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Autor(en): 
  • Eelco Doornbos
  • Thermospheric Density and Wind Determination from Satellite Dynamics 
     

    (Buch)
    Dieser Artikel gilt, aufgrund seiner Grösse, beim Versand als 3 Artikel!


    Übersicht

    Auf mobile öffnen
     
    Lieferstatus:   Auf Bestellung (Lieferzeit unbekannt)
    Genre:  Naturwissensch., Medizin, Technik 
     
    Aerospace & aviation technology / Aerospace engineering / Aerospace Technology and Astronautics / astronautics / Atmospheric Sciences / B / Classical and Continuum Physics / Earth and Environmental Science / Earth System Sciences / Fluid mechanics / Fluid- and Aerodynamics / Fluids
    ISBN:  9783642442643 
    EAN-Code: 
    9783642442643 
    Verlag:  Springer Nature EN 
    Einband:  Kartoniert  
    Sprache:  English  
    Serie:  Springer Theses  
    Dimensionen:  H 235 mm / B 155 mm / D  
    Gewicht:  314 gr 
    Seiten:  184 
    Zus. Info:  Previously published in hardcover 
    Bewertung: Titel bewerten / Meinung schreiben
    Inhalt:
    The Earth's atmosphere is often portrayed as a thin and finite blanket covering our planet, separate from the emptiness of outer space. In reality, the transition is gradual and a tiny fraction of the atmophere gases is still present at the altitude of low orbiting satellites. The very high velocities of these satellites ensure that their orbital motion can still be considerably affected by air density and wind. This influence can be measured using accelerometers and satellite tracking techniques. The opening chapters of this thesis provide an excellent introduction to the various disciplines that are involved in the interpretation of these observations: orbital mechanics, satellite aerodynamics and upper atmospheric physics. A subsequent chapter, at the heart of this work, covers advances in the algorithms used for processing satellite accelerometry and Two-Line Element (TLE) orbit data. The closing chapters provide an elaborate analysis of the resulting density and wind products,which are generating many opportunities for further research, to improve the modelling and understanding of the thermosphere system and its interactions with the lower atmosphere, the ionosphere-magnetosphere system and the Sun.

      
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