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19992025
most citedGlobal Energetics of Thirty-Eight Large Solar Eruptive Events

491 citations · 6.8k across the 109 of their papers we have counts for

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physics.space-ph2020★ 20 cited

Propagating Conditions and the Time of ICMEs Arrival: A Comparison of the Effective Acceleration Model with ENLIL and DBEM Models

Evangelos Paouris, Jasa Calogovic, Mateja Dumbovic +5

The Effective Acceleration Model (EAM) predicts the Time-of-Arrival (ToA) of the Coronal Mass Ejection (CME) driven shock and the average speed within the sheath at 1 AU. The model…

physics.space-ph2014★ 121 cited

Three-dimensional evolution of flux rope CMEs and its relation to the local orientation of the heliospheric current sheet

Alexey Isavnin, Angelos Vourlidas, Emilia K. J. Kilpua

Flux ropes (FRs) ejected from the Sun may change their geometrical orientation during their evolution which directly affects their geoeffectiveness. Therefore, it is crucial to und…

physics.space-ph2009★ 67 cited

Solar-Terrestrial Simulation in the STEREO Era: The January 24-25, 2007 Eruptions

N. Lugaz, A. Vourlidas, I. I. Roussev +1

The SECCHI instruments aboard the recently launched STEREO spacecraft enable for the first time the continuous tracking of coronal mass ejections (CMEs) from the Sun to 1 AU. We an…

physics.space-ph2008★ 36 cited

The Brightness of Density Structures at Large Solar Elongation Angles: What is Being Observed by STEREO/SECCHI?

N. Lugaz, A. Vourlidas, I. I. Roussev +3

We discuss features of coronal mass ejections (CMEs) that are specific to heliospheric observations at large elongation angles. Our analysis is focused on a series of two eruptions…