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keywords:(Coronal mass ejections)
Testing the asymmetric cone model for halo CMEs using STEREO/SECCHI coronagraphic observations
Large non-radial propagation of a coronal mass ejection on 2011 January 24
Trends and characteristics of high-frequency type II bursts detected by CALLISTO spectrometers
The characteristics of flare- and CME-productive solar active regions
Particle acceleration and transport at an oblique CME-driven shock
Separating the effects of earthside and far side solar events. A case study
CME–flare association during the 23rd solar cycle
A statistical study of post-flare-associated CME events
Flux emergence and generation of flare-productive active regions
Some characteristics of Coronal Mass Ejections associated with Prominence Eruptions
Coronal mass ejections: Solar cycle aspects
Transit time of CME/shock associated with four major geo-effective CMEs in solar cycle 24
Analyzing deflection of multiple Solar Coronal Mass Ejections from the same active region
Implementation and validation of the FRi3D flux rope model in EUHFORIA
Large scale MHD properties of interplanetary magnetic clouds
Comparison of CME characteristics for SEP and non-SEP related events
Properties of structured coronal mass ejections in solar cycle 23
ICMEs and CIRs monitored in IPS data at a frequency of 111 MHz
Evolution of coronal mass ejections in the early stage
Comparison of force-free flux rope models with observations of magnetic clouds
An atlas of solar events: 1996-2005
Solar neutron events in association with large solar flares in November 2003
The scaler mode in the Pierre Auger Observatory to study heliospheric modulation of cosmic rays
Large-scale waves in the solar corona: The continuing debate
Objective CME detection over the solar cycle: A first attempt
Injection and propagation of solar protons to high heliospheric latitudes: Ulysses Ket observations
Two candidate homologous CMEs on 2002 May 22
Some features of the sources of relativistic particles at the Sun in the solar cycles 21-23
Composition and magnetic structure of interplanetary coronal mass ejections at 1AU
Coronal mass ejections associated with polar crown filaments
Why are there stationary EIT wave fronts
Field configuration around large flux ropes in the solar corona and inner heliosphere
Propagation of interplanetary shocks through the solar wind and magnetosheath