Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
SOT: Synoptic
2015-03-04T18:04:30 to 2015-03-04T18:04:53
Science Goal: Synoptic
Program: Synoptic BFI NFI (revised: small, no mask, Na D cont.)
Target: Sun Center
xcen=19 ycen=26
Instrument: SOT
HOP/JOP: 0
Description: Sunspots often show bright fan loops in the AIA 171 channel, and these are clearly seen in upper transition region lines of EIS where they exhibit downflows of 10-40 km/s. Sunspot plumes are identified as redshifted features seen in transition region lines, and are particularly clearly seen in the IRIS O IV lines, which show velocities of 70-100 km/s. Sunspot plumes are usually narrower than fan loops, but are found in the same locations so they may represent one stage in the evolution of the strands that compose fan loops. This IHOP will take coordinated observations between Hinode and IRIS to investigate the relationship between sunspot plumes and fan loops.

Annotations:
Hits: 46
Chief Observer
DeRosa (RCO)
Related Links
Cites: Synoptic     
Timeline: gif use
See also
Datasets
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saaIntervals hiIntervals

wavelength: CN bandhead 3883 cadence: -1 min fov: 223,111 images: 1 JavaScript Landing Page
wavelength: G band 4305 cadence: 0.05 min fov: 223,111 images: 2 JavaScript Landing Page
wavelength: TF Na I 5896 base cadence: -1 min fov: 327,163 images: 1 JavaScript Landing Page
wavelength: red cont 6684 cadence: -1 min fov: 223,111 images: 1 JavaScript Landing Page
wavelength: green cont 5550 cadence: -1 min fov: 223,111 images: 1 JavaScript Landing Page
wavelength: blue cont 4504 cadence: -1 min fov: 223,111 images: 1 JavaScript Landing Page
wavelength: Ca II H line cadence: -1 min fov: 223,111 images: 1 JavaScript Landing Page
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