Contains:  Solar system body or event
Solar remnants of AR3664 - Set 2 of 3, DWS 23

Solar remnants of AR3664 - Set 2 of 3

Acquisition type: Lucky imaging
Solar remnants of AR3664 - Set 2 of 3, DWS 23

Solar remnants of AR3664 - Set 2 of 3

Acquisition type: Lucky imaging

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Description

Time lapse of Solar activity from the region of AR3664 as it passes the Suns limb showing the areas large magnetic fields at work. If we look carfully, part of Sunspot AR3664 is still visible at the edge. AR3664 was the sunspot that produced the beautiful Northern Lights on May 10-11, 2024. The time lapse consists of 18 images combined, spanning 36 minutes, starting at 19:41UT to 20:17UT. The height of the largest loop spans to about 40,000 miles above the surface. For a more detailed explanation about the physics of the activity, my dear friend Andrew Rosado, who is pursuing his PhD in Solar Astro-Physics, has given me a much better understanding of what is happening.  I hope you find his description interesting and educational. I know I always do!

From Andrew:

These solar filaments follow a near-perfect magnetic loop emanating from the chromosphere. The loops formed as large magnetic regions of the surface, divided into different polarities, interact. At intersections of these different polarity regions, Polarity Inversion Lines form. When following PILs’; magnetic breakout can occur due to violent magnetic interactions, forming a filament above. This facilitates the substantial quantity of comparatively cooler and dense plasma, supported by the resultant magnetic fields against solar gravity. This makes the structure you see in this data, a near perfect example of the magnetic interaction at work at the Sun’s surface.

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