Solar Radius Determination from Total Solar Eclipse Observations on 29 March 2006

Details Solar Radius Determination from Total Solar Eclipse Observations on 29 March 2006 Solar Radius Determination from Total Solar Eclipse Observations on 29 March 2006

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009soph..257..237k&link_type=abstract

Solar Physics, Volume 257, Issue 2, pp.237-250

Physics

4

Sun: Activity, Sun: Diameter, Sun: Eclipses

Scientific paper

Solar diameter measurements have been made nearly continuously through different techniques for more than three centuries. They were obtained mainly with ground-based instruments except for some recent estimates deduced from space observations. One of the main problems in such space data analysis is that, up to now, it has been difficult to obtain an absolute value owing to the absence of an internally calibrated system. Eclipse observations provide a unique opportunity to give an absolute angular scale to the measurements, leading to an absolute value of the solar diameter. However, the problem is complicated by the Moon limb, which presents asphericity because of the mountains. We present a determination of the solar diameter derived from the total solar eclipse observation in Turkey and Egypt on 29 March 2006. We found that the solar radius carried back to 1 AU was 959.22±0.04 arcsec at the time of the observations. The inspection of the compiled 19 modern eclipses data, with solar activity, shows that the radius changes are nonhomologous, an effect that may explain the discrepancies found in ground-based measurements and implies the role of the shallow subsurface layers (leptocline) of the Sun.

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