Dr. G. Chris Boynton
	Research Assistant Professor
	Fall 09 Classes:   PHY 101
	voice: (305) 284 2326 ext 1
	Fax: (305) 284 4222
	Rm 303, James L. Knight Physics Building
	1320 Campo Sano Ave., Coral Gables, Fl. 33146

My research uses computers (numerical solutions or simulations) to better understand issues in two different areas of physics: plasma MagnetoHydroDynamics (MHD*) and Radiative Transfer. We use computers to solve MHD models of the Sun's outer atmosphere, the solar corona. The solar corona presents a long standing mystery - its temperature is millions of Kelvin, whereas the sun's photosphere (visible surface) is a relatively cool 6000 Kelvin. We study how the Corona might be heated to these extreme temperatures by MHD forms of energy such as MHD waves and shocks that originate at the solar surface. In the area of Radiative Transfer I'm interested in is the study of lights propagation, scattering and absorption through the earth's atmosphere, seas and other natural media. In particular, we use computer simulations of these processeses to derive information about inherent conditions within the atmosphere or ocean from measured data about the distribution of light. Much of this work is motivated by the desire to remotely (ie. via satellite) measure conditions in the Earth's atmosphere and oceans.

For more details see my web site.

*Magnetohydrodynamics is used in the study of plasmas (ionized gasses), treating them as fluids. Magneto "fluids" are interesting because they can carry electrical currents that will then generate and interact with magnetic fields which inturn will alter the electrical currents.