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What can be expected with solar filters?
Hi all.
After geting strong advice from s.a.a not to risk the telscope and eyepice on solar projection, I would like to check out solar filters to be mounted in front of the telescope objective. From what I understand, there are at least two types of filters. The first is one that merely reduces the amount of light that enters the telescope. The example pictures I have seen essentially show the solar disc with some sun spots. Some people I have talked to, said that these types of filters were very popular (in terms of sold units) just before eclipses. Now, we just had an eclipse a couple of months ago, and I don't know when the next is to be expected. I have seen some mentioning of "Hydrogen Alpha" filters, that only let specific parts of the hydrogen spectrum through. There is some vague mentioning of these filters being "expensive!", but, on the other hand, there may be way more detail to be seen on the sun than with the more ordinary filters. The prospect of watching the sun almost every day, to get an impression of the dynamics of the sun, does have a stronger appeal to me than merely having a quick look every eclipse or so. All of this put the following questions to mind: - What types of details can one expect to see with Hydrogen Alpha filters that don't appear with the "ordinary" filters? I have the impression protuberances and surface granularity would be visible. What about flares? Other details? Would one see dynamic features i.e. instant movement on the surface as opposed to sunspot positions that change over hours and days? The telescope in question is of 80 mm aperture with a 20-60x eyepiece. - How much more expensive are the Hydrogen Alpha filters than ordinary ones? 2 times? 10 times? Any opinions much appreciated. Rune |
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What can be expected with solar filters?
Hi there. You posted:
What types of details can one expect to see with Hydrogen Alpha filters that don't appear with the "ordinary" filters? I have the impression protuberances and surface granularity would be visible. What about flares? Other details? Would one see dynamic features i.e. instant movement on the surface as opposed to sunspot positions that change over hours and days? There is a *huge* difference between the views in white light (ie: ordinary broad-band solar filters) and those in a sub-angstrom H-alpha filter (passband of less than one Angstrom in width). In white light, you can see sunspots and some brighter patches on the disk toward the limb known as faculae, but that's about it. Its fun to watch and relatively inexpensive, so white-light filters are pretty popular. However, in H-alpha, you are viewing the thin layer of the sun's atmosphere known as the Chromosphere. On the limb, you will see the gigantic streamers of gas known as prominences while, on the disk, the prominences become dark and are known as "filaments". You will also see a mass of fine fibril detail on the disk, as well as brighter patches known as "plage" seen around active regions. Sunspots can be visible as well, but there is a great deal of detail around them which is not visible in white light filters. The surface is in almost constant turmoil and with careful study, small-scale changes can easily be noticed in only a few minutes. Solar flares are visible in H-alpha filters as well (not usually seen in white light), and some move quite rapidly so that you can actually see things move in a few minutes time. I have seen some solar flares erupt in only a few *seconds* of time, and they are a lot of fun to watch. Some of these events are quite spectacular, so the views you may have seen in some H-alpha movies are not far off from what is seen viewing with the eye. If you want to compare the view in H-alpha to that of white light, go to the web page of Big Bear Solar Observatory http://www.bbso.njit.edu and click on the "Latest Images". They also have "live" images in H-alpha which are updated every few minutes when the sun is up over Big Bear, California. The telescope in question is of 80 mm aperture with a 20-60x eyepiece. - How much more expensive are the Hydrogen Alpha filters than ordinary ones? 2 times? 10 times? A good 80mm "white light" solar filter might run you something like $40 to $60 and is well worth the money. An H-alpha filter with an 80mm aperture will run you considerably more than this even if you use one which is quite small like the SolarMax 40mm model, which is around $1250. There are two companies which currently market decent H-alpha filters (ie: those with bandwidths of less than one Angstrom, which is required to see much on the disk). These are DayStar Filters and Coronado. The DayStar filters can be somewhat less expensive, but require *long* focal length telescopes to work properly (f/ratios of f/30 or longer). The least expensive of the DayStar line of filters (the T-Scanner) starts at around $1600, not including the energy rejection filter which has to be mounted in front of the objective. I have used my T-Scanner for about 17 years and I really enjoy it. The Coronado filters are a bit simpler and will work at almost any focal length, although again, if you want any significant aperture, the price is rather high (their 60mm model is over $2500 and their 90mm aperture model is over $5000). These filters also take a while to make, so if you are considering getting an H-alpha filter, be prepared for a wait which can last months. For those who are interested solar observing in Hydrogen-alpha light, check out the on-line publication: OBSERVING THE SUN IN H-ALPHA, available on the Web page of the Prairie Astronomy Club: http://www.prairieastronomyclub.org It is a guide containing a useful intoduction to observing equipment and techniques, coupled with a comprehensive look at the terminology and behavior of solar H-alpha features which the amateur might see. The information was compiled from the text ASTROPHYSICS OF THE SUN by Harold Zirin (Cal. Tech), and provides a review of features such as Prominences H-alpha disk detail, H-alpha sunspot development and behavior, solar activity, and solar flares. The guide also contains a glossary of the most common H-alpha terms used by many observers. For those who do not have H-alpha equipment but still want to follow the sun's activity, these web sites provide quality images and information. "EYES ON THE SKIES" ROBOTIC SOLAR TELESCOPE OBSERVATORY: http://sunmil1.uml.edu/eyes/index.html This site is run by amateur astronomer Mike Rushford, and produces "Live" H-alpha images with a small solar scope and a sub-angstrom filter. The scope produces medium to high resolution images, and can be moved by the user, with changable image parameters. Since it is only one site (California), there will be times when no images will be present due to weather conditions. There is also a limited archive of interesting movies and images of H-alpha solar activity. In addition, an extensive solar observing FAQ is provided, covering equipment and some solar terms. Astro-USON WebTV Observatorio "CarlSagan" (Sonora, Mexico) http://cosmos.astro.uson.mx/webtv/webtv.htm Live high-resolution (754x487 pixels) images from a 125 mm aperture f/10 Catadioptric telescope using a 0.6 Angstrom H-alpha filter are provided from this Mexican site, including occasional longer exposures on the limb to provide better coverage of limb prominences and activity (it is helpful if you can read Spanish, although you can still get around without knowing the language). The schedule is Monday through Saturday from 15 hrs to 22 hrs UTC weather permitting. BIG BEAR SOLAR OBSERVATORY (BBSO) http://www.bbso.njit.edu/ Big Bear provides high resolution (up to 2024 x 2024 pixels) full-disk images of the sun in both white light and H-alpha, along with current information on solar activity. They also provide their "live" moderate resolution images (updated about every minute) along with a plot of current solar X-ray emission. However, since this is only one observatory, and is mainly a research facility, there will be times when images will not be updated due to weather conditions or research projects. In addition, Big Bear is part of the Global H-alpha Newtwork, so at least a few images may be available when the sun is not up over Big Bear. They provide a wealth of information concerning active region history, location, type, and current level of activity, which is very useful for keeping track of things when you can't observe every day. Big Bear also has an extensive archive of images and movies (including a "daily movie" when it was clear at the observatory) which demonstrate some interesting solar phenomenon. NATIONAL SOLAR ASTRONOMY OBSERVATORY http://www.sunspot.noao.edu/ This site provides "near-live" full-disk medium resolution images of the sun in H-alpha updated every few minutes, and solar images in Calcium and white light every ten minutes from the National Solar Astronomy Observatory at Sunspot, New Mexico. These images are of somewhat higher resolution than those from the Space Environment Laboratory, but are not as high as those from sites like BBSO or the "Eyes on the Skies" telescope. In addition, archived images and movies of solar activity are available, along with information on solar activity and useful links. SPACE ENVIRONMENT CENTER http://www.sel.noaa.gov/ This site is probably the best one for complete information on current and future solar/terrestrial conditions and activity. They provide lower-resolution "colorized" full-disk H-alpha images several times per day from observing sites in New Mexico and Australia, along with selected higher resolution active region images. There is also an extensive archive of past images and information, along with a glossary of solar terms. Clear skies to you. -- David W. Knisely Prairie Astronomy Club: http://www.prairieastronomyclub.org Hyde Memorial Observatory: http://www.hydeobservatory.info/ ********************************************** * Attend the 10th Annual NEBRASKA STAR PARTY * * July 27-Aug. 1st, 2003, Merritt Reservoir * * http://www.NebraskaStarParty.org * ********************************************** |
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