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Spiral Rainbands in a Numerical Simulation of Hurricane Bil Spiral Rainbands in a Numerical Simulation of Hurricane Bil

Spiral Rainbands in a Numerical Simulation of Hurricane Bil - PowerPoint Presentation

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Spiral Rainbands in a Numerical Simulation of Hurricane Bil - PPT Presentation

Comparisons to Observations Yumin Moon and David S Nolan 2014 Rainband Classification Data amp Methodology Principal Rainband Secondary Rainband Distant Rainband Inner Rainband Four types of rainbands primary secondary distant and inner ID: 552033

side radial secondary rainband radial side rainband secondary updraft circulation outwards overturning tilt outward convection downdraft distant eyewall similar

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Presentation Transcript

Slide1

Spiral Rainbands in a Numerical Simulation of Hurricane Bill (2009). Part I: Structures and

Comparisons

to Observations

Yumin

Moon and David S. Nolan 2014

Rainband Classification

Data & Methodology

Principal Rainband

Secondary Rainband

Distant Rainband

Inner Rainband

Four types of rainbands: primary, secondary, distant, and inner

Simulation of Hurricane Bill 2009 was done using the WRF 3.2.1

over a 3 day

period of max

intensity from

1200 UTC 18 August to 1200 UTC 21 August

Graphs are radius-height cross sectional averages for each rainband

1.Radial tilt outwards

2. Overturning secondary circulation

3. Enhanced tangential velocity on radial outward side

4. Higher theta-e in updraft

Updraft

Downdraft

Radial inflow from outward side z=2-4km that descends to surface

or

Indirect overturning circulation on inward side called inner-edge downdraft (IED)

Stratiform

1. Found on downwind sector of band

2. Radial tilt outwards with bright band at 5 km

Updraft

1.Radial tilt outwards

2. More mature convection with higher vertical extent found on downwind side

3. Overturning circulation on radial outward side

Downdraft

Left side displays descending midlevel radial flow and right side is indirect overturning circulation on inward side

1.Radial tilt inwards

2. Updraft on radial outward side

3. Strong horizontal convergence at base of updraft and divergence above

4. Structure similar to squall lines

1. Shallow convection below 5 km

2. Reflectivity above 7km is condensates from eyewall convection

3. Hypothesized to

form close

to the eyewall and

propagate outwards

-Primary and secondary are very similar

except with primary being more stationary-Distant has convection similar to squall lines -Inner, not shown in the diagram, are found in closer proximity to the eyewall than the secondary

Houze(2010)