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This paper presents a detailed description of various subsystems of CALLISTO solar radio spectrograph installed at the USO/PRL. In the front-end system, a log periodic dipole antenna (LPDA) is designed for the frequency range of 40-900 MHz. In this paper LPDA design, its modifications, and simulation results are presented. We also present some initial observations taken by CALLISTO at Udaipur.
A CALLISTO spectrometer to monitor solar radio transient emissions from $approx 0.8-1.6~R_{odot}$ (above photosphere) is installed at IISER, Pune, India (longitude $73^{circ} 55$ E and latitude $18^{circ}31$ N). In this paper, we illustrate the instr
Our knowledge of the Sun, its atmosphere, long term activity and space weather potential is severely limited by the lack of good observations of the polar and far-side regions. Observations from a polar vantage point would revolutionize our understan
The Askaryan Radio Array (ARA) reports an observation of radio emission coincident with the Valentines Day solar flare on Feb. 15$^{rm{th}}$, 2011 in the prototype Testbed station. We find $sim2000$ events that passed our neutrino search criteria dur
The observation and research of the solar radio emission have unique scientific values in solar and space physics and related space weather forecasting applications, since the observed spectral structures may carry important information about energet
NASAs WB-57 High Altitude Research Program provides a deployable, mobile, stratospheric platform for scientific research. Airborne platforms are of particular value for making coronal observations during total solar eclipses because of their ability