arXiv (All)
open access
Comparing turbulent cascades and heating vs spectral anisotropy in solar wind via direct simulations
In a previous work (MGV18), we showed numerically that the turbulent cascade generated by quasi-2D structures (with wave vectors mostly-perpendicular to the mean magnetic field) is able to generate a temperature profile close to the one observed in solar wind ($\simeq 1/R$) in the range 0.2 $\le R \
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Disentangling non-thermal electron injection and decay in solar flares using multi-wavelength radio observations#422453
- Negative and Positive Cascade Rates of Slow Alfvénic Turbulence in Switchback and Non-switchback Intervals: \emph{Wind} Observations#1115842
- MATLAB Code for Evaluating Wave Dissipation by Typical Coastal Vegetation#296728
- How Magnetic Fields Regulate Cooling and Mixing in Turbulent Radiative Mixing Layers#1077709
- Efficient spectral Galerkin framework for nonlinear transient heat transfer in finite domains#1036951
Record · ID 1143548
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive