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      "name": "Rosetta - LAP - photosaturation current (PHO)",
        "alternateName": "Photosaturation current derived collectively from multiple sweeps",
      "dateModified": "2019-09-02",
      
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    "description": "There are two estimates of the photoemission current from LAP1 sweeps of a sunlit probe. \nI_PH0_60M in PH0 files is a statistical estimate from several sweeps (over 60 minute \nwindows), while I_PH0_S in the ASW files is an estimate from a single sweep with larger \nuncertainties but higher time resolution (usually 160 s). As LAP1 has shown no significant \ncontamination effects, these estimates should be directly proportional to the EUV flux at the \nRosetta position in the 20-130 nm band [Johansson et al, 2017]. For LAP2, the same \ntechniques have revealed a lower photoemission at the start of the cometary phase of the \nemission, and a sharp drop in photoemission after significant thruster firings (e.g. dayside \nexcursion, 60% decrease) with sporadic recoveries and relapses. We therefore only use LAP1 \nbased values. \n\nWhile there is no other source of photoemission measurements than LAP, its value is \ncontrolled by solar EUV radiation which is known from e.g. TIMED and SDO at Earth and \nMAVEN at Mars. Photoemission values by both methods were presented by Johansson et al. \n[2017] and compared to Earth and Mars data. The two methods were found to give consistent \nresults, also in agreement with a third independent method immune to instrument offsets. \nHowever, around perihelion all methods returned about 50% less photoemission than \nexpected from the Earth and Mars EUV fluxes. This may be a real effect, for example because \nof attenuation of solar EUV radiation by large numbers of small dust grains at large distance \nfrom the nucleus. It is also possible that this somehow relates to probe surface contamination, \nthough no other such effects have been noted on LAP1.\n\nThis is a preliminary data set which will be replaced by another in a few months.\n            ",
    "abstract": "There are two estimates of the photoemission current from LAP1 sweeps of a sunlit probe. \nI_PH0_60M in PH0 files is a statistical estimate from several sweeps (over 60 minute \nwindows), while I_PH0_S in the ASW files is an estimate from a single sweep with larger \nuncertainties but higher time resolution (usually 160 s). As LAP1 has shown no significant \ncontamination effects, these estimates should be directly proportional to the EUV flux at the \nRosetta position in the 20-130 nm band [Johansson et al, 2017]. For LAP2, the same \ntechniques have revealed a lower photoemission at the start of the cometary phase of the \nemission, and a sharp drop in photoemission after significant thruster firings (e.g. dayside \nexcursion, 60% decrease) with sporadic recoveries and relapses. We therefore only use LAP1 \nbased values. \n\nWhile there is no other source of photoemission measurements than LAP, its value is \ncontrolled by solar EUV radiation which is known from e.g. TIMED and SDO at Earth and \nMAVEN at Mars. Photoemission values by both methods were presented by Johansson et al. \n[2017] and compared to Earth and Mars data. The two methods were found to give consistent \nresults, also in agreement with a third independent method immune to instrument offsets. \nHowever, around perihelion all methods returned about 50% less photoemission than \nexpected from the Earth and Mars EUV fluxes. This may be a real effect, for example because \nof attenuation of solar EUV radiation by large numbers of small dust grains at large distance \nfrom the nucleus. It is also possible that this somehow relates to probe surface contamination, \nthough no other such effects have been noted on LAP1.\n\nThis is a preliminary data set which will be replaced by another in a few months.\n            ",
    
    "temporalCoverage": "2014-03-24T09:30:00Z/2016-09-29T00:30:00Z",

    "genre": "ThermalPlasma",
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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://cdaweb.gsfc.nasa.gov/registry/hdp/hapi/hapiHtml.html#url=https://amda.irap.omp.eu/service/hapi&amp;id=ros-lap-pho">HAPI: CDPP/AMDA HAPI Server</a>
                            </li>
                            <li class="list">
                                <a target="_blank" href="https://amda.cdpp.eu">CDPP/AMDA Web application</a>
                            </li>
                        </ul>
                    </div>
                    <div class="citation inset">
                        <h1>
                            <a name="spase://CNES/NumericalData/CDPP-AMDA/Rosetta/LAP/ros-lap-pho">Rosetta - LAP - photosaturation current (PHO)</a>
                        </h1>
                        <p>
                            <div class="term">ResourceID</div>
                            <div class="definition">spase://CNES/NumericalData/CDPP-AMDA/Rosetta/LAP/ros-lap-pho</div>
                        </p>
                        <p>
                            <div class="term">Description</div>
                            <div class="definition">There are two estimates of the photoemission current from LAP1 sweeps of a sunlit probe. 
I_PH0_60M in PH0 files is a statistical estimate from several sweeps (over 60 minute 
windows), while I_PH0_S in the ASW files is an estimate from a single sweep with larger 
uncertainties but higher time resolution (usually 160 s). As LAP1 has shown no significant 
contamination effects, these estimates should be directly proportional to the EUV flux at the 
Rosetta position in the 20-130 nm band [Johansson et al, 2017]. For LAP2, the same 
techniques have revealed a lower photoemission at the start of the cometary phase of the 
emission, and a sharp drop in photoemission after significant thruster firings (e.g. dayside 
excursion, 60% decrease) with sporadic recoveries and relapses. We therefore only use LAP1 
based values. 

While there is no other source of photoemission measurements than LAP, its value is 
controlled by solar EUV radiation which is known from e.g. TIMED and SDO at Earth and 
MAVEN at Mars. Photoemission values by both methods were presented by Johansson et al. 
[2017] and compared to Earth and Mars data. The two methods were found to give consistent 
results, also in agreement with a third independent method immune to instrument offsets. 
However, around perihelion all methods returned about 50% less photoemission than 
expected from the Earth and Mars EUV fluxes. This may be a real effect, for example because 
of attenuation of solar EUV radiation by large numbers of small dust grains at large distance 
from the nucleus. It is also possible that this somehow relates to probe surface contamination, 
though no other such effects have been noted on LAP1.

This is a preliminary data set which will be replaced by another in a few months.
</div>
                        </p>
                        <p/>
                    </div>
                </div>
                <div>
                    <p class="right">
                        <a target="_blank" href="/WS/hdp/1/Spase?ResourceID=spase://CNES/NumericalData/CDPP-AMDA/Rosetta/LAP/ros-lap-pho&amp;Format=spase_xml" download="ros-lap-pho.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-AMDA/Rosetta/LAP/ros-lap-pho&amp;Format=spase_xml">Edit</a>
                    </p>
                    <h1 class="detail">Details</h1>
                </div>
                <div>
                    <div class="product">
                        <p class="version">Version:2.4.1</p>
                        <h1>NumericalData</h1>
                        <div class="term">ResourceID</div>
                        <div class="definition">spase://CNES/NumericalData/CDPP-AMDA/Rosetta/LAP/ros-lap-pho</div>
                        <div class="term">ResourceHeader</div>
                        <div class="definition">
                            <div class="term">ResourceName</div>
                            <div class="definition">Rosetta - LAP - photosaturation current (PHO)</div>
                            <div class="term">AlternateName</div>
                            <div class="definition">Photosaturation current derived collectively from multiple sweeps</div>
                            <div class="term">ReleaseDate</div>
                            <div class="definition">2019-09-02 13:17:49Z</div>
                            <div class="term">Description</div>
                            <div class="definition">There are two estimates of the photoemission current from LAP1 sweeps of a sunlit probe. 
I_PH0_60M in PH0 files is a statistical estimate from several sweeps (over 60 minute 
windows), while I_PH0_S in the ASW files is an estimate from a single sweep with larger 
uncertainties but higher time resolution (usually 160 s). As LAP1 has shown no significant 
contamination effects, these estimates should be directly proportional to the EUV flux at the 
Rosetta position in the 20-130 nm band [Johansson et al, 2017]. For LAP2, the same 
techniques have revealed a lower photoemission at the start of the cometary phase of the 
emission, and a sharp drop in photoemission after significant thruster firings (e.g. dayside 
excursion, 60% decrease) with sporadic recoveries and relapses. We therefore only use LAP1 
based values. 

While there is no other source of photoemission measurements than LAP, its value is 
controlled by solar EUV radiation which is known from e.g. TIMED and SDO at Earth and 
MAVEN at Mars. Photoemission values by both methods were presented by Johansson et al. 
[2017] and compared to Earth and Mars data. The two methods were found to give consistent 
results, also in agreement with a third independent method immune to instrument offsets. 
However, around perihelion all methods returned about 50% less photoemission than 
expected from the Earth and Mars EUV fluxes. This may be a real effect, for example because 
of attenuation of solar EUV radiation by large numbers of small dust grains at large distance 
from the nucleus. It is also possible that this somehow relates to probe surface contamination, 
though no other such effects have been noted on LAP1.

This is a preliminary data set which will be replaced by another in a few months.
</div>
                            <div class="term">Contacts</div>
                            <div class="definition">
                                <table class="nested" cellspacing="0">
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                                        <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-AMDA/Anders.Eriksson.html">spase://CNES/Person/CDPP-AMDA/Anders.Eriksson</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
                                        </tr>
                                        <tr>
                                            <td>2.</td>
                                            <td>DataProducer</td>
                                            <td>
                                                <a target="_blank" href="https://spase-metadata.org/CNES/Person/CDPP-AMDA/Erik.Johansson.html">spase://CNES/Person/CDPP-AMDA/Erik.Johansson</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
                                        </tr>
                                    </tbody>
                                </table>
                            </div>
                            <div class="definition">
                                <p/>
                                <p/>
                            </div>
                            <div class="term">InformationURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">RPC User Guide</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="http://amda.irap.omp.eu/help/parameters/RPC_USER_GUIDE.PDF">http://amda.irap.omp.eu/help/parameters/RPC_USER_GUIDE.PDF</a>
                                </div>
                            </div>
                            <div class="term">InformationURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">RPC LAP User Guide</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="http://amda.irap.omp.eu/help/parameters/RO-IRFU-LAP-UG.PDF">http://amda.irap.omp.eu/help/parameters/RO-IRFU-LAP-UG.PDF</a>
                                </div>
                            </div>
                            <div class="term">InformationURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">RPC-LAP to Planetary Science Archive Interface Control Document</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="http://amda.irap.omp.eu/help/parameters/RO-IRFU-LAP-EAICD.PDF">http://amda.irap.omp.eu/help/parameters/RO-IRFU-LAP-EAICD.PDF</a>
                                </div>
                            </div>
                            <div class="term">InformationURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">RPC-LAP Report on cross-calibration of LAP data to measurements by other RPC instruments</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="http://amda.irap.omp.eu/help/parameters/RO-IRFU-LAP-XCAL_1_0_PDF_A-1b.PDF">http://amda.irap.omp.eu/help/parameters/RO-IRFU-LAP-XCAL_1_0_PDF_A-1b.PDF</a>
                                </div>
                            </div>
                        </div>
                        <div class="term">AccessInformation</div>
                        <div class="definition">
                            <div class="term">RepositoryID</div>
                            <div class="definition">
                                <a href="https://spase-metadata.org/SMWG/Repository/CDPP/AMDA.html">spase://SMWG/Repository/CDPP/AMDA</a>
                            </div>
                            <div class="term">Availability</div>
                            <div class="definition">Online</div>
                            <div class="term">AccessRights</div>
                            <div class="definition">Open</div>
                            <div class="term">AccessURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">CDPP/AMDA HAPI Server</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://amda.irap.omp.eu/service/hapi">https://amda.irap.omp.eu/service/hapi</a>
                                </div>
                                <div class="term">Style</div>
                                <div class="definition">HAPI</div>
                                <div class="term">ProductKey</div>
                                <div class="definition">ros-lap-pho</div>
                                <div class="term">Description</div>
                                <div class="definition">Web Service to this product using the HAPI interface.</div>
                            </div>
                            <div class="term">Format</div>
                            <div class="definition">CSV</div>
                            <div class="term">Acknowledgement</div>
                            <div class="definition">Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.</div>
                        </div>
                        <div class="term">AccessInformation</div>
                        <div class="definition">
                            <div class="term">RepositoryID</div>
                            <div class="definition">
                                <a href="https://spase-metadata.org/SMWG/Repository/CDPP/AMDA.html">spase://SMWG/Repository/CDPP/AMDA</a>
                            </div>
                            <div class="term">Availability</div>
                            <div class="definition">Online</div>
                            <div class="term">AccessRights</div>
                            <div class="definition">Open</div>
                            <div class="term">AccessURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">CDPP/AMDA Web application</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://amda.cdpp.eu">https://amda.cdpp.eu</a>
                                </div>
                                <div class="term">Description</div>
                                <div class="definition">Access to Data via CDPP/AMDA Web application.</div>
                            </div>
                            <div class="term">Format</div>
                            <div class="definition">CSV</div>
                            <div class="term">Format</div>
                            <div class="definition">VOTable</div>
                            <div class="term">Format</div>
                            <div class="definition">CDF</div>
                            <div class="term">Format</div>
                            <div class="definition">PNG</div>
                            <div class="term">Acknowledgement</div>
                            <div class="definition">Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.</div>
                        </div>
                        <div class="term">ProviderName</div>
                        <div class="definition">PSA</div>
                        <div class="term">ProviderResourceName</div>
                        <div class="definition">RO-C-RPCLAP-5-xxx-DERIV2-V1.0</div>
                        <div class="term">InstrumentIDs</div>
                        <div class="definition">
                            <a target="_blank" href="https://spase-metadata.org/CNES/Instrument/CDPP-AMDA/Rosetta/LAP.html">spase://CNES/Instrument/CDPP-AMDA/Rosetta/LAP</a>
                        </div>
                        <div class="term">MeasurementType</div>
                        <div class="definition">ThermalPlasma</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">2014-03-24 09:30:00Z</div>
                                <div class="term">StopDate</div>
                                <div class="definition">2016-09-29 00:30:00Z</div>
                            </div>
                            <div class="term">Cadence</div>
                            <div class="definition">PT60S</div>
                        </div>
                        <div class="term">Caveats</div>
                        <div class="definition">
            Quality Flag : 
            
            A quality flag is a (base 10) integer that is constructed in the two steps below:
            * Add together the constants associated with the relevant quality-related effects listed below. Note that these constants are chosen such that every digit represents up to three true/false values for the presence/absence of three specific separate quality-related effects.
            * Should the three quality-related effects be irrelevant for the given data product, then that digit is replaced by the digit “9”.
            
            Quality flag event description :
            * +1 - Low quality sweep analysis model fit
            * +2 - One of two meanings: (1) Low sample size; an average is based on fewer data points than nominal (due to filtering or otherwise) and applies to sweep steps and downsampled time series. (2) zero-padding; zeros replace lost samples for the purpose of calculating PSD.
            * +10 - One of two meanings: (1) Sweep data product and data products based on sweeps: SAA rotation of more than 0.05° during sweep. (2) Downsampled time series data product: Bias change within the 32 s downsampling period.
            * +20 - Probe in partial or full shadow
            * +100 - Rosetta wheel off-loading (WOL) or Orbit-control-maneuver (OCM)
            * +200 - One of two meanings: (1) For LAP1: LDL disturbance (LAP2 in LDL mode); (2) For LAP2: Contamination signature possibly present
            * +400 - Saturation
            
            Example: suppose that one encounters the quality flag “109”. 109 = 100 + 9 means (1) that there is an ongoing wheel off-loading (+100), and (2) that the quality-related effects associated with +1 and +2 cannot occur even in principle for the kind of data that one is looking at.           
            
        </div>
                        <div class="parameter">Parameter #1</div>
                        <div class="definition">
                            <div class="term">Name</div>
                            <div class="definition">i_ph0_60m</div>
                            <div class="term">ParameterKey</div>
                            <div class="definition">ros_lap_pho</div>
                            <div class="term">Description</div>
                            <div class="definition">Photosaturation current derived collectively from multiple sweeps</div>
                            <div class="term">Units</div>
                            <div class="definition">A</div>
                            <div class="term">RenderingHints</div>
                            <div class="definition">
                                <div class="term">DisplayType</div>
                                <div class="definition">TimeSeries</div>
                            </div>
                            <div class="term">FillValue</div>
                            <div class="definition">-1.e9</div>
                            <div class="term">Support</div>
                            <div class="definition">
                                <div class="term">SupportQuantity</div>
                                <div class="definition">Other</div>
                            </div>
                        </div>
                        <div class="parameter">Parameter #2</div>
                        <div class="definition">
                            <div class="term">Name</div>
                            <div class="definition">i_ph0_60m : qual</div>
                            <div class="term">ParameterKey</div>
                            <div class="definition">ros_lap_pho_q</div>
                            <div class="term">Description</div>
                            <div class="definition">Quality value in the range 0 (worst) to 1 (best). 
Corresponds to goodness of fit or how well the model fits the data.</div>
                            <div class="term">RenderingHints</div>
                            <div class="definition">
                                <div class="term">DisplayType</div>
                                <div class="definition">TimeSeries</div>
                            </div>
                            <div class="term">Support</div>
                            <div class="definition">
                                <div class="term">SupportQuantity</div>
                                <div class="definition">Other</div>
                            </div>
                        </div>
                        <div class="parameter">Parameter #3</div>
                        <div class="definition">
                            <div class="term">Name</div>
                            <div class="definition">quality flag</div>
                            <div class="term">ParameterKey</div>
                            <div class="definition">ros_lap_pho_f</div>
                            <div class="term">Description</div>
                            <div class="definition">Quality flag constructed as the sum of multiple terms, 
depending on what quality related effects are present. Each digit is either in 
the range 0 (best) to 7 (worst), or 9 (not used)</div>
                            <div class="term">RenderingHints</div>
                            <div class="definition">
                                <div class="term">DisplayType</div>
                                <div class="definition">TimeSeries</div>
                            </div>
                            <div class="term">Support</div>
                            <div class="definition">
                                <div class="term">SupportQuantity</div>
                                <div class="definition">Other</div>
                            </div>
                        </div>
                    </div>
                </div>
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