activity
20122018
most citedPredicting the magnetic vectors within coronal mass ejections arriving at Earth: 1. Initial Architecture

83 citations · 387 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2017★ 61 cited

Planar magnetic structures in coronal mass ejection-driven sheath regions

Erika Palmerio, Emilia K. J. Kilpua, Neel P. Savani

Planar magnetic structures (PMSs) are periods in the solar wind during which interplanetary magnetic field vectors are nearly parallel to a single plane. One of the specific region…

astro-ph.SR2015★ 51 cited

Propagation of the 7 January 2014 CME and Resulting Geomagnetic Non-Event

M. L. Mays, B. J. Thompson, L. K. Jian +8

On 7 January 2014 an X1.2 flare and CME with a radial speed 2500 km s was observed from near an active region close to disk center. This led many forecasters to est…

astro-ph.SR2015★ 22 cited

Observational Tracking of the 2D Structure of Coronal Mass Ejections Between the Sun and 1 AU

Savani, N. P., Davies +18

The Solar TErrestrial RElations Observatory (STEREO) provides high cadence and high resolution images of the structure and morphology of coronal mass ejections (CMEs) in the inner…

astro-ph.SR2013★ 9 cited

A Plasma β Transition Within a Propagating Flux Rope

Neel P. Savani, A. Vourlidas, D. Shiota +4

We present a 2.5D MHD simulation of a magnetic flux rope (FR) propagating in the heliosphere and investigate the cause of the observed sharp plasma beta transition. Specifically, w…

astro-ph.SR2012★ 83 cited

Magnetic Field Configuration Models and Reconstruction Methods for Interplanetary Coronal Mass Ejections

N. Al-Haddad, T. Nieves-Chinchilla, N. P. Savani +6

This study aims to provide a reference to different magnetic field models and reconstruction methods for interplanetary coronal mass ejections (ICMEs). In order to understand the d…

astro-ph.SR2012★ 21 cited

A study of the Heliocentric dependence of Shock Standoff Distance and Geometry using 2.5D MHD Simulations of CME-driven shocks

Neel P. Savani, Daikou Shiota, Kanya Kusano +2

We perform four numerical magnetohydrodynamic simulations in 2.5 dimensions (2.5D) of fast Coronal Mass Ejections (CMEs) and their associated shock fronts between 10Rs and 300Rs. W…