Category: Besorolatlan

Some other handy solar stuff

because google is no longer our friend when it comes to finding stuff

Solar spectrum, with tellurics https://hs5000.vo.aip.de/

SOLAR-ISS: A new reference spectrum based on SOLAR/SOLSPEC observations https://www.aanda.org/articles/aa/pdf/2018/03/aa31316-17.pdf

GOES X-Ray Flux https://www.swpc.noaa.gov/products/goes-x-ray-flux

Infrared Helium Sun: https://iopscience.iop.org/article/10.1088/1674-4527/ad37f4/pdf

Databases: https://data.nas.nasa.gov/helio/portals/solarflares/datasources.html

Flares and stuff: https://www.lmsal.com/isolsearch

Flare prediction forecast https://www.solarmonitor.org/forecast.php

Liege https://fermi.jhuapl.edu/liege/s08_0085.html

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A great spiral on the Sun, 2025-03-01

Cloudy and hazy sky, but hey, what else to do. The He I D3 enhanced signal clearly reflects what the corona is doing, according to NASA/SDO/AIA

https://sdo.gsfc.nasa.gov/assets/img/browse/2025/03/01/20250301_100911_1024_0211.jpg

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Hunting the Calcium II triplet

The Sun at around 850 nm infrared*, false color

With my usual setup, the EQ3-mod, mountpusher, Baader Astrosolar ND3.8 Film, TS-Optics 76/342 TS76EDPH, ?filters?, ASI 178MM (cooled), I though what if I got creative. I put in the IRpass 850 filter from ZWO, and added an additional ND1.3 filter, because the ND5 front filter was a bit out of reach. Afterthought: I don’t know the transmittance curve of the ND filter, so maybe what I photographed is actually undefined-ish.

With the above in mind, the transmittance curve of the ZWO IR pass filter, along with the response curve of the camera, gives us a gentle hill around the magic 850 nanometer region, which is where the Calcium II triplet resides, and should draw the active regions in a similar way the CaK does. No matter what filters I used, these active regions show up in all of them, from UV, through CaK, deep blue, even in oxygen III, solar continuum, and 7nm Hα.

Digging out the details did take a good while, since the granulation (I guess it is that) on the surface of the Sun causes a sort of pixel noise to appear that doesn’t fare well with my emphasizing solutions. This „pixelnoise” is also present in my CaK images, and looks exactly the same on the DSO resources I checked at 160 and 170 nanometers.

ND1.3 and telescope glass aside, this is the wavelength-intensity area that should be in the photo. Telluric absorption is not that interesting in this region, and is uniform across the solar disk anyway.

(tovább…)

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Fotótervező 7. rész: a hasonló a hasonlót vonzza

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Műhelytitkok 3. — élességállítási tippek bolygófotózáshoz

 

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Saturn 2019-09-20

HEQ5, N250/1200, TSO ADC, ASI 224MC (cooled), home observatory, mountpusher, very bad seeing conditions

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Jupiter and Europa 2019-09-20

HEQ5, N250/1200, TSO ADC, ASI 224MC (cooled), home observatory, mountpusher very bad seeing conditions

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Jupiter, Io 2019-07-15

Jupiter and Io. I just realized why I don’t have a TV: I can see live interplanetary feeds from my balcony. And while there is less action and it’s considerably slower, Galileo Galilei did stuff like this – just a tad more low tech. ASI 224MC, TSO ADC, N250/1200, HEQ5 guided by the soapbox project.
(tovább…)

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Saturn, bad seeing

Let me post a bad picture of mine, Saturn as it looks through bad seeing and some thin clouds. In a way, this is the normal for me. Datetime: 2019-07-14-21-58Z, long video. ASI 224MC, TSO ADC, N250/1200, HEQ5

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Mars 2018-09-10

N 150/750, 2x Barlow, TS Optics ADC, 20cm extension tubes, ASI 224MC, PIPP, Registax, 1500 out of 20k frames.

Mars 2018-09-10

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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.).