Ryuho Kataoka

2 ta ish

Tokyo Institute of Technology

1. Why are relativistic electrons persistently quiet at geosynchronous orbit in 2009?

   Ryuho Kataoka, Yoshizumi Miyoshi

   Maqola20102 iqtibos

   ABIABI:AkademIndex/2026.other.532536

2. Average profiles of the solar wind and outer radiation belt during the extreme flux enhancement of relativistic electrons at geosynchronous orbit

   Ryuho Kataoka, Yoshizumi Miyoshi

   Maqola20082 iqtibos

   ABIABI:AkademIndex/2026.other.783287