Other
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh41a1625m&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #SH41A-1625
Other
[0604] Electromagnetics / Antenna Arrays, [0609] Electromagnetics / Antennas, [0694] Electromagnetics / Instruments And Techniques, [7999] Space Weather / General Or Miscellaneous
Scientific paper
The Mexican Array Radio Telescope (MEXART) has an antenna composed by 4096 full-wavelength dipoles, covering about 9800 square meters. The instrument is primary devoted to carry out observations of compact stelar radio sources presenting Interplanetary Scintillation (IPS) at 140 MHz. The IPS technique is a very useful tool to perform observations of large-scale solar wind density disturbances in the inner heliosphere at heliocentric ranges where no other instruments can cover. These observations can help to track the evolution of CMEs and shocks in the interplanetary medium. We present the first catalog of IPS sources detected with the MEXART. We show the power spectrum analysis to obtain information of solar wind velocity and density.
Aguilar-Rodriguez Ernesto
Andrade-Mascote E.
Carrillo-Vargas Armando
Gonzalez-Esparza Americo
Mejia Ambriz J. C.
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