Results From Observations Taken During The Total Solar Eclipse of 2006

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Using the Multi-Aperture Coronal Spectrometer (MACS) we measured the K-coronal spectrum in the visible wavelength range at multiple locations in the low solar corona during the total solar eclipse, which occured on 29 March 2006 In Libya. The purpose of these measurements was to obtain the thermal electron temperature, and its flow speed at those locations. The observed K-coronal spectrum was matched with models to obtain the best fit to the data. These observations could be easily performed from a space-based platform to produce global maps of the electron density, temperature, and flow speed at the base of the solar wind.

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