2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Rosetta/IES/ros-ion-az azimuthal spectra : countrate ion azimuthal spectra : countrate 2017-03-18T00:15:14Z Ion azimuthal (16 anodes) spectra : Counts summed over energies and elevations. * Azimuth 45 - 90 - Anode #0 * Azimuth 00 - 45 - Anode #1 * Azimuth 315-360 - Anode #2 * Azimuth 310-315 - Anode #3 * Azimuth 305-310 - Anode #4 * Azimuth 300-305 - Anode #5 * Azimuth 295-300 - Anode #6 * Azimuth 290-295 - Anode #7 * Azimuth 285-290 - Anode #8 * Azimuth 280-285 - Anode #9 * Azimuth 275-280 - Anode #10 * Azimuth 270-275 - Anode #11 * Azimuth 225-270 - Anode #12 * Azimuth 180-225 - Anode #13 * Azimuth 135-180 - Anode #14 * Azimuth 90-135 - Anode #15 Principal Investigator : James L. Burch, SwRI spase://SMWG/Person/James.L.Burch PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/Ray.Goldstein CoInvestigator spase://CNES/Person/CDPP-AMDA/Brad.Trantham DataProducer ros-ion-all PartOf ions spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi ros-ion-az 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 https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application https://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 https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. SwRI / ImperialCollege Uncalibrated spase://CNES/Instrument/CDPP-AMDA/Rosetta/IES ThermalPlasma 2010-11-29T23:18:19Z 2016-09-30T23:58:44Z PT128S Comet Sometimes anode data are combined on board in certain operating modes because of telemetry limitations. In those cases each of the anodes is given identical values (sum/number of anodes). Anodes 13 and 14 are often noisy so caution is recommended when using data from them. The so-called "fine anodes" (3 - 11) are sometimes combined on board in certain operating modes because of telemetry limitations. In those cases each of these 9 anodes are given identical values (the sum/9). The data from individual fine anodes, when provided, suffer from crosstalk between these anodes and thus may not be reliable. It was discovered after launch, apparently as a result of a light leak, that when the sun is incident between anodes 2 and 3, a high count rate is seen in anode 12. It is also seen in anode 13 when counts in 12 and 13 are combined. ion countrate ros_ion_az s**-1 Spectrogram 16 -1 Ion CountRate