112 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Goddard Space Flight CenterUS10 papers
- Catholic University of AmericaUS4 papers
- University of MichiganUS4 papers
- GeoSphere Austria3 papers
- University of GrazAT3 papers
- University of New HampshireUS3 papers
- Central Institution for Meteorology and GeodynamicsAT2 papers
- HeliophysicsUS2 papers
- University of AmericaUS2 papers
- University of California, BerkeleyUS2 papers
- Adnet Systems (United States)US1 paper
- Aryabhatta Research Institute of Observational SciencesIN1 paper
10 papers
Investigating potential benefits of future sub-L1 missions with STEREO-A
Eva Weiler, Emma E. Davies, Christian Möstl +4
We present the first statistical study of geomagnetic storm forecasting using in situ data from the STEREO-A spacecraft as a sub-L1 monitor. Between November 2022 and June 2024, ST…
First observations of a geomagnetic superstorm with a sub-L1 monitor
Eva Weiler, Christian Möstl, Emma E. Davies +10
Forecasting the geomagnetic effects of solar coronal mass ejections (CMEs) is currently an unsolved problem. CMEs, responsible for the largest values of the north-south component o…
Probing Velocity Dispersion inside CMEs in Inner Corona: New Insights on CME Initiation
Satabdwa Majumdar, Elke D' Huys, Marilena Mierla +4
This work studies the kinematics of the leading edge and the core of 6 Coronal Mass Ejections (CMEs) in the combined field of view of Sun Watcher using Active Pixel System detector…
Flux rope modeling of the 2022 Sep 5 CME observed by Parker Solar Probe and Solar Orbiter from 0.07 to 0.69 au
Emma E. Davies, Hannah T. Rüdisser, Ute V. Amerstorfer +19
As both Parker Solar Probe (PSP) and Solar Orbiter (SolO) reach heliocentric distances closer to the Sun, they present an exciting opportunity to study the structure of CMEs in the…
Which Upstream Solar Wind Conditions Matter Most in Predicting Bz within Coronal Mass Ejections
Pete Riley, M. A. Reiss, C. Mostl
Accurately predicting the z-component of the interplanetary magnetic field, particularly during the passage of an interplanetary coronal mass ejection (ICME), is a crucial objectiv…
Kamodo: Simplifying Model Data Access and Utilization
Rebecca Ringuette, Lutz Rastaetter, Darren De Zeeuw +2
To address the lack of user-friendly software needed to simplify the utilization of model data across Heliophysics, the Community Coordinated Modeling Center (CCMC) at NASA Goddard…
Writhed Analytical Magnetic Flux Rope Model
Andreas J. Weiss, Teresa Nieves-Chinchilla, Christian Möstl +3
Observations of magnetic clouds, within interplanetary coronal mass ejections (ICMEs), are often well described by flux rope models. Most of these assume either a cylindrical or to…
The STONE curve: A ROC-derived model performance assessment tool
Michael W. Liemohn, Abigail R. Azari, Natalia Ganushkina +1
A new model validation and performance assessment tool is introduced, the sliding threshold of observation for numeric evaluation (STONE) curve. It is based on the relative operati…
Toward Quantitative Model for Simulation and Forecast of Solar Energetic Particles Production during Gradual Events - I: Magnetohydrodynamic Background Coupled to the SEP Model
D. Borovikov, I. V. Sokolov, I. Roussev +2
Solar Energetic Particles (SEPs) are an important aspect of space weather. SEP events posses a high destructive potential, since they may cause disruptions of communication systems…
Data Constrained Coronal Mass Ejections in A Global Magnetohydrodynamics Model
M. Jin, W. B. Manchester, B. van der Holst +6
We present a first-principles-based coronal mass ejection (CME) model suitable for both scientific and operational purposes by combining a global magnetohydrodynamics (MHD) solar w…