Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Computer Sciences Corp., Silver Spring, Md.
Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA 90009, USA
Aerospace Corp., Los Angeles, CA
Aerospace Corp., Space Sciences Laboratory, El Segundo, CA
The Aerospace Corporation, Los Angeles, CA, USA;
Space Science Applications Laboratory, The Aerospace Corporation, El Segundo, CA, USA;
The Aerospace Corporation, El Segundo, CA, USA;
Space Sci Dept M2-260, The Aerospace Corporation, Los Angeles, CA, USA;
Space Science Applications Laboratory, Aerospace Corp, M2-260, Los Angeles, CA, USA;
Dixie State College, St. George, UT, USA;
Space and Environment Technology Center, The Aerospace Corporation, Los Angeles, USA
Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, California, USA
Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA 90009 Space Science Applications Laboratory, The Aerospace Corporation, Los Angeles, CA 90009 Space Science Applications Laboratory, The Aerospace Corporation, Mail Stop M2-260, PO Box 92957, Los Angeles, CA 90009
Aerospace Corporation, El Segundo, California, USA
The Aerospace Corp, MS M2-259 PO Box 92957, Los Angeles, CA 90009, USA
Computational Physics, Inc., Fairfax, VA, US
The Aerospace Corporation, Mail Stop M2-260 PO Box 92957, Los Angeles, CA 90009, USA
The Aerospace Corporation, P. O. Box 92957 Mail Station M2 / 260, Los Angeles, CA 90009, USA Aerospace Corporation, Mail Stop M2-260, PO Box 92957, Los Angeles, CA 90009, USA Science Applications Laboratory, The Aerospace Corporation Mail Stop M2-260 PO Box 92957, Los Angeles, CA 90009, USA
Aerospace Corporation, Space Environment and Technology Center, Los Angeles, CA 90009, USA
The Aerospace Corporation, M2-259 PO Box 92957, Los Angeles, CA 90009, USA j
A Climatology of Ripple Instabilities in the OH Airglow at Maui, HI
A comparison between auroral particle characteristics and atmospheric composition inferred from analyzing optical emission measurements alone and in combination with incoherent scatter radar measurements
A Comparison of Electron Density Profiles Derived from the Low Resolution Airglow and Aurora Spectrograph (LORAAS) Ultraviolet Measurements: Resolution of the 911 Å Conundrum
A comparison of the morphology of instability features seen at the Andes Lidar Observatory with those observed over Maui
A downward revision of a recently reported proton auroral LBH emission efficiency
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