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Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images
DOI: 10.1007/s11207-024-02370-3 Bibcode: 2025SoPh..300....4V

Susino, Roberto; Romoli, Marco; Burtovoi, Aleksandr +15 more

The Metis coronagraph onboard Solar Orbiter and the LASCO-C2 coronagraph onboard SoHO both acquire white light polarized brightness (pB) images of the solar corona. When the Sun–Solar Orbiter distance is less than 0.85 AU, i.e., outside orbital segments around aphelia, the range of elongations covered by the fields-of-view of the two instruments o…

2025 Solar Physics
SOHO SolarOrbiter 0
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind
DOI: 10.1007/s11207-024-02300-3 Bibcode: 2024SoPh..299...54W

Wang, Y. -M.

The tendency for low-speed solar wind to show greater spatiotemporal variability and different compositional properties from high-speed wind has led to the prevailing idea of a bimodal solar wind, in which fast wind comes from coronal holes and slow wind comes from coronal streamers. We present observational evidence that most of the slow wind ori…

2024 Solar Physics
SolarOrbiter 7
Multiwavelength Observations of Quasiperiodic Pulsations in the Impulsive Phase of an Eruptive Flare with the Hard X-Ray Imager On Board ASO-S and Other Instruments
DOI: 10.1007/s11207-024-02272-4 Bibcode: 2024SoPh..299...30S

Chen, Wei; Warmuth, Alexander; Su, Yang +7 more

We investigated the quasiperiodic pulsations (QPPs) of the X1.2 solar flare (SOL2023-01-06T00:57) based on multi-instrument observations, especially the Hard X-ray Imager (HXI) on board the Advanced Space-based Solar Observatory (ASO-S). The quasiperiod of ≈27 s was identified in hard X-rays (HXR) and microwaves using the Markov Chain Monte Carlo …

2024 Solar Physics
SolarOrbiter 3
Tomography of the Solar Corona with the Metis Coronagraph II: Three-Dimensional Reconstructions of the Electron Density and Comparison with Reconstructions Based on LASCO-C2
DOI: 10.1007/s11207-024-02410-y Bibcode: 2024SoPh..299..165V

Susino, Roberto; Romoli, Marco; De Leo, Yara +13 more

We carried out tomographic reconstructions of the three-dimensional distribution of the electron density of the solar corona based on white light polarized brightness (pB) images taken by the Metis coronagraph on board the Solar Orbiter (SolO) mission. We selected three different time intervals during 2022, and further implemented independent sync…

2024 Solar Physics
SolarOrbiter 2
Spectral and Imaging Observations of a C2.3 White-Light Flare from the Advanced Space-Based Solar Observatory (ASO-S) and the Chinese HαSolar Explorer (CHASE)
DOI: 10.1007/s11207-024-02313-y Bibcode: 2024SoPh..299...73L

Lei, Shijun; Chen, Wei; Feng, Li +27 more

Solar white-light flares are characterized by an enhancement in the optical continuum, which are usually large flares (X- and M-class flares). Here, we report a small C2.3 white-light flare (SOL2022-12-20T04:10) observed by the Advanced Space-based Solar Observatory and the Chinese HαSolar Explorer (CHASE). This flare exhibits an increase of ≈ 6.4…

2024 Solar Physics
SolarOrbiter 1
Triangulation of Hard X-Ray Sources in an X-Class Solar Flare with ASO-S/HXI and Solar Orbiter/STIX
DOI: 10.1007/s11207-024-02341-8 Bibcode: 2024SoPh..299..114R

Massa, Paolo; Krucker, Säm; Chen, Wei +4 more

HXI on ASO-S and STIX onboard Solar Orbiter are the first simultaneously operating solar hard X-ray imaging spectrometers. ASO-S's low Earth orbit and Solar Orbiter's periodic displacement from the Sun–Earth line enables multi-viewpoint solar hard X-ray spectroscopic imaging analysis for the first time. Here, we demonstrate the potential of this n…

2024 Solar Physics
SolarOrbiter 1
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence
DOI: 10.1007/s11207-024-02336-5 Bibcode: 2024SoPh..299...89X

Feng, Li; Lu, Lei; Li, Qiao +31 more

Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here, we present two failed prominence eruptions on 26 October 2022 and explore their connections. Using stereoscopic observations, the South prominence (PRO-S) erupts with untwisting motions, flare ribbons occ…

2024 Solar Physics
SolarOrbiter 1
Asymmetric Hard X-ray Radiation of Two Ribbons in a Thermal-Dominated C-Class Flare
DOI: 10.1007/s11207-024-02349-0 Bibcode: 2024SoPh..299..104S

Lei, Shijun; Feng, Li; Lu, Lei +26 more

The asymmetry in hard X-ray (HXR) emission at the footpoints (FPs) of flare loops is a ubiquitous feature closely associated with nonthermal electron transport. In this study, we analyze the asymmetric HXR radiation at two flare ribbons, which is thermal-dominated during a long-duration C4.4 flare that occurred on March 20, 2023, combining multi-v…

2024 Solar Physics
SolarOrbiter 1
Kink-and-Disconnection Failed Eruption in 3D
DOI: 10.1007/s11207-024-02325-8 Bibcode: 2024SoPh..299...81M

Chen, Wei; Gan, Weiqun; Mrozek, Tomasz +4 more

We present a case study of a failed eruption that accompanied an M1.5 GOES class solar flare. It was observed by STIX onboard Solar Orbiter, HXI onboard the Advanced Space-based Solar Observatory, AIA onboard Solar Dynamics Observatory, and WAVES onboard the STEREO-A. The important input is from stereoscopic hard X-ray (HXR) observations obtained …

2024 Solar Physics
SolarOrbiter 0
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations
DOI: 10.1007/s11207-024-02280-4 Bibcode: 2024SoPh..299...41R

Hirzberger, Johann; Solanki, Sami K.; Inhester, Bernd +1 more

The orbit of the Solar Orbiter mission carries it and the Polarimetric and Helioseismic Imager (PHI), which is onboard, away from the Sun–Earth line, opening up the first ever possibility of doing stereoscopy of solar photospheric structures. We present a method for a stereoscopic analysis of the height variations in the solar photosphere. This me…

2024 Solar Physics
SolarOrbiter 0