Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
SOT: HOP73 Prominence
2008-09-18T10:02:00 to 2008-09-18T17:35:00
Science Goal: Quiescent Prominence Structure and Dynamics
Program: Ha 2WL core DG + CaH, for prominences, 30sec
Target: Prominence
xcen=575 ycen=742
Instrument: SOT
HOP/JOP: 73
Description: Scientific Objectives: This HOP seeks to further understand the structure and dynamics of QPs, and in particular the origin of the mysterious dark turbulent upflows and large bubble instabilities. Can we discern a thermal mechanism at work in these dynamics? Or are they caused, as the more classical explanation would have it, by magnetic field dynamics entraining the plasma in a low-?????? mode?

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Chief Observer
Tarbell
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contextwavelength: null cadence: fov: null,null images: null