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20082026
most citedA New Method of 3D Magnetic Field Reconstruction

53 citations · 119 across the 9 of their papers we have counts for

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physics.space-ph2026

Evolution of Coronal Mass Ejection Properties through Superposed Epoch Analysis from 0.2 to 2.2 au

Yakub Olufadi, Nada Al-Haddad, Florian Regnault +6

Coronal mass ejections (CMEs) are explosive and energetic events consisting of strong magnetic structures erupting from the solar corona. We use superposed epoch analysis to invest…

physics.space-ph2025

Influence of the Deformation of Coronal Mass Ejections on Their In-Situ Fitting with Circular-Cross-Section Flux Rope Models

Bin Zhuang, Noé Lugaz, Nada Al-Haddad +8

Understanding the properties, especially the magnetohydrodynamic (MHD) invariants, of coronal mass ejections (CMEs) measured in-situ is key to bridging the CME properties from the…

physics.space-ph2024

Can Alfvénic Fluctuations Affect the Correlation and Complexity of Magnetic Fields in Magnetic Ejecta? A Case Study Based on Multi-Spacecraft Measurements at 1~au

Camilla Scolini, Bin Zhuang, Noé Lugaz +4

We investigate whether Alfvénic fluctuations (AFs) can affect the structure of magnetic ejecta (MEs) within interplanetary coronal mass ejections (ICMEs). We study an ICME observed…

physics.space-ph2023

Multi-scale observation of magnetotail reconnection onset: 2. microscopic dynamics

K. J. Genestreti, C. Farrugia, S. Lu +23

We analyze the local dynamics of magnetotail reconnection onset using Magnetospheric Multiscale (MMS) data. In conjunction with MMS, the macroscopic dynamics of this event were cap…

physics.space-ph2023

Multi-scale observation of magnetotail reconnection onset: 1. macroscopic dynamics

K. J. Genestreti, C. Farrugia, S. Lu +22

We analyze a magnetotail reconnection onset event on 3 July 2017 that was observed under otherwise quiescent magnetospheric conditions by a fortuitous conjunction of six space and…

physics.space-ph201953 cited

A New Method of 3D Magnetic Field Reconstruction

R. B. Torbert, I. Dors, M. R. Argall +6

A method is described to model the magnetic field in the vicinity of constellations of multiple satellites using field and plasma current measurements. This quadratic model has the…