Context. Spectropolarimetry has the potential to provide us with important coronal plasma parameters. Aims. We test spectropolarimetric forward modelling by investigating whether it is possible to reproduce the only linear polarisation measurement made for the optically thin 1032 Å UV O v
Context. Progress in the solution to some of the most outstanding open problems of solar physics, su...
Ph.D. University of Hawaii at Manoa 2014.Includes bibliographical references.The dissertation focuse...
International audienceCurrent burning issues in stellar physics, for both hot and cool stars, concer...
Context. Spectropolarimetry has the potential to provide us with important coronal plasma parameters...
Talk delivered in Seminar Series of the Osservatorio Astrofisico di Catania (Virtual), 2020.Spectrop...
Context. Narrowband imaging spectropolarimetry is one of the most powerful tools available to infer ...
The coronal magnetic field creates the structure of the corona and is the source of heat and energy ...
International audienceHigh-resolution spectropolarimetry is a useful astronomical technique, in part...
International audienceMagnetic fields are important for stellar photospheres and magnetospheres, inf...
Prague, Czech Republic, 24-27 April 2017Polarimetry is a valuable technique to help us understand th...
One of the greatest future challenges in cosmic physics is the empirical investigation of the magnet...
Context. It has so far proven impossible to reproduce all aspects of the solar plage chromosphere in...
Context. Spectropolarimetry at high spatial and spectral resolution is a basic tool to characterize...
Linear spectropolarimetry of spectral lines is a neglected field in astronomy, largely because of th...
Spectropolarimetry is nowadays one of the most used tool to investigate small scale (100 km) magneti...
Context. Progress in the solution to some of the most outstanding open problems of solar physics, su...
Ph.D. University of Hawaii at Manoa 2014.Includes bibliographical references.The dissertation focuse...
International audienceCurrent burning issues in stellar physics, for both hot and cool stars, concer...
Context. Spectropolarimetry has the potential to provide us with important coronal plasma parameters...
Talk delivered in Seminar Series of the Osservatorio Astrofisico di Catania (Virtual), 2020.Spectrop...
Context. Narrowband imaging spectropolarimetry is one of the most powerful tools available to infer ...
The coronal magnetic field creates the structure of the corona and is the source of heat and energy ...
International audienceHigh-resolution spectropolarimetry is a useful astronomical technique, in part...
International audienceMagnetic fields are important for stellar photospheres and magnetospheres, inf...
Prague, Czech Republic, 24-27 April 2017Polarimetry is a valuable technique to help us understand th...
One of the greatest future challenges in cosmic physics is the empirical investigation of the magnet...
Context. It has so far proven impossible to reproduce all aspects of the solar plage chromosphere in...
Context. Spectropolarimetry at high spatial and spectral resolution is a basic tool to characterize...
Linear spectropolarimetry of spectral lines is a neglected field in astronomy, largely because of th...
Spectropolarimetry is nowadays one of the most used tool to investigate small scale (100 km) magneti...
Context. Progress in the solution to some of the most outstanding open problems of solar physics, su...
Ph.D. University of Hawaii at Manoa 2014.Includes bibliographical references.The dissertation focuse...
International audienceCurrent burning issues in stellar physics, for both hot and cool stars, concer...
DOI
Add to ORKG