SID Manual
Space Weather Report: July 23 to July 29
Ch 13 -uranus
Solar Energetic Particles and Shocks. What are Solar Energetic Particles? Electrons, protons, and heavier ions Energies – Generally KeV – MeV – Much less.
Radio Diagnostics of Energetic Electrons from Solar Flares, CMEs and Shocks: Nicole Vilmer LESIA Observatoire de Paris UMR 8109 CNRS, UPMC, Université.
Coronal IP Shocks Nat Gopalswamy NASA/GSFC Elmau CME Workshop, 2003 February 7 Plenary talk Sun Earth.
Stuart D. BaleFIELDS iCDR – Science Requirements Solar Probe Plus FIELDS Instrument CDR Science and Instrument Overview Science Requirements Stuart D.
Shock wave formation heights using 2D density and Alfvén maps of the corona ABSTRACT Coronal shock waves can produce decametric radio emission known Type.
1 THE RELATION BETWEEN CORONAL EIT WAVE AND MAGNETIC CONFIGURATION Speakers: Xin Chen 2015-10-17.
Collaborators:
To be published in ApJ: doi:10.1086/’521716’ Please email the author for preprints
A major proton event of 2005 January 20: propagating supershock or superflare?
