Astronomical site selection: on the use of satellite data for aerosol content monitoring

Varela, A. M.; Bertolin, C.; Muñoz-Tuñón, C.; Ortolani, S.; Fuensalida, J. J.
Bibliographical reference

Monthly Notices of the Royal Astronomical Society, Volume 391, Issue 2, pp. 507-520.

Advertised on:
12
2008
Number of authors
5
IAC number of authors
3
Citations
27
Refereed citations
22
Description
The main goal of this work is to analyse new approaches to the study of the properties of astronomical sites. In particular, satellite data measuring aerosols have recently been proposed as a useful technique for site characterization and searching for new sites to host future very large telescopes. Nevertheless, these data need to be critically considered and interpreted in accordance with the spatial resolution and spectroscopic channels used. In this paper, we have explored and retrieved measurements from satellites with high spatial and temporal resolutions and concentrated on channels of astronomical interest. The selected data sets are the Ozone Monitoring Instrument on board the NASA Aura satellite and the Moderate Resolution Imaging Spectroradiometer on board the NASA Terra and Aqua satellites. A comparison of remote-sensing and in situ techniques is discussed. As a result, we find that aerosol data provided by satellites up to now are not reliable enough for aerosol site characterization, and in situ data are required.
Related projects
Project Image
Starbursts in Galaxies GEFE

Starsbursts play a key role in the cosmic evolution of galaxies, and thus in the star formation (SF) history of the universe, the production of metals, and the feedback coupling galaxies with the cosmic web. Extreme SF conditions prevail early on during the formation of the first stars and galaxies, therefore, the starburst phenomenon constitutes a

Casiana
Muñoz Tuñón