A new astronomical parameter from remote sensing data: Astronomical clearness index (ACI)
-
Published:2021-06-30
Issue:1
Volume:63
Page:58-79
-
ISSN:1303-6009
-
Container-title:Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering
-
language:en
-
Short-container-title:Commun.Fac.Sci.Univ.Ank.Series A2-A3: Phys.Sci. and Eng.
Author:
KABA Kazım1ORCID, YEŞİLYAPRAK Cahit1ORCID, ŞATIR Onur1ORCID
Abstract
Eastern Anatolia Observatory (DAG) project was initiated in Erzurum/Turkey in 2011. DAG will have Turkey’s largest (4 m) and first infrared telescope. The installation process is planned to be by taking its first light in the end of 2021. This study was focused on a new analysis method about the atmospheric properties of DAG site in terms of the cloudiness as known the most vital atmospheric parameter for ground-based astronomical observatories. In this regard, the cloudiness for DAG site is comprehensively examined using the “Cloud Mask” (CMa) and “Cloud Type” (CT) products from Satellite Application Facility on Support to Nowcasting and Very Short-Range Forecasting (NWC SAF). Firstly, the cloudiness and the cloud types over DAG site were determined. Secondly, NWC SAF CMa and CT data have been redefined for astronomical purposes, and the pixel values/meanings in CMa and CT images have been reduced from 6 to 4 and from 21 to 4 pixels, respectively. Thirdly, these new data were used to define a new index named as “Astronomical Clearness Index” (ACI), and finally, the observable days for DAG site were determined using this newly defined index.
Funder
TÜBİTAK ve Atatürk Üni, Astrofizik Araştırma ve Uygulama Merkezi
Publisher
Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering
Reference19 articles.
1. McInnes, B., Walker, M.F., Astronomical site testing in the Canary Islands, Publications
of the Astronomical Society of the Pacific, 86 (512) (1974), 529-544.
https://doi.org/10.1086/129641 2. Calisse, P.G., Ashley, M.C.B., Burton, M.G., Phillips, M.A., Storey, J.W.V., Radford,
S.J.E., Peterson, J.B., Submillimeter site testing at Dome C, Antarctica, Publications of
the Astronomical Society of Australia, 21 (3) (2004), 256-263.
https://doi.org/10.1071/AS03018 3. Schöck, M., Els, S., Riddle, R., Skidmore, W., Travouillon, T., Blum, R., Bustos, E.,
Chanan, G., Djorgovski, S. G., Gillett, P., Gregory, B., Nelson, J., Otárola, A., Seguel, J.,
Vasquez, J., Walker, A., Walker, D., Wang, L., Thirty meter telescope site testing I:
overview, Publications of the Astronomical Society of the Pacific, 121 (878) (2009), 384-
395. https://doi.org/10.1086/599287 4. Vernin, J., Muñoz-Tuñón, C., Sarazin, M., Vazquez Ramió, H., Varela, A.M., Trinquet,
H., Delgado, J.M., Jiménez Fuensalida, J., Reyes, M., Benhida, A., Benkhaldoun, Z.,
Garcia Lambas, D., Hach, Y., Lazrek, M., Lombardi, G., Navarrete, J., Recabarren, P.,
Renzi, V., Sabil, M., Vrech, R., European extremely large telescope site characterization
I: overview, Publications of the Astronomical Society of the Pacific, 123 (909) (2011),
1334-1346. https://doi.org/10.1086/662995 5. Hidayat, T., Mahasena, P., Dermawan, B., Hadi, T. W., Premadi, P. W., Herdiwijaya, D.,
Clear sky fraction above Indonesia: an analysis for astronomical site selection, Monthly
Notices of the Royal Astronomical Society, 427 (3) (2012), 1903-1917.
https://doi.org/10.1111/j.1365-2966.2012.22000.x
|
|