Data Access
This data set contains the Cluster 3 WHISPER Prime Parameters : the electron density and plasma wave spectral density integrated over the frequency range, plus the status of operations.
Caveats
The WHISPER sounders operate on a duty cycle, so the electron density is sampled on neither a continuous nor a constant basis. This duty cycle covers situations from continuous active modes with one sounding occurring typically every 1-3 seconds, to natural mode operation only when no sounding is performed, and hence no density is provided for long periods. When many density values are available during a PPDB/SPDB interval, the averaged value is provided. When no value is available during such a time interval, the fill value (no data) is given. For example, in the typical WEC normal mode, a double sounding occurs over 3 s every 52 s. Thus, for PPDB, a density value, averaged over 2 spectra, is available followed by 6 fill values. For the SPDB, 2 averaged values are available 52 s apart. They are averaged for the SPDB slot.
Version:2.4.0
This data set contains the Cluster 3 WHISPER Prime Parameters : the electron density and plasma wave spectral density integrated over the frequency range, plus the status of operations.
Caveats
The WHISPER sounders operate on a duty cycle, so the electron density is sampled on neither a continuous nor a constant basis. This duty cycle covers situations from continuous active modes with one sounding occurring typically every 1-3 seconds, to natural mode operation only when no sounding is performed, and hence no density is provided for long periods. When many density values are available during a PPDB/SPDB interval, the averaged value is provided. When no value is available during such a time interval, the fill value (no data) is given. For example, in the typical WEC normal mode, a double sounding occurs over 3 s every 52 s. Thus, for PPDB, a density value, averaged over 2 spectra, is available followed by 6 fill values. For the SPDB, 2 averaged values are available 52 s apart. They are averaged for the SPDB slot.
Role | Person | StartDate | StopDate | Note | |
---|---|---|---|---|---|
1. | PrincipalInvestigator | spase://CNES/Person/CDPP-Archive/Pierrette.Decreau | |||
2. | CoInvestigator | spase://CNES/Person/CDPP-Archive/Patrick.Canu |
Access via CNES Data Archive for CDPP
Cluster 3 Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation electron number density derived from plasma frequency recognition at spin time resolution
Cluster 3 Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation electron number density quality of the resonance recognition flag at spin time resolution
Cluster 3 Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation electric field spectral density in the 4-10 kHz (f4) frequency range at spin time resolution
Cluster 3 Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation electric field spectral density in the 10-20 kHz (f5) frequency range at spin time resolution
Cluster 3 Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation electric field spectral density in the 20-80 kHz (f6) frequency range at spin time resolution
Cluster 3 Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation normalized electric field variance at spin time resolution
Cluster 3 Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation status at spin time resolution