Night Sky Brightness at Sites from DMSP-OLS Satellite Measurements
From: Joseph Lazio (jlazio_at_adams.patriot.net)
Date: 06/29/04
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Date: 29 Jun 2004 18:32:51 -0400
This paper appeared recently on astro-ph, and I thought that some in
this group might find it interesting:
Paper: astro-ph/0406610
Date: Mon, 28 Jun 2004 01:25:31 GMT (385kb)
Title: Night sky brightness at sites from DMSP-OLS satellite measurements
Authors: Pierantonio Cinzano (1,2), Cristopher D. Elvidge (3) ((1) Dipartimento
di Astronomia, Padova, Italy, (2) Istituto di Scienza e Tecnologia
dell'Inquinamento Luminoso (ISTIL), Italy, (3) NOAA National Geophysical Data
Center, Boulder, USA)
Comments: 14 pages, 12 figures, accepted for publication in MNRAS, 17 june 2004
\\
We apply the sky brightness modelling technique introduced and
developed by Roy Garstang to high-resolution DMSP-OLS satellite
measurements of upward artificial light flux and to GTOPO30 digital
elevation data in order to predict the brightness distribution of the
night sky at a given site in the primary astronomical photometric
bands for a range of atmospheric aerosol contents. This method, based
on global data and accounting for elevation, Earth curvature and
mountain screening, allows the evaluation of sky glow conditions over
the entire sky for any site in the World, to evaluate its evolution,
to disentangle the contribution of individual sources in the
surrounding territory, and to identify main contributing sources. Sky
brightness, naked eye stellar visibility and telescope limiting
magnitude are produced as 3-dimensional arrays whose axes are the
position on the sky and the atmospheric clarity. We compared our
results to available measurements.
\\ ( http://arXiv.org/abs/astro-ph/0406610 , 385kb)
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