×

Convective instability induced by gravity in a plasma with a frozen-in magnetic field. (English) Zbl 0103.43703


Keywords:

hydrodynamics
PDFBibTeX XMLCite
Full Text: DOI

References:

[1] K. Schwarzschild, Nachr. Kgl. Ges. Wiss. Göttingen, p. 41 (1906).
[2] Biermann, Z. Astrophys. 5 pp 117– (1932)
[3] Biermann, Astron. Nachr. 257 pp 270– (1935)
[4] Biermann, Ergeb. exakt. Naturw. 21 pp 1– (1945)
[5] Siedentopf, Astron. Nachr. 244 pp 273– (1932)
[6] Cowling, Monthly Notices Roy. Astron. Soc. 94 pp 768– (1934) · Zbl 0009.41502 · doi:10.1093/mnras/94.8.768
[7] Chandrasekhar, Proc. Natl. Acad. Sci. U.S. 23 pp 572– (1937)
[8] S. Chandrasekhar,An Introduction to the Study of Stellar Structure, (University of Chicago Press, Chicago, 1939). · JFM 65.1543.02
[9] Rayleigh, Phil. Mag. 32 pp 529– (1917) · doi:10.1080/14786441608635602
[10] Jeffreys, Phil. Mag. 2 pp 833– (1926) · doi:10.1080/14786442608564114
[11] Thompson, Phil. Mag. 42 pp 1417– (1951) · doi:10.1080/14786445108560961
[12] Chandrasekhar, Phil. Mag. 43 pp 501– (1952) · doi:10.1080/14786440508520205
[13] Chandrasekhar, Phil. Mag. 45 pp 1177– (1954) · doi:10.1080/14786441108520544
[14] Chandrasekhar, Proc. Roy. Soc. (London) A225 pp 173– (1954)
[15] Chandrasekhar, Proc. Roy. Soc. (London) A237 pp 476– (1956)
[16] Yu. A. Tserkovnikov, ”Convective instability of a rarefied plasma,” Division of Theoretical Physics, Mathematical Institute of V. A. Steklov, Academy of Sciences of the U. S. S. R., Moscow, Rept. No. T-2 (1960).
[17] Tserkovnikov, Doklady Akad. Nauk S. S. S. R. 130 pp 295– (1960)
[18] Tserkovnikov, Soviet Phys.–Doklady 5 pp 87– (1960)
[19] Kruskal, Proc. Roy. Soc. (London) A223 pp 348– (1954)
[20] Bernstein, Proc. Roy. Soc. (London) A244 pp 17– (1958)
[21] W. A. Newcomb, Ann. Phys. (N.Y.) (to be published).
[22] H. Grad, ”Propagation of magnetohydrodynamic waves without radial attenuation,” Institute of Mathematical Sciences, New York University, Rept. No. NYO-2537 (1959).
This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.