A stack of 40 scans obtained with ML Astro’s SHG 700 spectroheliograph.
A stack of 16 scans obtained with ML Astro’s SHG 700 spectroheliograph.
Ever tried posting a link under a youtube video? It may get auto-deleted, no matter if it is on topic. Tried talking about how to find the on-topic resource, to avoid deletion? Also gets deleted. What we get instead is AI-slop upon AI-slop and a control of the narrative, like those not really on youtube never even existed.
Just fuck that.
Google is not your friend.
Using the ML Astro SHG 700 (third batch) spectroheliograph, on a 80/540 refractor, ASI 678MM camera, I recorded seven scans of the Sun, in the singly ionized iron line, Fe II 5018.45Å.
This is what I got after getting rid of the artefacts and amplifying a bit the already strong signal (way stronger than He I D3).
I scanned the Sun into a cube, containing the Ba II line at 6141.73Å which, like we’ve seen with ionized metals before, turn the active regions dark, instead of letting them shine against a darker photosphere. The atmosphere was remarkably calm on 2025-04-21, and further, the disks were anti-jagged by an experimental feature in JSolEx. (tovább…)
From some of the data I recorded, among which there are quite a few comparatively wide cubes, I assembled the Atlas and published the software platform and the first cubes in it.
And the research note on the atlas: https://iopscience.iop.org/article/10.3847/2515-5172/adef50
Stuff I found on the net about this:
https://solarchatforum.com/viewtopic.php?t=50095
https://solarchatforum.com/viewtopic.php?p=476026
https://www.cloudynights.com/forums/topic/970675-first-ever-browsable-solar-spectrum-atlas/
Continuing my incursions into virtually (at least by amateurs) unexplored lines, on 2025-04-20 I went into the singly ionized Strontium at 407.77 nanometers (4077.7 Ångström).
Sol’Ex, JSol’Ex and imagemath scripts to dig out the weak signal.
And a trisolaran werk photo also, with the spectroheliograph’s three Suns.

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