This paper will review the input of 65 years of radio observations to our understanding of
solar and solar–terrestrial physics. It is focussed on the radio observations of phenomena …

Coronal mass ejections (CMEs) play an important role in space weather. The propagation
characteristics of CMEs in the Corona and interplanetary space determine whether, when …

In a previous study (Cane and Richardson, J. Geophys. Res. 108 (A4), SSH6-1, 2003), we
investigated the occurrence of interplanetary coronal mass ejections in the near-Earth solar …

Abstract We present the “Drag-Based Model”(DBM) of heliospheric propagation of
interplanetary coronal mass ejections (ICMEs). The DBM is based on the hypothesis that the …

We analyze the relationship between the coronal hole (CH) area/position and physical
characteristics of the associated corotating high-speed stream (HSS) in the solar wind at 1 …

We describe a geometric triangulation technique, based on time–elongation maps
constructed from imaging observations, to track coronal mass ejections (CMEs) continuously …

Context. The propagation of interplanetary coronal mass ejections (ICMEs) and the forecast
of their arrival on Earth is one of the central issues of space weather studies. Aims. We …

Aims. The Sun-Earth transit time of interplanetary coronal mass ejections (ICMEs) is one of
central issues of space weather forecasting. Our aim is to find out to what degree the ICME …

In this study, we use an ice‐cream cone model to analyze the geometrical and kinematical
properties of the coronal mass ejections (CMEs). Assuming that in the early phase CMEs …

The kinematics of CMEs are well characterized to 32 R☉ by height-time measurements from
existing space-based and ground-based coronagraphs. Although there has been long …