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20092026
most citedObservations of an extreme storm in interplanetary space caused by successive coronal mass ejections

298 citations · 2.9k across the 52 of their papers we have counts for

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15 papers · 1 filter

physics.space-ph2026★ 35 cited

A living catalog of stream interaction regions in the Parker Solar Probe era

R. C. Allen, G. C. Ho, L. K. Jian +15

Stream interaction regions (SIRs) and corotating interaction regions (CIRs) are important phenomena in heliospheric physics. These large-scale structures vary temporally and spatia…

physics.space-ph2023★ 21 cited

Using Solar Orbiter as an upstream solar wind monitor for real time space weather predictions

R. Laker, T. S. Horbury, H. O'Brien +11

Coronal mass ejections (CMEs) can create significant disruption to human activities and systems on Earth, much of which can be mitigated with prior warning of the upstream solar wi…

physics.space-ph2023★ 1 cited

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…

physics.space-ph2020★ 37 cited

Evaluation of CME Arrival Prediction Using Ensemble Modeling Based on Heliospheric Imaging Observations

Tanja Amerstorfer, Jürgen Hinterreiter, Martin A. Reiss +8

In this study, we evaluate a coronal mass ejection (CME) arrival prediction tool that utilizes the wide-angle observations made by STEREO's heliospheric imagers (HI). The unsurpass…

physics.space-ph2020★ 28 cited

Using gradient boosting regression to improve ambient solar wind model predictions

R. L. Bailey, M. A. Reiss, C. N. Arge +7

Studying the ambient solar wind, a continuous pressure-driven plasma flow emanating from our Sun, is an important component of space weather research. The ambient solar wind flows…

physics.space-ph2019★ 39 cited

Forecasting the Ambient Solar Wind with Numerical Models: I. On the Implementation of an Operational Framework

Martin A. Reiss, Peter J. MacNeice, Leila M. Mays +4

The ambient solar wind conditions in interplanetary space and in the near-Earth environment are determined by activity on the Sun. Steady solar wind streams modulate the propagatio…

physics.space-ph2019★ 11 cited

Tracking and Validating ICMEs Propagating Toward Mars Using STEREO Heliospheric Imagers Combined With Forbush Decreases Detected by MSL/RAD

Johan L. Freiherr von Forstner, Jingnan Guo, Robert F. Wimmer-Schweingruber +7

The Radiation Assessment Detector (RAD) instrument onboard the Mars Science Laboratory (MSL) mission's Curiosity rover has been measuring galactic cosmic rays (GCR) as well as sola…

physics.space-ph2019★ 81 cited

Generic magnetic field intensity profiles of interplanetary coronal mass ejections at Mercury, Venus and Earth from superposed epoch analyses

Miho Janvier, Reka Winslow, Simon Good +8

We study interplanetary coronal mass ejections (ICMEs) measured by probes at different heliocentric distances (0.3-1AU) to investigate the propagation of ICMEs in the inner heliosp…

physics.space-ph2018★ 6 cited

The Magnetic Field Geometry of Small Solar Wind Flux Ropes Inferred from their Twist Distribution

W. Yu, C. J. Farrugia, N. Lugaz +4

This work extends recent efforts on the force-free modeling of large flux rope-type structures (magnetic clouds, MCs) to much smaller spatial scales. We first select small flux rop…

physics.space-ph2018★ 31 cited

Correlation of ICME Magnetic Fields at Radially Aligned Spacecraft

S. W. Good, R. J. Forsyth, J. P. Eastwood +1

The B-field structures of two ICMEs each observed by a pair of spacecraft close to radial alignment have been analysed. The ICMEs were observed in situ by MESSENGER and STEREO-B in…

physics.space-ph2016★ 43 cited

Prediction of Geomagnetic Storm Strength from Inner Heliospheric In Situ Observations

M. Kubicka, C. Möstl, T. Amerstorfer +4

Prediction of the effects of coronal mass ejections (CMEs) on Earth strongly depends on knowledge of the interplanetary magnetic field southward component, Bz. Predicting the stren…

physics.space-ph2014★ 298 cited

Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections

Ying D. Liu, Janet G. Luhmann, Primož Kajdič +8

Space weather refers to dynamic conditions on the Sun and in the space environment of the Earth, which are often driven by solar eruptions and their subsequent interplanetary distu…

physics.space-ph2013★ 11 cited

Assessing the Constrained Harmonic Mean Method for Deriving the Kinematics of ICMEs with a Numerical Simulation

Tanja Rollett, Manuela Temmer, Christian Möstl +3

In this study we use a numerical simulation of an artificial coronal mass ejection (CME) to validate a method for calculating propagation directions and kinematical profiles of int…

physics.space-ph2012★ 172 cited

The Deflection of the Two Interacting Coronal Mass Ejections of 2010 May 23-24 as Revealed by Combined In situ Measurements and Heliospheric Imaging

N. Lugaz, C. J. Farrugia, J. A. Davies +4

In 2010 May 23-24, SDO observed the launch of two successive coronal mass ejections (CMEs), which were subsequently tracked by the SECCHI suite onboard STEREO. Using the COR2 coron…

physics.space-ph2010★ 113 cited

STEREO and Wind observations of a fast ICME flank triggering a prolonged geomagnetic storm on 5-7 April 2010

Christian Möstl, Manuela Temmer, Tanja Rollett +6

On 5 April 2010 an interplanetary (IP) shock was detected by the Wind spacecraft ahead of Earth, followed by a fast (average speed 650 km/s) IP coronal mass ejection (ICME). During…