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.
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Model calculations of electron precipitation induced ionization patches on the nightside of Mars
Matts O. Fillingim,Laura Peticolas,Robert Lillis,David Brain,Jasper Halekas,David L. Mitchell,Robert P. Lin,Dirk Lummerzheim,Stephen W. Bougher,D. L. Kirchner +9 more
TL;DR: In this paper, the effect of electron precipitation on the electron density and total electron content in the nightside ionosphere of Mars was investigated using an electron transport model, and the results showed a secondary electron density peak due to precipitation of several keV electrons not seen in previous modeling efforts.
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A large excess in apparent solar oblateness due to surface magnetism.
TL;DR: The shape of the Sun subtly reflects its rotation and internal flows and relates the larger radius values to magnetic elements in the enhanced network and uses the correlation to correct for it as a systematic error term in the oblateness measurement.
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A reconnection layer associated with a magnetic cloud
Charlie J. Farrugia,Bernard J. Vasquez,Ian G. Richardson,Roy B. Torbert,L. F. Burlaga,Helfried K. Biernat,S. Mühlbachler,K. W. Ogilvie,R. P. Lepping,J. D. Scudder,D. Berdichevsky,Vladimir Semenov,I. V. Kubyshkin,Tai Phan,Robert P. Lin +14 more
TL;DR: In this article, the authors examine a 3-hour interval on December 24, 1996, containing a magnetic hole associated with an interplanetary magnetic cloud and interpret the observations as MHD discontinuities arriving with varying delays from a reconnection site closer to the Sun.
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Interplanetary magnetic field connection to the sun during electron heat flux dropouts in the solar wind
Robert P. Lin,S. W. Kahler +1 more
TL;DR: In this article, observations of 2-to 8.5-keV electrons, made by measurements aboard the ISEE 3 spacecraft during the periods of heat flux decreases (HFDs) reported by McComas et al.
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RHESSI e + -e - Annihilation Radiation Observations: Implications for Conditions in the Flaring Solar Chromosphere
TL;DR: RHESSI has measured the positron-electron annihilation line and continuum in three solar flares: 2002 July 23, 2003 October 28, and 2003 November 2 as discussed by the authors, consistent with annihilation in an ambient ionized medium at temperatures above 105 K.