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A compilation of studies from Atmospheric Variability Experiment (AVE)Five methods for obtaining the sign of vertical motion at various levels in the atmosphere were investigated to determine which gave the best explanation for areas of rain and no-rain in the southeastern United States during the period February 19-22, 1964. The methods used were the terrain-induced vertical motion, the kinematic method including the terrain effect, the adiabatic method, the omega equation, and the vorticity equation combined with Dines' Compensation Principle. Stability and moisture availability were considered but not as extensively as vertical motion. Values of vertical motion obtained by the kinetic method, including orographic lifting produced the best agreement with the observed areas. When terms in the omega equation were added through use of constant multipliers, results comparable to the adiabatic method were obtained. Without this addition large uncertainties occurred. Maps showing areas where terms of the omega equation would indicate positive vertical motion did not correlate well with the observed rainfall patterns.
Document ID
19730022845
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Scoggins, J. R.
(Texas A&M Univ. College Station, TX, United States)
Fuelberg, H. E.
(Texas A&M Univ. College Station, TX, United States)
Carlson, R. D.
(Texas A&M Univ. College Station, TX, United States)
Phelps, R. W.
(Texas A&M Univ. College Station, TX, United States)
Bellue, D. G.
(Texas A&M Univ. College Station, TX, United States)
Date Acquired
September 2, 2013
Publication Date
August 1, 1973
Publication Information
Publisher: NASA
Subject Category
Meteorology
Report/Patent Number
NASA-CR-2304
Report Number: NASA-CR-2304
Accession Number
73N31577
Funding Number(s)
CONTRACT_GRANT: NAS8-26751
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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