HR: 1340h
AN: IN23A-0945    [Abstracts]
TI: Description Of Computational Routines For Accessing And Using Real Time Data In The Mexican Array Radiotelescope (MEXART)
AU: * Casillas-Perez, G
EM: gacp@geofisica.unam.mx
AF: Instituto de Geofisica Universidad Nacional Autonoma de Mexico, Instituto de Geofisica Ciudad Universitaria s/n Delegacion Coyoacan, Mexico, D.F 04510, Mexico
AU: Jeyakumar, S
EM: sjk@astro.ugto.mx
AF: Departamento de Astronomia Universidad de Guanajuato, Apartado postal 144, Guanajuato, Gto 36000, Mexico
AU: Carrillo-Vargas, A
EM: armando@geofisica.unam.mx
AF: Instituto de Geofisica Universidad Nacional Autonoma de Mexico, Instituto de Geofisica Ciudad Universitaria s/n Delegacion Coyoacan, Mexico, D.F 04510, Mexico
AU: Andrade-Mascote, E
EM: eandrade@geofisica.unam.mx
AF: Instituto de Geofisica Universidad Nacional Autonoma de Mexico, Instituto de Geofisica Ciudad Universitaria s/n Delegacion Coyoacan, Mexico, D.F 04510, Mexico
AU: Gonzalez-Esparza, A
EM: americo@geofisica.unam.mx
AF: Instituto de Geofisica Universidad Nacional Autonoma de Mexico, Instituto de Geofisica Ciudad Universitaria s/n Delegacion Coyoacan, Mexico, D.F 04510, Mexico
AB: The Mexican Array Radiotelescope (MEXART) is a 64x64 dipole antenna element array used to carry out IPS observations of various radio sources in the sky. This kind of observations are of importance for the construction of daily maps of the sky, and are helpful in the detection and trace of solar perturbations propagating througout the solar wind, which can reach the Earth. To obtain and to handle the MEXART data observations a lot of work of computation is required for the acquisition, storage and data processing. In this work we report the structure of the acquired data and programs implemented as a support tool for the real time data processing, that leads to some results in which some radio sources are observed.
DE: 7500 SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY
SC: Earth and Space Science Informatics [IN]
MN: 2007 Fall Meeting