Electron Temperature Maps of Low Solar Corona: Results from the Total Solar Eclipse of 29 March 2006 in Libya

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Scientific paper

We conducted an experiment in conjunction with the total solar eclipse of 29 March 2006 in Libya that measured the coronal intensity through two filters centered at 3850 and 4100 Angstroms with bandwidths of 40 Angstroms. The purpose of these measurements was to obtain the intensity ratio through these two filters to determine the electron temperature. The instrument, Imaging Spectrograph of Coronal Electrons (ISCORE), consisted of an 8-inch f/10 Schmidt Cassegrain telescope with a thermoelectrically cooled CCD camera at the focal plane. Results show temperatures of 105 K close to the limb to 3 MK at 1.3 solar radii. In the poster we describe this novel technique, and we compare our results to other relevant measurements. This technique could be easily implemented on a space-based platform using a coronagraph to produce global maps of the electron temperature of the solar corona.

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