Add to ORKGFlares are localized phenomena in active regions, but the magnetic and plasma responses may propagate to a larger area. In this work we investigate the temporal evolution of a flare in an active region with particular attention to the morphological details, and to the temperature and emission measure diagnostics allowed by Hinode/XRT
Abstract. In this paper we present the analysis of M 1.8 class (GOES SXR) limb flare and associated ...
Multiple ratios of Hinode/XRT filters showed evidence of a minor very hot emission measure component...
Context. Solar flares are associated with intense soft X-ray emission generated by the hot flaring p...
Flares are localized phenomena in active regions, but the magnetic and plasma responses may propagat...
Context. Flares are dynamic events which involve rapid changes in coronal magnetic topology end ener...
Context. Flares, eruptive prominences and coronal mass ejections are phenomena where magnetic reconn...
Context. We present observations of a B7.9-class flare that occurred on the 24th January, 2015, usin...
Aims.The aim of this paper is to understand the magnetic configuration and evolution of an active re...
Flare-prolific active region NOAA 12673 produced consecutive X2.2 and X9.3 flares on the 6 September...
In this paper we analyse an M 1.0 confined flare observed mainly during its gradual phase. We use th...
International audienceIn this paper we analyse an M 1.0 confined flare observed mainly during its gr...
Magnetohydrodynamic plasma turbulence is believed to play a vital role in the production of energeti...
We model in detail a flare observed on Proxima Centauri with the EPIC-PN on board XMM-Newton at high...
The interaction of magnetic structures and the conversion of magnetic free energy into heating of th...
Magnetohydrodynamic plasma turbulence is believed to play a vital role in the production of energeti...
Abstract. In this paper we present the analysis of M 1.8 class (GOES SXR) limb flare and associated ...
Multiple ratios of Hinode/XRT filters showed evidence of a minor very hot emission measure component...
Context. Solar flares are associated with intense soft X-ray emission generated by the hot flaring p...
Flares are localized phenomena in active regions, but the magnetic and plasma responses may propagat...
Context. Flares are dynamic events which involve rapid changes in coronal magnetic topology end ener...
Context. Flares, eruptive prominences and coronal mass ejections are phenomena where magnetic reconn...
Context. We present observations of a B7.9-class flare that occurred on the 24th January, 2015, usin...
Aims.The aim of this paper is to understand the magnetic configuration and evolution of an active re...
Flare-prolific active region NOAA 12673 produced consecutive X2.2 and X9.3 flares on the 6 September...
In this paper we analyse an M 1.0 confined flare observed mainly during its gradual phase. We use th...
International audienceIn this paper we analyse an M 1.0 confined flare observed mainly during its gr...
Magnetohydrodynamic plasma turbulence is believed to play a vital role in the production of energeti...
We model in detail a flare observed on Proxima Centauri with the EPIC-PN on board XMM-Newton at high...
The interaction of magnetic structures and the conversion of magnetic free energy into heating of th...
Magnetohydrodynamic plasma turbulence is believed to play a vital role in the production of energeti...
Abstract. In this paper we present the analysis of M 1.8 class (GOES SXR) limb flare and associated ...
Multiple ratios of Hinode/XRT filters showed evidence of a minor very hot emission measure component...
Context. Solar flares are associated with intense soft X-ray emission generated by the hot flaring p...