Zobrazeno 1 - 10
of 1 194
pro vyhledávání: '"M. Stix"'
Autor:
Nigel Weiss
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 97:421-423
Autor:
Michael J. Rycroft
Publikováno v:
Surveys in Geophysics. 25:183-184
Autor:
Tony Arber
Publikováno v:
International Journal of Astrobiology. 2:75-75
Publikováno v:
Solar Neutrinos ISBN: 9780429502811
Evolutionary sequences of solar models starting in a fully convective phase at the Hayashi line are described. An overshoot layer of ∼0.30 pressure scale heights is sufficient for the depletion of lithium by a factor 100. The destruction of Li occu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::489e4f9a72e5e2d3b31a35848f35eebe
https://doi.org/10.1201/9780429502811-24
https://doi.org/10.1201/9780429502811-24
Autor:
Arber, Tony
Publikováno v:
International Journal of Astrobiology; January 2003, Vol. 2 Issue: 1 p75-75, 1p
Publikováno v:
Astronomische Nachrichten. 326:223-226
We present some results of three-dimensional hydrodynamic simulations of a compressible flow under the influence of rotation. The code implements a three-layer (stably–unstably–stably stratified) rectangular box placed at various latitudes in a c
Autor:
M. Stix
Publikováno v:
Astronomische Nachrichten. 323:178-185
There are two kinds of questions that must be asked in the context of sunspots: those concerning the 22-year magnetic cycle, and those concerning individual spots. The magnetic cycle is probably the result of an αΩ dynamo, but the nature and the ma
Autor:
M. Stix
Publikováno v:
Astronomical & Astrophysical Transactions. 20:417-427
Mean-field theory appears appropriate to describe the solar dynamo. The αΩ dynamo yields a cyclic mean magnetic field, including the butterfly diagram. In spite of this apparent success many difficulties persist. The dynamo coefficients, especially
Publikováno v:
Astronomy & Astrophysics. 366:668-675
We present a model for the differential rotation of the present Sun as well as a solar-type star during its pre-main-sequence evolution. The model is based on the mixing-length theory of convective heat transport and a standard solar model. The resul
Autor:
D. Melrose, J. T. Mariska, S. Koutchmy, S. Baliunas, Petr Heinzel, D. Dravins, F. Deubner, Thomas L. Duvall, C. Fang, M. Stix, Yoshinori Suematsu, E. Kononovich, Sami K. Solanki, V. Gaizauskas, Peter Foukal
Publikováno v:
Transactions of the International Astronomical Union. 24:73-76
The focus of Commission 12 is on the solar interior, on global phenomena of the quiet Sun, and on the Sun’s radiative outputs, both spectral and total. These are the topics treated below in our discussion of Scientific Highlights. The many topics h