DocumentCode
1953308
Title
Sun noise measurement at low Earth orbiting satellite ground station
Author
Cakaj, Shkelzen ; Keim, Werner ; Malaric, Kresimir
Author_Institution
Post & Telecommun. of Kosovo, Prishtina
fYear
2005
fDate
8-10 June 2005
Firstpage
345
Lastpage
348
Abstract
The project "MOST" (microvariability and oscillations of stars) is a Canadian micro satellite space telescope mission. The micro satellite carries a Rumak-Maksutov telescope with an aperture of 15 cm. The size of the satellite is 65 cm times 65 cm times 30 cm and the mass is about 65 kg. The goals of the mission are to analyze the inner structure of stars, set a lower limit to the age of the universe and to search for Exoplanets. The project MOST consists of a low earth orbiting (LEO) satellite and three ground stations, one of them in Vienna [W. Weiss et al., 2003]. The Vienna ground station system was set up at the Institute for Astronomy of the University of Vienna in cooperation with the Institute of Communications and Radio-Frequency Engineering of the Vienna University of Technology. The downlink budget calculations are done for the worst propagation conditions. Among measurements related to the performance it is finally measured the figure of merit (G/Ts ) of the receiving system based on the sun flux density method
Keywords
Sun; noise measurement; satellite ground stations; Canadian microsatellite space telescope mission; Exoplanets; downlink budget calculations; low earth orbiting satellite ground station; microvariability and oscillations of stars; performance measurement; sun flux density method; sun noise measurement; Apertures; Density measurement; Extraterrestrial measurements; Low earth orbit satellites; Noise measurement; Satellite broadcasting; Satellite ground stations; Space missions; Sun; Telescopes;
fLanguage
English
Publisher
ieee
Conference_Titel
ELMAR, 2005. 47th International Symposium
Conference_Location
Zadar
Print_ISBN
953-7044-01-4
Type
conf
DOI
10.1109/ELMAR.2005.193714
Filename
1505715
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