STRUCTUREANDBEHAVIOROFSOL

http://verelcielonews.wordpress.com/

Contents1. Sol

* Structure- Parts- Description of (parts)> Core >Radiative Zone > Convective zone> Corona > Photosphere > Chromosphere> Sunspot > Granules > Prominence

* Behavior- geomagnetic storm- solar flare

It’s good that you used hyperlinks. However, you have to have a way of coming back to this slide. You can do this by inserting an action button that links to last slide viewed. You may consult with me in school if you’re not sure how to do this.

Sol - (in Latin for the sun) the star at the center of the Solar System. It is almost perfectly Spherical and consists of hot plasma interwoven with magnetic fields. It has a diameter of about 1,392,000 km, about 109 times that of Earth, and its mass. http://curio-world.blogspot.com/2012/02/sun.

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Too many words. Keywords only please.

1. Core 2. Radiative Zone3. Convective zone4. Photosphere5. Chromosphere6. Corona7. Sunspot8. Granules9. Prominence

STRUCTURE (Parts)

http://en.wikipedia.org/wiki/Sun

STRUCTURE1. The core of the Sun is considered to extend from the center to about 0.2 to 0.25 solar radius.

2. The radiation zone or radiative zone is a layer of a star's interior where energy is primarily transported toward the exterior by means of radiative diffusion , rather than by convection.

http://planetfacts.org/what-color-is-the-sun/

Please revise this according to my comments in your first draft.

3. The convection zone of a star is the range of radii in which energy is transported primarily by convection.

STRUCTURE

4. The photosphere of an astronomical objectis the region from which externally received light Originates.

http://planetfacts.org/what-color-is-the-sun/

STRUCTURE5. The chromosphere is the second of the three main layers in the Sun's atmosphere and is roughly 2,000 kilometers deep.

6. A corona is a type of plasma "atmosphere of the Sun or other celestial body, extending millions of kilometers into space, most easily seen during a total solar eclipse , but also observable in a coronagraph.

http://planetfacts.org/what-color-is-the-sun/

STRUCTURE7. Sunspots are temporary phenomenaon the photosphere of the Sun that appear visibly as dark spots compared to surrounding Regions.

8. Granules on the photosphere of the Sun are caused by convection currents within the Sun's convective zone.

http://planetfacts.org/what-color-is-the-sun/

STRUCTURE9. A prominence is a large, bright feature extending outward from the Sun's surface, often in a loop shape.

http://planetfacts.org/what-color-is-the-sun/

BEHAVIORA geomagnetic storm that is caused

by the sun is a temporary disturbance of the Earth's magnetosphere caused by a disturbance in the interplanetary medium. A geomagnetic storm is a major component of space weather and provides the input for many other components of space weather. A geomagnetic storm is caused by a solar windshock wave or cloud of magnetic field which interacts with the Earth's magnetic field. The increase in the solar wind pressure initially compresses the magnetosphere and the solar wind's magnetic field will interact with the Earth’s magnetic field and transfer An increased amount of energy into the magnetosphere.

http://oilismastery.blogspot.com/2008/12/giant-breach-in-earths-magnetic-field.html

Keywords only please. The animation is too slow. Please change it.

BEHAVIORA solar flare is a sudden brightening observed over the

Sun's surface or the solar limb, which is interpreted as a large energy release of up to 6 × 1025 joules of energy. These are not visible from Earth's surface.

http://www.bibliotecapleyades.net/imagenes_ciencia/conscious_universe50_01.jpg

THEE N D

THANK YOU FOR LISTENING!!!

http://www.boston.com/bigpicture/2008/10/the_sun.html

BY : Maria Rita Montserrat B. Fernandez-Cuervo

Year I – Agnes Bojaxiu

http://www.tarotelprada.com/2011/07/significado-de-los-suenos-el-sol.html