Solar Radius Determination from Total Solar Eclipse Observations on 29 March 2006 |
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Authors: | A Kilcik C Sigismondi J P Rozelot K Guhl |
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Institution: | 1.Faculty of Art and Science Department of Physics,Akdeniz University,Antalya,Turkey;2.ICRA International Center for Relativistic Astrophysics,Sapienza University of Rome,Rome,Italy;3.Fizeau Dept.,Université de Nice Sophia-Antipolis,Nice,France;4.Fizeau Department, OCA-CNRS UMR 6225,Université de Nice Sophia-Antipolis,Grasse,France;5.Archenhold Sternwarte, Berlin,IOTA/ES International Occultation Timing Association, European Section,Berlin,Germany |
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Abstract: | 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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Keywords: | Sun: activity Sun: diameter Sun: eclipses |
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