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20112026
most citedObservations of an extreme storm in interplanetary space caused by successive coronal mass ejections

298 citations · 3k across the 98 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR2022★ 20 cited

Shock-accelerated electrons during the fast expansion of a coronal mass ejection

D. E. Morosan, J. Pomoell, A. Kumari +2

Context. Some of of the most prominent sources for energetic particles in our Solar System are huge eruptions of magnetised plasma from the Sun called coronal mass ejections (CMEs)…

physics.space-ph2022★ 47 cited

Single-spacecraft techniques for shock parameters estimation: A systematic approach

Domenico Trotta, Laura Vuorinen, Heli Hietala +8

Spacecraft missions provide the unique opportunity to study the properties of collisionless shocks utilising in situ measurements. In the past years, several diagnostics have been…

physics.space-ph2022★ 30 cited

Multi-spacecraft observations of shocklets at an interplanetary shock

Domenico Trotta, Heli Hietala, Timothy Horbury +5

Interplanetary (IP) shocks are fundamental building blocks of the heliosphere, and the possibility to observe them \emph{in-situ} is crucial to address important aspects of energy…

physics.space-ph2022★ 14 cited

Small-scale flux ropes in ICME sheaths

J. Ruohotie, E. K. J. Kilpua, S. W. Good +1

Sheath regions of interplanetary coronal mass ejections (ICMEs) are formed when the upstream solar wind is deflected and compressed due to the propagation and expansion of the ICME…

physics.space-ph2022★ 17 cited

Cross helicity of interplanetary coronal mass ejections at 1 au

S. W. Good, L. M. Hatakka, M. Ala-Lahti +3

Interplanetary coronal mass ejections (ICMEs) contain magnetic field and velocity fluctuations across a wide range of scales. These fluctuations may be interpreted as Alfvénic wave…

astro-ph.SR2022

Eruption and Interplanetary Evolution of a Stealthy Streamer-Blowout CME Observed by PSP at 0.5~AU

Sanchita Pal, Benjamin J. Lynch, Simon W. Good +5

Streamer-blowout coronal mass ejections (SBO-CMEs) are the dominant CME population during solar minimum. Although they are typically slow and lack clear low-coronal signatures, the…