activity
20082026
most citedCME-CME Interactions as Sources of CME Geo-effectiveness: The Formation of the Complex Ejecta and Intense Geomagnetic Storm in Early September 2017

112 citations · 1.2k across the 62 of their papers we have counts for

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7 papers · 1 filter

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…

econ.GN2026

Participation, selection and indicative bidding in auctions with costly entry

Changxia Ke, Greg Kubitz, Yang Liu

We study auctions with costly entry in which bidders have incomplete information about their affiliated private valuations prior to entry. We examine whether indicative bidding--a…

astro-ph.SR2026

Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool

Markus Baumgartner-Steinleitner, Astrid M. Veronig, Karin Dissauer +1

We investigate the two-dimensional velocity field of the fast and complex large-scale coronal wave observed on September 6, 2011. We use both a classical perturbation profile appro…

astro-ph.SR2026

Magnetic Topology and Loop Statistics in Observed Coronal Holes Using Potential Field Modeling

Stephan G. Heinemann, Jens Pomoell, Manuela Temmer

Potential Field Source Surface (PFSS) models are widely used to study the solar corona and form the basis for solar wind forecasting, yet often fail to reproduce observed propertie…

astro-ph.SR2026

Turbulence-Driven Corrugation of Collisionless Fast-Magnetosonic Shocks

Immanuel Christopher Jebaraj, Mikhail Malkov, Nicolas Wijsen +4

Collisionless fast-magnetosonic shocks are often treated as smooth, planar boundaries, yet observations point to organized corrugation of the shock surface. A plausible driver is u…