Published January 23, 2023 | Version v1
Journal article Open

Supporting files for "Interchange reconnection as the source of the fast solar wind within coronal holes"

Authors/Creators

  • 1. Space Sciences Laboratory, University of California, Berkeley, CA, USA
  • 2. Department of Physics, the Institute for Physical Science and Technology and the Joint Space Institute, University of Maryland, College Park, MD, USA
  • 3. Physics Department, University of California, Berkeley, CA, USA
  • 4. Southwest Research Institute, San Antonio, TX, USA
  • 5. Institute for Research in Electronics and Applied Physics, University of Maryland, College Park, MD, USA
  • 6. The Blackett Laboratory, Imperial College London, London, UK
  • 7. Johns Hopkins Applied Physics Laboratory, Laurel, MD, USA
  • 8. Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA
  • 9. Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
  • 10. California Institute of Technology, Pasadena, CA, USA
  • 11. Advanced Heliophysics Inc., Los Angeles, CA, USA
  • 12. BWX Technologies, Inc., Washington, DC, USA

Description

IDL data files and code for generating the plots from the PIC simulations in the paper "Interchange reconnection as the source of the fast solar wind within coronal holes".  The full data set from the simulations is too large to upload, so only relevant snapshots are included here.  The complete data set is stored at the supercomputing centers at which the runs were performed and access can be arranged upon request.

Files

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