A. Kontogeorgos, P. Tsitsipis, C. Caroubalos, X. Moussas, P. Preka-Papadema, A. Hilaris, V. Petoussis, J.-L. Bougeret, C. E. Alissandrakis, G. Dumas, J. Polygiannakis
MEASURING SOLAR RADIO BURSTS IN THE 20-650 MHz RANGE. THE IMPROVED ARTEMIS IV MULTICHANNEL SOLAR RADIO SPECTROGRAPH OF THE UNIVERSITY OF ATHENS
We present the improved solar radiospectrograph of the University of Athens operating at the Thermopylae Satellite Station. Observations now cover the frequency range from 20 to 650 MHz. The spectrograph has a 7-meter moving parabola feeding by a log-period antenna for 100 to 650MHz and a stationary inverted V fat dipole antenna for the 20 to 100 MHz. Two receivers are operating in parallel, one sweep frequency for the whole range (10 spectra/sec, 630 channels/spectrum) and one acousto-optical receiver for the range 270 to 450 MHz (100 spectra/sec, 128 channels/spectrum). The data acquisition system consists of two PCs (equipped with 12 bit, 225ksamples/sec DAC, one for every receiver). The daily operation is fully automated: receiving universal time from a GPS, pointing the antenna to the sun, system calibration, starting and stopping the observations at preset times, data acquisition, and archiving on DVD. We can also control the whole system through modem or Internet. The instrument can be used either by itself or in conjunction with other instruments to study the onset and evolution of solar radio bursts and associated interplanetary phenomena.