activity
20092026
most citedPrediction of Geomagnetic Storm Strength from Inner Heliospheric In Situ Observations

43 citations · 87 across the 4 of their papers we have counts for

collaborators

5 papers

physics.space-ph2026

Structure of energy flux densities in Earth's magnetotail reconnection regions: Bridging simulation and observation

Cara L. Waters, Jonathan P. Eastwood, Harry C. Lewis +5

Magnetic reconnection is important in both space and laboratory contexts because it changes the topology of magnetic fields and converts magnetic energy into particle energies. Est…

astro-ph.IM2023

Multi-point Assessment of the Kinematics of Shocks (MAKOS): A Heliophysics Mission Concept Study

Katherine A. Goodrich, Lynn B. Wilson, Steven Schwartz +6

Collisionless shocks are fundamental processes that are ubiquitous in space plasma physics throughout the Heliosphere and most astrophysical environments. Earth's bow shock and int…

astro-ph.SR2020★ 19 cited

CMEs in the Heliosphere: III. A Statistical Analysis of the Kinematic Properties Derived from Stereoscopic Geometrical Modelling Techniques Applied to CMEs Detected in the Heliosphere from 2008 to 2014 by STEREO/HI-1

D. Barnes, J. A. Davies, R. A. Harrison +10

We present an analysis of coronal mass ejections (CMEs) observed by the Heliospheric Imagers (HIs) on board NASA's Solar Terrestrial Relations Observatory (STEREO) spacecraft. Betw…

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…

astro-ph.SR2009★ 25 cited

On the Brightness and Waiting-time Distributions of a Type III Radio Storm observed by STEREO/WAVES

J. P. Eastwood, M. S. Wheatland, H. S. Hudson +5

Type III solar radio storms, observed at frequencies below approximately 16 MHz by space borne radio experiments, correspond to the quasi-continuous, bursty emission of electron be…