We present a case study of an M4-class flare on 28 March 2022, near Solar Orbiter's first science perihelion (0.33 AU). Solar Orbiter was 83.5{\deg} west of the Sun-Earth line, making the event appear near the eastern limb, while Earth-orbiting spacecraft observed it near the disk center. The timing and location of the STIX X-ray sources were related to the plasma evolution observed in the EUV by the Extreme Ultraviolet Imager (EUI) on Solar Orbiter and the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory, and to the chromospheric response observed in 1600 {\AA} by AIA. We performed differential emission measure (DEM) analysis to further characterize the flaring plasma at different subvolumes. The pre-flare magnetic fiel...
We present SDO/AIA observations of an eruptive X-class flare of 2012 July 12, and compare its evolut...
Context. Coordinated observations of a GOES B4.8 microflare with SDO’s Atmospheric Imaging...
Solar flares are one of the most energetic events in the solar system, created by the explosive conv...
CONTEXT: The Solar Orbiter mission completed its first remote-sensing observation windows in the s...
MMW and SD acknowledge STFC for support via their PhD Studentships. DML is an Early-Career Fellow, f...
We present an analysis of multi-instrument space- and ground-based observations relevant to a C4.1 s...
P.S acknowledges financial support from the programme Aristotelis/SIEMENS at the NOA.Aims: We presen...
Context. The energy release in eruptive flares and the kinematics of the associated coronal mass eje...
A solar flare is composed of impulsive energy release events by magnetic reconnection, which forms a...
<p>We investigate the release of magnetic energy stored within the solar atmosphere, the driving for...
Context. During its commissioning phase in 2020, the Spectrometer/Telescope for Imaging X-rays (STIX...
We conduct a detailed analysis of an M1.3 limb flare occurring on 2017 July 3, which have the X-ray ...
Context. We present an analysis of a GOES M1.8 flare with excellent observational coverage in UV, ex...
Context. The Spectrometer/Telescope for Imaging X-rays (STIX) is the hard X-ray instrument onboard S...
Context. The Sun is very quiet with less sunspots and activity since the beginning of solar cycle 24...
We present SDO/AIA observations of an eruptive X-class flare of 2012 July 12, and compare its evolut...
Context. Coordinated observations of a GOES B4.8 microflare with SDO’s Atmospheric Imaging...
Solar flares are one of the most energetic events in the solar system, created by the explosive conv...
CONTEXT: The Solar Orbiter mission completed its first remote-sensing observation windows in the s...
MMW and SD acknowledge STFC for support via their PhD Studentships. DML is an Early-Career Fellow, f...
We present an analysis of multi-instrument space- and ground-based observations relevant to a C4.1 s...
P.S acknowledges financial support from the programme Aristotelis/SIEMENS at the NOA.Aims: We presen...
Context. The energy release in eruptive flares and the kinematics of the associated coronal mass eje...
A solar flare is composed of impulsive energy release events by magnetic reconnection, which forms a...
<p>We investigate the release of magnetic energy stored within the solar atmosphere, the driving for...
Context. During its commissioning phase in 2020, the Spectrometer/Telescope for Imaging X-rays (STIX...
We conduct a detailed analysis of an M1.3 limb flare occurring on 2017 July 3, which have the X-ray ...
Context. We present an analysis of a GOES M1.8 flare with excellent observational coverage in UV, ex...
Context. The Spectrometer/Telescope for Imaging X-rays (STIX) is the hard X-ray instrument onboard S...
Context. The Sun is very quiet with less sunspots and activity since the beginning of solar cycle 24...
We present SDO/AIA observations of an eruptive X-class flare of 2012 July 12, and compare its evolut...
Context. Coordinated observations of a GOES B4.8 microflare with SDO’s Atmospheric Imaging...
Solar flares are one of the most energetic events in the solar system, created by the explosive conv...