A new method for aerosol measurement using wide-field photometry

0550874 - FZÚ 2022 RIV GB eng J - Článek v odborném periodiku
Ebr, Jan - Karpov, Sergey - Eliášek, Jiří - Blažek, Jiří - Cunniffe, Ronan - Ebrová, I. - Janeček, Petr - Jelínek, Martin - Juryšek, Jakub - Mandát, Dušan - Mašek, Martin - Pech, Miroslav - Prouza, Michael - Trávníček, Petr
A new method for aerosol measurement using wide-field photometry.
Astronomical Journal. Roč. 162, č. 1 (2021), č. článku 6. ISSN 0004-6256. E-ISSN 1538-3881
Grant CEP: GA MŠMT EF15_003/0000437; GA MŠMT(CZ) EF18_046/0016007; GA MŠMT EF16_013/0001403; GA MŠMT(CZ) LM2018105; GA MŠMT LTT17006; GA MŠMT(CZ) LG13007
Grant ostatní: OP VVV - CoGraDS(XE) CZ.02.1.01/0.0/0.0/15_003/0000437; OP VVV - CTA-CZ II(XE) CZ.02.1.01/0.0/0.0/18_046/0016007
Institucionální podpora: RVO:68378271 ; RVO:67985815
Klíčová slova: aerosol measurement * wide-field photometry * vertical aerosol optical depth (VAOD) * CCD camera with a photographic lens
Obor OECD: Particles and field physics; Particles and field physics (ASU-R)
Impakt faktor: 5.491, rok: 2021
Způsob publikování: Open access

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 s 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 the 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 the details of stellar photometry and modeling of the dependence of the measured stellar flux, the star color, and the position within the field of view. The results obtained with robotic setups at the future sites of the Cerenkov Telescope Array show good internal consistency and agreement with simultaneous measurements from a Sun/Moon photometer located at the same sites.
Trvalý link: http://hdl.handle.net/11104/0326188