R
Robert P. Lin
Researcher at University of California, Berkeley
Publications - 525
Citations - 36803
Robert P. Lin is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Solar flare & Solar wind. The author has an hindex of 93, co-authored 525 publications receiving 34180 citations. Previous affiliations of Robert P. Lin include Kyung Hee University & Space Sciences Laboratory.
Papers
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The origin of complex organic ions in the coma of Comet Halley
TL;DR: The Giotto-PICCA instrument has obtained heavy-ion mass spectra in the inner coma of Comet Halley; the spectra exhibit a series of distinct mass groups separated by a constant about 15 amu, and extending to at least 120 amu.
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Observational Aspects of Particle Acceleration in Large Solar Flares
TL;DR: A review of observations that bear upon the acceleration mechanism can be found in this article, where the acceleration is usually associated with magnetic reconnection occurring high in the corona, though a shock produced by the Coronal Mass Ejection (CME) associated with a flare can also accelerate particles.
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RHESSI as a Hard X-Ray Polarimeter
TL;DR: The Ramaty High Energy Solar Spectroscopic Imager (RHESSI) as mentioned in this paper is capable of measuring the polarization of hard X-rays (20-100 keV) from solar flares.
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Simultaneous Geotail and Wind observations of reconnection at the subsolar and tail flank magnetopause
T. D. Phan,Hiroshi Hasegawa,Masaki Fujimoto,Marit Øieroset,Toshifumi Mukai,Robert P. Lin,W. Paterson +6 more
TL;DR: In this article, a two-spacecraft conjunction was reported when Geotail and Wind observed the occurrence of reconnection simultaneously at the subsolar and dawn tail flank magnetopause during stable By dominated IMF.
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The injection of ten electron/3He-rich SEP events
TL;DR: In this paper, the authors derived the particle injections at the Sun for ten good electron/3 He-rich solar energetic particle (SEP) events, using a 1.2 AU particle path length (suggested by analysis of the velocity dispersion).