Contains:  Solar system body or event
Prominence animation showing arching plasma being transferred between two active sets, DWS 23

Prominence animation showing arching plasma being transferred between two active sets

Acquisition type: Lucky imaging
Prominence animation showing arching plasma being transferred between two active sets, DWS 23

Prominence animation showing arching plasma being transferred between two active sets

Acquisition type: Lucky imaging

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Description

Processing some old data.

Animation showing a large prominence and some of the solar activity from 6-17-23. Animation consisting of 17 frames, starting at 14:25 UT, ending at 14:57 UT. As always, I should have gone longer but had an interruption in my data accumulation. The span of this prominence is about 120,000 miles with a height of approximately 10,000 miles . Part two of this animation is to follow.

For a more detailed explanation about the physics of the activity, I would like to hand that over to my dear friend Andrew Rosado, who is pursuing his PhD in Astro-Physics. He knows way more about the dynamics of what is going on and I hope you find his description interesting and educational. I know I will!

From Andrew:

This is a relatively interesting prominence, it's the most recent animation to present a prominence this low in the chromosphere. To cover a prominence are jets of plasma that are thermally insulated by the magnetic field containing them. As a result, the thermal gradient results in differing optical densities and therefore structure. Despite its relatively low altitude, the prominence is likely relatively cooler than a prominence that reaches out far into the corona. This is a product of the increasing temperature that exists with an increase in distance from the core. At the transition zone, which is about 8500km outwards from the convection zone. Temperatures in excess of 1,000,000 Kelvin.

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