2.4.1 spase://CNES/NumericalData/CDPP-AMDA/MAVEN/SWEA/mav-swea-kp electrons : key parameters SWEA : key parameters 2022-07-02T06:08:47Z Data follow a 4-second cadence when MAVEN is at an altitude of less than 500 km, otherwise the time cadence is 8 seconds. The in situ key parameters contain 235 parameters selected by the instrument leads and other MAVEN scientists. These data consist of values derived from L2 data provided by the in situ instruments. >Principal Investigator : David L. Mitchell, SSL, Berkeley spase://CNES/Person/CDPP-AMDA/David.L.Mitchell PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/P.Dunn DataProducer SWIA web page, Summary sheet http://lasp.colorado.edu/home/maven/science/instrument-package/swea/ spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server http://amda.irap.omp.eu/service/hapi Web Service to this product using the HAPI interface. CSV 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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application http://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG 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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. PDS /maven-insitu-calibrated spase://CNES/Instrument/CDPP-AMDA/MAVEN/SWEA ThermalPlasma 2014-10-06T00:00:00Z 2021-11-14T23:59:52Z PT4S PT8S Mars Quality indicates statistical uncertainty, (1 sigma) density mav_sweakp_n Density of solar wind or magnetosheath electrons based on moments of the electron distribution after correcting for the spacecraft potential phys.density;phys.atmol.ionStage cm-3 Electron NumberDensity density quality mav_sweakp_nqual Density statistical uncertainty, (1 sigma) phys.density;phys.atmol.ionStage cm-3 Other temperature mav_sweakp_t Temperature solar wind or magnetosheath electrons based on moments of the electron distribution after correcting for the spacecraft potential phys.temperature;phys.atmol.Ionstage eV Electron Temperature temperature quality mav_sweakp_tqual Temperature statistical uncertainty, (1 sigma) phys.density;phys.atmol.ionStage eV Other parallel flux 5-100 eV mav_sweakp_pf1 Electron energy flux parallel to the magnetic field vector (0-90 degrees pitch angle) eV/(cm^2 s sr) Electron EnergyFlux parallel flux 100-500 eV mav_sweakp_pf2 Electron energy flux parallel to the magnetic field vector (0-90 degrees pitch angle) eV/(cm^2 s sr) Electron EnergyFlux parallel flux 500-1000 eV mav_sweakp_pf3 Electron energy flux parallel to the magnetic field vector (0-90 degrees pitch angle) eV/(cm^2 s sr) Electron EnergyFlux anti-parallel flux 5-100 eV mav_sweakp_apf1 Electron energy flux anti-parallel to the magnetic field vector (90-180 degrees pitch angle) eV/(cm^2 s sr) Electron EnergyFlux anti-parallel flux 100-500 eV mav_sweakp_apf2 Electron energy flux anti-parallel to the magnetic field vector (90-180 degrees pitch angle) eV/(cm^2 s sr) Electron EnergyFlux anti-parallel flux 500-1000 eV mav_sweakp_apf3 Electron energy flux anti-parallel to the magnetic field vector (90-180 degrees pitch angle) eV/(cm^2 s sr) Electron EnergyFlux spectrum shape mav_sweakp_shape Energy spectrum shape parameter used to distingush between ionospheric photoelectrons and solar wind electrons Other