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Galileo Plasma Wave Sensors (PWS) Earth Flyby Daily Dynamic Spectrograms Electric

ResourceID
spase://NASA/DisplayData/Galileo/PWS/DS/Electric/P1D

Description

These PWS daily spectrograms cover the time range around the time of the Galileo spacecraft's two Earth flybys on its way to Jupiter. This dataset contains electric field spectrograms in units of electric field spectral density (V^2/m^2/Hz) spanning 6 Hz to 5.6 MHz. An associated dataset contains magnetic field spectrograms in units of magnetic field spectral density (nT^2/Hz) spanning 6 Hz to 75 kHz. The sources of this browse data set are the High Frequency Receiver, Sweep Frequency Receiver, and Spectrum Analyzer which make up the Low Rate Science portion of the PWS. The high frequency receiver data that appears in the uppermost panel of the spectrograms are only taken from the electric field antennas. During the time interval spanned by the first Earth flyby, Galileo approached Earth from the local early morning sector, made a close approach to Earth by passing through the magnetosphere, plasmasphere, ionosphere, and finally exited the Earth system in the local late morning. During the time interval spanned by the second Earth flyby, Galileo approached Earth from the local late evening sector, made a close approach to Earth by passing through the magnetosphere, plasmasphere, ionosphere, and finally exited the Earth system near local dawn. +-----------------------------------------------------+ Flyby 1 1990 November 8 1700 UT - dataset start 1990 December 8 - Earth closest approach 1990 December 18 1700 UT - dataset end +-----------------------------------------------------+ +-----------------------------------------------------+ Flyby 2 1992 November 6 2100 UT - dataset start 1992 December 8 - Earth closest approach 1992 December 17 0630 UT - dataset ends +-----------------------------------------------------+

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Details

Version:2.2.9

DisplayData

ResourceID
spase://NASA/DisplayData/Galileo/PWS/DS/Electric/P1D
ResourceHeader
ResourceName
Galileo Plasma Wave Sensors (PWS) Earth Flyby Daily Dynamic Spectrograms Electric
ReleaseDate
2020-07-07 19:48:33Z
Description

These PWS daily spectrograms cover the time range around the time of the Galileo spacecraft's two Earth flybys on its way to Jupiter. This dataset contains electric field spectrograms in units of electric field spectral density (V^2/m^2/Hz) spanning 6 Hz to 5.6 MHz. An associated dataset contains magnetic field spectrograms in units of magnetic field spectral density (nT^2/Hz) spanning 6 Hz to 75 kHz. The sources of this browse data set are the High Frequency Receiver, Sweep Frequency Receiver, and Spectrum Analyzer which make up the Low Rate Science portion of the PWS. The high frequency receiver data that appears in the uppermost panel of the spectrograms are only taken from the electric field antennas. During the time interval spanned by the first Earth flyby, Galileo approached Earth from the local early morning sector, made a close approach to Earth by passing through the magnetosphere, plasmasphere, ionosphere, and finally exited the Earth system in the local late morning. During the time interval spanned by the second Earth flyby, Galileo approached Earth from the local late evening sector, made a close approach to Earth by passing through the magnetosphere, plasmasphere, ionosphere, and finally exited the Earth system near local dawn. +-----------------------------------------------------+ Flyby 1 1990 November 8 1700 UT - dataset start 1990 December 8 - Earth closest approach 1990 December 18 1700 UT - dataset end +-----------------------------------------------------+ +-----------------------------------------------------+ Flyby 2 1992 November 6 2100 UT - dataset start 1992 December 8 - Earth closest approach 1992 December 17 0630 UT - dataset ends +-----------------------------------------------------+

Acknowledgement
When using this data please acknowledge the PI Donald A. Gurnett and Co-I William S. Kurth, NASA, The University of Iowa and the VWO.
Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://SMWG/Person/Donald.A.Gurnett
2.CoInvestigatorspase://SMWG/Person/William.S.Kurth
InformationURL
Name
Galileo Plasma Wave Investigation Page
URL
Description

Galileo Plasma Wave Investigation page maintained by The University of Iowa with descriptions of the instrument, press releases, publications and links to PWS and PLS data and data viewers.

Language
en
PriorIDs
spase://VWO/DisplayData/Galileo/PWS/DS.Electric.P1D
spase://VSPO/DisplayData/Galileo/PWS/DS/Electric/P1D
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
AccessURL
Format
GIF
Encoding
None
Acknowledgement
When using these data please acknowledge the PI Donald A. Gurnett and Co-I William S. Kurth, NASA, The University of Iowa and the VWO.
InstrumentIDs
MeasurementType
Waves.Passive
MeasurementType
Spectrum
MeasurementType
ElectricField
TemporalDescription
TimeSpan
StartDate
1990-11-08 17:00:00Z
StopDate
1992-12-17 06:30:00Z
Note
There is a gap of approximately two years between one Earth flyby and the next. See time span tables in the Description above.
DisplayCadence
P1D
ObservedRegion
Earth.Magnetosphere
ObservedRegion
Earth.NearSurface.Plasmasphere
ObservedRegion
Earth.NearSurface.AuroralRegion
ObservedRegion
Earth.NearSurface.PolarCap
ObservedRegion
Heliosphere.Inner
Keywords
Dynamic Spectrogram
Spectrogram
AKR
Auroral Kilometric Radiation
Chorus
Continuum radiation
Myriametric radiation
Solar radio burst
Terrestrial Kilometric Radiation
TKR
Type II Solar radio burst
Type III Solar radio burst
Parameter #1
Name
Electric Spectral Density
Units
V^2/m^2/Hz
Wave
WaveType
PlasmaWaves
Qualifier
Magnitude
Qualifier
Pseudo
WaveQuantity
ACElectricField
FrequencyRange
SpectralRange
RadioFrequency
Low
5.62
High
5620000
Units
Hz