Physics – Condensed Matter – Strongly Correlated Electrons
Scientist
Physics
Condensed Matter
Strongly Correlated Electrons
Scientist
National Research Council, Code 612.3 NASA / GSFC, Greenbelt, MD 20771, USA; Institute for Astronomy and Astrophysics, Scheinerstrasse 1, Munich, 81679 Germany
The Catholic University of America, Washington, DC, USA;
Department of Physics, The Catholic University of America, Washington, DC, USA;
ORAU / GSFC, Code 612.3, Grenbelt, MD 20771, USA / GSFC, NASA GSFC, Mail code 674, Greenbelt, MD 20771, USA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA; University Observatory, Faculty for Physics, Ludwig Maximilian University, Scheinerstr. 1, Munich, 81679, Germany The Catholic University of America / NASA Goddard Space Flight Center, Washington, DC, USA
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, Garching, 85741 Germany
The Catholic University of America, Washington, DC, USA
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany
Leningradskii Gosudarstvennyi Universitet, Leningrad, USSR
Munich
NAS / NRC at GSFC and Max Planck
CUA / LMU / GSFC, Mailcode 693, Greenbelt, MD 20771, USA Planck Institute
Institut für Astronomie and Astrophysik der Universität München, Scheinerstrasse 1 81679 München, Germany
Institut für Astronomie und Astrophysik der Universität München, Scheinerstrasse 1 81679 München, Germany currently NAS / NRC at NASA / GSFC
Catholic University of America, Institute for Astrophysics and Computational Sciences, Washington, DC 20064, USA; NASA / GSFC, Heliophysics Science Division, Code 674, Greenbelt, MD 20771, USA GSFC, NASA Goddard Space Flight Center, Greenbelt Rd, Greenbelt, MD 20771, USA; CUA, The Catholic University of America, Washington, DC 20064, USA
St. Petersburg Sta
A new general circulation model of the martian atmosphere: description and first results
A Non-LTE model for the atmosphere of Titan and implications for the Cassini CIRS experiment
A review of the scientific results from the CRISTA missions
Accurate and fast computation of the radiative transfer absorption rates for the infrared bands in the atmosphere of Titan
Additional Radiative Cooling of the Mesopause Region due to Small-Scale Temperature and [O] Fluctuations Associated with Gravity Waves
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