Velocity patterns inside magnetic clouds are regular. The velocity component along the Sun-Earth line can be fitted quite well, bu the remaining components often show a different behaviour than one would expect from a simple flux rope model and a simple expansion.
Velocity patterns inside magnetic clouds are regular. The velocity component along the Sun-Earth line can be fitted quite well, bu the remaining components often show a different behaviour than one would expect from a simple flux rope model and a simple expansion. (en)
Složky rychlosti plazmatu v magnetických oblacích mají pravidelný chod. Složka ve směru ke Slunci se dá dobře fitovat, ale zbývající složky se často chovají jinak, než lze očekávat z jednoduchého modelu expanze oblaku. (cs)