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You are in the convection zone. The vibrations you feel are due to the fact that the fluid (we call it plasma) which ... Imaginary trip; Convection zone: where, what, how, why, ...; 1. Where is the Convection Zone Located; 2. What do we see from it; 3. What is it; It is made out of plasma; It is convecting (boiling);
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www.cora.nwra.com/~werne/eos/text/convection_zone.html
www.cora.nwra.com/~werne/eos/text/convection_zone.html
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The most efficient means of energy transfer is now convection and we find ourselves in the region of the Sun's interior know as the convection zone. The hotter material near the top of the radiation zone (the bottom of the convection zone) rises up and the cooler material sinks to the bottom.
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solar.physics.montana.edu/ypop/Spotlight/SunInfo/Conzon...
solar.physics.montana.edu/ypop/Spotlight/SunInfo/Conzone.html
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The combination of what takes place in the convection zone and the differential rotation of the Sun creates something called the solar dynamo. This phenomenon is the true origin of solar activity.
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solar-heliospheric.engin.umich.edu/hjenning/ConvectiveZ...
solar-heliospheric.engin.umich.edu/hjenning/ConvectiveZone.html
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; The convection zone of the Sun; Click on image for full size (52K GIF); ... The convection zone is farther away from the core than the the radiative zone. At this point turbulent convective motions occur, similar to a pot of boiling water. The overturning (bubbling) motions inside the Sun are responsible for the...
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www.windows.ucar.edu/tour/link=/sun/Solar_interior/Sun_...
www.windows.ucar.edu/tour/link=/sun/Solar_interior/Sun_layers/Convection_zone/convection_zone.html
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The convection zone in the Sun occurs above the radiative zone, at about .7 to .8 solar radii from the center of the Sun. At this point the temperature gradient (the change in temperature with depth) becomes so large that turbulent convective motions occur, similar to a pot of boiling water.
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www.windows.ucar.edu/tour/link=/sun/Solar_interior/Sun_...
www.windows.ucar.edu/tour/link=/sun/Solar_interior/Sun_layers/Convection_zone/convection_zone.html&edu=high
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The Convection Zone ... Energy is generated in the core, the innermost 25%. This energy diffuses outward by radiation (mostly gamma-rays and x-rays) through the radiative zone and by convective fluid flows (boiling motion) through the convection zone, the outermost 30%. The thin interface layer (the "tachocline") between...
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solarscience.msfc.nasa.gov/interior.shtml
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CiteSeerX - Document Details (Isaac Councill, Lee Giles): Bipolar magnetic regions are believed to form when flux originating below the solar convection zone rises to the surface in the form of long thin loops. ... 1 Emergence of anchored flux tubes through the convection zone – Fisher, Chou, et al. - 1989...
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citeseer.ist.psu.edu/197898.html
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