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CHISLENNOE MODELIROVANIE RASPROSTRANENIYA VGV OT NESTATSIONARNYKH TROPOSFERNYKH ISTOCHNIKOV. / Gavrilov, N. M.; Yudin, V. A.

In: Izvestia Akademii nauk SSSR. Fizika atmosfery i okeana, Vol. 23, No. 3, 03.1987, p. 241-248.

Research output: Contribution to journalArticlepeer-review

Harvard

Gavrilov, NM & Yudin, VA 1987, 'CHISLENNOE MODELIROVANIE RASPROSTRANENIYA VGV OT NESTATSIONARNYKH TROPOSFERNYKH ISTOCHNIKOV.', Izvestia Akademii nauk SSSR. Fizika atmosfery i okeana, vol. 23, no. 3, pp. 241-248.

APA

Gavrilov, N. M., & Yudin, V. A. (1987). CHISLENNOE MODELIROVANIE RASPROSTRANENIYA VGV OT NESTATSIONARNYKH TROPOSFERNYKH ISTOCHNIKOV. Izvestia Akademii nauk SSSR. Fizika atmosfery i okeana, 23(3), 241-248.

Vancouver

Gavrilov NM, Yudin VA. CHISLENNOE MODELIROVANIE RASPROSTRANENIYA VGV OT NESTATSIONARNYKH TROPOSFERNYKH ISTOCHNIKOV. Izvestia Akademii nauk SSSR. Fizika atmosfery i okeana. 1987 Mar;23(3):241-248.

Author

Gavrilov, N. M. ; Yudin, V. A. / CHISLENNOE MODELIROVANIE RASPROSTRANENIYA VGV OT NESTATSIONARNYKH TROPOSFERNYKH ISTOCHNIKOV. In: Izvestia Akademii nauk SSSR. Fizika atmosfery i okeana. 1987 ; Vol. 23, No. 3. pp. 241-248.

BibTeX

@article{82ffc7e1571f4e848df2dfbeccd09f4e,
title = "CHISLENNOE MODELIROVANIE RASPROSTRANENIYA VGV OT NESTATSIONARNYKH TROPOSFERNYKH ISTOCHNIKOV.",
abstract = "Calculations are made of the propagation of internal gravity waves (IGW) from unsteady sources located in the troposphere. Taking the unsteadiness of the tropospheric sources into account leads to a decrease in the heights of the maximum amplitudes and energy characteristics of these waves, owing to energy capture in the mesospheric waveguide at z approximately equals 75 km. The filtering action of the background wind leads mainly to intensification of the IGW, which propagate counter to the wind, and to the formation of wave accelerations which hamper the background flow near the mesopause. For certain source parameters and at certain moments of time IGW traveling in the same direction as the background wind may prevail.",
author = "Gavrilov, {N. M.} and Yudin, {V. A.}",
year = "1987",
month = mar,
language = "русский",
volume = "23",
pages = "241--248",
journal = "Izvestiya - Atmospheric and Oceanic Physics",
issn = "0001-4338",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "3",

}

RIS

TY - JOUR

T1 - CHISLENNOE MODELIROVANIE RASPROSTRANENIYA VGV OT NESTATSIONARNYKH TROPOSFERNYKH ISTOCHNIKOV.

AU - Gavrilov, N. M.

AU - Yudin, V. A.

PY - 1987/3

Y1 - 1987/3

N2 - Calculations are made of the propagation of internal gravity waves (IGW) from unsteady sources located in the troposphere. Taking the unsteadiness of the tropospheric sources into account leads to a decrease in the heights of the maximum amplitudes and energy characteristics of these waves, owing to energy capture in the mesospheric waveguide at z approximately equals 75 km. The filtering action of the background wind leads mainly to intensification of the IGW, which propagate counter to the wind, and to the formation of wave accelerations which hamper the background flow near the mesopause. For certain source parameters and at certain moments of time IGW traveling in the same direction as the background wind may prevail.

AB - Calculations are made of the propagation of internal gravity waves (IGW) from unsteady sources located in the troposphere. Taking the unsteadiness of the tropospheric sources into account leads to a decrease in the heights of the maximum amplitudes and energy characteristics of these waves, owing to energy capture in the mesospheric waveguide at z approximately equals 75 km. The filtering action of the background wind leads mainly to intensification of the IGW, which propagate counter to the wind, and to the formation of wave accelerations which hamper the background flow near the mesopause. For certain source parameters and at certain moments of time IGW traveling in the same direction as the background wind may prevail.

UR - http://www.scopus.com/inward/record.url?scp=0023312577&partnerID=8YFLogxK

M3 - статья

AN - SCOPUS:0023312577

VL - 23

SP - 241

EP - 248

JO - Izvestiya - Atmospheric and Oceanic Physics

JF - Izvestiya - Atmospheric and Oceanic Physics

SN - 0001-4338

IS - 3

ER -

ID: 87735064