Monthly archives: szeptember, 2025

Flare in He I 5015.7

With a rather unusual setup, the SolEx coupled with the IMX 571 wielding Altair Astro 26C camera, I observed a bright solar flare at 2025-09-28 08:43Z (a longer time series actually) at to my surprise, the helium line also lit up. This is not a typical nor a recommended setup of the SolEx. I sacrificed spatial (either way, bad seeing) and spectral (…) resolution for bit depth.

With the Helium image, I cheated a bit: the perpetually changing thin clouds resulted in the helium wavelength’s disk center getting saturated from time to time, so data’s been taken from non-saturated takes, to fill that gap.

He I 5015, continuum-subtracted

He I 5015, continuum-subtracted

Fe II 5018, CLAHE-enhanced signal

Fe II 5018, CLAHE-enhanced signal

spectra, before and during

spectra, before and during


Green Helium Prominence — first detection of He I 5015

The He I 5015 prominence, probably the least significant bit in the data

Using the usual setup, an ML Astro SHG 700 on a 80/540 refractor and a cooled IMX 678 camera, with an in-cone interference filter as an ERF, letting through the oxygen line, and coincidentally, the Fe II 5018.45Å and also the He I 5015.7Å lines, I managed, for the first time, to dig out a bright-ish prom in the green (turquoise-something) Helium line.

This could well be among the first, if not the very first amateur observation of this line.

See

https://physics.nist.gov/PhysRefData/Handbook/Tables/heliumtable2.htm

Processed using JSolEx.

(tovább…)


H gamma

I stacked together some decent scans into this frame of hydrogen gamma. ML Astro SHG 700, with a 80/540 refractor, in-cone ERF, Ersatz-Obsi.


Jól kalibrált monitoron mindegyik számnál elkülönülő árnyalat látszik. Ha mégsem látszanak, akkor a megjelenített képek színhiányosan rajzolódnak ki. A monitort valószínűleg kalibrálni kell.

You should see distinct shades for each number. If those shades are not clearly visible, the displayed pictures will lack accuracy. Your display most likely needs to be calibrated (brightness, gamma, contrast etc.).