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SWS Cosmic Ray Data, Australasia (from Kingston and Mawson Stations) (2004 onwards)
Cosmic rays consist mainly of protons of extremely high energies. They can originate from galactic sources or from the Sun. Cosmic rays are observed indirectly. At the lowest... -
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SWS Solar Images from Culgoora (N.S.W.) and Learmonth (W.A) Solar...
Australia has made major contributions to research in solar physics for several decades. Solar images are a major kind of record of solar activities. The SWS has monitored and... -
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SWS Magnetometer Data, Southern Hemisphere (1995 onwards)
The magnetometer data provides a measure of variations of the Earth's magnetic field in 2 or 3 orthogonal directions, typically in the geomagnetic north-south and east-west... -
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SWS Riometer Data, Four Stations in Southern Hemisphere / Antarctica (1987 onwards)
The SWS WDC ( World Data Centre ) archives Riometer data obtained from Casey, Davis, Mawson and Macquarie Island in Antarctica. The first Riometer data file was obtained on... -
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SWS Ionospheric Scintillation Monitor Data (1999 onwards)
Ionospheric scintillation is a rapid fluctuation of radio-frequency signal phase and/or amplitude, which is generated as a signal passes through the ionosphere. Scintillation... -
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SWS Raw and Clean Ionogram, Scaled Ionspheric data ( 1938 onwards ), Australasia
Ionograms are an image of frequency versus time delay (virtual height) of HF echoes from the ionosphere recorded by an ionosonde. An ionosonde is a swept frequency HF pulsed... -
SWS Solar Radio Data from Learmonth (1991 onwards)
The discrete frequencies Solar Radio data, also known as Radio Interference Monitoring Sets (RIMS), is obtained from Learmonth Solar Observatory, Western Australia. Equipment: A... -
SWS Sunspot Numbers (1700 onwards)
The SWS sunspot number tables are based on the observed (definitive and provisional) monthly mean sunspot numbers from WDC-SILSO, Royal Observatory of Belgium, Brussels... -
SWS Solar Spectrograph Data from Culgoora (N.S.W.) and Learmonth (W.A.) (...
Culgoora and Learmonth Observatories' dynamic spectrogram plots display frequency in MHz on the vertical axis and time in UT on the horizontal axis. Each plot spans local...
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