Abstract:
We have obtained Fabry-Perot Interferograms of the solar corona during the 1995 total solar eclipse, in two emission lines, Fe X line at 6374Å and Fe XIV line at s303 Å.
We have also obtained a Fabry-perot-gram of the corona in the high temperature Ca XV Å line at 569 4 nm. The Co. XV FP-gram showed two concentrated blobs of emission from the equatorial regions of the Sun.