arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2101.03074astro-ph.IMhep-exphysics.ao-ph
收藏

一种利用宽视场Photometry测量气溶胶的新方法

A New Method for Aerosol Measurement using Wide-field Photometry

Jan Ebr, Sergey Karpov, Jiří Eliášek, Jiří Blažek, Ronan Cunniffe, Ivana Ebrová, Petr Janeček, Martin Jelínek, Jakub Juryšek, Dušan Mandat, Martin Mašek, Mirosl… 展开作者

Jan Ebr, Sergey Karpov, Jiří Eliášek, Jiří Blažek, Ronan Cunniffe, Ivana Ebrová, Petr Janeček, Martin Jelínek, Jakub Juryšek, Dušan Mandat, Martin Mašek, Miroslav Pech, Michael Prouza, Petr Travníček

摘要:

提出了一种利用宽视场成像仪--一台安装在赤道架上的带摄影镜头的CCD相机测量晴朗夜晚气溶胶垂直光学厚度的新方法。在地平线以上的不同高度拍摄的一系列30秒曝光可以用于在几分钟内测量VAOD,其精度优于0.008光学深度。这种测量不产生任何光,因此适合在其他天文仪器所在的地点使用。VAOD测量的精度取决于实验室校准的光谱特性的系统和相机的电子设备的响应,以不同的照明水平,以及仔细考虑的细节恒星测光和建模的依赖性测得的恒星通量恒星颜色和位置的视野内。在切伦科夫望远镜阵列的未来站点与机器人设置获得的结果显示出良好的内部一致性和协议,同时测量从太阳/月球光度计位于同一地点。

英文摘要:

We present a new method to measure the vertical aerosol optical depth (VAOD) during clear nights using a wide-field imager - a CCD camera with a photographic lens on an equatorial mount. A series of 30-second exposures taken at different altitudes above the horizon can be used to measure the VAOD with a precision better than 0.008 optical depths within a few minutes. Such a measurement does not produce any light and is thus suitable for use at sites where other astronomical instruments are located. The precision of the VAOD measurement depends on laboratory calibration of spectral properties of the system and of the response of the camera electronics to varying illumination levels, as well as careful considerations of details of stellar photometry and modelling of the dependence of measured stellar fluxes star color and position within the field of view. The results obtained with robotic setups at the future sites of the Cherenkov Telescope Array show good internal consistency and agreement with the simultaneous measurements from a Sun/Moon Photometer located at the same site.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑