this post was submitted on 10 Apr 2025
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Another cloud free day in Scotland let me catch almost 9 hours of this huge and lively prom. Taken with my home made 90mm modded Coronado PST and DMK21 camera. Software: CdC, Eqmod, DSSR, AutoStakkert!, Wavesharp, DVS, Shotcut and Gimp.

David Wilson on April 8, 2025 @ Inverness, Scotland

https://spaceweathergallery2.com/indiv_upload.php?upload_id=221951

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[–] 1luv8008135@lemmy.world 55 points 2 days ago (11 children)

So dumb question, but what’s causing the gap between the plasma cloud(?) and the surface? And is that gap filled with something that is invisible?

[–] niktemadur@lemmy.world 35 points 2 days ago (4 children)

The dynamics there due to sheer gravity, magnetism and levels of energy/radiation that are utterly alien to our daily experience.

[–] NikkiDimes@lemmy.world 21 points 2 days ago (1 children)

I get some of the basic underlying mechanics, but I absolutely cannot comprehend it. Incredible.

[–] perestroika@lemm.ee 20 points 2 days ago* (last edited 2 days ago) (1 children)

A guess: doubly ionized helium vs. singly ionized helium. They absorb different amounts of radiation (have different opacity). At high opacity it gathers heat and subsequently expands. At low opacity it lets the heat pass through, subsequently cools and condenses.

(This is the mechanism that makes Cepheid stars regularly and predictably change intensity. The same mechanism is probably present in other stars too, and causes local processes that we cannot observe from another star system... but can observe in the Sun.)

Alternatively, there could be a multitude of other effects doing something similar.

[–] niktemadur@lemmy.world 2 points 1 day ago (1 children)

This is the mechanism that makes Cepheid stars regularly and predictably change intensity

Doesn't it also make the Cepheid noticeably swell (then deflate) in circumference? Or does it maintain the same basic size, and it's just storing magnetic bubbles of hot plasma like a halo, before bursting and releasing all that accumulated material?

[–] perestroika@lemm.ee 2 points 1 day ago* (last edited 1 day ago)

To my understanding they do chance circumference. The opaque doubly ionized helium forms at high temperature, expands until temperature drops (change in circumference), drops to singly ionized after expansion, and gets doubly ionized again after contraction (another change in circumference). In Cepheids, it's uniform across the whole star.

Thus, your question makes me doubt my original speculation that it's helium changing ionization levels. The way some material "climbs up" into the arc in this video (from the right end, at one point of time) while other material "rains down" make a magnetic explanation (proposed by others here) seem more plausible.

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