Relevant bibliographies by topics / Photosphäre

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  1. Dissertations / Theses

Academic literature on the topic 'Photosphäre'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Dissertations / Theses on the topic "Photosphäre"

1

Okunev, Oleg. "Observations and modeling of polar faculae on the sun." Doctoral thesis, [S.l. : s.n.], 2004. http://deposit.ddb.de/cgi-bin/dokserv?idn=975320157.

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2

Cheung, Chung Ming Mark. "Magnetic flux emergence in the solar photosphere." Katlenburg-Lindau Copernicus GmbH, 2006. http://d-nb.info/981843441/34.

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3

Mostoslavsky, Michael. "Hawking radiation photosphere around microscopic black holes." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1998. http://www.collectionscanada.ca/obj/s4/f2/dsk1/tape11/PQDD_0004/MQ44227.pdf.

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4

RINCON, Francois. "Dynamique des grandes échelles de la convection dans la photosphère solaire." Phd thesis, Université Paul Sabatier - Toulouse III, 2004. http://tel.archives-ouvertes.fr/tel-00008710.

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Les mesures des champs de vitesse turbulents dans la photosphère solaire font apparaître trois échelles horizontales distinctes : la granulation (1~000~km), la mésogranulation (7~000~km), et la supergranulation (30~000~km). La granulation résulte du refroidissement radiatif brutal à la surface du gaz chaud et montant. En revanche, l'origine de la mésogranulation et de la supergranulation est en grande partie inconnue. Au cours de cette thèse, plusieurs modèles de convection ont été élaborés afin de mettre en évidence des mécanismes de formation de ces écoulements à grande échelle. Une première
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5

Danilović, Sanja. "Magnetic fine structure in the solar photosphere observations and MHD simulations." Berlin Uni-Ed, 2009. http://d-nb.info/1002469767/04.

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6

Zeuner, Franziska [Verfasser]. "High resolution scattering spectropolarimetry of the quiet solar photosphere / Franziska Zeuner." Göttingen : Niedersächsische Staats- und Universitätsbibliothek Göttingen, 2021. http://d-nb.info/1225121566/34.

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7

Rincon, François. "Dynamique des grandes échelles de la convection dans la photosphère solaire." Toulouse 3, 2004. http://www.theses.fr/2004TOU30254.

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Abstract:
Les mesures des champs de vitesse turbulents dans la photosphère solaire font apparaître trois échelles horizontales distinctes : la granulation (1~000~km), la mésogranulation (7~000~km), et la supergranulation (30~000~km). La granulation résulte du refroidissement radiatif brutal à la surface du gaz chaud et montant. En revanche, l'origine de la mésogranulation et de la supergranulation est en grande partie inconnue. Au cours de cette thèse, plusieurs modèles de convection ont été élaborés afin de mettre en évidence des mécanismes de formation de ces écoulements à grande échelle. Une première
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8

Gallagher, Peter Thomas. "Optical and EUV observations of the solar atmosphere." Thesis, Queen's University Belfast, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.322860.

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9

Cheung, Chung Ming Mark [Verfasser]. "Magnetic flux emergence in the solar photosphere / vorgelegt von Chun Ming Mark Cheung." Katlenburg-Lindau : Copernicus GmbH, 2006. http://d-nb.info/981843441/34.

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10

Ortiz, Carbonell Ada Natalia. "Solar Irradiance Variations Induced by Faculae and Small Magnetic Elements in the Photosphere." Doctoral thesis, Universitat de Barcelona, 2003. http://hdl.handle.net/10803/733.

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The aim of this thesis is the study of the total and spectral solar irradiance variability induced by the presence of small magnetic elements that emerge into the solar photosphere. It is important to study changes in the solar energy output because they reflect the existence of several physical processes in the solar interior, their interpretation helps to understand the solar cycle and because of their influence on the terrestrial climate. The work presented in this thesis is exclusively based on data provided by the SOHO spacecraft, specifically by the VIRGO and MDI instruments.<br/><br/>Ir
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