Evolution of solar and stellar coronal abundances owing to magnetic activity.
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| Title: | Evolution of solar and stellar coronal abundances owing to magnetic activity. |
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| Authors: | Brooks DH; Computational Physics, Inc. , Springfield, VA 22151, USA.; Mullard Space Science Laboratory, University College London , Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK., Baker D; Mullard Space Science Laboratory, University College London , Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK., Long DM; Centre for Astrophysics & Relativity, School of Physical Sciences, Dublin City University , Dublin D09 K2WA, Ireland., Testa P; Harvard-Smithsonian Center for Astrophysics , 60 Garden St., Cambridge, MA 02193, USA., Warren HP; US Naval Research Laboratory , Washington, DC 20375, USA. |
| Source: | Philosophical transactions. Series A, Mathematical, physical, and engineering sciences [Philos Trans A Math Phys Eng Sci] 2026 Jul 02; Vol. 384 (2323). |
| Publication Type: | Journal Article |
| Journal Info: | Publisher: The Royal Society Country of Publication: England NLM ID: 101133385 Publication Model: Print Cited Medium: Internet ISSN: 1471-2962 (Electronic) Linking ISSN: 1364503X NLM ISO Abbreviation: Philos Trans A Math Phys Eng Sci Subsets: MEDLINE; PubMed not MEDLINE |
| Database: | MEDLINE Ultimate |
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