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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Proceedings ArticleDOI
A uniform-twist magnetic flux rope in the solar wind
Charlie J. Farrugia,L. Janoo,Roy B. Torbert,J. M. Quinn,K. W. Ogilvie,R. P. Lepping,R. J. Fitzenreiter,John T. Steinberg,A. J. Lazarus,Robert P. Lin,Davin Larson,Sergio Dasso,Fausto T. Gratton,Yu Lin,D. B. Berdichevsky +14 more
TL;DR: In this article, the authors describe magnetic field, proton, electron, and α-particle observations made by WIND on 24 and 25 October 1995 of a structure consisting of a magnetic flux rope containing a relatively low beta plasma.
Journal ArticleDOI
A burst of energetic O+ ions during an upstream particle event
Eberhard Möbius,D. Hovestadt,Berndt Klecker,Manfred Scholer,F. M. Ipavich,C. W. Carlson,Robert P. Lin +6 more
TL;DR: In this paper, a brief burst of energetic O/sup +/ ions have been observed using the time-of-flight spectrometer SULEICA on the AMPTE/IRM spacecraft.
Journal ArticleDOI
First detection of a terrestrial MeV X-ray burst
J. E. Foat,Robert P. Lin,David M. Smith,F. R. Fenrich,Robyn Millan,Ilan Roth,K. R. Lorentzen,Michael P. McCarthy,George K. Parks,J. P. Treilhou +9 more
TL;DR: The first detection of a terrestrial X-ray burst extending up to MeV energies was made by a liquid-nitrogen-cooled germanium detector (∼2 keV FWHM resolution) on a high-altitude balloon at 65.5° magnetic latitude (L=5.7) in the late afternoon (1815 MLT) during low geomagnetic activity.
Journal ArticleDOI
Lunar surface magnetic field concentrations antipodal to young large impact basins
TL;DR: In this paper, the origin of the strong surface magnetic fields is discussed and the mechanisms yielding surface magnetic field concentrations antipodal to impact basins are not yet clear, the indicated period of strong lunar magnetic fields, at between about 3.85 and 3.6 aeons, is consistent with lunar paleomagnetic sample data.
Journal ArticleDOI
Evidence of electron impact ionization in the magnetic pileup boundary of Mars
D. Crider,Paul A. Cloutier,C. Law,P. Walker,Y. Chen,Mario H. Acuña,John E. P. Connerney,David L. Mitchell,Robert P. Lin,Kinsey A. Anderson,C. W. Carlson,J. P. McFadden,H. Rème,Christian Mazelle,Claude d’Uston,J. A. Sauvaud,D. Vignes,David Brain,Norman F. Ness +18 more
TL;DR: In this paper, the authors examined the characteristics of the evolution of the electron distribution function for one orbit and determined that the spectra can best be explained by electron impact ionization of oxygen and hydrogen.