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.
and Gonzalez, Walter D
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
years
2026 4representative citing papers
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.
Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
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.
citing papers explorer
-
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.
-
Validating a Non-conventional Method for Expansion of Coronal Mass Ejections (CMEs) and Investigating the Evolution of a CME Substructures Using Solar Orbiter and Wind Observations
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.
-
Energetic particle-mediated interplanetary shocks observed by Solar Orbiter
Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
-
"Corotating Interaction Regions (CIRs)", "Interaction Regions (IRs)" and "Stream Interaction Regions (SIRs)", which term should be used?
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.