Observations of the four Stokes parameters of a 430 MHz flare from the UV Ceti-type star AD Leonis are presented. The maximum amplitude of the event was 0.52 flux units and the durations at one-half and one-tenth maximum were 12 and 40 seconds, respectively. The degree of circular polarization at maximum intensity was approximately 56 percent and was later observed to be as high as 92 percent. Linear polarization was also observed at a level of about 21 percent at flare maximum which allowed an upper limit of 440 radians - sq m to be placed on the rotation measure
We present optical and near-IR linear polarimetry of V404 Cyg during its 2015 outburst and in quiesc...
The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio ...
We examine spectropolarimetric data from the Coronal Multi-channel Polarimeter (CoMP) instrument, ac...
We have detected four flares from UV Ceti at 154 MHz using the Murchison Widefield Array. The flares...
Sgr A* is variable at radio and submillimeter wavelengths on hourly timescales, showing time delays ...
The degree of linear polarization in solar flares has not yet been precisely determined despite mult...
The pioneering observational work in solar flare X-ray polarimetry was done in a series of satellite...
The goal for the SAMEX magnetograph's optical system is to accurately measure the polarization state...
We report Atacama Large Millimeter Array (ALMA) Band 6 full-polarization observations of the lensed ...
We searched for linear polarization in the H alpha line using the Stokes Polarimeter at Mees Solar O...
Instrumentation has been developed to measure the normalized V Stokes vector coincident with the Q a...
The progressive phases of three solar flares have beenobserv ed with THEMIS in July 2000, using the ...
Context. The impact polarization of optical chromospheric lines in solar flares is still b...
We report the results of a high temporal resolution spectroscopic monitoring of the flare star AD Le...
International audienceWe report here on the temporal and spatial evolution of the impact polarizatio...
We present optical and near-IR linear polarimetry of V404 Cyg during its 2015 outburst and in quiesc...
The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio ...
We examine spectropolarimetric data from the Coronal Multi-channel Polarimeter (CoMP) instrument, ac...
We have detected four flares from UV Ceti at 154 MHz using the Murchison Widefield Array. The flares...
Sgr A* is variable at radio and submillimeter wavelengths on hourly timescales, showing time delays ...
The degree of linear polarization in solar flares has not yet been precisely determined despite mult...
The pioneering observational work in solar flare X-ray polarimetry was done in a series of satellite...
The goal for the SAMEX magnetograph's optical system is to accurately measure the polarization state...
We report Atacama Large Millimeter Array (ALMA) Band 6 full-polarization observations of the lensed ...
We searched for linear polarization in the H alpha line using the Stokes Polarimeter at Mees Solar O...
Instrumentation has been developed to measure the normalized V Stokes vector coincident with the Q a...
The progressive phases of three solar flares have beenobserv ed with THEMIS in July 2000, using the ...
Context. The impact polarization of optical chromospheric lines in solar flares is still b...
We report the results of a high temporal resolution spectroscopic monitoring of the flare star AD Le...
International audienceWe report here on the temporal and spatial evolution of the impact polarizatio...
We present optical and near-IR linear polarimetry of V404 Cyg during its 2015 outburst and in quiesc...
The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio ...
We examine spectropolarimetric data from the Coronal Multi-channel Polarimeter (CoMP) instrument, ac...