Evolution of Coronal Mass Ejections in the Inner Heliosphere: A Study Using White-Light and Scintillation Images

174 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model (2013, methodology): “(2005) and the 30-event sample prepared by Manoharan (2006). Note that we consider only the arrival of the front boundary of the ejecta (not the ICME-driven shock).”
Ensemble Modeling of CMEs Using the WSA–ENLIL+Cone Model (2015, background): “Another improvement could be the use of real-time interplanetary scintillation (IPS) observations by the Ooty Radio Telescope (Manoharan, 2006).”
COMBINED STEREO/RHESSI STUDY OF CORONAL MASS EJECTION ACCELERATION AND PARTICLE ACCELERATION IN SOLAR FLARES (2010, background): “After the magnetic driving force of the eruption ceases, the CME is slowed down by the drag force until its velocity adjusts to the speed of the solar wind (e.g. Cargill 2004; Manoharan 2006; Vršnak et al. 2008, and references therein).”
The Physical Processes of CME/ICME Evolution (2017, background): “Later on, Manoharan et al. (2004), Manoharan (2006), and Gopalswamy (2009) extended the a(VCME) relationship to 2nd-degree polynomial forms.”