Is Convection in the Inner Core of Intense Hurricanes Buoyant Matthew D. Eastin

Oct 03, 2012

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Is Convection in the Inner Core of Intense Hurricanes Buoyant Matthew D. Eastin

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2002 Atlantic Intense Hurricanes ISIDORE and LILI

2002 Atlantic Intense Hurricanes ISIDORE and LILI. Pressure - Wind Relationships Intensity / Structure Satellite Images. LOWEST MINIMUM SEA-LEVEL PRESSURE (hPa) 1. Mitch 905 2. Opal 916 3. Floyd 921 4. Felix ‘95 929 5. Gert 930 6. Edouard 933 7. Lenny 933 8. Michelle 933

710 views • 44 slides

The Realities of Hurricanes

The Realities of Hurricanes . Robert D Macedo Director of Operations of the VoIP Hurricane Net ARES SKYWARN Coordinator for NWS Taunton Eastern Massachusetts ARES Section Emergency Coordinator Web: www.voipwx.net Email: kd1cy@voipwx.net

600 views • 36 slides

Inner Magnetospheric Modeling with the Rice Convection Model

Inner Magnetospheric Modeling with the Rice Convection Model. Frank Toffoletto, Rice University (with thanks to: Stan Sazykin, Dick Wolf, Bob Spiro, Tom Hill, John Lyon, Mike Wiltberger and Slava Merkin). Outline. Motivation Importance of the inner magnetosphere

729 views • 51 slides

Convection & Buoyant Force

Convection & Buoyant Force. By Ross Nuechterlein. Convection. Convection is the movement of molecules within fluids and is one of the major modes of heat and mass transfer in liquids and gas. Buoyancy .

485 views • 13 slides

Inner Core

Crust. Upper Mantle. asthenosphere. 1050 Km. Moho. Gutenburg. 2900 Km. Inner Core. 0 Km. 6371Km. 5000Km. Outer Core. Lower Mantle. Moho boundary is between 25 and 60 km deep beneath the continents and between 5 and 8 km deep beneath the ocean floor.

208 views • 4 slides

The Onset of Neutrino-Driven Convection in Core-Collapse Supernovae

The Onset of Neutrino-Driven Convection in Core-Collapse Supernovae. Brendan Krueger CEA Saclay 2013 October 18. Outline. Background Structure of CC SNe in the stalled-shock phase Instabilities in CC SNe Convective instability Standing accretion shock instability Research at CEA

398 views • 28 slides

inner core

inner core. outer core. mantle. crust. reverse fault. normal fault. strike-slip fault. thrust or reverse fault. normal fault. strike-slip fault. P Waves. push and pull motion fastest-moving waves travel in straight path move through solid and liquid material. S Waves.

595 views • 28 slides

Buoyant force

Buoyant force . buoyant force and fluid pressure. Imagine that you have a glass of ice water in front of you. Take your straw and push down the ice cubes. What happens to the ice cubes?. A force pushes the ice cubes back up This force is called buoyant force

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The Brains of Hurricanes

The Brains of Hurricanes. By: Davis . Where do hurricanes typically happen?.

168 views • 11 slides

Is inner core translation a good model ?

Is inner core translation a good model ?. Vernon Cormier, Lizzie Day, Zack Geballe, Marine Lasbleis , Mohammad Youssof , Han Yue. Does the inner core grows layer by layer?. Does it convect ?. Deguen , 2012. Summary of s eismic features. SLOW isotropic velocity

277 views • 16 slides

Convective-scale variations in the inner-core rainbands of tropical cyclones

Convective-scale variations in the inner-core rainbands of tropical cyclones. Houze 2010. Anthony C. Didlake, Jr. and Robert A. Houze, Jr. 30 th Conference on Hurricanes and Tropical Meteorology April 17, 2012. Hurricane Rita. S t r a t i f o r m. NCAR ELDORA radar.

257 views • 14 slides

Rescattering ionization of D 2 + in intense laser pulses

Rescattering ionization of D 2 + in intense laser pulses. M.Benis, A.Alnaser, T.Osipov, A.Wech, C.Wyant, J.Stuhlman, Erge Edgu-Fry, Z.Chang, B.Shan, C.Wang, M.Wells, A.Rankin, C.L.Cocke Purpose: To reveal rescattering ionization of a molecule in an intense laser pulse or

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What’s the “ Intense” in “ Intensive”?

What’s the “ Intense” in “ Intensive”?. The experience of Barnardos Australia in establishing Redfern/Waterloo Intensive Family Support Service Presentation by Kathleen Clark and Deirdre Cheers Intensive Family Services - Fifth National Practice Symposium - Bondi Beach - 2004.

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Matthew Antario D.

Matthew Antario D. Mechanical Engineering: The Code. The different languages used through a specific field. In mechanical engineering a lot of technical terms may be used therefore they may use many different acronyms and abbreviations. ASME -American society of mechanical engineers

257 views • 13 slides

Global Variability of Intense Convection

Global Variability of Intense Convection. Robert A. Houze, Jr. University of Washington. ISSCP at 30, New York, 22 April 2013. Radars in Space. CloudSat 2006-. TRMM 1997-. Epic Floods in Pakistan 2010, 2011, 2012. TRMM data showing storms producing the floods. 2010. 2011. 2012. 30N.

472 views • 36 slides

Home of the Hurricanes!

SOMERSET PREP NORTH LAUDERDALE 7101 Kimberly Boulevard North Lauderdale, FL, 33068 Phone: (954) 718-5065 Fax: (954) 718-5066 K-12 Broward County Public Charter School. Home of the Hurricanes!. WELCOME TO A NEW SCHOOL YEAR 2014-2015. Your Administrative team. Mr. Daniel Shourds, Principal

334 views • 22 slides

Inner-core diagnostics of HWRFx

Inner-core diagnostics of HWRFx. Robert Rogers (with many others, e.g., John Gamache , Gopal , Sylvie Lorsolo , Frank Marks, Dave Nolan, Paul Reasor , Jun Zhang, Xuejin Zhang) *thanks to Thiago Quirino and Kevin Yeh. Motivation.

225 views • 12 slides

CONVECTION IN THE ATMOSPHERE

Convection Requires: A Fluid Differential Heating Convection Produces: Low and High Pressure Zones Climate Zones Winds Rain-Shadow Desert Ocean Currents. CONVECTION IN THE ATMOSPHERE. MOLECULAR DESCRIPTIONS of SOLIDS, LIQUIDS, AND GASSES. SOLIDS LIQUIDS GASES

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The growth of plasma convection in Saturn ’ s inner magnetosphere

The growth of plasma convection in Saturn ’ s inner magnetosphere X. Liu; T. W. Hill; R. A. Wolf; Y. Chen Physics & Astronomy Department, Rice University, Houston, TX. Outline Rice Convection Model (RCM) 3 plasma source models Simulation results comparison with observations.

298 views • 21 slides

Convection in the Atmosphere

Convection in the Atmosphere. Chapter 6 Notes. Composition of the Atmosphere. Atmosphere: a mixture of gasses that surround the Earth Contains the oxygen you breathe and protects you from harmful rays from the sun.

409 views • 39 slides

What is the intense passionate Rafting in Rishikesh?

Rafting is a passion in river if you have to know swimming. visit: https://sacredexplorations.in/

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Is Convection in the Inner Core of Intense Hurricanes Buoyant Matthew D. Eastin

Is Convection in the Inner Core of Intense Hurricanes Buoyant Matthew D. Eastin

Presentation Transcript

2002 Atlantic Intense Hurricanes ISIDORE and LILI

The Realities of Hurricanes

Inner Magnetospheric Modeling with the Rice Convection Model

Convection &amp; Buoyant Force

Inner Core

The Onset of Neutrino-Driven Convection in Core-Collapse Supernovae

inner core

Buoyant force

The Brains of Hurricanes

Is inner core translation a good model ?

Convective-scale variations in the inner-core rainbands of tropical cyclones

Rescattering ionization of D 2 + in intense laser pulses

What’s the “ Intense” in “ Intensive”?

Matthew Antario D.

Global Variability of Intense Convection

Home of the Hurricanes!

Inner-core diagnostics of HWRFx

CONVECTION IN THE ATMOSPHERE

The growth of plasma convection in Saturn ’ s inner magnetosphere

Convection in the Atmosphere

What is the intense passionate Rafting in Rishikesh?

Convection & Buoyant Force