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Modelling radiative transfer in circuit-breaker arcs with the P-1 approximation

✍ Scribed by Eby, S D; Trépanier, J Y; Zhang, X D

Book ID
125534906
Publisher
Institute of Physics
Year
1998
Tongue
English
Weight
544 KB
Volume
31
Category
Article
ISSN
0022-3727

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## Abstract A protoplanetary disk is a quasi‐toroidal gas–dust mixture rotating around a protostar that creates a complex intensity field in the internal disk medium in which planets are believed to form. In this work we start to model an idealized disk describing the radiation intensity propagatin