Solar Activity Observatory early stages: Analysis of the diurnal variations in the amplitude strength at 20.1MHz

We present the results of the early stages of a Solar Activity Observatory: the continuous monitoring of 20.1MHz signal strength in order to study the solar activity. Since the project is quite young, as to say, we have 3 months of observations, in this sense, we were able to observe diurnal changes...

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Bibliographic Details
Published in2020 XXXIIIrd General Assembly and Scientific Symposium of the International Union of Radio Science pp. 1 - 3
Main Authors Escobedo-Galvan, C.R., Castro Nieto, C.P., Perez-Martinez, M.I.
Format Conference Proceeding
LanguageEnglish
Published URSI 01.08.2020
Subjects
Monitoring
Observatories
Time measurement
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Summary:We present the results of the early stages of a Solar Activity Observatory: the continuous monitoring of 20.1MHz signal strength in order to study the solar activity. Since the project is quite young, as to say, we have 3 months of observations, in this sense, we were able to observe diurnal changes. The difference between the day and night amplitude strength, the time it takes the amplitude to increase and decrease from day to night, and some special features such as a B class solar flare during May 6.
ISSN:2642-4339
DOI:10.23919/URSIGASS49373.2020.9232343