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.
Title resolution pending
6 Pith papers cite this work. Polarity classification is still indexing.
6
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 6roles
background 1polarities
background 1representative citing papers
MMS data from a 2023 CME show elevated electron temperatures with superthermal tails, depleted mid-energy electrons, and weak MHD-like turbulence with reduced intermittency in the rare sub-Alfvénic solar wind at 1 AU.
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.
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.
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.
This paper discusses observational, calibration, and imaging requirements for solar and heliospheric science with the SKA radio telescope.
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.
-
MMS Insights into CME Driven Sub-Alfv\'enic Solar Wind at 1 AU
MMS data from a 2023 CME show elevated electron temperatures with superthermal tails, depleted mid-energy electrons, and weak MHD-like turbulence with reduced intermittency in the rare sub-Alfvénic solar wind at 1 AU.
-
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.
-
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.
-
"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.
-
State-of-the-art Observation, Calibration, and Imaging Framework for Solar and Heliospheric Sciences with SKA
This paper discusses observational, calibration, and imaging requirements for solar and heliospheric science with the SKA radio telescope.