RTT150 high resolution spectral observations of Solar Corona during the solar eclipse on March 29, 2006

Details RTT150 high resolution spectral observations of Solar Corona during the solar eclipse on March 29, 2006 RTT150 high resolution spectral observations of Solar Corona during the solar eclipse on March 29, 2006

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..782....1b&link_type=abstract

The Astronomer's Telegram, #782

Astronomy and Astrophysics

Astronomy

Optical, The Sun

Scientific paper

On March 29, 2006, the total solar eclipse had a duration of totality of about 2 minutes at TUBITAK National Observatory, Antalya, Turkey. The Russian-Turkish 1.5-meter optical telescope (RTT150) equipped with a coude-echelle spectrometer and a 1040 x 1160 pixels nitrogen cooled CCD was used to get the spectra of solar Corona. We have obtained two high-resolution, high S/N spectra of a small region of the solar Corona situated approximately 3 arcmin Eastwards of the solar limb, with coordinates R.A.(2000.0) = 00h 32m 37s, Dec.(2000.0) = +03o 23' 55".

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