International audienceThis paper reviews solar flows and magnetic fields observed at the photospheric level. We first present the context in which these observations are performed. We describe the various temporal and spatial scales involved, and the coupling between them. Then we present small-scale flows, mainly supergranulation and flows around active regions. Flows at the global scale are then reviewed, again with emphasis on the flows, i.e. differential rotation, torsional oscillation and meridional circulation. In both small- and global-scale we discuss the coupling between flow fields and magnetic field and give an overview of observational techniques. Finally, the possible connection between studies of solar activity and stellar act...
Our present-day understanding of solar and stellar magnetic fields is discussed from both an observa...
Context. As the global magnetic field of the Sun has an activity cycle, one expects to observe some ...
In this review, our present day understanding of the Sun’s global photospheric and coronal magnetic ...
This review about solar photospheric magnetic fields will follow the two traditionnal approaches to...
Context. The Sun features on its surface typical flow patterns called the granulation, mesogranulati...
Context. The Sun features on its surface typical flow patterns called the granulation, mesogranulati...
Context. The Sun features on its surface typical flow patterns called the granulation, mesogranulati...
International audienceContext. As the global magnetic field of the Sun has an activity cycle, one ex...
We have developed a method to map large-scale horizontal velocity fields in the solar photosphere. ...
© ESO 2019. Context. The Sun features on its surface typical flow patterns called the granulation, m...
International audienceContext. As the global magnetic field of the Sun has an activity cycle, one ex...
International audienceContext. As the global magnetic field of the Sun has an activity cycle, one ex...
International audienceContext. As the global magnetic field of the Sun has an activity cycle, one ex...
Abstract We compare horizontal flow fields in the photosphere and in the subphoto-sphere (a layer 0....
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
Our present-day understanding of solar and stellar magnetic fields is discussed from both an observa...
Context. As the global magnetic field of the Sun has an activity cycle, one expects to observe some ...
In this review, our present day understanding of the Sun’s global photospheric and coronal magnetic ...
This review about solar photospheric magnetic fields will follow the two traditionnal approaches to...
Context. The Sun features on its surface typical flow patterns called the granulation, mesogranulati...
Context. The Sun features on its surface typical flow patterns called the granulation, mesogranulati...
Context. The Sun features on its surface typical flow patterns called the granulation, mesogranulati...
International audienceContext. As the global magnetic field of the Sun has an activity cycle, one ex...
We have developed a method to map large-scale horizontal velocity fields in the solar photosphere. ...
© ESO 2019. Context. The Sun features on its surface typical flow patterns called the granulation, m...
International audienceContext. As the global magnetic field of the Sun has an activity cycle, one ex...
International audienceContext. As the global magnetic field of the Sun has an activity cycle, one ex...
International audienceContext. As the global magnetic field of the Sun has an activity cycle, one ex...
Abstract We compare horizontal flow fields in the photosphere and in the subphoto-sphere (a layer 0....
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
Our present-day understanding of solar and stellar magnetic fields is discussed from both an observa...
Context. As the global magnetic field of the Sun has an activity cycle, one expects to observe some ...
In this review, our present day understanding of the Sun’s global photospheric and coronal magnetic ...