On the base of the top-of-atmosphere radiance calculations carried out with the use of an isotropic version of the CoxMunk model of sea surface slopes distribution and the Sobolev model of light scattering in the atmosphere, the sun glint quantitative characteristics such as its length, maximal width and maximal contrast are presented for measurements of scanning satellite instruments in the visible and near-infrared ranges from 0.4 to 1.6 μm for sea wind speeds from 2 to 14 m/s and atmospheric aerosol optical thicknesses from 0.03 to 0.33.
Access to the requested content is limited to institutions that have purchased or subscribe to SPIE eBooks.
You are receiving this notice because your organization may not have SPIE eBooks access.*
*Shibboleth/Open Athens users─please
sign in
to access your institution's subscriptions.
To obtain this item, you may purchase the complete book in print or electronic format on
SPIE.org.
INSTITUTIONAL Select your institution to access the SPIE Digital Library.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.