Physics – High Energy Physics – High Energy Physics - Theory
Scientist
Physics
High Energy Physics
High Energy Physics - Theory
Scientist
SSL-UCB, Berkeley, USA
SSL / UCB
Space Sciences Laboratory, University of California, Berkeley
CEA / UCB
University of California, Berkeley, CA, US
University of California / Berkeley, USA
University of California, Berkeley, Sanfrancisco, CA, USA;
UC-Berkeley
Space Sciences Lab, UC
Space Sciences Laboratory, University of California, Berkeley, CA 94720.
University of California Berkeley
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA
California, University, Berkeley
UC, Berkeley
Space Science Research Division, Korea Astronomy Observatory, Daejeon 305-348, Korea Sciences Lab., University of California, Berkeley
Spaces Sceinces Lab. U.C. Berkeley
UC Berkeley, Space Sciences Lab
Space Sciences Lab, UC-Berkeley
University of California Berkeley, Space Science Laboratory, 7 Gauss Way, Berkeley, CA 94720, USA
Satellite Technology Research Center, KAIST; Korea Astronomy Observatory; Space Sciences Lab., University of California, Berkeley, CA, USA
Korea Astronomy Observatory; Satellite Technology Research Center, KAIST; Space Sciences Lab., University of California, Berkeley, CA, USA
University of California, Berkeley, USA
University of California, Space Sciences Laboratory, Berkeley, 94720-7450, USA
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA of California, Berkeley, CA, USA
Space Sciences Laboratory, University of California, Berkeley, California, USA
Lawrence Berkeley National Lab
UC Berkeley Space Sciences Laboratory
Space Sciences, UC Berkeley
SSL, U.C. Berkeley
University of California, Berkeley, Space Sciences Laboratory, UCB, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, University of California, Berkeley, CA 94720
A high-throughput, high-resolution spectrometer for mapping the heliopause and 3-D Solar Wind using He+ 30.4nm
A Search For C IV Emission Line From Galactic SNRs With SPEAR/FIMS
Airglow Observation from STSAT-1
An EUV spectrometer for mapping the heliopause and solar wind
Analysis of auroras caused by precipitation of high energy electrons
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Profile ID: LFWR-SCP-P-55302