298 citations · 3k across the 98 of their papers we have counts for
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On the occurrence of type IV solar radio bursts in the solar cycle 24 and their association with coronal mass ejections
Anshu Kumari, D. E. Morosan, E. K. J. Kilpua
Solar activity, in particular coronal mass ejections (CMEs), are often accompanied by bursts of radiation at metre wavelengths. Some of these bursts have a long duration and extend…
On the Radial and Longitudinal Variation of a Magnetic Cloud: ACE, Wind, ARTEMIS and Juno Observations
E. E. Davies, R. J. Forsyth, S. W. Good +1
We present observations of the same magnetic cloud made near Earth by the Advance Composition Explorer (ACE), Wind, and the Acceleration, Reconnection, Turbulence and Electrodynami…
Electron acceleration and radio emission following the early interaction of two coronal mass ejections
D. E. Morosan, E. Palmerio, J. E. Räsänen +6
Context. Coronal mass ejections (CMEs) are large eruptions of magnetised plasma from the Sun that are often accompanied by solar radio bursts produced by accelerated electrons. Aim…
Cross Helicity of the November 2018 Magnetic Cloud Observed by the Parker Solar Probe
S. W. Good, E. K. J. Kilpua, M. Ala-Lahti +3
Magnetic clouds are large-scale transient structures in the solar wind with low plasma , low-amplitude magnetic field fluctuations, and twisted field lines with both ends often…
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…
Using radio triangulation to understand the origin of two subsequent type II radio bursts
Immanuel Christopher Jebaraj, Jasmina Magdalenic, Tatiana Podladchikova +7
Context: Eruptive events such as coronal mass ejections (CMEs) and flares accelerate particles and generate shock waves which can arrive at Earth and can disturb the magnetosphere.…