77 Supergranulation PPTs View free & download

Supergranulation-Scale Solar Convection Simulations PowerPoint PPT Presentation

Supergranulation-Scale Solar Convection Simulations - 3rd order Runga-Kutta. Equation of state. tabular ... Components Composite : Uz at 17.3 Mm. Mean Atmosphere State. Temperature, Density and Pressure ...

3rd order Runga-Kutta. Equation of state. tabular ... Components Composite : Uz at 17.3 Mm. Mean Atmosphere State. Temperature, Density and Pressure ...

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Numerical Simulations of Supergranulation and Solar Oscillations PowerPoint PPT Presentation

Numerical Simulations of Supergranulation and Solar Oscillations - fast about 5 CPU-microseconds / mesh-update. includes 4-bin ... vert. velocity, surface intensity. Velocity, as seen by VAPOR (top perspective) Sunspot, ...

fast about 5 CPU-microseconds / mesh-update. includes 4-bin ... vert. velocity, surface intensity. Velocity, as seen by VAPOR (top perspective) Sunspot, ...

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Small Magnetic Elements and Supergranulation PowerPoint PPT Presentation

Small Magnetic Elements and Supergranulation - Web interface to my 3D sound speed and flow kernel code will ... De-convolve magnetic field map from travel time map. Data. Model. HMI will help with the noise ...

Web interface to my 3D sound speed and flow kernel code will ... De-convolve magnetic field map from travel time map. Data. Model. HMI will help with the noise ...

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Superrotation of Supergranulation: The Sun does The Wave PowerPoint PPT Presentation

Superrotation of Supergranulation: The Sun does The Wave - Pattern of horizontal outflows, outlined by network of magnetic features ... SOHO/MDI movie of solar supergranulation (10 day sequence at 15 min image cadence) ...

Pattern of horizontal outflows, outlined by network of magnetic features ... SOHO/MDI movie of solar supergranulation (10 day sequence at 15 min image cadence) ...

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Summary - Supergranulation, and other convective scale realistic ... NS lanes. Latitudinal variations. Thermal/velocity/magnetic correlations. Torsional oscillations ...

Supergranulation, and other convective scale realistic ... NS lanes. Latitudinal variations. Thermal/velocity/magnetic correlations. Torsional oscillations ...

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GOALS - Summary - Sasha Kosovichev. Supergranulation Simulation. Density fluctuation. 48x48x20 Mm ... 5, 1, 1.5 kG (gray) 20 G (red/green) Initial uniform. vertical ...

Summary - Sasha Kosovichev. Supergranulation Simulation. Density fluctuation. 48x48x20 Mm ... 5, 1, 1.5 kG (gray) 20 G (red/green) Initial uniform. vertical ...

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Helioseismic%20holography%20of%20Solar%20Subsurface%20Flows%20:%20progress%20 PowerPoint PPT Presentation

Helioseismic%20holography%20of%20Solar%20Subsurface%20Flows%20:%20progress%20 - a full inversion taking into account horizontal, vertical flows, and ... OLA method. regularization by hand. solutions for two depths are shown (3Mm and 14 Mm) ...

a full inversion taking into account horizontal, vertical flows, and ... OLA method. regularization by hand. solutions for two depths are shown (3Mm and 14 Mm) ...

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Mission%20Operations%20and%20Data%20Analysis%20(MO PowerPoint PPT Presentation

Mission%20Operations%20and%20Data%20Analysis%20(MO - execute a random walk resulting in large-scale field fluctuations that are ... of the field lines execute a random walk in the photosphere, resulting in large ...

execute a random walk resulting in large-scale field fluctuations that are ... of the field lines execute a random walk in the photosphere, resulting in large ...

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Stars%20II.%20Stellar%20Physics PowerPoint PPT Presentation

Stars%20II.%20Stellar%20Physics - Stars II. Stellar Physics Overview of the structure of stars Still, First the Sun as an example Overview of basic processes Nuclear energy production energy transport ...

Stars II. Stellar Physics Overview of the structure of stars Still, First the Sun as an example Overview of basic processes Nuclear energy production energy transport ...

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From detailed magneto-convection simulations to modelling the convection zone-corona system PowerPoint PPT Presentation

From detailed magneto-convection simulations to modelling the convection zone-corona system - From detailed magneto-convection simulations to modelling the ... Institute of Theoretical Astrophysics, University of Oslo. Monterey February 14 2006 ...

From detailed magneto-convection simulations to modelling the ... Institute of Theoretical Astrophysics, University of Oslo. Monterey February 14 2006 ...

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Holography - Holography & HMI. NorthWest Research Associates, Inc. Colorado Research ... power between 5-7 mHz computed in subjacent vantage with focus at surface. ...

Holography & HMI. NorthWest Research Associates, Inc. Colorado Research ... power between 5-7 mHz computed in subjacent vantage with focus at surface. ...

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Simulations of Solar Convection Zone PowerPoint PPT Presentation

Simulations of Solar Convection Zone - Simulations of Solar Convection Zone Nagi N. Mansour Goals Provide numerical simulation models for interpretation of SDO data Develop understanding of physical ...

Simulations of Solar Convection Zone Nagi N. Mansour Goals Provide numerical simulation models for interpretation of SDO data Develop understanding of physical ...

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ASTRONOMY: Earth and Space Systems PowerPoint PPT Presentation

ASTRONOMY: Earth and Space Systems - ASTRONOMY: Earth and Space Systems Standard 8-4.2: Summarize the characteristics of the surface features of the Sun: Photosphere, corona, sunspots, prominences, and ...

ASTRONOMY: Earth and Space Systems Standard 8-4.2: Summarize the characteristics of the surface features of the Sun: Photosphere, corona, sunspots, prominences, and ...

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Dynamical Implications PowerPoint PPT Presentation

Dynamical Implications - Dynamics: Nic Brummell, Sacha Brun, Marc DeRosa, Mark Miesch. Just ... POLEWARD. FLOW NEAR. SURFACE. REVERSED. FLOW. AT DEPTH. 1997. 1996. Haber et al (2002) ...

Dynamics: Nic Brummell, Sacha Brun, Marc DeRosa, Mark Miesch. Just ... POLEWARD. FLOW NEAR. SURFACE. REVERSED. FLOW. AT DEPTH. 1997. 1996. Haber et al (2002) ...

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Relationship between the High and mid latitude Solar Magnetic Field PowerPoint PPT Presentation

Relationship between the High and mid latitude Solar Magnetic Field - Relationship between the High and mid latitude Solar Magnetic Field Elena E. Benevolenskaya J. Todd Hoeksema Stanford University Contents Introduction Zonal Structure ...

Relationship between the High and mid latitude Solar Magnetic Field Elena E. Benevolenskaya J. Todd Hoeksema Stanford University Contents Introduction Zonal Structure ...

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Physics 202: Introduction to Astronomy PowerPoint PPT Presentation

Physics 202: Introduction to Astronomy - Physics 202: Introduction to Astronomy Lecture 13

Physics 202: Introduction to Astronomy Lecture 13

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An Introduction to Astronomy Part IX: The Sun, Our Star PowerPoint PPT Presentation

An Introduction to Astronomy Part IX: The Sun, Our Star - Title: Science and a Christian World View A Christian View of Science: Part II: Ideas in Conflict. Author: Lambert E. Murray Description

Title: Science and a Christian World View A Christian View of Science: Part II: Ideas in Conflict. Author: Lambert E. Murray Description

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helioseismic holography of solar subsurface flows : progress PowerPoint PPT Presentation

helioseismic holography of solar subsurface flows : progress - Braun AIA/HMI Feb 2006. 1. helioseismic holography of ... ARs: faster rotation. ARs w. large spots: outflows. ARs: no net vorticity. all other ARs: inflows ...

Braun AIA/HMI Feb 2006. 1. helioseismic holography of ... ARs: faster rotation. ARs w. large spots: outflows. ARs: no net vorticity. all other ARs: inflows ...

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The solar dynamo PowerPoint PPT Presentation

The solar dynamo - Active regions, bi-polarity. systematic east-west orientation. opposite in the south ... Still helically forced turbulence. Shear driven by a friction term ...

Active regions, bi-polarity. systematic east-west orientation. opposite in the south ... Still helically forced turbulence. Shear driven by a friction term ...

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HMI H8: Flows TimeDistance - HMI H8: Flows TimeDistance

HMI H8: Flows TimeDistance

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I. OUR OWN SUN PowerPoint PPT Presentation

I. OUR OWN SUN - Atmosphere: Photosphere, Chromosphere, ... 3. Photosphere. Temperature ... Photosphere -- Sunspots. Harriot discovered (1610) w. telescope. Dark because ...

Atmosphere: Photosphere, Chromosphere, ... 3. Photosphere. Temperature ... Photosphere -- Sunspots. Harriot discovered (1610) w. telescope. Dark because ...

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Physics 681: Solar Physics and Instrumentation Lecture 22 PowerPoint PPT Presentation

Physics 681: Solar Physics and Instrumentation Lecture 22 - The volume force can be divided into a magnetic pressure gradient and a ... Steady state: time scale of field decay d 2 / ? equals time scale of advection l / u ...

The volume force can be divided into a magnetic pressure gradient and a ... Steady state: time scale of field decay d 2 / ? equals time scale of advection l / u ...

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The Sun as a Star PowerPoint PPT Presentation

The Sun as a Star - ... in X ray images ... isotope of C captures a proton and emits a gamma-ray producing the mass-13 ... to heavier elements up to Fe (iron) requires 5 x 108o K ...

... in X ray images ... isotope of C captures a proton and emits a gamma-ray producing the mass-13 ... to heavier elements up to Fe (iron) requires 5 x 108o K ...

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Status of current work on Faculae and Sunspots PowerPoint PPT Presentation

Status of current work on Faculae and Sunspots - Accurate: Comprehensive set of rays. Coronal physics. Equation of state ... v(k) = (k P(k))1/2. Velocity driving for corona sims. Voronoi tessellation. ensemble ...

Accurate: Comprehensive set of rays. Coronal physics. Equation of state ... v(k) = (k P(k))1/2. Velocity driving for corona sims. Voronoi tessellation. ensemble ...

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Session H1: Local Helioseismology I: Current Issues PowerPoint PPT Presentation

Session H1: Local Helioseismology I: Current Issues - Session H1: Local Helioseismology I: Current Issues 3:15-3:30 Turbulent magnetohydrodynamics of the Sun: big questions and key targets for HMI - J.Toomre

Session H1: Local Helioseismology I: Current Issues 3:15-3:30 Turbulent magnetohydrodynamics of the Sun: big questions and key targets for HMI - J.Toomre

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Prograde patterns in rotating convection and implications for the dynamo PowerPoint PPT Presentation

Prograde patterns in rotating convection and implications for the dynamo - from helioseismology. spoke-like at equ. dW/dr 0 at bottom ? ... In the days before helioseismology. Angular velocity (at 4o latitude): very young spots: 473 nHz ...

from helioseismology. spoke-like at equ. dW/dr 0 at bottom ? ... In the days before helioseismology. Angular velocity (at 4o latitude): very young spots: 473 nHz ...

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Holography - Holography & HMI D. Braun, C. Lindsey, A. Birch (NWRA/CoRA) collaborators: P. Cally, A. Donea, H. Schunker (Monash U.), J. Werne, M. Woodard (NWRA/CoRA)

Holography & HMI D. Braun, C. Lindsey, A. Birch (NWRA/CoRA) collaborators: P. Cally, A. Donea, H. Schunker (Monash U.), J. Werne, M. Woodard (NWRA/CoRA)

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Walking on the Sun by Smash Mouth PowerPoint PPT Presentation

Walking on the Sun by Smash Mouth - There are 2 ways stars convert H to He Proton-proton chain CNO cycle Both yield the same results 4H He + energy Where does the Sun s energy come from? For stars ...

There are 2 ways stars convert H to He Proton-proton chain CNO cycle Both yield the same results 4H He + energy Where does the Sun s energy come from? For stars ...

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The Virtual Solar Observatory 1 Solar Data Sets - The Virtual Solar Observatory 1 Solar Data Sets

The Virtual Solar Observatory 1 Solar Data Sets

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Physics 320: Astronomy and Astrophysics Lecture X PowerPoint PPT Presentation

Physics 320: Astronomy and Astrophysics Lecture X - At wavelength where the opacity is greatest, the value of s is smallest. ... the central one third of the spectrogram height, the slit crossed a magnetically ...

At wavelength where the opacity is greatest, the value of s is smallest. ... the central one third of the spectrogram height, the slit crossed a magnetically ...

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Our Star - 1400 W/m2 at Earth's surface. 10 billion 1-Mton nuclear bombs per second ... Helioseismology. The surface of the sun oscillates like a set of bells ...

1400 W/m2 at Earth's surface. 10 billion 1-Mton nuclear bombs per second ... Helioseismology. The surface of the sun oscillates like a set of bells ...

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HMI Investigation Overview - HMI Investigation Overview

HMI Investigation Overview

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Berrilli F., Del Moro D., Giordano S., Consolini G., Kosovichev, A. PowerPoint PPT Presentation

Berrilli F., Del Moro D., Giordano S., Consolini G., Kosovichev, A. - It is able to discern characteristic dimensions of particles and particles clustering. ... This probability is given relative to what expected for a uniform random ...

It is able to discern characteristic dimensions of particles and particles clustering. ... This probability is given relative to what expected for a uniform random ...

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Accurate Polar and small scale observations during the solar cycle PowerPoint PPT Presentation

Accurate Polar and small scale observations during the solar cycle - Accurate Polar and small scale observations during the solar cycle. Elena E. ... The values of the total polar magnetic flux are depended on the number of ...

Accurate Polar and small scale observations during the solar cycle. Elena E. ... The values of the total polar magnetic flux are depended on the number of ...

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Dynamo action in shear flow turbulence PowerPoint PPT Presentation

Dynamo action in shear flow turbulence - Nils Erland Haugen (Univ. Trondheim) Wolfgang Dobler ... In the days before helioseismology. Angular velocity (at 4o latitude): very young spots: 473 nHz ...

Nils Erland Haugen (Univ. Trondheim) Wolfgang Dobler ... In the days before helioseismology. Angular velocity (at 4o latitude): very young spots: 473 nHz ...

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Introductory Lectures on Solar Magnetism PowerPoint PPT Presentation

Introductory Lectures on Solar Magnetism - All in all, the Sun becomes our great physics laboratory in the sky. ... Eugene N. Parker. Outline. Overview of Solar Magnetism ...

All in all, the Sun becomes our great physics laboratory in the sky. ... Eugene N. Parker. Outline. Overview of Solar Magnetism ...

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HAO Science Objectives for HMI PowerPoint PPT Presentation

HAO Science Objectives for HMI - Solar Dermatology - A brief tour through the esoteric terminology Anemone Arcade Bright Point Coronal Hole Coronal Mass Ejection Coronal Rain Cusp

Solar Dermatology - A brief tour through the esoteric terminology Anemone Arcade Bright Point Coronal Hole Coronal Mass Ejection Coronal Rain Cusp

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REU Training The Solar Atmosphere Jerry Harder jerry'harderlasp'colorado'edu 303 492 1891 - REU Training The Solar Atmosphere Jerry Harder jerry'harderlasp'colorado'edu 303 492 1891

REU Training The Solar Atmosphere Jerry Harder jerry'harderlasp'colorado'edu 303 492 1891

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The creation of magnetic structures from velocity shear - The creation of magnetic structures from velocity shear

The creation of magnetic structures from velocity shear

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Solar Interior (continued) PowerPoint PPT Presentation

Solar Interior (continued) - Solar Interior (continued) Role of convection energy transport in the solar interior * * * Sun is fully convective up to 1.4 x106 years temperature throughout

Solar Interior (continued) Role of convection energy transport in the solar interior * * * Sun is fully convective up to 1.4 x106 years temperature throughout

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Physics 681: Solar Physics and Instrumentation PowerPoint PPT Presentation

Physics 681: Solar Physics and Instrumentation - Flux erupts in the form of loops (not always as bipolar structure) ... The sunspot atmosphere is compressible, stably stratified, and has a magnetic ...

Flux erupts in the form of loops (not always as bipolar structure) ... The sunspot atmosphere is compressible, stably stratified, and has a magnetic ...

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OUR ENIGMATIC SUN PowerPoint PPT Presentation

OUR ENIGMATIC SUN - Old Picture Atmosphere - static, T(r) E.g., old model of chromosphere: Temp (height) ... Stereoscopic images of corona. Solar Orbiter (ESA) * 3 times closer ...

Old Picture Atmosphere - static, T(r) E.g., old model of chromosphere: Temp (height) ... Stereoscopic images of corona. Solar Orbiter (ESA) * 3 times closer ...

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TOTAL SOLAR IRRADIANCE AND CLIMATE PowerPoint PPT Presentation

TOTAL SOLAR IRRADIANCE AND CLIMATE - ... and Gravity Oscillation Experiment (VIRGO) on the Solar and heliospheric Observatory (SOHO) ... besides natural causes, man-made activities are ...

... and Gravity Oscillation Experiment (VIRGO) on the Solar and heliospheric Observatory (SOHO) ... besides natural causes, man-made activities are ...

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OUR ENIGMATIC SUN - ECLIPSE Movie. ECLIPSE in Turkey, 1999. In corona B dominates plasma ... Guitar string can oscillate in different normal modes. Sun too ...

ECLIPSE Movie. ECLIPSE in Turkey, 1999. In corona B dominates plasma ... Guitar string can oscillate in different normal modes. Sun too ...

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1' FPP Science Goals PowerPoint PPT Presentation

1' FPP Science Goals - Solar & Astrophysics Laboratory. FPP Overview. Primary FPP Science Goals. Magnetic Flux ... Solar & Astrophysics Laboratory. FPP Overview. Level 0 Requirements ...

Solar & Astrophysics Laboratory. FPP Overview. Primary FPP Science Goals. Magnetic Flux ... Solar & Astrophysics Laboratory. FPP Overview. Level 0 Requirements ...

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Solar Magnetism - Solar Magnetism

Solar Magnetism

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CDP Workshop on Magnetic Fields and Structures Magnetic fields on Normal i'e', nondegenerate Stars PowerPoint PPT Presentation

CDP Workshop on Magnetic Fields and Structures Magnetic fields on Normal i'e', nondegenerate Stars - ... for stellar magnetic cycles from the Mt. Wilson Ca II index program (Baliunas et ... Applied to the chemically peculiar star 53 Cam. ...

... for stellar magnetic cycles from the Mt. Wilson Ca II index program (Baliunas et ... Applied to the chemically peculiar star 53 Cam. ...

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Solar%20Energy%20II PowerPoint PPT Presentation

Solar%20Energy%20II - ... where D is the distance across the reflector and ... to produce a p-n junction p-n ... depletion region where electric field ...

... where D is the distance across the reflector and ... to produce a p-n junction p-n ... depletion region where electric field ...

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Solar Science Workshop PowerPoint PPT Presentation

Solar Science Workshop - An Introduction to the Physics of Our Star: The Sun Distance from Earth 1 AU Travel time for Light to Earth About 8 minutes Travel time for solar wind to 1 AU

An Introduction to the Physics of Our Star: The Sun Distance from Earth 1 AU Travel time for Light to Earth About 8 minutes Travel time for solar wind to 1 AU

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Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). - What evidence do we have that the granulation seen on the Sun's surface is caused by convection? a.

What evidence do we have that the granulation seen on the Sun's surface is caused by convection? a.

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Solar Energy II PowerPoint PPT Presentation

Solar Energy II - Solar Energy II Lecture #9 HNRT 228 Energy and the Environment Chapter 4 Summary Energy from the Sun Spoke way too much about this in our last meeting Today s focus ...

Solar Energy II Lecture #9 HNRT 228 Energy and the Environment Chapter 4 Summary Energy from the Sun Spoke way too much about this in our last meeting Today s focus ...

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R. Komm - Kinetic Helicity Density (v curl v) Physical Parameters ... Kinetic Helicity Density. Zonal flow and north-south asymmetry. Corrected for annual variations ...

Kinetic Helicity Density (v curl v) Physical Parameters ... Kinetic Helicity Density. Zonal flow and north-south asymmetry. Corrected for annual variations ...

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Seismology of the Solar Atmosphere PowerPoint PPT Presentation

Seismology of the Solar Atmosphere - Seismology of the Solar Atmosphere HELAS Roadmap Workshop, OCA Nice Wolfgang Finsterle, PMOD/WRC, Davos, Switzerland Seismology of the Solar Atmosphere Conceptual ...

Seismology of the Solar Atmosphere HELAS Roadmap Workshop, OCA Nice Wolfgang Finsterle, PMOD/WRC, Davos, Switzerland Seismology of the Solar Atmosphere Conceptual ...

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Our Star, the Sun PowerPoint PPT Presentation

Our Star, the Sun - Title: PowerPoint Presentation Author: Sumanas Last modified by: Shalom Fisher Created Date: 12/24/2002 1:08:46 AM Document presentation format: On-screen Show (4:3)

Title: PowerPoint Presentation Author: Sumanas Last modified by: Shalom Fisher Created Date: 12/24/2002 1:08:46 AM Document presentation format: On-screen Show (4:3)

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Turbulent Origins of the Solar Wind PowerPoint PPT Presentation

Turbulent Origins of the Solar Wind - Basal acoustic flux: 108 erg/cm2/s (equiv. ' piston' v = 0.3 km/s) ... http://cfa-www.harvard.edu/~scranmer/ Turbulent Origins of the Solar Wind. Steven R. Cranmer ...

Basal acoustic flux: 108 erg/cm2/s (equiv. ' piston' v = 0.3 km/s) ... http://cfa-www.harvard.edu/~scranmer/ Turbulent Origins of the Solar Wind. Steven R. Cranmer ...

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A Model of the Chromosphere: Heating, Structures, and Convection PowerPoint PPT Presentation

A Model of the Chromosphere: Heating, Structures, and Convection - A Model of the Chromosphere: Heating, Structures, and Convection P. Song1, and V. M. Vasyli nas1,2 Center for Atmospheric Research and Department of Environmental ...

A Model of the Chromosphere: Heating, Structures, and Convection P. Song1, and V. M. Vasyli nas1,2 Center for Atmospheric Research and Department of Environmental ...

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Supergranulation PowerPoint PPT Presentations