This volume is devoted to the dynamics and diagnostics of solar magnetic fields and plasmas in the Sun’s atmosphere. Five broad areas of current research in Solar Physics are presented: (1) New techniques for incorporating radiation transfer effects into three-dimensional magnetohydrodynamic models of the solar interior and atmosphere, (2) The connection between observed radiation processes occurring during flares and the underlying flare energy release and transport mechanisms, (3) The global balance of forces and momenta that occur during flares, (4) The data-analysis and theoretical tools needed to understand and assimilate vector magnetogram observations and (5) Connecting flare and CME phenomena to the topological properties of the mag...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
Solar flares are prominent eruptive phenomenon happening in the solar atmosphere. Major flares usual...
Sunspots are regions of decreased brightness on the visible surface of the Sun (photosphere) that ar...
The book contains lecture papers and contributed papers on different aspects of magnetic phenomena i...
The Sun is a magnetically active star and is the source of the solar wind, electromagnetic radiation...
The areas of emphasis are: (1) develop theoretical models of the transient release of magnetic energ...
The physical processes, which drive powerful solar eruptions, play an important role in our understa...
Abstract This publication provides an overview of magnetic fields in the solar atmo-sphere with the ...
This paper outlines the current understanding of solar flares, mainly focused on magne-tohydrodynami...
Solar magnetism is responsible for the several active phenomena that occur in the solar atmosphere. ...
The defining physical property of the Sun's corona is that the magnetic field dominates the plasma. ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
Solar flares are prominent eruptive phenomenon happening in the solar atmosphere. Major flares usual...
Sunspots are regions of decreased brightness on the visible surface of the Sun (photosphere) that ar...
The book contains lecture papers and contributed papers on different aspects of magnetic phenomena i...
The Sun is a magnetically active star and is the source of the solar wind, electromagnetic radiation...
The areas of emphasis are: (1) develop theoretical models of the transient release of magnetic energ...
The physical processes, which drive powerful solar eruptions, play an important role in our understa...
Abstract This publication provides an overview of magnetic fields in the solar atmo-sphere with the ...
This paper outlines the current understanding of solar flares, mainly focused on magne-tohydrodynami...
Solar magnetism is responsible for the several active phenomena that occur in the solar atmosphere. ...
The defining physical property of the Sun's corona is that the magnetic field dominates the plasma. ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
International audienceSolar magnetism is responsible for the several active phenomena that occur in ...
Solar flares are prominent eruptive phenomenon happening in the solar atmosphere. Major flares usual...