Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientist
Physics
High Energy Physics
High Energy Physics - Phenomenology
Scientist
Ifae
Universidad Nacional Autonoma de Mexico, Villa Obregon.
Universidad Nacional Autonoma de Mexico
Universidad Nacional Autonoma de Mexico, Coyoacan, Mexico
Universidad Nacional Autonoma de Mexico, Mexico City, Mexico
Instituto de Geofísica, UNAM
Instituto de Geofisica, Universidad Nacional Autónoma de México Coyoacán, D.F. 04510, México
UNAM, Coyoacan, Mexico
Instituto de Geofísica, UNAM, México, D.F.
Instituto de Geofísica, UNAM, México
Universidad Nacional Autonoma de Mexico, Alvaro Obregon, Mexico
Instituto de Geofísica, Universidad Nacional Autónoma de México, Coyoacán, D.F., 04510, México
Instituto de Geofísica, Universidad Nacional Autónoma de México Coyoacán, D.F., 04510, México
Instituto de Geofísica, Universidad Nacional Autónoma de México Ciudad Universitaria, Coyoacán, México D.F. 04510, Mexico
Inst. de Geofisica, Coyoacan, D.F., Mexico
Universidad Nacional Autonoma de Mexico, Coyoacan
Departimento de Física Espacial, Instituto de Geofísica, UNAM, Coyoacán, D.F. 04510, México
A discussion about the geometry of the SKYLAB north polar coronal hole
A Solar Scenario for the Associated Occurrence of Flares, Eruptive Prominences, Coronal Mass Ejections, Coronal Holes, and Interplanetary Shocks
Actividad de LOS Hoyos Coronales Solares de Baja Latitud
Characteristics of coronal mass ejections associated with interplanetary shocks
Characteristics of interplanetary magnetic clouds in relation to their solar association
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