Physics
Optics
Scientist
Institute of Geophysics and Planetary Physics, University of California
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, California, USA
Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA, USA
Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences, University of California, Los Angeles, CA 90095-1567, USA
University of California, Institute of Geophysics and Planetary Physics, Los Angeles, CA, USA
UCLA, Institute of Geophysics and Planetary Physics, Earth and Space Sciences, Los Angeles, USA
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, 595 Charles E. Young Dr. East 6862 Slichter Hall, Los Angeles, CA 90095, USA
IGPP, UCLA, Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, 405 Hilgard Ave, LA, CA 90095, USA
ESS, UCLA
Institute of Geophysics and Planetary Physics / UCLA, Institute of Geophysics and Planetary Physics / UCLA, Los Angeles, CA 90095-1567 UCLA, UCLA, Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics / UCLA, UCLA, Los Angeles, CA 90095 of California, Los Angeles, IGPP, Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics; Department of Earth and Space Sciences; University of California, Los Angeles, 595 Charles E. Young Dr. East, 6862 Slichter Hall, Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095-1567, USA
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA
IGPP, University of California, Los Angeles, California, USA
Institute of Geophysics and Planetary Physics, University of California Los Angeles
An unusual current sheet in an ICME: Possible association with C/2006 P1 (McNaught)
Behavior of current sheets at directional magnetic discontinuities in the solar wind at 0.72 AU
Characteristic size and shape of the mirror mode structures in the solar wind at 0.72 AU
Comparing Solar Minimum 23/24 with Historical Solar Wind Records at 1 AU
Comparison of Observations at ACE and Ulysses with Enlil Model Results: Stream Interaction Regions During Carrington Rotations 2016 - 2018
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