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- W1539069504 abstract "The weakly ionized plasmas that occur in protostellar disks and in the cores of molecular clouds generally have a dust component. This chapter takes a look at the effects of the presence of charged dust on magnetic reconnection process. The chapter investigates the dynamics of two current loops coalescence, for both cases; partial and complete magnetic reconnection. Finally, it is shown that the field-free gas produced during the two loops coalescence with complete magnetic reconnection is able to initiate star formation." @default.
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- W1539069504 date "2000-01-01" @default.
- W1539069504 modified "2023-09-23" @default.
- W1539069504 title "Current Loop Coalescence in Dusty Plasmas" @default.
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- W1539069504 doi "https://doi.org/10.1016/b978-044450398-5/50039-7" @default.
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