Abstract

Extratropical cyclones draw energy from the horizontal variation of temperature in the atmosphere; i.e., from the baroclinic structure of the atmosphere. Clouds form in response to the vertical air motions within baroclinic waves and are usually concentrated along warm, cold, and occluded fronts. The air motions within baroclinic waves are frontogenetical, meaning that they tend to bring isotherms together into sharp zones of horizontal temperature contrast to define frontal zones. Frontogenetic zones have strong secondary circulations that keep the flow in force balance. This overturning produces nimbostratus clouds along most fronts. These clouds are unique in the atmosphere because they are produced by the dynamics of frontogenesis. However, the frontal clouds exhibit considerable variability. They break down into mesoscale precipitation features known as narrow cold frontal rainbands, wide cold frontal rainbands, occlusion bands, and surge rainbands. The narrow cold frontal rainbands are associated with gravity wave dynamics at the edge of sharp cold fronts. Wide cold and warm frontal rainbands are connected with moist conditional symmetric instability. The rainbands of extratropical cyclones often contain embedded convective elements. These observed structures and associated dynamics are all reviewed in this chapter.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.