Data Access
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 radar used to monitor the ionosphere. SWS WDC has archived ionogram data from 26 stations, 12 of them are still active at present. An IPS 5D ionosonde has been sounding since 30/06/1999 at Darwin. The 5D vertical sounding ionosondes normally sweep in frequency from about 1 to 21.5 MHz. Frequency step resolution for the 5D is 5kHz, with up to 4095 steps available. The step interval is variable, becoming more coarse at higher frequencies as ionograms are generally displayed on a logarithmic scale. Every five minutes, a Ionogram data file is recorded, cleaned and the cleaned ionogram is transfered to SWS Sydney head office for autoscaling and further analysis. The raw ionogram file is recorded in a DVD monthly, which will be posted to Sydney SWS head office every month. Except the current 5D ionosonde, During 24/08/1994 to 26/11/2002, SWS also had an IPS 4D ionosonde, During 16/05/1995 to 31/10/1998, an IPS 5C ionosonde, and during 04/06/1999 to 07/06/1999, a CADI ionosonde, only four days. SWS WDC archives all raw ionogram files and cleaned ionogram files. The Darwin digital clean ionogram data is available since 16/05/1995, and digital raw ionogram data since 24/08/1994. The Darwin scaled hourly ionospheric data include parameters of foF2, foF1, FoE, foEs, fbEs, fmin, fxl, f'scaling F/s, M(3000)F2, h'F2, h'F, h'E, h'Es, h'Scaling R/S and Type Es. They are avalable from 01/01/1982 to 30/11/2014. The Darwin median data of foF2 and M(3000)F2 are available from 12/1982 to 11/2014.
Version:2.3.2
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 radar used to monitor the ionosphere. SWS WDC has archived ionogram data from 26 stations, 12 of them are still active at present. An IPS 5D ionosonde has been sounding since 30/06/1999 at Darwin. The 5D vertical sounding ionosondes normally sweep in frequency from about 1 to 21.5 MHz. Frequency step resolution for the 5D is 5kHz, with up to 4095 steps available. The step interval is variable, becoming more coarse at higher frequencies as ionograms are generally displayed on a logarithmic scale. Every five minutes, a Ionogram data file is recorded, cleaned and the cleaned ionogram is transfered to SWS Sydney head office for autoscaling and further analysis. The raw ionogram file is recorded in a DVD monthly, which will be posted to Sydney SWS head office every month. Except the current 5D ionosonde, During 24/08/1994 to 26/11/2002, SWS also had an IPS 4D ionosonde, During 16/05/1995 to 31/10/1998, an IPS 5C ionosonde, and during 04/06/1999 to 07/06/1999, a CADI ionosonde, only four days. SWS WDC archives all raw ionogram files and cleaned ionogram files. The Darwin digital clean ionogram data is available since 16/05/1995, and digital raw ionogram data since 24/08/1994. The Darwin scaled hourly ionospheric data include parameters of foF2, foF1, FoE, foEs, fbEs, fmin, fxl, f'scaling F/s, M(3000)F2, h'F2, h'F, h'E, h'Es, h'Scaling R/S and Type Es. They are avalable from 01/01/1982 to 30/11/2014. The Darwin median data of foF2 and M(3000)F2 are available from 12/1982 to 11/2014.
Role | Person | StartDate | StopDate | Note | |
---|---|---|---|---|---|
1. | GeneralContact | spase://ASWS/Person/Kehe.Wang | |||
2. | MetadataContact | spase://ASWS/Person/Kehe.Wang |
includes descriptions of data format of raw ionogram data and clean ionogram data
Softwares to view clean ionogram data with scaling function
includes browse display interface, button to get yearly data file and link to data availability chart
includes browse display interface, button to get the median data file and link to data availability chart
Online viewer of Real Time clean ionogram data
Access to the raw and clean ionogram data of Darwin IPS 4D (cdn4d), 5C (cdn5c) and IPS 5D (cdn5d) ionosondes and CADI ionosonde (cdncd)
Frequencies used to sonde ionopshere
The apparent height of an ionospheric layer deduced from the time delay of a reflected radio pulse upon the assumption that it travelled at the speed of light over its entire path. However, the radio wave actually slows down as it is refracted so that the virtual height is greater than the true height of the refracting layer.