Other
Scientist
Big Bear Solar Observatory, Pasadena, CA
California Institute of Technology, Pasadena
Characteristics of solar coronal source regions producing He-3-rich particle events
Coronal mass ejections and associated X-ray flare durations
Emerging flux in active regions
He D3 as a diagnostic for the hard and soft X-rays from solar flares
Impulsive microwave burst and solar noise storm emission resolved with the VLA
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Profile ID: LFWR-SCP-P-430379