arXiv (All)
open access
Widespread plasma jets in the Martian magnetosheath revealed by dual-spacecraft observations
Plasma jets in planetary magnetosheaths are transient, high dynamic pressure structures capable of strongly perturbing downstream magnetospheres and modulating solar wind energy transfer. Although recently identified at Mars, their formation mechanisms and global occurrence remain poorly constrained
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
- Ultimate large- Rm regime of the solar dynamo#1090656
- Volcanic Satellites and Ion Escape in the Magnetospheres of Ultra-Cool and Brown Dwarf Stars#1049936
- Magnetic Field Spreading from Stellar and Galactic Dynamos into the Exterior#161371
- Experimental Study of Dusty Flow-Surface Interactions on Heat-Shield Materials at Martian Atmospheric Entry Conditions / Ciro Salvi ; Deutsches Zentrum für Luft- und Raumfahrt - Institut für Aerodynamik und Strömungstechnik#1154255
- The Physical Origin of Periodic Density Structures in the Solar Wind: Coronal Streamers as Magnetohydrodynamic Resonators#974251
Record · ID 1014373
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