The two STEREO radio receivers measure wave intensity, source direction and angular size in the frequency
range 40 kHz to 16 MHz, corresponding to heliocentric source distances of about 1 Rs to 1 AU. One 10-40 kHz
receiver measures radio and plasma waves near the 1 AU electron plasma frequency. One receiver makes high
time resolution measurements at 50 MHz. Time Domain Samplers make simultaneous wideband waveform measurements
on three electric components. Antenna systems include three mutually orthogonal 6-meter monopoles.
Version:2.3.1
The two STEREO radio receivers measure wave intensity, source direction and angular size in the frequency
range 40 kHz to 16 MHz, corresponding to heliocentric source distances of about 1 Rs to 1 AU. One 10-40 kHz
receiver measures radio and plasma waves near the 1 AU electron plasma frequency. One receiver makes high
time resolution measurements at 50 MHz. Time Domain Samplers make simultaneous wideband waveform measurements
on three electric components. Antenna systems include three mutually orthogonal 6-meter monopoles.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Jean-Louis.Henry.Bougeret | |||
| 2. | MetadataContact | spase://SMWG/Person/James.M.Weygand |
NASA STEREO SWAVE resources information.
NASA STEREO SWAVE instrument information.
WAVES Experiment on the STEREO Mission.
FTPS access to SWAVES ASCII data
HTTPS access to SWAVES ASCII data
High frequency data in 48 channels.
This is the first 48 values in the daily file.
The 48 background value used in (currently) arbitrary decibel (dB) units.
The 48 background value used in (currently) arbitrary decibel (dB) units.
The 2-dimensional (# of frequencies X 1440 minutes per day) array of averages in dB above the average (i.e. value-average in dB). Missing data is indicated by a value less than 0.
This is the next 1440 by 320 values in the daily file.