I recorded 30 scans of the Sun, using the SHG 700 with a 678MM camera.






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
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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