Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
SOT: HOP 95 NBPs
2009-02-07T13:55:00 to 2009-02-07T14:14:35
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 line scan 40mA step, 1 min
Target: Disk Center, Network bright points
xcen=-48 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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Timeline: gif use
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saaIntervals hiIntervals
contextwavelength: null cadence: fov: null,null images: null