Tor Vergata Earth Observation Laboratory
 

Improving satellite antenna temperature estimation
by high-resolution emission model of the Earth

G. Schiavon, P. Ferrazzoli, L. Guerriero, R. Jørgensen, S. Badessi, P. de Maagt, and H. Fenech

 


Abstract

This paper describes the recent results of a study aimed at accurately determining the antenna noise temperature used to calculate uplink G/T for satellite-borne receivers. The antenna noise temperature is calculated from a brightness temperature database of the Earth which, for each surface pixel (I deg x 1 deg). includes the effects of season, observation angle and frequency. Good correlation has been found by comparison with In-Orbit Test (IOT) measurements


Index Terms - Microwave emission uplink satellite antenna temperature brightness database

This paper appears in: Antennas and Propagation Society International Symposium, 1999. IEEE
Publication Date: Aug 1999
Volume: 3, On page(s): 2174-2177 vol.3
Meeting Date: 07/11/1999 - 07/16/1999
Location: Orlando, FL, USA
ISBN: 0-7803-5639-x
References Cited: 5
INSPEC Accession Number: 6489700
Digital Object Identifier: 10.1109/APS.1999.788393

© 1999 IEEE. Personal use of this material is permitted. However, permission to reprint/republish this material for advertising or promotional purposes or for creating new collective works for resale or redistribution to servers or lists, or to reuse any copyrighted component of this work in other works must be obtained from the IEEE

 

|| full paper || earth observation laboratory ||