Go Out: Look Up!A Guide to the Sky, Telescopes, and Telescope Programs |
Looking at the SunFirst, never look at the sun without an appropriate filter in place. Instant and permanent eye damage can occur. Solar Astronomy is by far the easiest way to connect to the universe in a school setting. It takes only a few minutes, it’s not after school, nor past anyone’s bedtime. A bright sky in an urban setting is no hindrance.. Sure, there is only one thing to look at, but it’s different every day. It’s dynamic. It moves. It rotates a bit every day. With a Hydrogen-alpha solar telescope, you can watch the Sun’s weather. Over the course of a week you can see a loopy solar prominence or flare transit across the face of the sun to become a prominence on the other side. Much like a beautiful sunset makes you feel really blessed to witness the beauty of nature, watching a big storm playing out over a the face of the Sun does make you feel like you’re connected to something big. The universe itself reveals itself to be alive and dynamic. All this can be experienced in a couple of minutes any time the sun is visible. There are two common types of Solar Observing available to the amateur: White Light and Hydrogen-alpha. White LightPros: White-light Solar Filters for your telescope are cheap (anywhere from $30 to $100 for small to medium scopes), Sunspots are easy to see with them.
The cons of detachable solar filters is that if they detach while you're viewing them (unlikely, but not inconceivable) eye damage will occur. For telescope programs, this is a liability to be weighed heavily. For school programs for younger children, presenting habit of looking at the sun may task their judgment too heavily. Another alternative is a special diagonal called a Hershel Wedge, which safely eliminates the excess radiation and can be used immediately on just about any refractor or SCT telescope. Sunspot info is updated daily at: http://spaceweather.com/ Hydrogen-AlphaHydrogen-Alpha is a very specific wavelength of light. Blocking out all other wavelengths of light allows us to see a very active region of the sun. In addition to sunspots, bright Active Regions and Prominences are visible (see the photo at the top of this page). Prominences are loops and flares of gas extending outward from the surface of the sun. They are bright when backed by dark space. When a prominence is in front of the sun's disk they instead resemble dark threads and feathers. This is because, while hot, they are cooler and darker than the sun's surface. Watching the sun of the course of a week, you can see prominences on the eastern limb of the sun become filaments and the re-emerge as a prominence on the western limb. Some cool solar photos and info is at: http://sdo.gsfc.nasa.gov/ Live H-alpha shots are at http://halpha.nso.edu/ Observing goals can include
|
| Here's a
Coronado PST Hydrogen-Alpha scope mounted on a
8" dobsonian (Orion XT8i) fitted with a white-light mylar filter.
While not at all sophisticated, this setup allows switching between white light and h-alpha by simply moving your head. The white-light filter material cost $35 and the cell (allowing the filter to be mounted on the telescope was home-made from cardboard). While not recommended (due to air turbulence which can blur the views), you can observe the sun from indoors (here a sliding-glass door is open).
Always use appropriate filters! |
|
|
Questions or comments? Email:Jeff Martin |