activity
20192026
most citedBaryonic effects for weak lensing. Part I. Power spectrum and covariance matrix

85 citations · 760 across the 29 of their papers we have counts for

collaborators
Showing 2021Show all

10 papers · 1 filter

physics.geo-ph2021★ 21 cited

Forecasting GICs and geoelectric fields from solar wind data using LSTMs: application in Austria

R. L. Bailey, R. Leonhardt, C. Möstl +4

The forecasting of local GIC effects has largely relied on the forecasting of dB/dt as a proxy and, to date, little attention has been paid to directly forecasting the geoelectric…

astro-ph.SR2021★ 52 cited

Multipoint interplanetary coronal mass ejections observed with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind and STEREO-A

C. Möstl, A. J. Weiss, M. A. Reiss +12

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 (Sol…

astro-ph.SR2021★ 19 cited

Drag-based CME modeling with heliospheric images incorporating frontal deformation: ELEvoHI 2.0

J. Hinterreiter, T. Amerstorfer, M. Temmer +7

The evolution and propagation of coronal mass ejections (CMEs) in interplanetary space is still not well understood. As a consequence, accurate arrival time and arrival speed forec…

astro-ph.SR2021★ 7 cited

Predicting CMEs using ELEvoHI with STEREO-HI beacon data

Maike Bauer, Tanja Amerstorfer, Jürgen Hinterreiter +6

Being able to accurately predict the arrival of coronal mass ejections (CMEs) at Earth has been a long-standing problem in space weather research and operations. In this study, we…

physics.space-ph2021★ 25 cited

Machine learning for predicting the Bz magnetic field component from upstream in situ observations of solar coronal mass ejections

Martin A. Reiss, Christian Möstl, Rachel L. Bailey +6

Predicting the Bz magnetic field embedded within ICMEs, also known as the Bz problem, is a key challenge in space weather forecasting. We study the hypothesis that upstream in situ…

astro-ph.SR2021★ 29 cited

Solar origins of a strong stealth CME detected by Solar Orbiter

Jennifer O'Kane, Lucie M. Green, Emma E. Davies +6

Aims.We aim to locate the origin of a stealth coronal mass ejection (CME) detected in situ by the MAG instrument on board Solar Orbiter, and make connections between the CME observ…

astro-ph.SR2021★ 41 cited

Multi point analysis of coronal mass ejection flux ropes using combined data from Solar Orbiter, BepiColombo and Wind

A. J. Weiss, C. Moestl, E. E. Davies +15

The recent launch of Solar Orbiter and BepiColombo opened a brief window in which these two spacecraft were positioned in a constellation that allows for the detailed sampling of a…

astro-ph.SR2021★ 21 cited

Radial Evolution of the April 2020 Stealth Coronal Mass Ejection between 0.8 and 1 AU -- A Comparison of Forbush Decreases at Solar Orbiter and Earth

Johan L. Freiherr von Forstner, Mateja Dumbović, Christian Möstl +40

Aims. We present observations of the first coronal mass ejection (CME) observed at the Solar Orbiter spacecraft on April 19, 2020, and the associated Forbush decrease (FD) measured…

astro-ph.SR2021★ 19 cited

Why are ELEvoHI CME arrival predictions different if based on STEREO-A or STEREO-B heliospheric imager observations?

Jürgen Hinterreiter, Tanja Amerstorfer, Martin A. Reiss +9

Accurate forecasting of the arrival time and arrival speed of coronal mass ejections (CMEs) is a unsolved problem in space weather research. In this study, a comparison of the pred…

astro-ph.SR2021★ 35 cited

CME Magnetic Structure and IMF Preconditioning Affecting SEP Transport

Erika Palmerio, Emilia K. J. Kilpua, Olivier Witasse +15

Coronal mass ejections (CMEs) and solar energetic particles (SEPs) are two phenomena that can cause severe space weather effects throughout the heliosphere. The evolution of CMEs,…