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pro vyhledávání: '"Pino, Jesse Ethan"'
Autor:
Pino, Jesse Ethan, 1981
The Magnetorotational Instability (MRI) is believed to be the primary mechanism for angular momentum transfer in astrophysical accretion disks. This instability, which exists in ionized disks in the presence of weak magnetic fields, can either transf
Externí odkaz:
http://hdl.handle.net/2152/18376
Autor:
Pino, Jesse Ethan
Thesis (Ph. D.)--University of Texas at Austin, 2009.
Title from PDF title page (University of Texas Digital Repository, viewed on Sept. 9, 2009). Vita. Includes bibliographical references.
Title from PDF title page (University of Texas Digital Repository, viewed on Sept. 9, 2009). Vita. Includes bibliographical references.