Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

Cosmic-Ray Ionization Rate in Protoplanetary Disks with Sheared Magnetic Fields

  • Authors: Yuri I. Fujii, Shigeo S. Kimura

Yuri I. Fujii and Shigeo S. Kimura 2022 The Astrophysical Journal Letters 937 .

  • Provider: AAS Journals

Caption: Figure 1.

Schematic view of our scenario. An hourglass-shaped magnetic-field configuration focuses cosmic rays from a molecular cloud core to a protoplanetary disk. The purple oval represents the area from which the disk can receive cosmic-ray particles. The magnetic fields are stretched to azimuthal direction by shearing motion.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse