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Download Solar Instruments for Observing the Sun for Amateurs
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Solar Instruments for Observing the Sun David Groski Mt Cuba Observatory •Why Observe The Sun ? It is the only Star were we can directly observe the surface The Sun is very Dynamic. Surface features can change in as little as a few minutes Observation can be used to explain a number of concepts in Physics, Chemistry and Astrophysics The Sun directly effects us. It’s WARM and Sunny in the daytime ! Safety ! The Sun is bright ! Magnitude -23 Never leave your telescope unattended Cap the finder scope Make sure your filters are secularly attached The Filter needs to reduce the brightness by 10,000 to 1 across the FULL spectrum How To Observe the Sun Projection White Light Filters Color Filters Dedicated telescope Coronagraph Narrow Band Filter Spectroscopic Projection The Simplest Fairly Safe Gives Good Resolution Use with Apertures of 4” or less Don’t use with Expensive eyepieces ! Don’t use with SCT or Maks ! White Light Filters Metalized Film Safe Gives an excellent image for money Can be used with any type of telescope Can be used at the full aperture of the telescope White Lights Filters Herschel Wedge Gives Excellent Image, better then Film Needs to used with telescopes of 4” or less Needs additional Filtration Some Safety Concerns Color Filters Colored Filters Must be Used with Additional Filter Green filters like Wratten #58 used to improve Sunspot Detail Blue filters used improve faculae Also can improve general image sharpness by narrowing the spectrum Dedicated Solar Telescope Designed to give the best possible image Built in Safety Uncoated Primary, Secondary and Herschel Wedge Easily Tune the brightness by the use of crossed Polarized Light Coronagraph (Promscope) Blocks the Disk of Sun Greatly reduces stray light Gives the best views of Prominences Narrow Band filters For H-alpha need below 1 Angstrom ( 1 x 10^-10 meters) For Calcium K need below 10 Angstroms Usually Expensive ($500 to $10,000) Spectroscopic Shows 100’s of absorption lines Was used to observe Prominences without an Eclipse Helium was discovered on the Sun before being found on the Earth Zeeman effect used to determine the magnetic fields of Sun spots