Zobrazeno 1 - 10
of 22
pro vyhledávání: '"N L, Isaeva"'
Publikováno v:
Труды по прикладной ботанике, генетике и селекции, Vol 179, Iss 4, Pp 82-90 (2019)
Background. One of the main tasks of the present-day breeding practice is the development of high-yielding intensive-type fodder crop cultivars for indoor feeding of livestock. Alfalfa, as a productive and high-protein crop, deserves special attentio
Externí odkaz:
https://doaj.org/article/9a61d6f8ab0d4813abc6d37617e80d5e
Autor:
N. L. Isaeva, Luís Campos
Publikováno v:
Journal of Plasma Physics. 70:271-302
Alfven waves are considered in a radial flow and external magnetic field, which relates to some features of the solar wind near the critical point. The Alfven wave equation for the velocity perturbation is derived, showing that it has in general two
Autor:
N. L. Isaeva, L. M. B. C. Campos
Publikováno v:
Physics of Plasmas. 10:2486-2500
The application to the solar wind motivates the consideration of Alfven waves in a radial background magnetic field and radial mean flow, in two cases, viz., with velocity and magnetic field perturbations along parallels, or also with perturbations a
On three-dimensional magnetosonic waves in an isothermal atmosphere with a horizontal magnetic field
Publikováno v:
Journal of Plasma Physics. 68:331-361
Magnetosonic-gravity waves in an isothermal non-dissipative atmosphere, with a uniform horizontal external magnetic field have been considered in the literature in two cases: (i) one-dimensional' magnetosonic-gravity waves, in the case of zero horizo
Publikováno v:
Scopus-Elsevier
Alfven waves are considered in a radially inhomogeneous medium under a radial background magnetic field: In order for the latter to be divergence free, the magnetic field strength must decay like the inverse square of the distance; for the radial dep
Autor:
N. L. Isaeva, Luís Campos
Publikováno v:
Scopus-Elsevier
This paper considers Alfvén waves in a radially stratified medium where all background quantities, namely mass density, magnetic field strength and mean flow velocity, depend only on the distance from the centre, the latter two being assumed to lie
Autor:
N. L. Isaeva, L. M. B. C. Campos
Publikováno v:
Journal of Plasma Physics. 48:415-434
We derive the Alfvén-wave equation for an atmosphere in the presence of a non-uniform vertical magnetic field and the Hall effect, allowing for Alfvén speed and ion gyrofrequency that may vary with altitude; the pair of coupled second-order differe
Publikováno v:
Nonlinear MHD Waves and Turbulence ISBN: 9783540666974
The linear propagation of Alfven waves in the solar wind is considered for arbitrary wavelengths, which may exceed the lengthscales of variation of (i) the mass density of the medium, (ii) strength and direction of the external magnetic field, (iii)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5905c9b9e1cd23f2662ea7d4772480e3
https://doi.org/10.1007/3-540-47038-7_5
https://doi.org/10.1007/3-540-47038-7_5
Publikováno v:
AIP Conference Proceedings.
The present paper considers Alfven waves in an inhomogeneous medium, under a non-uniform external magnetic field and in the presence of a non-uniform flow, to obtain the wave equations for the velocity and magnetic field perturbations in the case of
Autor:
N. L. Isaeva, Luís Campos
Publikováno v:
AIP Conference Proceedings.
Alfven waves are considered in a radial flow and external magnetic field, which relates to some features of the solar wind. Particular emphasis is put on the role of the Alfvenic critical point and propagation of the Alfven waves across this critical