logging in or signing up EAS GradExpo06 poster aSGuest49714 Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINT lite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 11 Category: Entertainment License: All Rights Reserved Like it (1) Dislike it (0) Added: June 18, 2010 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript Slide 1: The Mechanics of Falling Hailstones and Hailswaths Kevin Vermeesch and Ernest Agee Department of Earth and Atmospheric Sciences, Purdue University Objectives Develop a set of mechanical equations for calculating hailstone fall velocities and characteristics for a variety of thunderstorm and atmospheric conditions Plot hailswaths for real atmospheric events and compare with model results Physical Properties in the Model Equations Density profile of atmosphere Diameter and mass of spheroidal hailstones Drag coefficient for subcritical Reynolds number flow Translational speed of supercell thunderstorm Updraft velocity profile of the supercell thunderstorm Rotational velocity profile of embedded mesocyclone Spherical vs. non-spherical hailstone and related Re and CD Cases and Model Results Cases Testing Fall Speeds 3 April 1974 tornado tracks and hailswath in Indiana In a size-sorted hailswath, the largest hail lands closest to the mesocyclone (or tornado track if present). The dimensions of the swath are a function of the thunderstorm’s rotational velocity (vθ), translational velocity (u), and mesocyclone radius. The image on the right shows a portion of the mesocyclone and underlying wall cloud, flanked by a spectacular hailshaft that produces the hailswath. Graphical verification of model terminal velocity with Knight and Knight (2001) Hailstone shapes range from being nearly spherical and smooth to very irregular, containing knobs, lobes, or spikes on their surface. The smooth stones fall under conditions of subcritical Reynolds flow, while the irregular shapes may achieve supercritical flow conditions. Re < Rec Size-sorted hailswath produced by model References Knight, C.A. and N.C. Knight, 2001: Hailstorms. Severe Convective Storms, Meteor. Monogr., No. 50, Amer. Meteor. Soc., 223-249. Knight, C.A. and N.C. Knight, 2005: Very large hailstones from Aurora, Nebraska. Bull. Amer. Meteor. Soc., 86, 1773-1781. Re > Rec Knight and Knight (2005), Figure 9 Knight and Knight (2001), Figure 6.2 Hailswaths You do not have the permission to view this presentation. In order to view it, please contact the author of the presentation.
EAS GradExpo06 poster aSGuest49714 Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINT lite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 11 Category: Entertainment License: All Rights Reserved Like it (1) Dislike it (0) Added: June 18, 2010 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript Slide 1: The Mechanics of Falling Hailstones and Hailswaths Kevin Vermeesch and Ernest Agee Department of Earth and Atmospheric Sciences, Purdue University Objectives Develop a set of mechanical equations for calculating hailstone fall velocities and characteristics for a variety of thunderstorm and atmospheric conditions Plot hailswaths for real atmospheric events and compare with model results Physical Properties in the Model Equations Density profile of atmosphere Diameter and mass of spheroidal hailstones Drag coefficient for subcritical Reynolds number flow Translational speed of supercell thunderstorm Updraft velocity profile of the supercell thunderstorm Rotational velocity profile of embedded mesocyclone Spherical vs. non-spherical hailstone and related Re and CD Cases and Model Results Cases Testing Fall Speeds 3 April 1974 tornado tracks and hailswath in Indiana In a size-sorted hailswath, the largest hail lands closest to the mesocyclone (or tornado track if present). The dimensions of the swath are a function of the thunderstorm’s rotational velocity (vθ), translational velocity (u), and mesocyclone radius. The image on the right shows a portion of the mesocyclone and underlying wall cloud, flanked by a spectacular hailshaft that produces the hailswath. Graphical verification of model terminal velocity with Knight and Knight (2001) Hailstone shapes range from being nearly spherical and smooth to very irregular, containing knobs, lobes, or spikes on their surface. The smooth stones fall under conditions of subcritical Reynolds flow, while the irregular shapes may achieve supercritical flow conditions. Re < Rec Size-sorted hailswath produced by model References Knight, C.A. and N.C. Knight, 2001: Hailstorms. Severe Convective Storms, Meteor. Monogr., No. 50, Amer. Meteor. Soc., 223-249. Knight, C.A. and N.C. Knight, 2005: Very large hailstones from Aurora, Nebraska. Bull. Amer. Meteor. Soc., 86, 1773-1781. Re > Rec Knight and Knight (2005), Figure 9 Knight and Knight (2001), Figure 6.2 Hailswaths