No CrossRef data available.
Article contents
Properties of the Solar Granulation
Published online by Cambridge University Press: 08 February 2017
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Until recently the theory of the photospheric structure has had a modest role. This situation has qualitatively changed with the appearance of the numerical simulations of Nordlund [1], Uus [2], Gadun [3], and others.
- Type
- II. Photospheric Fine Structure
- Information
- Copyright
- Copyright © Kluwer 1990
References
6.
Nordlund, Å. (1984) in ‘Small-Scale Dynamical Processes in Quiet Stellar Atmospheres’ (ed. Keil, S.), 135–137.Google Scholar
12.
Bray, R.J., Loughhead, R.E., and Durrant, C.J. (1984)
The Solar Granulation
(Cambridge University Press), p. 256.Google Scholar
14.
Kneer, F. (1984) in ‘Small-Scale Dynamical Processes in Quiet Stellar Atmospheres’ (ed. Keil, S.), 110–129.Google Scholar
16.
Sveshnikov, A. (1968)
Prikladnye Metody Teorii Sluchainych Funktsyi
, Nauka, Moscow, p. 464.Google Scholar
20.
Mandelbrot, B. (1982)
The Fractal Geometry of Nature
, Freeman and Co., New-York, p. 480.Google Scholar
25.
Title, A.M. et al. (1988) ‘Statistical Properties of Solar Granulation Derived from the Soup Instrument on Spacelab 2’, LPARL, p. 51.Google Scholar
52.
Bialko, A.V., Avrett, E.H. (1985) ‘A Mechanism for Chromospheric Heating by Fast Electrons Generated in the Temperature Minimum Region’
(Preprint), The Academy of Sciences of the USSR, L.D. London Institute for Theoretical Physics, Chernogolovka.Google Scholar
You have
Access