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pro vyhledávání: '"ZHANG Wenjia, MA Xin"'
Autor:
ZHANG Wenjia, MA Xin
Publikováno v:
Shanghai Jiaotong Daxue xuebao, Vol 56, Iss 11, Pp 1461-1469 (2022)
When the deep space probe approaches the target planet, due to the rapid increase of the gravity of the target planet, the orbital dynamics model will have a rapid acceleration change. Because the noise covariance is not completely known, the traditi
Externí odkaz:
https://doaj.org/article/80a33afcfccd45b8a1781f7ad8b90d39
