HR: 0800h
AN: SH41A-12    [Abstracts]
TI: 3D Simulations of Solar Observations in Radio, Millimeter and Submillimeter Wavelengths.
AU: * De la Luz, V H
EM: vdelaluz@inaoep.mx
AF: Instituto Nacional de Astrofisica Optica y Electronica, Luis Enrique Erro #1, Tonantzintla, Puebla, Mexico., 72000,
AU: Lara, A
EM: alara@geofisica.unam.mx
AF: Instituto de Geofisica, UNAM, Ciudad Universitaria SN, Del. Coyoacan, Mexico D.F., 04510,
AU: Mendoza, E
EM: mend@inaoep.mx
AF: Instituto Nacional de Astrofisica Optica y Electronica, Luis Enrique Erro #1, Tonantzintla, Puebla, Mexico., 72000,
AB: In this work we present 3D simulations of solar radio emission at different frequencies (1.4, 3.9, 17, 34, 43, 110GHz and 12GHz), in the centimeter - submilimeter wavelength range. We build a 3D, spherically symetric, solar model and solve the clasical equation of radiative transfer using quiet Sun temperature and electron density models. We compare our results with observations from Nobeyama Radio Heliograph and SMT submillimeter telescope at CASILEO. The 3.9 and 43 GHz images will be useful to calibrate the observations of new millimeter telescope (RT5) which is being constructed at "Sierra Negra" Volcano, in the state of Puebla, Mexico, at an altitude of 4,600 m. This project is a collaboration between Universidad Nacional Autonoma de Mexico (UNAM) and Instituto Nacional de Astrofisica Optica y Electronica (INAOE).
DE: 0545 Modeling (4255)
DE: 0560 Numerical solutions (4255)
DE: 7546 Transition region
DE: 7847 Radiation processes
DE: 7859 Transport processes
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2007 Joint Assembly