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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3 Pith papers cite this work. Polarity classification is still indexing.
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Dual-spacecraft observations of a November 2021 CME confirm that the CAAP method reliably estimates instantaneous expansion speed from single-point data while revealing unexpected evolution in shock strength and magnetic flux.
Authors advocate precise terminology for interplanetary phenomena like CIRs over the broader SIR label and introduce Super CIR as a new category for exceptionally strong events from coronal hole jets.
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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.