Contains:  Solar system body or event
Animation of Solar Surface Activity 2023-06-09 (Sorry for the large file) Mono, DWS 23

Animation of Solar Surface Activity 2023-06-09 (Sorry for the large file) Mono

Acquisition type: Lucky imaging
Animation of Solar Surface Activity 2023-06-09 (Sorry for the large file) Mono, DWS 23

Animation of Solar Surface Activity 2023-06-09 (Sorry for the large file) Mono

Acquisition type: Lucky imaging

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Description

This surface animation shows a lot of activity with some very bright areas. The duration of the animation is only about 30 minutes. 
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
We will be looking at and understanding a bit of what is happening in the animation. The first point of note is the detailed contrast in the spicules within the chromosphere. These spicules are the almost hair-like structures observed while viewing the animation, these spicules rise directly out of the chromosphere over the course of 10-20 minutes. Spicules are massive energetic jets of plasma traveling upward from the photosphere beneath the chromosphere at 20-120 km/s. The result is extremely visible surface dynamics, as in this timelapse the chromosphere can be seen to transform near constantly over the course of an hour. Of further interest is the dark filament traveling across the center. It could be assumed that it is merely a hole, however it is actually a magnetic loop that has formed above the Polarity Inversion Line and parallel to it. It’s extremely fascinating because the dark region is cooling plasma being channeled across the magnetic loop. This cooling plasma presents as an optically dense and, therefore, dark spot when held against the surrounding temperature and optical densities.

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