2.0.1 spase://vspo/numericalData/P_ACE_HDR_EPAM_1HR ACE EPAM L2 1-hour particle flux data 2007-06-01T00:00:00 ACE EPAM L2 1-hour, 1-day and 27-day averaged electron, proton and alpha particle fluxes at ASC spase://SMWG/Person/Robert.E.Gold GeneralContact spase://SMWG/Repository/ACE_SC Online Open ACE Science Center (ASC) http://www.srl.caltech.edu/ACE/ASC/level2/lvl2DATA_EPAM.html in HDF via ftp from ASC ftp://mussel.srl.caltech.edu/pub/ace/level2/epam/ CDAWeb http://cdaweb.gsfc.nasa.gov in CDF via ftp from CDAWeb ftp://cdaweb.gsfc.nasa.gov/pub/istp/ace/epm_h2 Text CALIBRATED spase://SMWG/Instrument/ACE/EPAM EnergeticParticles IonComposition 1997-08-30T00:00:00 -P21D Data are presently current within few weeks PT3600S Heliosphere.NearEarth spase://SMWG/Observatory/ACE ACE Advanced Composition Explorer 1997-045A Explorer 71 2009-05-20T20:00:12Z The objective of the Advanced Composition Explorer (ACE) is to collect observations of particles of solar, interplanetary, interstellar, and galactic origins, spanning the energy range from that of KeV solar wind ions to galactic cosmic ray nuclei up to 600 MeV/nucleon. Definitive studies will be made of the abundances of essentially all isotopes from H to Zn (Z = 1-30), with exploratory isotope studies extending to Zr (Z = 40). The ACE payload includes six high resolution spectrometers, each designed to provide the optimum charge, mass, or charge-state resolution in its particular energy range. Each spectrometer has a geometry factor optimized for the expected flux levels, so as to provide a collecting power greater by a factor of 10-1000 times that of previous or planned experiments. The payload also includes three additional instruments of standard design to monitor energetic electrons, H and He ions, and a magnetometer. The ACE spacecraft is based on the design of the Charge Composition Explorer, built at JHU/APL for the Active Magnetospheric Particle Tracer Explorer (AMPTE) program. The spacecraft spin axis is pointed towards the Sun to within +/- 20 degrees, and it occupies a halo orbit about the L1 Earth-Sun libration point. Powered by solar cells, the spacecraft has a design life of at least five years, and it returns data in daily tape recorder dumps, received through NASA JPL's Deep Space Network and initially processed at NASA-GSFC. The average data telemetry rate is 6.7 Kbs. spase://SMWG/Person/Edward.C.Stone.Jr PrincipalInvestigator ACE Home Page http://www.srl.caltech.edu/ACE/ ACE mission home page at Caltech with data download NSSDC's Master Catalog http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=1997-045A Information about the ACE mission spase://vspo/observatory/2 Heliosphere.NearEarth Heliosphere.Inner spase://SMWG/Instrument/ACE/EPAM ACE Electron Proton Alpha Monitor ACE EPAM 1997-045A-08 2009-05-20T21:10:13Z EPAM is composed of five telescope apertures of three different types. Two Low Energy Foil Spectrometers (LEFS) measure the flux and direction of electrons above 30 keV (geometry factor = 0.397 cm^2 sr), two Low Energy Magnetic Spectrometers (LEMS) measure the flux and direction of ions greater than 50 keV (geometry factor = 0.48 cm^2 sr), and the Composition Aperture (CA) measures the elemental composition of the ions (geometry factor = 0.24 cm^2 sr). The telescopes use the spin of the spacecraft to sweep the full sky. Solid-state detectors are used to measure the energy and composition of the incoming particles. spase://SMWG/Person/Dennis.Haggerty TechnicalContact spase://SMWG/Person/Robert.E.Gold CoInvestigator Instrument description http://sd-www.jhuapl.edu/ACE/EPAM Description of the ACE EPAM instrument design and instrument characteristics, with links to data and other documentation NSSDC's Master Catalog http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1997-045A-08 Information about the EPAM experiment on the ACE mission. spase://SMWG/instrument/1997-045A-08 EnergeticParticleInstrument Electron Proton and Alpha Monitor (EPAM) on ACE spase://SMWG/Observatory/ACE spase://SMWG/Repository/ACE_SC SRL ACE Science Center ASC 2008-06-18T06:07:48Z ACE Science Center Please acknowledge the ACE instrument teams and the ACE Science Center in publications and presentations that use these data spase://SMWG/Person/Andrew.J.Davis PrincipalInvestigator GeneralContact ACE Science Center http://www.srl.caltech.edu/ACE/ASC spase://SMWG/Person/Robert.E.Gold Dr. Robert E. Gold Applied Physics Laboratory spase://SMWG/Person/Andrew.J.Davis Dr. Andrew J. Davis California Institute of Technology spase://SMWG/Person/Dennis.Haggerty 2007-11-27T19:26:30Z Dr. Dennis Haggerty Applied Physics Laboratory dennis.haggerty@jhuapl.edu spase://SMWG/Person/Edward.C.Stone.Jr 2001-04-02T00:00:00Z Prof. Edward C. Stone, Jr. California Institute of Technology ecs@srl.caltech.edu +1-626-395-8321