2.3.2 spase://ASWS/NumericalData/Solar_Radio/Lem_Solar_Radio Australian Space Weather Services Learmonth Solar Observatory Solar Radio Data 2021-03-29T17:14:50Z The discrete frequencies Solar Radio data, also known as Radio Interference Monitoring Sets (RIMS), is obtained from Learmonth Solar Observatory, Western Australia, Australia. A radio telescope with three parabolic dish antennae to monitor solar radio flux on 8 discrete frequencies in the range 245-15400 MHz. The three parabolic dish antennae feed eight, single frequency, radio telescopes. The largest antenna, 28 feet (8.5 meters) diameter, is used to monitor 245, 410 and 610 MHz. An 8 feet (2.4 meters) dish is used to monitor the microwave frequencies of 1415, 2695, 4995 and 8800 MHz. A small 3 feet (1 meter) dish monitors the high microwave frequency of 15400 MHz. Radio telescope outputs are digitised (1 Hz sampling rate), collected by computer and transferred to Sydney SWS head Office WDC for process and archive. Observers in Learmonth also send DVDs with RIMS (2 DVD per year) to SWS as backup for the FTP data. Up to date, we have archived four different formats of RIMS data. They are SRD (from 2005), APL (1999-2008), LSR (1991-2006) and rdata (2003-2005). All of them are available on our FTP server and SWS website. All of the data files are online plottable and downloadable. We are thankful to the United States Air Force at Learmonth Solar Observatory for supplying the RIMS instrumentation and data flow, as well as the USAF staff and Bureau of Meteorology of Australia staff for maintaining and providing the solar radio data in near real time. spase://ASWS/Person/Kehe.Wang GeneralContact spase://ASWS/Person/Kehe.Wang MetadataContact spase://SMWG/Person/Lee.Frost.Bargatze MetadataContact Documentation https://www.sws.bom.gov.au/World_Data_Centre/2/8/9 includes descriptions of Observation Log format, data format en spase://ASWS/DisplayData/Solar_Radio/Lem_Solar_Radio spase://SMWG/Repository/SWS Online Open Real Time Display https://www.sws.bom.gov.au/Solar/3/4 Real Time display of solar radio (245-15400 MHz) during daylight hours in Learmonth, Display Cadence: 12 hr en World Data Centre: Data Display and Download https://www.sws.bom.gov.au/World_Data_Centre/1/10 includes browse display interface, and link to data availability chart en Access to dynamic spectra plots (not with most browsers) https://downloads.sws.bom.gov.au/wdc/wdc_solradio/data/learmonth/ Access to the Learmonth Solar Radio data files en Text None spase://ASWS/Instrument/Ground/Learmonth/Solar_Radio Waves.Passive 1991-01-01T05:00:00Z -P2D Data are current to within a day or two. PT1S Sun Earth.Magnetosphere Heliosphere.Inner Heliosphere.Outer The time span for each plot varies, generally spanning daylight hours. Discrete frequency solar radio Radio telescope Solar radio burst Solar radio flux Frequency Eight discrete frequencies used to monitor solar radio flux. PT1S Electromagnetic Magnitude Pseudo ACElectricField RadioFrequency 254 15400 MHz Solar Radio Flux Value(SFU) The Solar Flux Unit (SFU) is a convenient measure of spectral flux density often used in solar radio observations: 1 SFU = 10^4 Jy = 10^-22 Watts meter^-2 Hz^-1 = 10^-19 erg s^-1 cm^-2 Hz^-1. A local radio interference, clouds (for high frequence) etc. PT1S SFU 0 500,000 Spectral Electromagnetic