Friday, December 15, 2006
Computer science
Computer science, or computing science, is the study of the theoretical basics of information and calculation and their execution and application in computer systems. Computer science has lot of sub-fields; a few highlight the calculation of exact consequences (such as computer graphics), whereas others (such as computational complexity theory) relate to properties of computational difficulties. Still others focus on the challenges in applying calculations. For instance, programming language theory studies move toward to describe calculations, whereas computer programming applies precise programming languages to answer precise computational difficulties.
Wednesday, December 06, 2006
Convection zone
Structure of the SunFrom about 0.7 solar radii to the Sun's visible surface, the material in the Sun is not dense enough or hot enough to transfer the heat energy of the interior outward via radiation. As a result, thermal convection occurs as thermal columns carry hot material to the surface (photosphere) of the Sun. Once the material cools off at the surface, it plunges back downward to the base of the convection zone, to receive more heat from the top of the radiative zone. Convective overshoot is thought to occur at the base of the convection zone, carrying turbulent downflows into the outer layers of the radiative zone.
The thermal columns in the convection zone form an imprint on the surface of the Sun, in the form of the solar granulation and supergranulation. The turbulent convection of this outer part of the solar interior gives rise to a "small-scale" dynamo that produces magnetic north and south poles all over the surface of the Sun.
The thermal columns in the convection zone form an imprint on the surface of the Sun, in the form of the solar granulation and supergranulation. The turbulent convection of this outer part of the solar interior gives rise to a "small-scale" dynamo that produces magnetic north and south poles all over the surface of the Sun.
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