Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
SOT: HOP 95 NBPs
2009-02-07T10:11:12 to 2009-02-07T11:54:46
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: 5250 sh-less line center and GB for HOP 95
Target: Disk Center, Network bright points
xcen=-46 ycen=0
Instrument: SOT
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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Hits: 37
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Related Links
Cites: HOP 95 NBPs     
Timeline: gif use
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saaIntervals hiIntervals

wavelength: G band 4305 cadence: 1 min fov: 111,111 images: 105 JavaScript Landing Page