e-Callisto
MEXICO-UANL-INFIERNILLO


The Callisto solar spectrometer is a programmable heterodyne receiver designed in 2006 by Christian Monstein, a member of the Radio Astronomy Group
at ETH Zurich, Switzerland. Several Callisto receivers are installed worldwide and are part of the e-Callisto network. You can access the data for the
entire network here
The Callisto MEXICO-UANL-INFIERNILLO station is located in the Galeana mountain range, Nuevo León. It is located in the Galeana Mountains, Nuevo León.
The station belongs to the Faculty of Physical and Mathematical Sciences (FCFM) of the Autonomous University of Nuevo León (UANL). It is configured to
monitor the 45-90 MHz band, at 200 frequencies, four times per second. It uses an LWA crossed dipole antenna. It also has a power coupler with a quadrature
(LWAPC-Q) that feeds the crossed dipole antenna's active balun array through the coaxial transmission lines. The LWAPC-Q has two identical RF circuits and is
inserted between the antenna array and the receivers. This allows for discrimination of circular polarizations received by linearly polarized crossed dipoles.
The MEXICO-UANL-INFIERNILLO dataset has a DOI:
If you use the dataset in a publication, please cite it as:
Peralta-Mendoza, I. A.; Romero-Hernandez, E.; Perez-Tijerina, E.; (2025), e-Callisto (MEXICO-UANL-INFIERNILLO). Universidad Autónoma de Nuevo León, doi:
© Hecho en México. Universidad Nacional Autónoma de México (UNAM). Todos los derechos reservados (2025).