Sun in Hydrogen Alpha

With Coronado PST

Uploaded 7/17/11

 The sun had a great many features today, and the seeing was fairly decent so I was able to use the 5x barlow again to gain some details. Clouds interfered with the first few frames, and the latest version of Registax 6 has more problems dealing with moving dark vapors moving over the sun than version 4. Once the clouds cleared (for a short while) I was able to use the much superior version 6 for full disk registrations. One of the sunspots has a nice flare on it too, appearing as a very brilliant white burned out region. Also, a very nice flame shaped prom was on one edge and had plenty of internal details as well.

Processing: For the most part, two images of each field were taken, one normal exposure and the second over exposed to show the very dim prominences. These were combined if the edge of the sun was present most of the time to show the full compliment of features. As is usual, no prime focus images are possible with the PST since the back focus is not sufficient.

Images with the Coronado 2x barlow:

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The big flame like prom is seen off to the left, and on the disk is an active region around a very tiny sunspot. The dark smudges around the spot are called filaments, and are proms seen in silhouette against the suns disk.

This image had some cloud issues!

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Now here is a white light image taken on the other side of the sun. To do a white light image with the PST, you crank the band pass adjust all the way to the end and get basically a view in red light with no hydrogen alpha features just like a white light view. compare this image with the one below!

A single small sunspot is seen here, with some faculae (white areas in the photosphere)

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Now here is the view in hydrogen alpha light. The details on the sun are quite a bit more interesting. The white faculae are much more prominent in this wavelength. The disk is covered with granulation. Remember - you are no longer looking at the photosphere of the sun. This is the basal Chromosphere, and the granulation is much larger to see. The proms on the edge and the fuzz all around the edge of the sun (spicules) are in the mid chromosphere. You cannot image the outer photosphere from earths surface unless there is a total eclipse.

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Moving the sun to the right we can see another spot here in white light coming on to the disk on the left. A bit of cloud is on the right side. (darn monsoon!)

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Here the same view as above in H-Alpha light. We can now see a bit of faculae around the spot on the left, but look in between the two spots - some nice filaments are starting to show up. The clouds went away at this point, and this image and those that follow will have much better overall disk registration since I used version 6. Look how nicely the program was able to register even the granulation automatically. NONE of the older versions did very well for me on this.

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The sunspot that was on the left in the above image is now on the right. There is some amazing activity going on disturbing the magnetic fields of the granulation here. I will have a 5x close up below.

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The lower right side of the Sun had some significant but small prom details. I was not able to get a clear shot of the disk due to clouds, so I darkened out the disk which is quite overexposed to show only the spicules fringe, and the proms. Believe me, if you don't do this the blasted solar disk really takes away from the faint prominences!

 

Images with the Televue 5x powermate barlow:

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Now were talking more details. The flame like big prom on the edge was stunning to say the least at 5x. This is a single frame, the prom was so bright I did not have to stack in the over exposed background. I did however continue the standard "tradition" of coloring the spicules and proms their correct blood red color.

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The active region imaged above on the center of the disk is quite nicely detailed at 5x. Seeing was starting to degrade a bit, but this shot still shows far more resolution than the 2x barlow. What an amazing tortured region on the sun...

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The sunspot on the right edge on closer examination was flaring. It is only a small B class flare, nothing to get excited about as far as aurora, but it was so brilliant that the area burned in pure white. An hour later, it was gone. Wow.

Look at the lumpy texture to the spicules on the edge here too.

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The other sunspot with the attending filament looks quite a bit more detailed here, You can imagine the twisting field lines of the sun spot which are seen very well in H alpha.

I hope you enjoyed this small presentation. I had fun making this, and am slowly creeping up the learning curve on this solar imaging stuff. As I get better at it, Ill certainly share my results with all of you as they come in...

Instrument: Coronado PST 40mm Platform: Astrophysics 1200 Camera: DMK 1024 Location: Payson, Arizona Elevation: 5150 ft. Sky: Seeing 6/10, Transparency 5/10 Outside Temperature: 80F Processing: Registax 4 and 6, Photoshop CS HOME SCHMIDT GALAXIES EMISSION NEBS REFLECTION NEBS COMETS GLOBULARS OPEN CLUST PLANETARIES LINKS