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keywords:(Coronal mass ejections)
Why are there stationary EIT wave fronts
Viewing radiation signatures of solar energetic particles in interplanetary space
Variation of SEP event occurrence with heliospheric magnetic field magnitudes
Variability of solar eruptions during cycle 23
Two energy release processes for CMEs: MHD catastrophe and magnetic reconnection
Two candidate homologous CMEs on 2002 May 22
Trends and characteristics of high-frequency type II bursts detected by CALLISTO spectrometers
Transit time of CME/shock associated with four major geo-effective CMEs in solar cycle 24
The STEREO heliospheric imager: how to detect CMEs in the heliosphere
The speed of halo Coronal Mass Ejections and properties of associated active regions
The Solar Terrestrial Relations Observatory (STEREO) Education and Outreach (E/PO) Program
The scaler mode in the Pierre Auger Observatory to study heliospheric modulation of cosmic rays
The Plasma and Suprathermal Ion Composition (PLASTIC) Investigation on the STEREO Observatories
The Low-Energy Telescope (LET) and SEP Central Electronics for the STEREO Mission