THICKNESS OF PLANETARY BOUNDARY LAYER

被引：61

作者：

HANNA, SR

机构：

[1] Air Resources Atmospheric Turbulence and Diffusion Laboratory, ESSA Oak Ridge

来源：

ATMOSPHERIC ENVIRONMENT | 1969年 / 3卷 / 05期

关键词：

D O I：

10.1016/0004-6981(69)90042-0

中图分类号：

X [环境科学、安全科学];

学科分类号：

08 ; 0830 ;

摘要：

Many different methods for estimating the thickness H of the planetary boundary layer are summarized and applied to the 1953 O'Neill boundary layer observations. The observed variation of the thickness H is best explained by Latkhtman's (1961) formula, which states that H is directly proportional to the free-stream or geostrophic wind speed and inversely proportional to the square root of the average vertical gradient of potential temperature within the boundary layer. © 1969.

引用

页码：519 / &

共 21 条

[1]

[Anonymous], NYT MAG F NATURVID

[2] VERTICAL DISTRIBUTION OF WIND AND TURBULENT EXCHANGE IN A NEUTRAL ATMOSPHERE [J].

BLACKADAR, AK .

JOURNAL OF GEOPHYSICAL RESEARCH, 1962, 67 (08) :3095-+

[3]

Davidson, 1957, EXPLORING ATMOSPHERE

[4]

ELLISON TH, 1956, SURVEYS MECHANICS, P400

[5]

GALADZHII NM, 1963, T MET GEOPHYS OBS, P101

[6]

Holzworth G. C., 1964, J APPL METEOROL, V6, P1039, DOI [10.1175/1520-0450(1967)006<1039:mdwsaa>2.0.co

[7]

2, DOI 10.1175/1520-0450(1967)006<1039:MDWSAA>2.0.CO

[8]

[9]

Holzworth G. C., 1964, MON WEATHER REV, V92, P235, DOI DOI 10.1175/1520-0493(1964)092%3C0235:EOMMMD%3E2.3.CO

[10]

← 1 2 3 →