ISTA Publications
metadata only
Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars
Magnetic fields in the stellar interiors are key candidates to explain observed core rotation rates inside solar-like stars along their evolution. Recently, asteroseismic estimates of radial magnetic field amplitudes near the hydrogen-burning shell (H-shell) inside about 24 red giants (RGs) have bee
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
- Magnetic field measurements in a sample of Class I and flat-spectrum protostars observed with SPIRou#408687
- Spin-current symmetries generated by the ferrimagnet Gd - Fe - Co across its magnetization-compensation temperature#330190
- Sustainable vortex-assisted magnetic micro-solid phase extraction using lithium ferrite/carboxylated nanodiamonds for ultra-trace determination of cadmium and lead in food and water samples#194257
- Front sign at the Seabrook Factory#1017407
- Magnetohydrodynamic mixed convection within a ventilated cavity crossed by a nanofluid: Effect of the obstacle position#940610
Record · ID 1492954
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