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Observational Relationship Between Meso-Sized Convection and 5-Min Oscillation in the Solar Atmosphere

Published online by Cambridge University Press:  08 February 2017

S. Ueno  and
R. Kitai
S. Ueno
Affiliation:
Kwasan Observatory, Kyoto University, Yamashina, Kyoto, Japan 607
R. Kitai
Affiliation:
Hida Observatory, Kyoto University, Yoshiki-gun, Gifu, Japan 506-13

Extract

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Solar convection has been studied theoretically and observationally for very long time. At present, three kinds of solar surface structures are supposed as manifestations of solar convection; granulation, mesogranulation, supergranulation, in increasing order of spatial size. Among them, observations of mesogranulation, however, do not have long history, yet, since November's discovery (1981). Their basic characteristics such as lifetime, velocity field, radial size, and relation to other kinds of convection, have not been precisely determined, yet.

Type
VII. The Solar Atmosphere
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 457 - 458
Copyright
Copyright © Kluwer 1998 

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