PPT-A Babcock-Leighton type solar dynamo working in the bulk of the convection zone

Beihang University China Key points The toroidal fields are produced in the bulk of the convection zone by the latitudinal shear The tachocline is unimportant in our model Zebin Zhang amp . The Swan 1050 1300 1512 Eaton Bray Northall Road 1055 1305 1514 Edlesborough opp Combined School 1100 1310 1517 Edlesborough Combined School 0845 Eaton Bray Northall Road 0850 Northall The Swan 0855 Dagnall Village Hall 1105 1315 Solar interior. Standard solar model. Solar evolution, past, present and future. The solar interior. Solar interior cannot be directly observed, information is from:. Theoretical models. Helioseismology. Webinar . Series. Dynamics of the Madden-Julian Oscillation Field Campaign. Climate Variability. . & Predictability. Shipboard Measurements of Aerosol Chemical, Physical, and Optical Properties during . David M. Romps. Workshop on Large-Scale Circulations. in Moist Convecting Atmospheres. October. 17, 2009. The bulk. -plume equations. , when used to diagnose large-eddy simulations, underestimate convective entrainment.. WE CAN SEE IT REALLY WELL.. The Sun is the basis for all of our knowledge of stars. Why?. temperature . kelvin. . degree Celsius . degree Fahrenheit . symbol . K . °C . °F . boiling point of water . Bjerknes. Memorial Lecture, AGU, San Francisco, 4 December 2012. Robert Houze. University of Washington. A personal story of three great field campaigns and the evolution of meteorological satellites . AMIE/DYNAMO. Angela Rowe and Robert . Houze. , Jr.. University of Washington. ASR Science Team Meeting. Potomac, MD. 13 March 2014. AMIE/DYNAMO. Zuluaga. and . Houze. (2013). Active periods: Increased rainfall/organization. Kepler. B. öhm-Vitense. 2007, . ApJ. , 657, 486. Asteroseismology. 101. Mean . density. Age. Mean . density. Size. of the . convection. zone. Mean . density. Age. 10. 11. Depth of the convection zone. The Sun and the Stars. Stellar Lifecycle. Starbirth. Young Stars. Globular Clusters. Star Death. Star Death. Star Death. Star Death. Aims and Objectives. To introduce you to the properties of . t. he Sun and the stars, and their evolution. Contents. Introduction. General . information. Structure. Formation. Life and Death. Features. Observation. introduction. Great ball of hydrogen plasma. Gravitational centre of . system. 99.8% the mass of the entire solar system. T. Tomm 2019. Heat Transfer. This Photo. by Unknown Author is licensed under . CC BY-NC-ND. What type of camera can measure temperatures?. A. Spectral B. Conductive C. Thermal. Which type of heat transfer occurs when heat moves through a piece of metal, such as a metal spoon? . CORE. The sun produces an enormous amount of energy in its core, or central region. The sun's energy comes from nuclear fusion. During nuclear fusion, hydrogen atoms join together to form helium. Nuclear fusion only can take place under conditions of extremely high pressure and temperature. The temperature inside the sun's core reaches 15 million C, high enough for nuclear fusion to take place. . Exoplanets. Kazunari. Shibata. . Kwasan. and . Hida. observatories, . Kyoto University. Hiroaki Isobe. Unit of Synergetic Studies for Space, Kyoto University. isobe@kwasan.kyoto. -. u.ac.jp. COSPAR2014, . O. f . F. ields and . F. lows in the . I. nterior and . E. xterior of the . S. un. A Heliophysics DRIVE Science Center. J. Todd Hoeksema, Stanford University. 1. COFFIES. . C. onsequences . o. f . F.