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Precipitation and kinematic structure of microburst producing storms

NASA NTRS · Conference Paper · 19860038175 · Published 2011-08-18 · Legacy CDMS · 2 authors

Abstract and citation only, verbatim from NASA NTRS; full text lives there. All credit to the authors and Legacy CDMS.

Abstract

Single Doppler radar techniques are used to study the precipitation and kinematic structure of microburst-producing storms. Radar data collected by NCAR radars during the Joint Airport Weather Studies (JAWS) experiment are presented along with rawinsonde data taken at Denver, Colorado near the times of microburst occurrence. The radar reflectivity and velocity structure of the storms exhibited great variability, with no unique signature indicating a microburst was imminent. Detection of descending divergent flow is probably not a microburst forecasting tool, nor can the presence of rotation be used as a precursor at present. Convergent flow aloft was a prominent feature in all events. Its occurrence with a descending precipitation shaft and/or at high altitudes is a good indicator of a downdraft. It is concluded that convergent flow is a very important microburst forecasting clue, particularly when coupled with the entrainment of Theta(e) air and a dry-adiabatic lapse rate below cloud base.

Authors

  • Roberts, R. D. National Center for Atmospheric Research
  • Wilson, J. W. Natonal Center for Atmospheric Research

Citation

Roberts, R. D., Wilson, J. W. (2011). Precipitation and kinematic structure of microburst producing storms. Legacy CDMS. NASA NTRS ID 19860038175. https://ntrs.nasa.gov/citations/19860038175 ↗