arXiv (All)
open access
Coherent radio bursts, polarity reversal, and quiescent emission from the M4V dwarf WW PsA
Coherent radio emission from magnetically active M dwarfs is largely observed in two varieties: stochastic solar-like bursts and beamed, rotationally modulated emission including auroral pulses. Detailed monitoring of these stars is critical for probing the plasmas and magnetic fields driving the em
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
- Detection of fine-structured radio bursts during a superflare on EQ Peg#1142214
- Image 4 of Evening star (Washington, D.C.), July 4, 1930#22263
- Image 2 of Evening star (Washington, D.C.), December 27, 1917#22353
- Image 159 of Evening star (Washington, D.C.), February 6, 1955#22391
- Image 15 of Evening star (Washington, D.C.), April 26, 1936#22277
Record · ID 1202374
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