic flux tubes. The NFI will provide the full Stokes IQUV in one of the wings of FeI 5250.2 A (high Lande factor g = 3), or in the line center.

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Related Links
Cited By: Get Data
Timeline: gif use
See also
Datasets
saaIntervals hiIntervals