Fig. 2 from Magnetorotational Instability in Protoplanetary Disks. II. Ionization State and Unstable Regions

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Magnetorotational Instability in Protoplanetary Disks. II. Ionization State and Unstable Regions

Authors: Takayoshi Sano, Shoken M. Miyama, Toyoharu Umebayashi, and Takenori Nakano

Sano et al. 2000 The Astrophysical Journal 543 486.

Provider: AAS Journals

Caption: Fig. 2.

Electrical conductivity ﹩\sigma _{c}﹩ on the midplane of the fiducial model (same as in Fig. 1) as a function of the distance r from the star. Also shown are the contributions of electrons, ions, and charged grains to the conductivity.

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