Structure and Dynamics of Solar Atmosphere
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Pavel Ambroz
Basic information
RNDr. Pavel Ambroz CSc. (*1941)
e-mail: pambroz@asu.cas.cz
Research fields: Large-scale and global properties of solar magnetic
and velocity fields, structure of patterns, kinetic energy
distribution, solar differential rotation and meridional circulation.
Dynamical properties of the solar convection zone and of the solar
atmosphere. Structure of the solar corona, models of the solar magnetic
field structure and time variations. Stationary models of the solar
corona and coronal radiation related to the observed brightness
distribution.
1958-1963 - study of physics, graduated from the Natural
Sciences Faculty of the J.E. Purkyne University, Brno.
Since 1964 in the Astronomical Institute.
1972 - PhD in astrophysics.
1981 - graduated in
astronomy from the Faculty of Mathematics and Physics of the Charles University, Prague.
1977-1990 - Deputy Head and Head of the Solar Department.
Since 1985 external lecturer on Solar Physics at the Faculty of
Mathematics and Physics.