A Dicke-type microwave radiometer has been developed for daily measurement of solar flux at 2800 MHz. The antenna system, consists of a 5 foot parabolic dish with horn feed, is equatorially mounted and is capable of tracking the sun for about 8 hours each day. The dynamic range of the radiometer is such that even strong solar bursts (flux = 10,000 × 10-22 Watts m-2 Hz-1) can be recorded by using the receiver in the AGC mode. The calibration procedure and the errors involved in the measurement of the solar flux are briefly discussed. Some sample records of solar bursts made by means of this equipment are presented
The interference radiotelescope for receiving of the solar radio waves at frequency 220 MHz and cont...
Simple thermopiles formed by copper-plating a constantan wire were used to build a solarimeter and a...
An area of increasing interest is the establishment of a significant research program in microwave r...
Abstract: We report the development of solar flux receivers operating at 2.8 GHz to monitor solar ra...
In this paper we present an overview of solar radio observations at 11.2 GHz on Metsähovi Radio Obse...
Data on disturbed sun emission at different microwave frequencies observed at Sagamore Hill Solar Ra...
In studies of solar active regions and bursts, the ability to obtain spatially resolved radio spectr...
196-198Data on disturbed sun emission at different microwave frequencies observed at Saga nore Hill ...
53-60A solar radio spectrograph (SRS), constructed at our School of Physics to study the dynamic act...
The Sun is considered as one of the strongest radio sources and observation in radio region can prov...
International audienceDecameter wavelength radio emission is finely structured in solar bursts. For ...
Observations of the solar radio spectrum have been made at the Harvard Radio Astronomy Station, Fort...
We report on the study and successful application of an improved measurement method for solar flares...
In this article, an evaluation of the flux density of the solar radio burst is presented. A rod alum...
Tabulations of the daily values of solar radio and burst observed on a frequency of 2800MHz at the A...
The interference radiotelescope for receiving of the solar radio waves at frequency 220 MHz and cont...
Simple thermopiles formed by copper-plating a constantan wire were used to build a solarimeter and a...
An area of increasing interest is the establishment of a significant research program in microwave r...
Abstract: We report the development of solar flux receivers operating at 2.8 GHz to monitor solar ra...
In this paper we present an overview of solar radio observations at 11.2 GHz on Metsähovi Radio Obse...
Data on disturbed sun emission at different microwave frequencies observed at Sagamore Hill Solar Ra...
In studies of solar active regions and bursts, the ability to obtain spatially resolved radio spectr...
196-198Data on disturbed sun emission at different microwave frequencies observed at Saga nore Hill ...
53-60A solar radio spectrograph (SRS), constructed at our School of Physics to study the dynamic act...
The Sun is considered as one of the strongest radio sources and observation in radio region can prov...
International audienceDecameter wavelength radio emission is finely structured in solar bursts. For ...
Observations of the solar radio spectrum have been made at the Harvard Radio Astronomy Station, Fort...
We report on the study and successful application of an improved measurement method for solar flares...
In this article, an evaluation of the flux density of the solar radio burst is presented. A rod alum...
Tabulations of the daily values of solar radio and burst observed on a frequency of 2800MHz at the A...
The interference radiotelescope for receiving of the solar radio waves at frequency 220 MHz and cont...
Simple thermopiles formed by copper-plating a constantan wire were used to build a solarimeter and a...
An area of increasing interest is the establishment of a significant research program in microwave r...