Tag Archives: Sunspot

CNYO Observers Log: Green Lakes State Park Solar Session (7 March 2015) and Monthly Baltimore Woods Session (13 March 2015)

Greetings fellow astrophiles,

A quick observing log combining two recent events hosted by Central New York’s own Bob Piekiel. As everyone who’s been local all winter knows, conditions were less than ideal for lots of observing. For those sessions that cloud cover (and snow) didn’t ruin, the Arctic Chill that hit CNY in the middle of February really did a number on even the most determined observers.

Solar Session – Green Lakes State Park – 7 March 2015

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Having put off and re-put off a solar observing session at Green Lakes State Park bus to lousy conditions, the powers that be wanted to go forward with a session on Saturday afternoon, March 7th. With H-alpha and Baader’ed scopes in tow, Bob (and I helping run the Baader’ed scope) hosted a session in the parking lot behind the main building at Green Lakes. Over the course of about 90 minutes, perhaps 10 good minutes of observing were had. Clear skies to the East couldn’t be coaxed to shift West and the upcoming mild snow storm that afternoon even provided some advanced warning. Still, about 10 people either showed specifically for the solar or made their way off the skiing path to take in a few sights of our nearest star.

2015march19_sunspots_1024_20150307The Sun itself wasn’t particularly busy that afternoon, with a major sunspot region having just fallen off the Sun’s edge, leaving a small speck of dark spots just within scopesight (see the March 7th image at right from NASA SOHO. Click for a larger view). As with all sessions, the observing was complemented by good introductory astronomy discussions and direction to the CNYO site for upcoming events (including upcoming solar sessions).

For those keeping additional track, the Sun did provide quite a show over the past few days in the form of fantastic aurora after an X-class solar flare fired up ionization in our atmosphere. For those looking for a gallery of what everyone by Central New Yorkers (it seems) saw over this past St. Patrick’s Day, I encourage you to let google do the work for the following image search: solar storm st. patricks 2015.

Baltimore Woods Monthly Session – 13 March 2015

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A panorama from the Baltimore Woods Session start. Click for a larger view.

A decidedly more fruitful session was had in the thawing parking lot of Baltimore Woods on Friday, March 13th. This evening was also first light for 2015 of my 12.5” NMT Dob (Bob’s SCT having already seen action with a few observing sessions this year). The sky (mostly) did not disappoint! Jupiter and Venus were easy and excellent targets, Mars was at the horizon at session start but still observable (Uranus having slipped too low to see), and a dozen eager observers attended to take in the sights. The only real letdown for the evening was the persistent cloud cover that obstructed all of Orion throughout, giving only a few passing views of the Orion Nebula. To Jupiter, Venus, Mars, and the Orion Nebula (sort of), a very double-centric crowd were treated to views of the double cluster in Perseus, Alcor and Mizar in Ursa Major, and Castor (a sextuplet star system that resolves to a bright binary pair) and Pollux in Gemini. Cloud cover was just persistent and wide-ranging enough to make galaxy views all but impossible, making the whole session a real hopscotch survey of the brightest available at the time. After a solid 80 minutes of observing, we finally packed up with plans for the next sessions made.

For those wanting to check out one of Bob Piekiel’s many events this year, please see his calendar on the CNYO website. We hope to see you!

Partial Solar Eclipse On October 23rd – Attendance And Location Update

Greetings fellow astrophiles,

The forecast for Thursday (Oct. 23rd) presently isn’t all that pleasant for observing the upcoming partial solar eclipse, but 3 days is a long time for CNY forecasting. We will keep track of the weather over the next few days and will announce on this site and our Facebook Page accordingly.

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The views of the partial solar eclipse from Starry Night Pro’s predictions.

The current location for the session will be the very southern end of the Onondaga Lake Parkway, just below the baseball diamond shown in the google map below.

For those willing to brave that left-hand turn at the main entrance, you need only loop left on the Parkway to get to the large parking lot at the southern end. For those NOT interested in fighting any rush hour traffic, we advise making a driving map that has you going past Heid’s, turning left onto 1st Street, making the left onto Lake Drive, then meander your way along to Onondaga Lake Parkway to get to the south end.

All of the data I’ve found so far for New York indicates the eclipse will start at 5:43 p.m. And go well past sunset (at which point it does’t matter to us anyway). The CNYO board will have several solar scopes and solar glasses there, so all you need do is show up! If you’ve solar equipment you want to bring, by all means do so.

Attendees may even be in for a special treat, as there’s currently a MASSIVE sunspot gracing the Sun’s surface. Seriously, look at the size of that thing in the image from NASA SOHO below:

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As always, keep track of this website for weather updates, with the final call being made on Thursday afternoon. We hope you can join us!

NASA Space Place – The Power of the Sun’s Engines

Poster’s Note: One of the many under-appreciated aspects of NASA is the extent to which it publishes quality science content for children and Ph.D.’s alike. NASA Space Place has been providing general audience articles for quite some time that are freely available for download and republishing. Your tax dollars help promote science! The following article was provided for reprinting in April, 2014.

By Dr. Ethan Siegel

2013february2_spaceplaceHere on Earth, the sun provides us with the vast majority of our energy, striking the top of the atmosphere with up to 1,000 Watts of power per square meter, albeit highly dependent on the sunlight’s angle-of-incidence. But remember that the sun is a whopping 150 million kilometers away, and sends an equal amount of radiation in all directions; the Earth-facing direction is nothing special. Even considering sunspots, solar flares, and long-and-short term variations in solar irradiance, the sun’s energy output is always constant to about one-part-in-1,000. All told, our parent star consistently outputs an estimated 4 × 1026 Watts of power; one second of the sun’s emissions could power all the world’s energy needs for over 700,000 years.

That’s a literally astronomical amount of energy, and it comes about thanks to the hugeness of the sun. With a radius of 700,000 kilometers, it would take 109 Earths, lined up from end-to-end, just to go across the diameter of the sun once. Unlike our Earth, however, the sun is made up of around 70% hydrogen by mass, and it’s the individual protons — or the nuclei of hydrogen atoms — that fuse together, eventually becoming helium-4 and releasing a tremendous amount of energy. All told, for every four protons that wind up becoming helium-4, a tiny bit of mass — just 0.7% of the original amount — gets converted into energy by E=mc2, and that’s where the sun’s power originates.

You’d be correct in thinking that fusing ~4 × 1038 protons-per-second gives off a tremendous amount of energy, but remember that nuclear fusion occurs in a huge region of the sun: about the innermost quarter (in radius) is where 99% of it is actively taking place. So there might be 4 × 1026 Watts of power put out, but that’s spread out over 2.2 × 1025 cubic meters, meaning the sun’s energy output per-unit-volume is just 18 W / m3. Compare this to the average human being, whose basal metabolic rate is equivalent to around 100 Watts, yet takes up just 0.06 cubic meters of space. In other words, you emit 100 times as much energy-per-unit-volume as the sun! It’s only because the sun is so large and massive that its power is so great.

It’s this slow process, releasing huge amounts of energy per reaction over an incredibly large volume, that has powered life on our world throughout its entire history. It may not appear so impressive if you look at just a tiny region, but — at least for our sun — that huge size really adds up!

Check out these “10 Need-to-Know Things About the Sun”: solarsystem.nasa.gov/planets/profile.cfm?Object=Sun.

Kids can learn more about an intriguing solar mystery at NASA’s Space Place: spaceplace.nasa.gov/sun-corona.

This article was provided by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

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Caption: Composite of 25 images of the sun, showing solar outburst/activity over a 365 day period; NASA / Solar Dynamics Observatory / Atmospheric Imaging Assembly / S. Wiessinger; post-processing by E. Siegel.

About NASA Space Place

The goal of the NASA Space Place is “to inform, inspire, and involve children in the excitement of science, technology, and space exploration.” More information is available at their website: http://spaceplace.nasa.gov/

Highlights From Bob Piekiel’s Green Lakes Solar Observing Session, 8 February 2014

Greetings fellow astrophiles,

A decent-sized group of appropriately-dressed observers braved the mid-winter cold to attend a solar observing session at Green Lakes State Park this past Saturday, February 8th (approx. 1 to 3 p.m.). The event, organized by Baltimore Woods favorite Bob Piekiel, was wing-observered by Ryan Goodson, Larry Slosberg, and Steve Capp. Observers were treated to a reasonably busy solar surface, with the massive sunspot 1967 and the small constellation of sunspots around 1968 just disappearing out of the field of view with the Sun’s rotation (and our revolution), then several smaller sunspots working their way across the Sun’s equator (that said, note the Earth size in the image below. Sunspots 1973 and 1974 are large enough to swallow the Earth whole!).

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The Sun on 8 February 2014. Image from NASA/SOHO.

Below is a gallery of images from the event (our first attempt at a CNYO gallery. If you have issues loading images or just don’t like how it works on the site, please let us know) featuring photos by Ryan Goodson and Cindi Farrell. Another session is coming up from 1 to 3 p.m. on February 22 (with the 23rd as the weather alternate) at Baltimore Woods. We hope you can join us for that one as well!


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CNYO Observing Log: Baltimore Woods Solar Session, 24 August 2013

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The gathered crowd at Baltimore Woods.

Greetings fellow astrophiles!

As CNY completes a remarkable span of bright days and clear nights around this year’s Harvest Moon, we finally catch up on our observing logs with a recap of Baltimore Wood’s Solar Session held on an equally bright and clear August 24th.

Despite its importance as the primary reason we and this Solar System are here at all, the Sun often gets neglected by some amateur astronomers who opt out of expensive solar equipment in favor of expensive deep sky equipment. The Sun, like all stars, is a seemingly simple ball of light that reveals great complexity depending on what you use to observe it. Some filters knock down all but 0.001%(ish) of the Sun’s light to provide great Sunspot detail, while other filters let only very specific wavelengths of light through – these filters then providing insights into the surface structure of the Sun based on the excitation of specific atoms on the Sun’s surface or in its corona.

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An observer at a Coronado H-alpha scope.

Despite its close proximity and constant activity, the Sun is just like any other astronomical object – patience is the key to appreciating the view. At low magnification and over only a few minutes, Sunspots and prominences appear to drift slowly, if at all, in the field of view. Changing to high magnification reveals dynamic views around Sunspots as they undulate or merge with other spots, with changes that are apparent to trained eyes occurring over many seconds. Observers with good memories can return to their scopes over several minutes to see very obvious changes to large prominences. While the differences may be subtle to the eye, they are anything but subtle on the Sun. Keeping in mind that 107 Earths fit across the diameter of the Sun, seeing changes to large prominence over the course of minutes means that plasma on the Sun’s surface is racing at dizzying speeds. The drama only seems slow from our safe distance.

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The gathered scopes (and gathering observers).

The two hour session at Baltimore Woods provided ample time to sample both the range of filters and the range of timescales, thanks primarily to the ever well-equipped Bob Piekiel and his Baader, CaK, and H-alpha scopes. To this list of equipment was added Larry Slosberg and his Baader-filtered New Moon Telescope 12″ Dobsonian (the big primary mirror of the session), then myself with a Coronado PST (H-alpha). And speaking of filters (and taken from CNYO’s A Guide For Solar Observing brochure)…

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A solar projecting scope (left) and Larry Slosberg’s Baader’ed NMT Dob.

Baader Filter – The Baader (“Bah-der”) filter works by reflecting 99.999% of all of the incoming light (almost a mirror), leaving you with a pale yellow disk. You’ll see no prominences or fine surface detail, but Baader filters are excellent for observing sunspots.

CaK (Calcium K-line) – The CaK filter lets through a wavelength corresponding to the 393.4 nm Ca K-line transition (you see it as violet). These filters provide excellent surface detail.

H-alpha (Hydrogen-alpha) – This filter lets through a hydrogen electronic transition corresponding to a wavelength of 656.28 nm (you see it as a rich red). H-alpha filters are excellent for prominences and good for surface detail.

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The Sun through different filters (see above).

Thanks to the SOHO (Solar And Heliospheric Observatory) satellite and its website, it is easy to find the Sun’s snapshot on August 24th to see exactly what we were looking at, complete with a week’s worth of images from the days before to see how the positions of Sunspots changed as the Sun’s plasma rotated about its axis (the final image in yellow is the view from the 24th).

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The week before the solar session (images from NASA/SOHO).

Technical details aside, the session was an excellent one, with approximately 30 people enjoying many views of the Sun and all the solar details Bob, Larry, and I could remember. Of specific note was a prominence that started small at the beginning of the session but grew to contain a clear, dark hole more than one Earth diameter wide over only an hour’s time. The fun wasn’t restricted to scope observers, either. With filtered binoculars and simple Baader glasses, the dimmed ball of light itself was just as interesting a target.

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The unmagnified (and nearly unmagnified) view of the Sun through Baader glasses.

While I didn’t hear it mentioned, it is worth noting that the unmagnified (but filtered) Sun appears to be about the same diameter as the unmagnified (and unfiltered) Moon – a point of no small significance during Solar Eclipses. And as the Moon is slipping away from us at a rate of 1.5 inches per year, the Solar Eclipse is also (very, very slowly) becoming a thing of the past in favor of what will become Lunar Transits. All the more reason why it’s a great time to be observing!

I leave you with the most informative 30 seconds on the website (so far). To demonstrate the dangers of observing the Sun without some kind of filter, Bob and Larry set to work reproducing the fabled ship-burning apparatus of Archimedes (also of Syracuse) by burning one sheet of paper and one dark leaf at low magnification. As Bob explains, this same burning would occur on your retina without something to greatly knock down the Sun’s brightness. I even found myself jumping rather anxiously at one intrepid observer trying to look through the eyepiece of Bob’s projecting scope. Solar safety (and eye safety in general) is no joke!

It’s as informative and definitive a video on solar safety as you’ll find on youtube, so feel free to pass the link along to any and all.