Energetic Particle Observations during the 2000 July 14 Solar Event

By J. Bieber, W. Dröge, P. Evenson, R. Pyle, D. Ruffolo, U. Pinsook, P. Tooprakai, M. Rujiwarodom, T. Khumlumlert, S. Krucker. 2002

156 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

A Global Picture of CMEs in the Inner Heliosphere (2004, background): “Multiple shocks and CMEs can form configurations that can enhance the SEP intensity significantly (Kallenrode and Cliver, 2001; Bieber et al., 2002).”
Modeling Shock-accelerated Solar Energetic Particles Coupled to Interplanetary Alfvén Waves (2003, unknown): “Such regions are known to exist as corotating interaction regions produced by stream-stream interaction, as enhanced turbulence and magnetic field enhancement near CME-driven IP shocks (e.g., Bieber et al. 2002), or simply as magnetic bottles from CMEs (Reames 2002).”
Properties of Ground Level Enhancement Events and the Associated Solar Eruptions During Solar Cycle 23 (2012, methodology): “Subsequently, several case studies were performed on individual GLE events from cycle 23 (Bieber et al. 2002, 2004, 2005, 2008; Grechnev et al. 2008; Tylka and Dietrich 2010).”
SOLAR RELEASE TIMES OF ENERGETIC PARTICLES IN GROUND-LEVEL EVENTS (2009, background): “Neutron monitor onsets are again well determined (e.g., Bieber et al. 2002).”