Mathematical analysis of temperature results of the total solar eclipse in China on 22 July 2009

Physics

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The paper is on mathematical analysis of the measured temperature values obtained during the total solar eclipse in China on 22 July 2009. A group from the Slovak Central Observatory (SCO), in co-operation with Bulgarian experts, observed this eclipse right next to its central line, close to Shanghai. As a result of these observations, we got data from three different sources and six measuring points, including temperature data taken at different heights and also under the ground level. We received details on air humidity during the phenomenon. Following the analysis of the total solar eclipse in Turkey 2006, we have examined the relation between the measured temperature values and the area of the visible arc of the Sun during the solar eclipse. We have determined key functions like the temperature as a function of time, and the area of the visible solar arc - under the partial sections of the solar eclipse - as a function of time. We have compared the coherent functions, and examined the process of the temperature change. We also paid attention to humidity changes during the phenomenon as a function of time, compared with the coverage of the Sun. We present the details of the analysis including the derived functions, pre- and final results. We draw conclusions from the results of our examination and confront them with the results of past solar eclipses. The results are the product of the Hungarian (NYME-SEK) and Slovak (SCO) cooperation.

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