Solitons in a magnetized relativistic electron-positron plasma
Nonlinear equations for the interaction of the Langmuir wave field and the transverse electromagnetic field in the pulsar magnetosphere are derived. These equations take into account the modulational instability of plasma waves and its decay into two transversal waves. © 1984.
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
1984
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 02935caa a22004457a 4500 | ||
|---|---|---|---|
| 001 | PAPER-1149 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250321092134.0 | ||
| 008 | 190411s1984 xx ||||fo|||| 00| 0 eng|d | ||
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| 100 | 1 | |a Verga, A.D. | |
| 245 | 1 | 0 | |a Solitons in a magnetized relativistic electron-positron plasma |
| 260 | |c 1984 | ||
| 270 | 1 | 0 | |m Verga, A.D.; Instituto de Astronomia y Fisica del Espacio, CC 67, Suc. 28, 1428 Buenos Aires, Argentina |
| 504 | |a Cordes, (1979) Space Sci. Rev., 24, p. 567 | ||
| 504 | |a Ruderman, Sutherland, Theory of pulsars - Polar caps, sparks, and coherent microwave radiation (1975) The Astrophysical Journal, 196, p. 51 | ||
| 504 | |a Arons, Scharlemann, Pair formation above pulsar polar caps - Structure of the low altitude acceleration zone (1979) The Astrophysical Journal, 231, p. 854 | ||
| 504 | |a Rylov, (1981) Astrophys. Space Sci., 75, p. 423 | ||
| 504 | |a Lominadze, Mikhailovskii, (1979) Sov. Phys. JETP, 49, p. 483 | ||
| 504 | |a Buti, (1978) Astrophys. Space Sci., 58, p. 89 | ||
| 504 | |a Pataraya, Melikidze, (1980) Astrophys. Space Sci., 68, p. 61 | ||
| 504 | |a ter Haar, Tsytovich, (1981) Phys. Rep., 73, p. 175 | ||
| 504 | |a Mikhailovskii, (1980) Sov. J. Plasma Phys., 6, p. 336 | ||
| 504 | |a Kakutani, Sugimoto, (1974) Phys. Fluids, 17, p. 1617 | ||
| 504 | |a Makhankov, (1978) Phys. Rep., 35, p. 1 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a Nonlinear equations for the interaction of the Langmuir wave field and the transverse electromagnetic field in the pulsar magnetosphere are derived. These equations take into account the modulational instability of plasma waves and its decay into two transversal waves. © 1984. |l eng | |
| 593 | |a Instituto de Astronomia y Fisica del Espacio, CC 67, Suc. 28, 1428 Buenos Aires, Argentina | ||
| 593 | |a Facultad de Ciencias Exactas y Naturales, Dto. Física, Ciudad Universitaris, 1428 Buenos Aires, Argentina | ||
| 700 | 1 | |a Ferro Fontán, Constantino | |
| 773 | 0 | |d 1984 |g v. 101 |h pp. 494-496 |k n. 9 |p Phys Lett Sect A Gen At Solid State Phys |x 03759601 |w (AR-BaUEN)CENRE-348 |t Physics Letters A | |
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| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_03759601_v101_n9_p494_Verga |x handle |y Handle |
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| 961 | |a paper_03759601_v101_n9_p494_Verga |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
| 963 | |a VARI | ||