Staring @ the Sun, 47

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05/16/2012. I asked for some clear skies, and
here they are. Clearish in the morning and brilliant for a while in the early afternoon. The Sun is idling along at low x-ray levels, but there are several interesting formations playing here and there on the disk. AR1476 is disappearing, but several smaller, less-complex regions are taking its place.

I had the RiteAV ethernet cable bagged up on top of my office trash bin when the housekeepers came. One suggested it would make a good clothes line. Go for it, says I. Recycling in action.

The Cables to Go ethernet cable works fine for telescope and camera control, but the transfer speeds from the computer out by the telescope to my desktop remain disappointing. They are faster, but not by much. The remaining "air gap" of about five feet from the wireless router to the computer must be more of a bottleneck than I suspected. I've (just now) bridged it with a short Cat5 patch, so we'll see about transfering videos again soon. In the meantime, today's solar review:

 

sun

Surface: 17ms x 400, 5db. Best 40% selected.
Limb: 48ms x 400, 9db. Best 40% selected.

 

sun

17ms x 400, 6db. Best 50% selected.
Surface and limb detail processed separately.

 

Sun

8ms x 400, 5db. Best 50%.

 

 

5/17/2012. Commanded, acquired, and downloaded to the desktop all via the network, no trotting back and forth with flash or portable hard drives, no waiting to bring the notebook inside. The wired connection works great. Transfering a pair of 1GB files took 3-4 minutes total. Concatenated them, selected the best 500 out of 1,700 frames, stacked them and massaged the result all without leaving my desk or letting my coffee get cold.

 

sun

ARs 1482 & 1479
17ms x 1700, 6db.
Best 500 frames stacked.

 

This stack defeated big, slow seeing in the early morning. Near noon, with a smaller airmass, the amplitude of the seeing was much smaller but instead of "boiling and roiling" the air was "shimmering." I kept the solar image on my second monitor, watching flares play around (big but not particularly intense) 1479. I was also watching to see when the seeing was particularly steady. Once or twice, it was so still that I thought the capture software or the remote desktop had frozen, and at those times I grabbed a couple of 400 frame captures and built an image from the best 200 frames. The result falls short of the 500 frame example above only in the finest grained noise characteristics -- that is, only because electronic noise was be reduced in the 2.5x taller stack (by a factor of the square root of 2.5, actually). I think the image from the afternoon clip shows gradations very nearly as well and detail just as fine as the morning image distilled from more data. When all is said and done, seeing matters.

We've reached a lovely and problematic point: the images look better at higher resolution than is convenient to share via the Slow Blog.

 

 

 

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Except where noted, solar photos are made with a Point Grey Research Chameleon camera behind a Lunt Solar Systems 60mm THa solar telescope double-stacked wtih a 50mm front etalon for an achieved bandwidth of about 0.55 Angstroms. The telescope uses a B600 blocking filter and is mounted piggyback with an Astro-Tech 10-inch Ritchey-Chretien (carefully capped!) on an Astro-Physics Mach1GTO mount. An Acer Aspire One netbook running Point Grey's Flycap software provides camera control and capture services via USB 2.0. Images typically begin as 20 second AVI's captured at 15 fps. 300 frame clips are aligned and stacked using Registax 6 or AVIStack 2.0. The resulting files are processed via wavelet functions in Registax and / or the FocusMagic 3.0.2 deconvolution plug-in in Photoshop CS4. (PixInsight is rapidly supplanting some of those steps.) The imaging train usually includes an Orion "Shorty" 2x barlow screwed into the 1.25-inch prime-focus snout. Exposures are on the order of 4-8 ms with gain set to 10-12 db, or 12-18ms at 0 gain. The barlow is sometimes replaced by an Antares 0.5x telecompressor sandwiched between the 1.25-inch snout and the C-adapter on the PGR Chameleon; this produces a full-disk image (during most of the year) and allows exposures in the 1ms range with slightly less gain. A RoboFocus motor with a timing belt looped around the stock (or, sometimes, a Feathertouch) focus knob enables remote operation.


 

 


                   © 2011, David Cortner