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Unexpected major geomagnetic storm caused by faint eruption of a solar trans-equatorial flux rope
DOI: 10.1038/s41467-024-53538-1 Bibcode: 2024NatCo..15.9198T

Zhang, Qingmin; Ji, Haisheng; Su, Yingna +1 more

Some geomagnetic storms' solar origins are ambiguous, making them hard to predict. On March 23, 2023, a severe geomagnetic storm occurred, however, forecasts based on remote-sensing observations failed to predict it. Here, we show clear evidence that this storm originates from the eruption of a trans-equatorial, longitudinal and low-density magnet…

2024 Nature Communications
Hinode SOHO SolarOrbiter 1
Ultra-high-resolution observations of persistent null-point reconnection in the solar corona
DOI: 10.1038/s41467-023-37888-w Bibcode: 2023NatCo..14.2107C

Barczynski, K.; Peter, H.; Chitta, L. P. +21 more

Magnetic reconnection is a key mechanism involved in solar eruptions and is also a prime possibility to heat the low corona to millions of degrees. Here, we present ultra-high-resolution extreme ultraviolet observations of persistent null-point reconnection in the corona at a scale of about 390 km over one hour observations of the Extreme-Ultravio…

2023 Nature Communications
IRIS SolarOrbiter 28
Polarisation of decayless kink oscillations of solar coronal loops
DOI: 10.1038/s41467-023-41029-8 Bibcode: 2023NatCo..14.5298Z

Antolin, Patrick; Berghmans, David; Chitta, Lakshmi Pradeep +4 more

Decayless kink oscillations of plasma loops in the solar corona may contain an answer to the enigmatic problem of solar and stellar coronal heating. The polarisation of the oscillations gives us a unique information about their excitation mechanisms and energy supply. However, unambiguous determination of the polarisation has remained elusive. Her…

2023 Nature Communications
SolarOrbiter 19
BepiColombo mission confirms stagnation region of Venus and reveals its large extent
DOI: 10.1038/s41467-022-35061-3 Bibcode: 2022NatCo..13.7743P

André, N.; Fedorov, A.; Barabash, S. +42 more

The second Venus flyby of the BepiColombo mission offer a unique opportunity to make a complete tour of one of the few gas-dynamics dominated interaction regions between the supersonic solar wind and a Solar System object. The spacecraft pass through the full Venusian magnetosheath following the plasma streamlines, and cross the subsolar stagnatio…

2022 Nature Communications
BepiColombo SolarOrbiter 4