Solar and stellar measurements using accurate spectroscopic techniques
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چکیده
We propose to use low-cost optics equipment in order to (1) generate a Hertzsprung-Russell diagram for the 24 brightest stars visible in Beaumont, (2) analyze the polarization of stellar and solar light and the effect a telescope's optics have on these measurements, and (3) analyze the absorption spectrum due to Earth’s atmosphere on the Sun’s blackbody radiation spectrum.
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