Measurement of Aureole and Suppression of Internal Stray Light of Aureole Photometer

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• 作者：Nian-Ping Liu¹ ;   ; ² ; Yu Liu¹ ;   ; ^{lyu@ynao.ac.cn} ; Yun-Deng Shen¹ ;   ; ² ; Xue-Fei Zhang¹ ; Wen-Da Cao³ ; Jean Arnaud⁴
• 关键词：instrumentation ; photometers ; sun ; corona
• 刊名：Chinese Astronomy and Astrophysics
• 出版年：2011
• 出版时间：October-December 2011
• 年：2011
• 卷：35
• 期：4
• 页码：428-438
• 全文大小：423 K

文摘

A modern aureole photometer (AP) was developed for the site survey inWest China, in preparation for the installation of future large solar equipments. The performance of this new AP was tested in preliminary observations, and a lot of sky brightness data were accumulated at a few sites in Yunnan Province. The result of data analysis shows that the aureole near the noon time on Jiaozi Snow Mountain is as low as a few millionths of the intensity at the solar disk center, indicating the low internal stray light level of our instrument. The internal stray light of the AP comes mainly from two parts: the edge diffraction of the ferrule for fixing the ND4 filter in the front end of the telescope tube, causing the stray light distributed in the inner region of the field of view, and the edge diffractions of the diaphragms placed inside the telescope tube, causing the stray light distributed in the outer region of the field of view. In order to suppress the stray light of the latter part, the experiment to change the aperture size of an additional diaphragm was performed. The result shows that the stray light in the outer region of the field of view can be effectively suppressed by reducing properly the aperture size of the diaphragm.