skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: The correction of infrasound signals for upper atmospheric winds

Conference ·
OSTI ID:6812452

Infrasound waves propagate in the atmosphere by a well known mechanism produced by refraction of the waves, return to earth, and reflection at the surface into the atmosphere for subsequent bounces. In this instance three rays are returned to earth from a region centered at about 50 kilometers in altitude and two from a region near 110 kilometers in altitude. The control of the wave refraction is largely dominated by the temperature-height profile and inversions; however, a major influence is also produced by the atmospheric wind profile. It obviously can be expected that infrasonic signal amplitudes will be greatly influenced by the winds in the atmosphere. The seasonal variation of the high altitude atmospheric winds is well documented. The very strong seasonal variation has the ability to exert a major seasonal influence on infrasonic signals. It is our purpose to obtain a method for the correction of this effect.

Research Organization:
Los Alamos National Lab., NM (USA)
Sponsoring Organization:
DOE/DP
DOE Contract Number:
W-7405-ENG-36
OSTI ID:
6812452
Report Number(s):
LA-UR-90-1997; CONF-9005236-2; ON: DE90013177
Resource Relation:
Conference: 4. international symposium on long range sound propagation at NASA Langley Research Center, Hampton, VA (USA), 15-17 May 1990
Country of Publication:
United States
Language:
English