Presentation is loading. Please wait.

Presentation is loading. Please wait.

“Dynamical Effects of Convection” Kathryn Saussy Meteorology 515: Analysis & Pred. of Severe Storms March 1 2006 Bluestein, Howard: Synoptic-Dynamic Meteorology.

Similar presentations


Presentation on theme: "“Dynamical Effects of Convection” Kathryn Saussy Meteorology 515: Analysis & Pred. of Severe Storms March 1 2006 Bluestein, Howard: Synoptic-Dynamic Meteorology."— Presentation transcript:

1 “Dynamical Effects of Convection” Kathryn Saussy Meteorology 515: Analysis & Pred. of Severe Storms March 1 2006 Bluestein, Howard: Synoptic-Dynamic Meteorology in Midlatitudes, Vol. II. Oxford Press, 594 pp. Johnson, Richard H., Mapes, Brian E, 2001: Mesoscale Processes and Severe Convective Weather. Meteor. Mon. 28 (50), Amer. Meteor. Soc., Boston. Monteverdi, John. Advanced Weather Analysis Lectures, Spring 2005.

2 Dynamical Effects of Convection I.Development & dynamical consequences of rotation II. Cold pool-shear interactions

3 I. Development & dynamical consequences of rotation Pressure perturbation forces develop. 2 perturbation dynamic pressures are associated with the wind field: The linear, p´ L, and the nonlinear part, p´ NL. ( p´  perturbation upward-directed pressure gradient force that adds to the synoptic-scale upwards directed force…or subtracts from the perturbation pressure change that would occur at that level. )

4 Nonlinear pressure perturbation, p´ NL p´ NL    2 This says that pressure falls are proportional & opposite in sign to the square of the vertical vorticity.

5 Nonlinear pressure perturbation, p´ NL (con’d) Unidirectional shear  Initial stage shows pressure falls (on either flank) that augment the updraft.

6 Nonlinear pressure perturbation, p´ NL (con’d) Unidirectional shear  Splitting stage shows downdraft forming; equal preference for R and L-moving storms.

7 Nonlinear pressure perturbation, p´ NL (con’d) On radar, it appears that the storm splits into mirror images. Note the unidirectional shear on the hodograph.

8 Linear pressure perturbation, p´ L p´ L   v/  z   2 w´ Unidirectional shear  If the wind shear vector (  v/  z) lies transverse a buoyant updraft, then pressures rise on the upshear side and fall on the downshear side. This results in no preferential growth to either of the flanks lying across the shear.

9 Linear pressure perturbation, p´ L (con’d) Clockwise shear vector  Leads to pressure falls on the right flank of the storm…and pressure rises on the left. New growth is favored on the right.

10 Linear pressure perturbation, p´ L (con’d) On radar, it appears that new storm growth favors the right flank. Note the clockwise shear indicated on the hodograph.

11 II. Cold pool-shear interactions Vertical shear  enhances ability of outflow (or cold pool) to trigger new storms Increasing shear  interaction between shear and cold pool enhances lifting on preferred storm flank.

12 Evolution of a Convective System: Stage 1 The initial updraft leans downshear in response to the surrounding vertical shear. (C is the strength of the cold pool; D u is the strength of surrounding vertical shear. Circular arrows show the most significant horizontal vorticity.)

13 Evolution of a Convective System: Stage 2 The circulation generated by the storm-induced cold pool balances the surrounding shear, and the system becomes upright.

14 Evolution of a Convective System: Stage 3 The cold pool dominates the surrounding shear and the system tilts upshear, producing a rear-inflow jet. (The rear-inflow jet is indicated by the thick, black arrow.)

15 Thank you.


Download ppt "“Dynamical Effects of Convection” Kathryn Saussy Meteorology 515: Analysis & Pred. of Severe Storms March 1 2006 Bluestein, Howard: Synoptic-Dynamic Meteorology."

Similar presentations


Ads by Google