Physics – Condensed Matter – Mesoscale and Nanoscale Physics
Scientist
Physics
Condensed Matter
Mesoscale and Nanoscale Physics
Scientist
Instituto de Geofisica, UNAM, Instituto de Geofisica, D.F., 04510 Mexico
Instituto De Geofisica, UNAM, C.U.Mexico, Mexico City, 04510
Instituto de Geofísica, UNAM, México
Center for Solar Physics and Space Weather, Catholic University of America, Washington, D. C., USA
Instituto de Geofisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico;
Instituto de Geofisica, Mexico, Mexico;
Universidad Nacional Autonoma, C.U. Mexico D.F., Mexico;
Instituto de Geofísica UNAM, Ciudad Universitaria, 04510, México D.F., México
Instituto de Geofisica, Universidad Nacional Autónoma de México, Mexico City, Mexico
Instituto de Geofisica UNAM, Instituto de Geofisica UNAM, C.U. Mexico D.F., 04510, Mexico
Instituto de Geofisica, UNAM, Ciudad Universitaria SN, Del. Coyoacan, Mexico D.F., 04510
Department of Physics, Catholic University of America, 200 Hannan Hall, Washington, DC 20064; On leave from the Instituto de Geofísica, UNAM, Mexico.
Instituto de Geofísica UNAM, Ciudad Universitaria, Delegacion de Coyoacan, 04510 DF, Mexico, Mexico
Instituto de Geofísica, Universidad Nacional Autónoma de México, México
The Catholic University of America
The Catholic University of America, 620 Michigan Ave, Washington, DC 20064, USA de Geofisica, National Autonomous University of Mexico, Mexico City, Mexico
I. de Geofísica, UNAM, Cd. Universitaria, Coyoac n, México, DF 04510 Mexico de Geofísica, UNAM, 04510 Mexico de Geofísica, UNAM, Ciudad Universitaria, México DF, 04510 Mexico; Center for Solar Physics and Space Weather, The Catholic University of America, Washington, DC 2100, USA of Maryland
Instituto de Geofisica, UNAM, Ciudad Universitaria, Mexico, DF 04510 Mexico
"Driverless" Shocks in the Interplanetary Medium
17 GHz Mode Coupling in the Solar Corona
3-D model of ICME in the interplanetary medium
3D Simulations of Solar Observations in Radio, Millimeter and Submillimeter Wavelengths.
3D Simulations of the Quiet Sun Radio Emission at Millimeter and Submillimeter Wavelengths
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