2.4.1 spase://CNES/NumericalData/CDPP-AMDA/ULYSSES/SWICS/ulys-swi-rat abundance ratios 2020-06-24T16:09:54Z Selected charge states and abundance ratios : Alpha particle speed: Repeated from previous archive for comparison. - C6+/C5+ and O7+/O6+ ratios: These two ratios are essentially redundant, with the former being ~10 times higher than the latter on average. At high values the O ratio is more reliable (because C5+ is getting rare) whereas at low values the C ratio is preferable (because O7+ gets rare). Low ratios are indicative of fast streams. - Fe/O abundance ratio: This is a proxy for the strength of the FIP fractionation if divided by the solar Fe/O ratio of ~0.05. - Average charge state of Fe: Weighted average of all charge states from Fe6+ to Fe16+, normally between 9 and 12 both in slow and in fast wind. High values are a good CME indicator. - Number of instrument cycles that were accumulated to obtain the 3-hour average value. Each instrument cycle takes 13 minutes, so values of 12-14 are normal, whereas low values should be considered as a warning. spase://SMWG/Person/Rudolf.Von.Steiger DataProducer Instrument and data portal at Cosmos https://www.cosmos.esa.int/web/ulysses/swics-instrument spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi ulys-swi-rat 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. ESA uswimatbYY.dat spase://CNES/Instrument/CDPP-AMDA/Ulysses/SWICS ThermalPlasma 1990-12-07T20:02:48Z 2009-06-29T06:15:49Z PT3H Heliosphere C6+/C5+ ratio ulys_swi_crat ratio of carbon 6+ to 5+ TimeSeries Ion ChargeState O7+/O6+ ratio ulys_swi_orat ratio of oxygen 7+ to 6+ TimeSeries Ion ChargeState Fe/O ratio ulys_swi_ferat abundance ratio of iron to oxygen TimeSeries Ion ChargeState Fe charge ulys_swi_fech average charge state of iron in e- = 1.6022e-19 C e- TimeSeries Ion ChargeState