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      Solar wind flow past nonmagnetic planets—Venus and Mars

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      Planetary and Space Science
      Elsevier BV

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          Plasma flow around the magnetosphere

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            The interaction of the terrestrial magnetic field with the solar corpuscular radiation

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              Theoretical determination of the form of the boundary of the solar corpuscular stream produced by interaction with the magnetic dipole field of the Earth

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                Author and article information

                Journal
                Planetary and Space Science
                Planetary and Space Science
                Elsevier BV
                00320633
                September 1970
                September 1970
                : 18
                : 9
                : 1281-1299
                Article
                10.1016/0032-0633(70)90139-X
                17e1bdac-38bd-47c8-942d-5a5db5f160aa
                © 1970

                http://www.elsevier.com/tdm/userlicense/1.0/

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