The main problem in the orbit determination of the space debris population orbiting our planet is the identification of two or more set of data. The observations of a given object during a passage above an observing station are called a Too Short Arc (TSA): data from a TSA cannot allow for a complete determination of an orbit. A new method for solving the identification problem, finding two or more observational TSA belonging to the same physical object and an orbit fitting all the observations is outlined.
Orbit determination methods for space debris
Rossi A
2006
Abstract
The main problem in the orbit determination of the space debris population orbiting our planet is the identification of two or more set of data. The observations of a given object during a passage above an observing station are called a Too Short Arc (TSA): data from a TSA cannot allow for a complete determination of an orbit. A new method for solving the identification problem, finding two or more observational TSA belonging to the same physical object and an orbit fitting all the observations is outlined.File in questo prodotto:
| File | Dimensione | Formato | |
|---|---|---|---|
|
prod_120334-doc_130454.pdf
accesso aperto
Descrizione: Orbit determination methods for space debris
Tipologia:
Versione Editoriale (PDF)
Dimensione
123.99 kB
Formato
Adobe PDF
|
123.99 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


