Numerical simulation and analysis of a prefrontal squall line. Part II: propagation of the squall line as an internal gravity wave

41Citations
Citations of this article
9Readers
Mendeley users who have this article in their library.

Abstract

The squall line was collocated with a surface front during its initial development (at 0000 UTC 18 June 1978), but then propagated faster than the front, resulting in a separation of approximately 200 km by 0300 UTC and 300-400 km by 0600 UTC. In this paper (Part II), the movement of the squall line in the model is shown to be due to the propagation of a deep tropospheric internal gravity wave in a wave-CISK-like (Conditional Instability of the Second Kind) process. The thermal and dynamic perturbations associated with the hypothesized wave are shown to be consistent with internal gravity wave theory, and the characteristics of the wave are compared to similar results from other wave-CISK studies. -from Authors

Cited by Powered by Scopus

A comprehensive meteorological modeling system-RAMS

1468Citations
N/AReaders
Get full text

Mesoscale convective systems

1057Citations
N/AReaders
Get full text

RAMS 2001: Current status and future directions

827Citations
N/AReaders
Get full text

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Cite

CITATION STYLE

APA

Cram, J. M., Pielke, R. A., & Cotton, W. R. (1992). Numerical simulation and analysis of a prefrontal squall line. Part II: propagation of the squall line as an internal gravity wave. Journal of the Atmospheric Sciences, 49(3), 209–225. https://doi.org/10.1175/1520-0469(1992)049<0209:NSAAOA>2.0.CO;2

Readers' Seniority

Tooltip

PhD / Post grad / Masters / Doc 5

56%

Researcher 3

33%

Professor / Associate Prof. 1

11%

Readers' Discipline

Tooltip

Earth and Planetary Sciences 8

89%

Environmental Science 1

11%

Save time finding and organizing research with Mendeley

Sign up for free