Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
California, University, La Jolla, Calif.
University of California San Diego
California, University, La Jolla, CA
Owens Valley Radio Observatory, Big Pine, Calif.
Electrical and Computer Engineering, University of California, San Diego, California 92093-0407
California Univ., La Jolla
Electrical Engineering, University of California, San Diego
E.C.E. Department, University of California at San Diego, La Jolla
Electrical and Computer Engineering, University of California at San Diego
California Univ., La Jolla.
UCSD
California, University, La Jolla
California, University, San Diego
Electrical and Computer Engineering Department, University of California, La Jolla, California 92093-0407
Electrical and Computer Engineering, University of California at San Diego, 9500 Gilman Drive, La Jolla, CA 92093-0407, USA
UC San Diego, Department of Elec. and Comp. Eng. Mail Code 0407, La Jolla, CA 92093-0407, USA University, San Diego, Calif.
University of California at San Diego, Electrical and Computer Engineering, MC 0407, La Jolla, CA 92093-0407, USA
UC-San Diego, Department of Elec. and Comp. Eng., La Jolla, CA 92093-0407, USA
California Univ., San Diego, La Jolla.
Electrical and Computer Engineering, University of California at San Diego, La Jolla, California, USA
Electrical and Computer Engineering, University of California at San Diego, La Jolla, California 92093, USA
California, University, San Diego, CA
University of California, E.C.E. Dept., La Jolla, CA 92093-0407, USA
E. C. E. Dept., University of California
University of Calif. at San Diego
California, Univ., San Diego
Department of Electrical and Computer Engineering, University of California, San Diego, La Jolla, California 92093
California University
Department of Electrical and Computer Engineering, University of California at San Diego
933 MHz IPS velocity measurements at EISCAT
A Bimodal Model of the Solar Wind Speed
A comparison of mean density and microscale density fluctuations in a CME at 10 Rsolar
A New Method for Studying the Solar Wind Using Radio Scintillations (IPS)
A New UHF Antenna for IPS and Pulsar Observations
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