H. Kunow – författare
Visar alla böcker från författaren H. Kunow. Handla med fri frakt och snabb leverans.
6 produkter
Coronal Mass Ejections
Av H. Kunow, N.U. Crooker m. fl.
Inbunden, 2007
1643 kr
Lägg i varukorg
It is well known, that the Sun as central star of our solar system gravitationally controls the orbits of planets and minor bodies. Much less known is the domain of plasma fields and charged particles, however, in which the Sun with a radius of less than 0.7 Million km governs the heliosphere out …
Coronal Mass Ejections
Av R. Von Steiger, R. Schwenn m. fl.
E-bok, 2007
2111 kr
Lägg i varukorg
It is well known, that the Sun as central star of our solar system gravitationally controls the orbits of planets and minor bodies. Much less known is the domain of plasma fields and charged particles, however, in which the Sun with a radius of less than 0.7 Million km governs the heliosphere out …
Corotating Interaction Regions
Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland
Av Andre Balogh, A. Balogh m. fl.
Inbunden, 2000
1643 kr
Lägg i varukorg
A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. …
Coronal Mass Ejections
Av H. Kunow, N.U. Crooker m. fl.
Häftad, 2010
1643 kr
Lägg i varukorg
It is well known, that the Sun as central star of our solar system gravitationally controls the orbits of planets and minor bodies. Much less known is the domain of plasma fields and charged particles, however, in which the Sun with a radius of less than 0.7 Million km governs the heliosphere out …
Corotating Interaction Regions
Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland
Av A. Balogh, J.T. Gosling m. fl.
Häftad, 2010
1643 kr
Lägg i varukorg
A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. …
Corotating Interaction Regions
Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland
Av H. Kunow, R. Kallenbach m. fl.
E-bok, 2013
2111 kr
Lägg i varukorg
A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. …
