Solar Awakening

H-Alpha Sun

Solar Prominences
Sketch and Details by Les Cowley

After weeks of inactivity the sun stirred at the end of September ’08. The 28th saw a huge but faint prominence on the Southeast limb and the next morning revealed two large and bright prominences almost diametrically opposite each other on the SE and Northern limbs. They are pictured here as viewed from England through a Coronado 60mm H-Alpha single-stacked telescope at 50 and 80X. The sketches were made at the eyepiece with Derwent Studio, Watercolour (dry) and Drawing pencils on black Canford paper. A black hood blocked out extraneous light. Each had to be finished within 10 minutes because the prominences, particularly the southern one, were evolving quickly.

Eclipse’s Delicate Blossom

2008 Eclipse

Total Solar Eclipse – August 2, 2008
Sketch by Serge Vieillard

Serge Vieillard made this sketch of the total solar eclipse of 2008 from the Gobi Desert in China. In the minutes leading up to totality, clouds threatened to hide the event from his eyes. He raced 1000 meters from his initial location to find a clear spot, only to have the clouds drift there as well. In the final moments however, the clouds broke and he was able to spend an ecstatic 2 minutes drawing the view through his Kowa TSN-2 77 mm spotting scope at 20X. As the seconds passed and his eyes adapted, he crafted the increasingly complex, asymmetrical contours of the Solar corona and noted a bright star in Cancer. During the final few seconds of totality, the pink bloom of a prominence emerged and topped off an exciting and memorable observation.

Solar Prominences – September 1, 2008

Solar Collage

Sun in H-Alpha
Sketch and details by Erika Rix

2008 September 01
solar
Erika Rix

Sketch media: black Cranford paper, white Conte’ and Prang pencils

It was a good day. I shared some solar views and was repaid with lunch!

After having walked the dogs up the road and through some fields first thing this morning, the skies were clear and I was looking forward to observing. I dragged the LXD mount outside in front of the observatory to see if the seeing improved. I didn’t set it back up inside to compare with, but I was a lot cooler, which in turn made an improved comfort level temperature wise. The downside was moving all my gear outside, putting up with a little wind, and observing on a slope. The views were worth it.

Half way through the session, my neighbor honked when she drove up the road to her house, so when I was finished with my sketches, I called her to see if she’d like to come down and have her first look at the sun through a telescope. Paul came down to join us and we had a really enjoyable time. He just came back from imaging the Sun with the Maxscope so I’m looking forward to comparing our views. His session was a few hours behind me, so I reckon there will be a few changes.

Being the thoughtful person that she is, our neighbor came back from her solar session with lunch for Paul and me.

Siberian Solar Eclipse

Solar Eclipse

Solar Eclipse
Sketch and Details by Ernest Shekolyan

That was so great event! I do not know what was more exiting in this solar eclipse – just one hour clear sky over Novosibirsk or magic view of black sun in shining coronary ring. Whole day before this short eclipse were partial or continuous clouds, but no one after the first contact! In comparison to eclipse 29 april 2006 corona was not so bright and contrast.

Draft of the sketch (pencil on white paper) was made in few minutes after end of the total phase. Then in 12 hours it was made final version of the sketch (the same pencil, but with better quality).

Ernest

Soaring Across the Solar Aviary

Sun H-Alpha

Sun (H-Alpha)
Sketch and Details by Ernest Shekolyan

Hi!

That is my picture of Sun on 7 May 2007 (13:40 msc). PST Coronado + 10 mm Super (Synta).
Interesting features: bird-like active chromispheric flash in center of solar disc and a number prominences on the limb. Graphite pencil, white paper, then photocopy and processing in ACDSee (coloring, soft, some additional manual drawing).

Sincerely yours, Ernest Shekolyan

Protubérances Solaires

Prom 1

Solar prominences
Sketches and Details by Cyprien Pouzenc

Bonjour !

Some prominences drawn at the 9 mm Nagler eyepiece, mounted on the
coronograph 107/1200 of the Sirene Observatory (www.obs-sirene.com) at
around 12pm on May 18, 2007 (! Yes, I was somewhat forgotten this
picture :o)

Prom 2

Lace… very difficult to render with graphite pencil !

Arch: drawn from 12:13 to 12:20 local time.
Shrubs: drawn from 11:57 to 12:06 local time.


Cyp

La Roque d’Anthéron (Bouches du Rhône, France)
+43° 43′ 03″ Nord, 5° 18′ 05″ Est, 175 m

CypASTROuille
Observatoire Sirene
Site NGC

The Sun, Pencils or Camera?

H-Alpha Sun

H-Alpha Sun
Sketch and Details by Les Cowley
Comparison Photos by Pete Lawrence

The Sun is an ever-changing target. In H-alpha light, prominences light and
dim, shift and change literally by the minute. Fascinating to watch and
sketch but just how accurate are drawings grabbed in a few minutes during
variable seeing and under a black hood?

May 7th was an opportunity to find out when Cloudy Nights held an
“International Day of the Sun”. Expert UK photographers Peter Lawrence and
Nick Howes suggested imaging or sketching a prominence every 30 minutes on
the hour and half hour!

The day dawned clear and after breakfast the selected prominence was viewed.
It was the ugliest assortment of filaments, clouds and loops that you could
imagine with parts changing and dancing about even as you watched. The
‘scope was a Coronado Solarmax60 mounted on a manual altazimuth. Seeing
started fairly good so I used an 8mm Radian, I need eyeglasses to sketch and
the Radian gives enough eye relief. The drawings were on A4 black Canford
paper filling half the sheet per sketch with Derwent Watercolour pencils
used sharp and dry.

Serious observing started about 8 minutes before each time mark with the
main proportions starting to be put in 5 minutes before the mark. Then finer
and finer details were quickly added, not in any order just wherever good
seeing happened to show them. This quickly brought the time to the mark and
then the whole view was assessed for accuracy. It was changing so fast!
Finally 3-5 minutes after the mark were spent getting the relative
intensities right and generally tidying up.

By 09:45 there were frequent periods of superlative seeing and I changed to
a 5mm Radian and clutched the dark hood around close to shield the daylight.
For long periods (but never, ever during the allocated 10 minute slots!) the
visible structures were exquisitely resolved into delicate stacked filaments
with even those sometimes doubling and breaking into knots – you would need
an hour or hours to capture all that! After 10:30 the seeing deteriorated
and that combined with not a little fatigue ended the sketching run.

Pete Lawrence was imaging some 150 miles to the south with about the same
seeing conditions. He used a Solarscope SF-70, a Rolls-Royce of H-alpha
filters. His images for the same times are on a reduced scale at the base
but you need to see the originals (http://www.digitalsky.org.uk/ and Cloudy
Nights) to really appreciate their superlative quality.

So can sketching such ephemeral objects ever be accurate? I’m still
deciding. There is maybe a tremendous amount to be leaned from a careful
comparison of sketch fragments with simultaneous photographs about how the
eye-brain interprets fine details and tends to join others into spurious
larger structures. If some of that can be understood then hopefully it might
improve the sketching accuracy.

Les Cowley, England

May 4, 2008 Solar Collage

Sun

H-Alpha Sun
Sketch and Details by Erika Rix

PCW Memorial Observatory, Zanesville, Ohio, USA, Lat: 40.01 / Long: -81.56

Erika Rix

Temp: 54.0°F / 12.2 °C
Winds: 5.8 mph NW, clear turning to partly cloudy
Humidity: 53%
Seeing: very poor 2/6
Transparency: 4/6

Equipment:
Internally double stacked Maxscope 60mm, LXD75, 40mm ProOptic Plossl, 21-7mm Zhumell, ETX70AT, 8mm TV Plossl

Sketch Media:
H-alpha – Black Strathmore Artagain paper, white Conte’ and Prang pencils, white vinyl eraser.

White light pores created in Photoshop.

New active region in the ESE quadrant was visible with two crescent shaped plage facing each other during the h-alpha observing session. In white light, seeing was very poor making it invisible at first glance. Eventually my eyes were able to see two dark specks in the AR, appearing to be only umbrae, with the more easterly one slightly darker and thicker.

No faculae were noted in white light.

Of the prominence activity in h-alpha, the long line of southern prominences had filament reaching out over the disk on the far western edge. The large eastern edged prom in this line was leaning at a crook to the east (right) in my FOV. It was also the faintest of the four more prominent prominences around the Sun’s limb.

A Freckle on the Sun

Mercury-Solar Transit

Mercury-Solar Transit
Sketch and Commentary by Jeremy Perez
Move cursor over sketch to see labels.

On Wednesday, November 8th, 2006, Mercury was due for a solar transit. Now, in my neck of the woods, that just happens to be a work day. So I planned to set up the scope during lunch in the parking lot, or outside the lunchroom. The only thing I needed was a solar filter. A couple years ago, a very kind and generous amateur astronomer from Phoenix, Scott Kroeppler, sent me a couple small Baader solar film samples. Other than some casual, unmagnified looks at the sun, I hadn’t put them to good use. Until now. I stayed up the night before, rigging these two 1-inch square pieces of solar film and a sewing hoop to an 8 inch square piece of foam core. I wasn’t sure if it would work, but the next morning, I pulled into the parking lot at work, put my mangy, home-made solar cap on the front, and got a handheld look at the sun for the first time through my own scope. Not only did it work great, but I was pleasantly surprised to see a huge sun spot easing over the solar limb.

So I got to work, and then about 15 minutes before the beginning of the transit, I put it all together on the patio outside the lunch room where I had the best opening between all the trees. I didn’t start quite early enough, because by the time I got everything set up and the solar cap taped on securely, Mercury was already well inside the solar disc. It looked just like a printed period against blue-white filtered circle of the sun. It had entered just south of the massive sunspot I noticed earlier. A couple fainter sunspots rested on the opposite side. At that point, I made my first solar sketch, and noted how easy it would be to really exaggerate distances and proportions across the sun’s face. I was excited to see that light, textured, filamentary features were visible around the sunspots. As I studied these features, I noticed that it didn’t take long for Mercury’s motion to become apparent.

Over the next 45 minutes, I invited passing coworkers to have a look. They all seemed happy to get a look at the transit, particularly after reading about it in the newspaper the day before. As folks walked up to the eyepiece, I tried to coach them a bit with the sketch to be sure they didn’t confuse the sunspot for Mercury. Quite a few commented on how very tiny the little planet appeared. Several of them were even able to make out the two relatively faint sunspots over on the western limb as well. After a little more than an hour, I moved the scope to an out-of-the-way spot, and went back to work.

At about 20 minutes before the end of the transit, I raced outside to find that the sun was completely hidden behind trees where I had the scope set up. With a bit of scouting, I moved the whole thing into the parking lot about a hundred yards to the north where I had a clear vantage. And here I got to watch that perfect little dot edge closer to the western edge of the sun. At about four Mercury diameters from the edge, the whole shebang began to sink behind a tree-lined ridge a mile to the west. So I missed seeing Mercury merge with and disappear into the darkness on the other side of the sun. It was still a fascinating event to witness, and since Mercury won’t do this again until 2016, I’m glad I was able to fit it in.

The sketch at the top of this post was overlayed onto a digitally generated disc with limb darkening that estimates what I saw through the eyepiece. The next time I sketch the sun this way, I’m sure I’ll want to include the lighter features, which will mean generating that limb darkening manually and erasing through it.

Subject Mercury – Solar Transit
Classification Planetary/Solar
Date/Time November 8, 2006, 12:33 – 04:54 PM MST (November 8, 2006, 07:33 – 11:54 UT)
Observing Loc. Flagstaff, AZ
Instrument Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)
Eyepieces/Mag. 25 mm (48X)
Conditions Clear, breezy
Seeing Ant. IV