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Multipoint Interplanetary Coronal Mass Ejections Observed with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind, and STEREO-A
DOI: 10.3847/2041-8213/ac42d0 Bibcode: 2022ApJ...924L...6M

Möstl, Christian; Davies, Emma E.; Freiherr von Forstner, Johan L. +12 more

We report the result of the first search for multipoint in situ and imaging observations of interplanetary coronal mass ejections (ICMEs) starting with the first Solar Orbiter (SolO) data in 2020 April-2021 April. A data exploration analysis is performed including visualizations of the magnetic-field and plasma observations made by the five spacec…

2022 The Astrophysical Journal
BepiColombo SOHO SolarOrbiter 40
Observation of a Magnetic Switchback in the Solar Corona
DOI: 10.3847/2041-8213/ac8104 Bibcode: 2022ApJ...936L..25T

Telloni, Daniele; Zank, Gary P.; Adhikari, Laxman +58 more

Switchbacks are sudden, large radial deflections of the solar wind magnetic field, widely revealed in interplanetary space by the Parker Solar Probe. The switchbacks' formation mechanism and sources are still unresolved, although candidate mechanisms include Alfvénic turbulence, shear-driven Kelvin-Helmholtz instabilities, interchange reconnection…

2022 The Astrophysical Journal
SolarOrbiter 38
The first widespread solar energetic particle event of solar cycle 25 on 2020 November 29. Shock wave properties and the wide distribution of solar energetic particles
DOI: 10.1051/0004-6361/202142515 Bibcode: 2022A&A...660A..84K

Lario, D.; Vainio, R.; Kilpua, E. K. J. +13 more

Context. On 2020 November 29, an eruptive event occurred in an active region located behind the eastern solar limb as seen from Earth. The event consisted of an M4.4 class flare, a coronal mass ejection, an extreme ultraviolet (EUV) wave, and a white-light (WL) shock wave. The eruption gave rise to the first widespread solar energetic particle (SE…

2022 Astronomy and Astrophysics
SOHO SolarOrbiter 32
The relativistic solar particle event on 28 October 2021: Evidence of particle acceleration within and escape from the solar corona
DOI: 10.1051/0004-6361/202243903 Bibcode: 2022A&A...663A.173K

Krucker, Säm; Dresing, Nina; Klein, Karl-Ludwig +6 more


Aims: We analyse particle, radio, and X-ray observations during the first relativistic proton event of solar cycle 25 detected on Earth. The aim is to gain insight into the relationship between relativistic solar particles detected in space and the processes of acceleration and propagation in solar eruptive events.
Methods: To this end, …

2022 Astronomy and Astrophysics
SOHO SolarOrbiter 32
Flux rope and dynamics of the heliospheric current sheet. Study of the Parker Solar Probe and Solar Orbiter conjunction of June 2020
DOI: 10.1051/0004-6361/202142381 Bibcode: 2022A&A...659A.110R

Fedorov, A.; Parenti, S.; Lavraud, B. +19 more

Context. Solar Orbiter and Parker Solar Probe jointly observed the solar wind for the first time in June 2020, capturing data from very different solar wind streams: calm, Alfvénic wind and also highly dynamic large-scale structures. Context. Our aim is to understand the origin and characteristics of the highly dynamic solar wind observed by the t…

2022 Astronomy and Astrophysics
SolarOrbiter 30
Solar coronal heating from small-scale magnetic braids
DOI: 10.1051/0004-6361/202244170 Bibcode: 2022A&A...667A.166C

Barczynski, K.; Peter, H.; Chitta, L. P. +19 more

Relaxation of braided coronal magnetic fields through reconnection is thought to be a source of energy to heat plasma in active region coronal loops. However, observations of active region coronal heating associated with an untangling of magnetic braids remain sparse. One reason for this paucity could be the lack of coronal observations with a suf…

2022 Astronomy and Astrophysics
Hinode SolarOrbiter 30
CMEs and SEPs During November-December 2020: A Challenge for Real-Time Space Weather Forecasting
DOI: 10.1029/2021SW002993 Bibcode: 2022SpWea..2002993P

Maksimovic, Milan; Möstl, Christian; Galvin, Antoinette B. +20 more

Predictions of coronal mass ejections (CMEs) and solar energetic particles (SEPs) are a central issue in space weather forecasting. In recent years, interest in space weather predictions has expanded to include impacts at other planets beyond Earth as well as spacecraft scattered throughout the heliosphere. In this sense, the scope of space weathe…

2022 Space Weather
MEx SOHO SolarOrbiter 29
The magnetic drivers of campfires seen by the Polarimetric and Helioseismic Imager (PHI) on Solar Orbiter
DOI: 10.1051/0004-6361/202142873 Bibcode: 2022A&A...660A.143K

Schmidt, W.; Woch, J.; Peter, H. +56 more

Context. The Extreme Ultraviolet Imager (EUI) on board the Solar Orbiter (SO) spacecraft observed small extreme ultraviolet (EUV) bursts, termed campfires, that have been proposed to be brightenings near the apexes of low-lying loops in the quiet-Sun atmosphere. The underlying magnetic processes driving these campfires are not understood.
Aim…

2022 Astronomy and Astrophysics
SolarOrbiter 29
What drives decayless kink oscillations in active-region coronal loops on the Sun?
DOI: 10.1051/0004-6361/202244403 Bibcode: 2022A&A...666L...2M

Teriaca, Luca; Solanki, Sami K.; Long, David M. +19 more

Here, we present a study of the phenomena of decayless kink oscillations in a system of active-region (AR) coronal loops. Using high-resolution observations from two different instruments, namely the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter and the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory, we follow…

2022 Astronomy and Astrophysics
SolarOrbiter 27
Two-spacecraft detection of short-period decayless kink oscillations of solar coronal loops
DOI: 10.1093/mnras/stac2545 Bibcode: 2022MNRAS.516.5989Z

Berghmans, David; Nakariakov, Valery M.; Verbeeck, Cis +2 more

Decayless kink oscillations of an ensemble of loops are captured simultaneously by the High Resolution Imager (HRI) of the Extreme Ultraviolet Imager (EUI) and the Atmospheric Imaging Assembly (AIA) from 22:58 UT on 2021 November 5 to 00:27 UT on 2021 November 6. Oscillations are analysed by processing image sequences taken by the two instruments …

2022 Monthly Notices of the Royal Astronomical Society
SolarOrbiter 26