Applications of fractal geometry to dynamical evolution of sunspots
- Auteur
- MILOVANOV, A. V; ZELENYI, L. M
Space res. inst., dep. space plasma physics, Moscow 117810, Russian Federation - Titre de la conférence
- American Physical Society. div. plasma physics. Annual Meeting
- Nom de la conférence
- American Physical Society. div. plasma physics. Annual Meeting (34 ; Seattle WA 1992-11-26)
- Auteur (monographie)
- CHUAN SHENG LIU (Editor)
American Physical Society. div. plasma div, United States (Funder/Sponsor)
Univ. Maryland, lab. plasma res., College Park MD 20742, United States - Source
Physics of fluids. B, Plasma physics. 1993, Vol 5, Num 7, pp 2609-2615 ; 2 ; ref : 21 ref
- CODEN
- PFBPEI
- ISSN
- 0899-8221
- Domaine scientifique
- Plasma physics
- Editeur
- American Institute of Physics, New York, NY
- Pays de publication
- United States
- Type de document
- Conference Paper
- Langue
- Russian
- Mot clé (fr)
- Dynamique Etude théorique Flux magnétique Fractale Photosphère Tache solaire Tube flux
- Mot clé (en)
- Dynamics Theoretical study Magnetic flux Fractals Photosphere Sunspots Flux tubes
- Classification
- Pascal
- 001 Sciences exactes et technologie / 001B Physique / 001B40 Domaines classiques de la physique (y compris les applications) / 001B40G Mécanique des fluides / 001B40G53 Fractals
- Pascal
- 001 Sciences exactes et technologie / 001E Terre, ocean, espace / 001E03 Astronomie / 001E03B Système solaire / 001E03B60 Physique solaire / 001E03B60Q Taches solaires, facules, plages faculaires
- Pacs
- 4753
- Pacs
- 9660Q
- Discipline
- Astronomy Physics : fluid mechanics
- Provenance
- Inist-CNRS
- Base de données
- PASCAL
- Identifiant INIST
- 3924986
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1063/1.860698 
https://dx.doi.org/10.1063/1.860698
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