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650.#.4.x: Físico Matemáticas y Ciencias de la Tierra

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336.#.#.3: Artículo de Investigación

336.#.#.a: Artículo

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270.1.#.p: Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

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850.#.#.a: Universidad Nacional Autónoma de México

856.4.0.u: https://www.revistascca.unam.mx/atm/index.php/atm/article/view/8291/7761

100.1.#.a: Wiin Nielsen, A.; Marshall, H.

524.#.#.a: Wiin Nielsen, A., et al. (1990). On the structure of transient atmospheric waves. Part III. Atmósfera; Vol. 3 No. 2, 1990. Recuperado de https://repositorio.unam.mx/contenidos/4121523

245.1.0.a: On the structure of transient atmospheric waves. Part III

502.#.#.c: Universidad Nacional Autónoma de México

561.1.#.a: Instituto de Ciencias de la Atmósfera y Cambio Climático, UNAM

264.#.0.c: 1990

264.#.1.c: 2009-10-05

506.1.#.a: La titularidad de los derechos patrimoniales de esta obra pertenece a las instituciones editoras. Su uso se rige por una licencia Creative Commons BY-NC 4.0 Internacional, https://creativecommons.org/licenses/by-nc/4.0/legalcode.es, para un uso diferente consultar al responsable jurídico del repositorio por medio del correo electrónico editora@atmosfera.unam.mx

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041.#.7.h: eng

520.3.#.a: In the third and final paper in the series on the relative structure of transient atmospheric waves we consider a model atmosphere with a continuous specification of the zonal wind and the static stability in the basic state. The vertical variations of the parameters in the basic state (except the stability) and in the perturbations will be represented as series expansions in functions appropriate to the vertical variation of the static stability parameter. For the stability we shall consider two cases. The first is a constant static stability in the whole model, and the second is a case where the stability varies as inversely proportional to the square of the pressure. In the first case we may use trigonometric functions to describe the vertical variation. In the second case we derive the appropriate structure functions in the paper, but it turns out that to satisfy the upper boundary condition it is necessary to assume that the top of the atmosphere is located at a pressure larger than zero. The relative structure is in each case obtained as a solution to the stationary equations for the relative amplitude and the relative phase angle. Such solutions are in simple cases obtained directly, but in more complicated cases by numerical integrations carried out to a point where an asymptotic steady state is obtained.

773.1.#.t: Atmósfera; Vol. 3 No. 2 (1990)

773.1.#.o: https://www.revistascca.unam.mx/atm/index.php/atm/index

046.#.#.j: 2021-10-20 00:00:00.000000

022.#.#.a: ISSN electrónico: 2395-8812; ISSN impreso: 0187-6236

310.#.#.a: Trimestral

264.#.1.b: Instituto de Ciencias de la Atmósfera y Cambio Climático, UNAM

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harvesting_date: 2023-06-20 16:00:00.0

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245.1.0.b: On the structure of transient atmospheric waves. Part II

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Artículo

On the structure of transient atmospheric waves. Part III

Wiin Nielsen, A.; Marshall, H.

Instituto de Ciencias de la Atmósfera y Cambio Climático, UNAM, publicado en Atmósfera, y cosechado de Revistas UNAM

Licencia de uso

Procedencia del contenido

Entidad o dependencia
Instituto de Ciencias de la Atmósfera y Cambio Climático, UNAM
Revista
Repositorio
Contacto
Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

Cita

Wiin Nielsen, A., et al. (1990). On the structure of transient atmospheric waves. Part III. Atmósfera; Vol. 3 No. 2, 1990. Recuperado de https://repositorio.unam.mx/contenidos/4121523

Descripción del recurso

Autor(es)
Wiin Nielsen, A.; Marshall, H.
Tipo
Artículo de Investigación
Área del conocimiento
Físico Matemáticas y Ciencias de la Tierra
Título
On the structure of transient atmospheric waves. Part III
Fecha
2009-10-05
Resumen
In the third and final paper in the series on the relative structure of transient atmospheric waves we consider a model atmosphere with a continuous specification of the zonal wind and the static stability in the basic state. The vertical variations of the parameters in the basic state (except the stability) and in the perturbations will be represented as series expansions in functions appropriate to the vertical variation of the static stability parameter. For the stability we shall consider two cases. The first is a constant static stability in the whole model, and the second is a case where the stability varies as inversely proportional to the square of the pressure. In the first case we may use trigonometric functions to describe the vertical variation. In the second case we derive the appropriate structure functions in the paper, but it turns out that to satisfy the upper boundary condition it is necessary to assume that the top of the atmosphere is located at a pressure larger than zero. The relative structure is in each case obtained as a solution to the stationary equations for the relative amplitude and the relative phase angle. Such solutions are in simple cases obtained directly, but in more complicated cases by numerical integrations carried out to a point where an asymptotic steady state is obtained.
Idioma
eng
ISSN
ISSN electrónico: 2395-8812; ISSN impreso: 0187-6236

Enlaces