English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

In this paper, we review the preliminary results on the propagation effectsand interplanetary consequences of fast and wide coronal mass ejection (CME)events, occurred during 18--25 June 2015, in the Sun-Earth distance range. Theinterplanetary scintillation (IPS) images reveal that the large-scalestructures of CME-driven disturbances filled nearly the entire innerheliosphere with a range of speeds, $\sim$300--1000 {\kmps}. The comparison ofspeed data sets, from IPS technique results in the inner heliosphere and {\itin-situ} measurements at 1 AU, indicates that the drag force imposed by thelow-speed wind dominated heliosphere on the propagation of CMEs may not beeffective. The arrival of shocks at 1 AU suggests that a shock can be driven inthe interplanetary medium by the central part of the moving CME and also by adifferent part away from its centre. The increased flux of proton at energies$>$10 MeV is consistent with the acceleration of particles by the shock aheadof the CME.

Interplanetary Consequences of Coronal Mass Ejection Events occurred during 18--25 June 2015