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      "name": "GALILEO PWS EXTR",
        
      "dateModified": "2022-03-22",
      
    "identifier": "https://doi.org/10.24400/802406/sh75-z63a",
    "publication": ", GALILEO PWS EXTR,  ()",
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    "creditText": "
        Users of these data are encouraged to acknowledge NASA, CNES (Centre National d'Etudes Spatiales) and, CNRS (Centre National de la Recherche Scientifique) for their support to the GALILEO-PWS team, and the CDPP (Centre des Données de la Physique des Plasmas) for the distribution of the GALILEO-PWS data, in all publications.

If PI/coI are not part of the publication list, then we suggest to also acknowledge Donald A. Gurnett, the late Alain Roux, Charles Kennel and Scott Bolton for use of GALILEO-PWS data.	  
	  ",
    "description": "This data set contains ASCII version of the EDR data set (one file contains one day of PWS data) :  wideband waveform measurements from the Galileo plasma wave receiver obtained during Venus encounter (1990/02/10), the first Earth encounter (1990/11/08 – 1990/12/16) and the second Earth encounter (1992/11/08 – 1992/12/20).\nThese measurements are electric or magnetic waveforms obtained by rapidly sampling the potential at the input to the receiver from either the electric dipole antenna or the magnetic search coil antenna.\n\nThe sample rates are 201,600 s^-1, 25, 200 s^-1, or 3,150 s^-1 taken through bandpass filters of 80, 10, or 1 kHz, respectively.\n\nEach sample is a 4-bit measurement after an automatic gain control (AGC) amplifier designed to keep the signal amplitude in a range commensurate with the optimal analog-to-digital converter dynamic range with a time constant of about 500 msec.\n\nAs such, the measurements are not absolutely calibrated, although it is possible to determine the approximate AGC gain from a digital performance parameter available every 2.667 seconds, assuming the signal amplitude does not vary appreciably over the 2.667 second interval.\n\nAlternately, the sweep frequency receiver (low rate) portion of the instrument can be used to determine the absolute amplitude of waves.\n\nIn many cases, the waveform data are used without any calibration for the purposes of identifying characteristic frequencies of the plasma via resonances or cutoffs, observing discrete emissions such as chorus or whistlers, or looking at the detailed form of the waveforms.",
    "abstract": "This data set contains ASCII version of the EDR data set (one file contains one day of PWS data) :  wideband waveform measurements from the Galileo plasma wave receiver obtained during Venus encounter (1990/02/10), the first Earth encounter (1990/11/08 – 1990/12/16) and the second Earth encounter (1992/11/08 – 1992/12/20).\nThese measurements are electric or magnetic waveforms obtained by rapidly sampling the potential at the input to the receiver from either the electric dipole antenna or the magnetic search coil antenna.\n\nThe sample rates are 201,600 s^-1, 25, 200 s^-1, or 3,150 s^-1 taken through bandpass filters of 80, 10, or 1 kHz, respectively.\n\nEach sample is a 4-bit measurement after an automatic gain control (AGC) amplifier designed to keep the signal amplitude in a range commensurate with the optimal analog-to-digital converter dynamic range with a time constant of about 500 msec.\n\nAs such, the measurements are not absolutely calibrated, although it is possible to determine the approximate AGC gain from a digital performance parameter available every 2.667 seconds, assuming the signal amplitude does not vary appreciably over the 2.667 second interval.\n\nAlternately, the sweep frequency receiver (low rate) portion of the instrument can be used to determine the absolute amplitude of waves.\n\nIn many cases, the waveform data are used without any calibration for the purposes of identifying characteristic frequencies of the plasma via resonances or cutoffs, observing discrete emissions such as chorus or whistlers, or looking at the detailed form of the waveforms.",
    
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    "temporalCoverage": "1990-02-10T00:00:00Z/1992-12-14T00:00:00Z",

    "genre": "Waves.Passive",
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        <div class="header">
            <div class="middle">HDPWS</div>
        </div>
        <div class="page">
            <div class="spase">
                <div class="abstract">
                    <div class="access">
                        <p class="box-title">
                    Data Access
                </p>
                        <ul class="list">
                            <li class="list">
                                <a target="_blank" href="https://regards.cnes.fr/user/cdpp/modules/1777?sp=DatasetName;q=DatasetName:GALILEO_PWS_EXTR">REGARDS</a>
                            </li>
                        </ul>
                    </div>
                    <div class="citation inset">
                        <h1>
                            <a name="spase://CNES/NumericalData/CDPP-Archive/Galileo/PWS/EXTR/GALILEO_PWS_EXTR">GALILEO PWS EXTR</a>
                        </h1>
                        <p>
                            <div class="term">ResourceID</div>
                            <div class="definition">spase://CNES/NumericalData/CDPP-Archive/Galileo/PWS/EXTR/GALILEO_PWS_EXTR</div>
                        </p>
                        <p>
                            <div class="term">Description</div>
                            <div class="definition">This data set contains ASCII version of the EDR data set (one file contains one day of PWS data) :  wideband waveform measurements from the Galileo plasma wave receiver obtained during Venus encounter (1990/02/10), the first Earth encounter (1990/11/08 – 1990/12/16) and the second Earth encounter (1992/11/08 – 1992/12/20).
These measurements are electric or magnetic waveforms obtained by rapidly sampling the potential at the input to the receiver from either the electric dipole antenna or the magnetic search coil antenna.

The sample rates are 201,600 s^-1, 25, 200 s^-1, or 3,150 s^-1 taken through bandpass filters of 80, 10, or 1 kHz, respectively.

Each sample is a 4-bit measurement after an automatic gain control (AGC) amplifier designed to keep the signal amplitude in a range commensurate with the optimal analog-to-digital converter dynamic range with a time constant of about 500 msec.

As such, the measurements are not absolutely calibrated, although it is possible to determine the approximate AGC gain from a digital performance parameter available every 2.667 seconds, assuming the signal amplitude does not vary appreciably over the 2.667 second interval.

Alternately, the sweep frequency receiver (low rate) portion of the instrument can be used to determine the absolute amplitude of waves.

In many cases, the waveform data are used without any calibration for the purposes of identifying characteristic frequencies of the plasma via resonances or cutoffs, observing discrete emissions such as chorus or whistlers, or looking at the detailed form of the waveforms.</div>
                        </p>
                        <p/>
                    </div>
                </div>
                <div>
                    <p class="right">
                        <a target="_blank" href="/WS/hdp/1/Spase?ResourceID=spase://CNES/NumericalData/CDPP-Archive/Galileo/PWS/EXTR/GALILEO_PWS_EXTR&amp;Format=spase_xml" download="GALILEO_PWS_EXTR.xml">View XML</a> |
              <a target="_blank" href="https://spase-editor.heliocloud.org/?edit=https://heliophysicsdata.gsfc.nasa.gov/WS/hdp/1/Spase?ResourceID=spase://CNES/NumericalData/CDPP-Archive/Galileo/PWS/EXTR/GALILEO_PWS_EXTR&amp;Format=spase_xml">Edit</a>
                    </p>
                    <h1 class="detail">Details</h1>
                </div>
                <div>
                    <div class="product">
                        <p class="version">Version:2.4.0</p>
                        <h1>NumericalData</h1>
                        <div class="term">ResourceID</div>
                        <div class="definition">spase://CNES/NumericalData/CDPP-Archive/Galileo/PWS/EXTR/GALILEO_PWS_EXTR</div>
                        <div class="term">ResourceHeader</div>
                        <div class="definition">
                            <div class="term">ResourceName</div>
                            <div class="definition">GALILEO PWS EXTR</div>
                            <div class="term">DOI</div>
                            <div class="definition">https://doi.org/10.24400/802406/sh75-z63a</div>
                            <div class="term">ReleaseDate</div>
                            <div class="definition">2022-03-22 11:28:57Z</div>
                            <div class="term">Description</div>
                            <div class="definition">This data set contains ASCII version of the EDR data set (one file contains one day of PWS data) :  wideband waveform measurements from the Galileo plasma wave receiver obtained during Venus encounter (1990/02/10), the first Earth encounter (1990/11/08 – 1990/12/16) and the second Earth encounter (1992/11/08 – 1992/12/20).
These measurements are electric or magnetic waveforms obtained by rapidly sampling the potential at the input to the receiver from either the electric dipole antenna or the magnetic search coil antenna.

The sample rates are 201,600 s^-1, 25, 200 s^-1, or 3,150 s^-1 taken through bandpass filters of 80, 10, or 1 kHz, respectively.

Each sample is a 4-bit measurement after an automatic gain control (AGC) amplifier designed to keep the signal amplitude in a range commensurate with the optimal analog-to-digital converter dynamic range with a time constant of about 500 msec.

As such, the measurements are not absolutely calibrated, although it is possible to determine the approximate AGC gain from a digital performance parameter available every 2.667 seconds, assuming the signal amplitude does not vary appreciably over the 2.667 second interval.

Alternately, the sweep frequency receiver (low rate) portion of the instrument can be used to determine the absolute amplitude of waves.

In many cases, the waveform data are used without any calibration for the purposes of identifying characteristic frequencies of the plasma via resonances or cutoffs, observing discrete emissions such as chorus or whistlers, or looking at the detailed form of the waveforms.</div>
                            <div class="term">Acknowledgement</div>
                            <div class="definition">
        Users of these data are encouraged to acknowledge NASA, CNES (Centre National d'Etudes Spatiales) and, CNRS (Centre National de la Recherche Scientifique) for their support to the GALILEO-PWS team, and the CDPP (Centre des Données de la Physique des Plasmas) for the distribution of the GALILEO-PWS data, in all publications.

If PI/coI are not part of the publication list, then we suggest to also acknowledge Donald A. Gurnett, the late Alain Roux, Charles Kennel and Scott Bolton for use of GALILEO-PWS data.	  
	  </div>
                            <div class="term">Contacts</div>
                            <div class="definition">
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                                    <tr>
                                        <th/>
                                        <th class="center">Role</th>
                                        <th class="center">Person</th>
                                        <th class="center">StartDate</th>
                                        <th class="center">StopDate</th>
                                        <th class="center">Note</th>
                                    </tr>
                                    <tbody>
                                        <tr>
                                            <td>1.</td>
                                            <td>PrincipalInvestigator</td>
                                            <td>
                                                <a target="_blank" href="https://spase-metadata.org/CNES/Person/CDPP-Archive/Donald.A.Gurnett.html">spase://CNES/Person/CDPP-Archive/Donald.A.Gurnett</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
                                        </tr>
                                        <tr>
                                            <td>2.</td>
                                            <td>CoInvestigator</td>
                                            <td>
                                                <a target="_blank" href="https://spase-metadata.org/CNES/Person/CDPP-Archive/Philippe.Louarn.html">spase://CNES/Person/CDPP-Archive/Philippe.Louarn</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
                                        </tr>
                                        <tr>
                                            <td>3.</td>
                                            <td>CoInvestigator</td>
                                            <td>
                                                <a target="_blank" href="https://spase-metadata.org/CNES/Person/CDPP-Archive/William.S.Kurth.html">spase://CNES/Person/CDPP-Archive/William.S.Kurth</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
                                        </tr>
                                        <tr>
                                            <td>4.</td>
                                            <td>GeneralContact</td>
                                            <td>
                                                <a target="_blank" href="https://spase-metadata.org/CNES/Person/CDPP-Archive/CDPP.general.contact.html">spase://CNES/Person/CDPP-Archive/CDPP.general.contact</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
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                        <div class="term">AccessInformation</div>
                        <div class="definition">
                            <div class="term">RepositoryID</div>
                            <div class="definition">
                                <a href="https://spase-metadata.org/CNES/Repository/CDPP-Archive/REGARDS-CDPP.html">spase://CNES/Repository/CDPP-Archive/REGARDS-CDPP</a>
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                            <div class="definition">Online</div>
                            <div class="term">AccessURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">REGARDS</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://regards.cnes.fr/user/cdpp/modules/1777?sp=DatasetName;q=DatasetName:GALILEO_PWS_EXTR">https://regards.cnes.fr/user/cdpp/modules/1777?sp=DatasetName;q=DatasetName:GALILEO_PWS_EXTR</a>
                                </div>
                                <div class="term">Description</div>
                                <div class="definition">Access via CNES Data Archive for CDPP</div>
                            </div>
                            <div class="term">Format</div>
                            <div class="definition">Text.ASCII</div>
                        </div>
                        <div class="term">ProcessingLevel</div>
                        <div class="definition">Uncalibrated</div>
                        <div class="term">InstrumentIDs</div>
                        <div class="definition">
                            <a target="_blank" href="https://spase-metadata.org/CNES/Instrument/CDPP-Archive/Galileo/PWS.html">spase://CNES/Instrument/CDPP-Archive/Galileo/PWS</a>
                        </div>
                        <div class="term">MeasurementType</div>
                        <div class="definition">Waves.Passive</div>
                        <div class="term">MeasurementType</div>
                        <div class="definition">ElectricField</div>
                        <div class="term">TemporalDescription</div>
                        <div class="definition">
                            <div class="term">TimeSpan</div>
                            <div class="definition">
                                <div class="term">StartDate</div>
                                <div class="definition">1990-02-10 00:00:00Z</div>
                                <div class="term">StopDate</div>
                                <div class="definition">1992-12-14 00:00:00Z</div>
                            </div>
                        </div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Jupiter</div>
                        <div class="parameter">Parameter #1</div>
                        <div class="definition">
                            <div class="term">Name</div>
                            <div class="definition">GALILEO PWS EXTR electric waveforms uncalibrated data</div>
                            <div class="term">Description</div>
                            <div class="definition">GALILEO PWS EXTR uncalibrated    electric   waveforms obtained by rapidly sampling the potential at the input to the receiver from either the electric dipole antenna</div>
                            <div class="term">Wave</div>
                            <div class="definition">
                                <div class="term">WaveType</div>
                                <div class="definition">PlasmaWaves</div>
                                <div class="term">WaveQuantity</div>
                                <div class="definition">ACElectricField</div>
                            </div>
                        </div>
                        <div class="parameter">Parameter #2</div>
                        <div class="definition">
                            <div class="term">Name</div>
                            <div class="definition">GALILEO PWS EXTR magnetic waveforms uncalibrated data</div>
                            <div class="term">Description</div>
                            <div class="definition">GALILEO PWS EDR uncalibrated    magnetic waveforms obtained by rapidly sampling the potential at the input to the receiver from the magnetic search coil antenna.</div>
                            <div class="term">Wave</div>
                            <div class="definition">
                                <div class="term">WaveType</div>
                                <div class="definition">PlasmaWaves</div>
                                <div class="term">WaveQuantity</div>
                                <div class="definition">ACMagneticField</div>
                            </div>
                        </div>
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