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March 24th 2012
The LS230T are shipping.

Stephen Ramsden’s Corner

Outreach, Imaging, and Reviewsbr>

Thanks Stephen for all your hard work.

Image of the week

Here is the Solar Image of the Week.
Thanks to: Howard
Lunt Solar CaK Filter

A very nice image from Florida.

Real Time Images: The Very Latest from SOHO

SOHO, the Solar & Heliospheric Observatory, is a project of international collaboration between ESA and NASA to study the Sun from its deep core to the outer corona and the solar wind.

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Open discussion forum regarding Solar equipment. A great place to ask questions.

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Lunt Solar Image Gallery
Visit this link to enter our image gallery area. View images by product.

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Lunt Solar Systems will be attending NEAF 2012.

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The Sun is our Star!

.......and as you would expect, our Star is hot, bright, dynamic, and sometimes quite violent.

At 93 million miles away, we are ideally placed at a point where the Sun provides just enough warmth and energy essential to our living planet, Earth.
At only 93 million miles, the Sun is close enough for us to view it's surface thru a relatively inexpensive scope from the comfort and relative safety (Sunscreen please) of our backyards on a clear and warm day.

What! Astronomy during the day? Lunt Solar wants to show you how.

References

Prominences:
These look like eruptions from the edge of the Solar disk. Prominences can be small spikey looking details, or large cloud-like detail with fine feather-like features.

They are, in fact, ionized Hydrogen-alpha emissions being projected from the linb.

Prominences are anchored to the Sun's surface in the Mesosphere, and extend outward into the Sun's Troposhere.
They typically measure many earth diameters.

Filaments:
These are strin-like features on the surface of the Sun.

At high resultion they take on a 3D effect due to the coller aspect of the suspended filament contrasted against the bright, hotter Sun.

They are actually prominences being viewed against the surface.

Spicules
A Spicule is a dynamic jet of gas about 500km long.
They move outward at about 20km/second thru the Chromosphere.

Father Angelo Secchi of the Vatican Observatory discovered them in 1877.

The Chromosphere is entirely composed of Spicules. These features can be seen as "fur"around the edge of the disk.


There's definately stuff to look at :)

Archive for the ‘Star Parties’ Category

June 17th, 2010

Author: Kevin LeGore

The Grand Canyon Star Party (GCSP), one, if not the largest public outreach star party in the United States.  Every year in June this massive annual event takes place at Yavapai Point on the south rim of the Grand Canyon and at the North Rim Lodge on the Grand Canyon’s northern rim.  This event offers astronomers a chance to enjoy a week of some of Arizona’s most beautiful scenery and skies; also being able to share it with others from all over the world.

During the evenings of the week-long event telescopes are aimed at all kinds of objects from galaxies to the bright planets; thousands of people with questions about the sky and the things they see in the telescopes.

But what about during the day?  After all this is a week-long event?  For most astronomers they are busy sleeping, preparing for the next nights crowds, but for some they taking advantage of the day time to inform people about the nights events.  Some use their powerful binoculars and small refractors to point out wonders in the Canyon, others spend time showing the public Venus and the Moon during the day, and then some spend time observing the sun!

This year the GCSP had a new addition to the day time events, an Lunt LS100T-Ha. At an elevation of nearly 7000 feet above sea level the seeing at the Canyon is normally very nice, this could be seen with the LS100T.  The Pressure Tuner performed beautifully at such a high elevation!  The views were sharp and packed with detail, one astronomer said, “The scope has resolution with a capital R”! Many astronomers were eager to sneak a peak through the monster solar scope, a scope such as this is rarely ever seen at the GCSP.

But the real reason for the LS100T was to use it for public outreach as this is what the GCSP is all about!  Over the four days I was present at the star party nearly 700 people viewed the sun!  Passer by were in awe of the prominences lifting off the sun’s surface and the explosive views of active regions!  While some were a bit hesitant to view, others jumped at the chance to take a glimpse at the sun, some even getting back in line to view again.  Some even tried their had at some  photography, leaving with some rather impressive shots of the prominences!  Towards the weeks end the weather became iffy, low temperatures and chances of rain but I still managed to get people a view of the sun!

All in all it was a great event, the views were incredible through the scope.   The coordinator of the GCSP south rim, Jim O’ Connor, called the LS100T a “solar masterpiece” on one of his Cloudy Nights posts, him and many others were all very impressed with the scope.  It was a joy to use as well and a great public outreach tool!

About Lunt Solar Systems LLC…

Lunt Solar Systems is a manufacturing and sales facility located in Tucson, Arizona. Lunt Solar design, fabricate, assemble, and test solar telescopes and solar filters. Whether you are looking for a dedicated solar telescope or a solar filter for attachment to you own astronomy telescope, we can help. Solar telescopes models start at $499 for an LS35T (telescope) or the only slightly more expensive LS50F (filter), all the way thru the 152T and the 160F. Solar observing is both fun and educational. Don’t miss out on Solar Maximum. Feel free to contact us with question or comments and we’d be happy to help.

Lunt Solar Systems LLC

2520 N. Coyote Drive
Suite 111
Tucson AZ 85745

luntsolarsystems.com

Telephone: 1-877-344-7348
Telephone: 520-344-7348
Fax: 520-344-7352
e-mail: sales@luntsolarsystems.com