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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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astro-ph.SR2026

Tracking a solar energetic eruption and associated energetic particles from Sun to spacecraft

D. E. Morosan, M. Baumgartner-Steinleitner, K. Bhandari +17

Context. Solar energetic particles (SEPs) in the heliosphere are produced by flaring processes on the Sun or shocks driven by coronal mass ejections (CMEs). Electrons, in particula…

astro-ph.SR2026

Integration of a CME Flux Rope Model with Magnetic Field Draping in Heliospheric Simulations

Ranadeep Sarkar, Jens Pomoell, Emilia Kilpua +1

Accurate prediction of the magnetic structure of interplanetary coronal mass ejections (ICMEs) remains a key challenge in space weather forecasting. Despite several efforts using g…

astro-ph.SR2026

Tracing magnetic flux rope footpoints in AR 12975 with coronal dimmings and data-driven magnetofrictional simulations

Andreas Wagner, Amaia Razquin, Astrid M. Veronig +3

Coronal mass ejections (CMEs) are driven by the eruption of magnetic flux ropes (MFRs) whose footpoints are often observed indirectly as coronal dimming regions. However, the relat…

astro-ph.SR2026

Spectral properties of mesoscale fluctuations in interplanetary coronal mass ejections

Anna-Sofia Jylhä, Simon Good, Emilia Kilpua

Magnetic fields in interplanetary coronal mass ejections (ICMEs) often display a flux rope structure at large scales and a turbulent cascade of fluctuations at smaller scales. Howe…

astro-ph.SR2026

Radial and angular evolution of magnetic cloud signatures in the turbulent solar wind: virtual spacecraft analysis

M. Sangalli, E. K. J. Kilpua, A. Verdini +3

Interplanetary coronal mass ejections (ICMEs) carry magnetic clouds (MCs), large-scale structures with average radial widths about a fifth of an astronomical unit at Earth's orbit.…

astro-ph.SR2026

The Correlation Length of Turbulence in Magnetic Clouds

S. W. Good, J. Lalueza Puértolas, A. -S. M. Jylhä +1

The large-scale limit or outer scale of turbulence in the solar wind is associated with the correlation length of the magnetic field. Determining correlation lengths from magnetic…