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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.
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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PubType: Academic Journal
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  Data: Evolution of solar and stellar coronal abundances owing to magnetic activity.
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  Data: <searchLink fieldCode="AU" term="%22Brooks+DH%22">Brooks DH</searchLink>; Computational Physics, Inc. , Springfield, VA 22151, USA.; Mullard Space Science Laboratory, University College London , Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK.<br /><searchLink fieldCode="AU" term="%22Baker+D%22">Baker D</searchLink>; Mullard Space Science Laboratory, University College London , Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK.<br /><searchLink fieldCode="AU" term="%22Long+DM%22">Long DM</searchLink>; Centre for Astrophysics & Relativity, School of Physical Sciences, Dublin City University , Dublin D09 K2WA, Ireland.<br /><searchLink fieldCode="AU" term="%22Testa+P%22">Testa P</searchLink>; Harvard-Smithsonian Center for Astrophysics , 60 Garden St., Cambridge, MA 02193, USA.<br /><searchLink fieldCode="AU" term="%22Warren+HP%22">Warren HP</searchLink>; US Naval Research Laboratory , Washington, DC 20375, USA.
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  Data: <searchLink fieldCode="JN" term="%22101133385%22">Philosophical transactions. Series A, Mathematical, physical, and engineering sciences</searchLink> [Philos Trans A Math Phys Eng Sci] 2026 Jul 02; Vol. 384 (2323).
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  Data: <i>Publisher: </i><searchLink fieldCode="PB" term="%22The+Royal+Society%22">The Royal Society </searchLink><i>Country of Publication: </i>England <i>NLM ID: </i>101133385 <i>Publication Model: </i>Print <i>Cited Medium: </i>Internet <i>ISSN: </i>1471-2962 (Electronic) <i>Linking ISSN: </i><searchLink fieldCode="IS" term="%221364503X%22">1364503X </searchLink><i>NLM ISO Abbreviation: </i>Philos Trans A Math Phys Eng Sci <i>Subsets: </i>MEDLINE; PubMed not MEDLINE
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        Value: 10.1098/rsta.2025.0188
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      – Code: eng
        Text: English
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      – TitleFull: Evolution of solar and stellar coronal abundances owing to magnetic activity.
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              Text: 2026 Jul 02
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              Y: 2026
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