Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Raytheon ITSS, 4400 Forbes Blvd., Lanham, MD 20706, USA
Catholic University of America and NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
Hughes STX, Inc.
Catholic University of America, Washington, DC; and NASA Goddard Space Flight Center, Greenbelt, MD
Science Applications Research, Lanham, MD
Raytheon Information Technology and Scientific Services, 4400 Forbes Boulvard, Lanham, MD 20706.
The Catholic University of America, Washington, DC, USA; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Catholic University and NASA / GSFC, Goddard Space Flight Center, Greenbelt, MD 20771, USA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA; The Catholic University of America, 620 Michigan Ave., N.E., Washington, DC 20064, USA University and NASA / GSFC, Code 695, Greenbelt, MD 20771, USA Catholic University of America; and NASA Goddard Space Flight Center, Greenbelt, MD 20771
NASA, GSFC, Greenbelt, MD 20770, USA Univ. & NASA / GSCF, Code 674, Greenbelt, MD 20771, USA Goddard Space Flight, USA and The Catholic University of America, USA
Hughes STX Corp., Lanham; NASA, Goddard Space Flight Center, Greenbelt, MD
Hughes STX, 4400 Forbes Blvd., Lanham, Maryland 20706
Catholic University, Greenbelt, MD 20771; NASA / Goddard Space Flight Center, Greenbelt, MD 20771
NASA / GSFC, Laboratory for Extraterrestrial Physics, Greenbelt, MD 20771, USA; The Catholic University of America, 620 Michigan Ave., NE, Washington, DC 20064, USA
Catholic University & NASA / GSFC, NASA / GSFC Code 690.2, Greenbelt, MD 20771, USA Catholic University of America and NASA / Goddard Space Flight Center
Hughes STX Corp., Lanham, MD; NASA, Goddard Space Flight Center, Greenbelt, MD
Hughes STX, Lanham, MD
NASA. Goddard Space Flight Center, Greenbelt, MD, US
Catholic University and NASA / GSFC, Code 69
A Highly Circularly Polarized Solar Radio Emission Component Observed at Hectometric Wavelengths
A new component of Jovian kilometric radio emission
A new method for reconstructing type III trajectories
A new method for studying remote type II radio emissions from coronal mass ejection-driven shocks
A test of magnetospheric radio tomographic imaging with IMAGE and WIND
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