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STRUCTURE

STRUCTURE. AND. BEHAVIOR. OF. SOL. Please change the title (think of a more exciting one). Also, the title animation takes too long- modify or animate the text all at once (and not by level). Sol - (in Latin for the sun) the star at the center of the Solar System.

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STRUCTURE

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  1. STRUCTURE AND BEHAVIOR OF SOL Please change the title (think of a more exciting one). Also, the title animation takes too long- modify or animate the text all at once (and not by level).

  2. 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. Image looks very similar to the one in the first slide. Change it so you add variety to your report. Also, cite the source of your image. There are too many words in this report. Use keywords only- see suggested changes in the next slide.

  3. Animation is too slow- change the timing. • Latin for Sun • Central star • Almost perfectly spherical • Hot plasma with magnetic fields • Diameter of 1,392,000 km (109x Earth’s)

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

  5. STRUCTURE 1. Thecore of the Sun is considered to extend from the center to about 0.2 to 0.25 solar radius. 2. Theradiation zone orradiative 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. Too crowded. One part = one slide. This way you can maximize the picture and the info. See how I changed this slide into the next two slides.

  6. CORE • 0.2 to 0.25 solar radius • add more info here (What happens in the core?)

  7. RADIATION ZONE • Energy transported via radiation • Add more info (What exactly is radiation?) Choose an image with better resolution. This one is pixilated.

  8. CONVECTION ZONE 3. The convection zone  of a star is the range of  radii in which energy is transported primarily by  convection. 4. Thephotosphere of an astronomical object is the region from which externally received light Originates.

  9. STRUCTURE 5. Thechromosphere is the second of the three main layers in the Sun's atmosphere and is roughly 2,000 kilometers deep.  6. Acorona 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.

  10. STRUCTURE 7. Sunspotsare temporary phenomena on 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.

  11. STRUCTURE 9. Aprominence is a large, bright feature extending outward from the Sun's surface, often in a loop shape.

  12. BEHAVIOR Ageomagnetic stormthat is caused by the sun is a temporary disturbance of the  Earth'smagnetospherecaused 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. Too many words! Cite the source of your image. Paste the URL here.

  13. BEHAVIOR A 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. Please make a concluding slide. What is the most important message in your report? What do you want your audience to remember? THANK YOU FOR LISTENING!!!

  14. THE E N D

  15. BY : Maria Rita Montserrat B. Fernandez-Cuervo Add the following to your report: How does the Sun make life possible on Earth? How should we behave in response to the Sun’s activities? (UV radiation, etc.) Year I – Agnes Bojaxiu

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