ATHARV is a tool that converts in-situ ICME time series into spatial maps assuming self-similar anisotropic expansion, demonstrated on 2023 multipoint data showing coherent flux-rope rotation with mesoscale inhomogeneity.
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2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2representative citing papers
CMEs during active solar phases are faster with stronger magnetic fields than in quiet phases (even after speed matching), while toroidal and poloidal field components decay similarly with distance and front-to-rear asymmetry increases.
citing papers explorer
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Visualizing the Magnetic Structure in Interplanetary Coronal Mass Ejections with ATHARV
ATHARV is a tool that converts in-situ ICME time series into spatial maps assuming self-similar anisotropic expansion, demonstrated on 2023 multipoint data showing coherent flux-rope rotation with mesoscale inhomogeneity.
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Evolution of Coronal Mass Ejection Properties through Superposed Epoch Analysis from 0.2 to 2.2 au
CMEs during active solar phases are faster with stronger magnetic fields than in quiet phases (even after speed matching), while toroidal and poloidal field components decay similarly with distance and front-to-rear asymmetry increases.