This page summarizes information about the selected resource and its origin based on SPASE metadata.
SPASE version 2.0.0
ACE EPAM Electron Proton Alpha Monitor (EPAM) intensities at 1-hour time resolution. Calibrated science quality data.
A web site hosting instrument information, data release notes, as well as web utilities for plotting and downloading data
ACE level 2 data rules of use, and caveats
Please acknowledge the ACE/EPAM instrument team and the ACE Science Center
| Role | Person | |
|---|---|---|
| 1. | Technical contact | Dr. Dennis Haggerty |
| 2. | CoInvestigator | Dr. Robert E. Gold |
FTP repository of 1-hour ACE/EPAM data in CDF format at CDAWeb
The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.
Number of milliseconds since CDF_EPOCH: 0000-01-01T00:00:00.000. Timestamp marks beginning of interval
Time of observation in year, day of year, and milliseconds. Timestamp marks beginning of interval
| Index | Name | Valid min | Valid max | Fill value |
|---|---|---|---|---|
| 1 | Year | 1997 | 2020 | -2147483648 |
| 2 | Day of year | 1 | 366 | -2147483648 |
| 3 | Milliseconds of day | 0 | 86401000 | -2147483648 |
LEMS30 0.047-0.065 MeV Ion Flux
LEMS30 0.065-0.112 MeV Ion Flux
LEMS30 0.112-0.187 MeV Ion Flux
LEMS30 0.187-0.310 MeV Ion Flux
LEMS30 0.310-0.580 MeV Ion Flux
LEMS30 0.580-1.06 MeV Ion Flux
LEMS30 1.06-1.91 MeV Ion Flux
LEMS30 1.91-4.75 MeV Ion Flux
Fractional uncertainty (statistical) in the P1 flux
Fractional uncertainty (statistical) in the P2 flux
Fractional uncertainty (statistical) in the P3 flux
Fractional uncertainty (statistical) in the P4 flux
Fractional uncertainty (statistical) in the P5 flux
Fractional uncertainty (statistical) in the P6 flux
Fractional uncertainty (statistical) in the P7 flux
Fractional uncertainty (statistical) in the P8 flux
DE 0.038-0.053 MeV Electron Flux
DE 0.053-0.103 MeV Electron Flux
DE 0.103-0.175 MeV Electron Flux
DE 0.175-0.315 MeV Electron Flux
Fractional uncertainty (statistical) in the DE1 flux
Fractional uncertainty (statistical) in the DE2 flux
Fractional uncertainty (statistical) in the DE3 flux
Fractional uncertainty (statistical) in the DE4 flux
CA60 0.389-1.28 MeV/nuc. He Flux)
CA60 1.28-6.98 MeV/nuc. He Flux)
CA60 0.465-1.71 MeV/nuc. CNO Flux)
CA60 1.71-19.1 MeV/nuc. CNO Flux)
CA60 0.239-0.840 MeV/nuc. Fe (9 lt Z lt 29) Flux)
CA60 0.840-92.7 MeV/nuc. Fe (9 lt Z lt 29) Flux)
Fractional uncertainty (statistical) in the W3 flux
Fractional uncertainty (statistical) in the W4 flux
Fractional uncertainty (statistical) in the W5 flux
Fractional uncertainty (statistical) in the W6 flux
Fractional uncertainty (statistical) in the W7 flux
Fractional uncertainty (statistical) in the W8 flux
LEFS60 0.045-0.062 MeV Electron Flux
LEFS60 0.062-0.103 MeV Electron Flux
LEFS60 0.103-0.175 MeV Electron Flux
LEFS60 0.175-0.312 MeV Electron Flux
LEFS60 0.546-0.761 MeV Ion Flux
LEFS60 0.761-1.22 MeV Ion Flux
LEFS60 1.22-4.97 MeV Ion Flux
Fractional uncertainty (statistical) in the E1p flux
Fractional uncertainty (statistical) in the E2p flux
Fractional uncertainty (statistical) in the E3p flux
Fractional uncertainty (statistical) in the E4p flux
Fractional uncertainty (statistical) in the FP5p flux
Fractional uncertainty (statistical) in the FP6p flux
Fractional uncertainty (statistical) in the FP7p flux
WARTD Z>1 E>0.7 MeV Ion Flux
WARTD Z>7 E>7.5 MeV Ion Flux
WARTD Z>5 E>2.5 MeV Ion Flux
WARTD Z>10 E>9.0 MeV Ion Flux
Fractional uncertainty (statistical) in the Z2 flux
Fractional uncertainty (statistical) in the Z2A flux
Fractional uncertainty (statistical) in the Z3 flux
Fractional uncertainty (statistical) in the Z4 flux
LEMS120 0.047-0.066 MeV Ion Flux
LEMS120 0.066-0.114 MeV Ion Flux
LEMS120 0.114-0.190 MeV Ion Flux
LEMS120 0.190-0.310 MeV Ion Flux
LEMS120 0.310-0.580 MeV Ion Flux
LEMS120 0.580-1.05 MeV Ion Flux
LEMS120 1.05-1.89 MeV Ion Flux
LEMS120 1.89-4.75 MeV Ion Flux
Fractional uncertainty (statistical) in the P1p flux
Fractional Uncertainty (statistical) in the P2p flux
Fractional uncertainty (statistical) in the P3p flux
Fractional uncertainty (statistical) in the P4p flux
Fractional uncertainty (statistical) in the P5p flux
Fractional uncertainty (statistical) in the P6p flux
Fractional uncertainty (statistical) in the P7p flux
Fractional uncertainty (statistical) in the P8p flux
LEFS150 0.045-0.062 MeV Electron Flux
LEFS150 0.062-0.102 MeV Electron Flux
LEFS150 0.102-0.175 MeV Electron Flux
LEFS150 0.175-0.312 MeV Electron Flux
LEFS150 0.540-0.765 MeV Ion Flux
LEFS150 0.765-1.22 MeV Ion Flux
LEFS150 1.22-4.94 MeV Ion Flux
Fractional uncertainty (statistical) in the E1 flux
Fractional uncertainty (statistical) in the E2 flux
Fractional uncertainty (statistical) in the E3 flux
Fractional uncertainty (statistical) in the E4 flux
Fractional uncertainty (statistical) in the FP5 flux
Fractional uncertainty (statistical) in the FP6 flux
Fractional uncertainty (statistical) in the FP7 flux
SPASE version 2.0.0
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.
Description of the ACE EPAM instrument design and instrument characteristics, with links to data and other documentation
Information about the EPAM experiment on the ACE mission.
| Role | Person | |
|---|---|---|
| 1. | Technical contact | Dr. Dennis Haggerty |
| 2. | CoInvestigator | Dr. Robert E. Gold |
SPASE version 2.0.0
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.
ACE mission home page at Caltech with data download
Information about the ACE mission
| Role | Person | |
|---|---|---|
| 1. | Principal investigator | Prof. Edward C. Stone, Jr. |
SPASE version 2.0.0
SPASE version 2.0.0
SPASE version 2.0.0
SPASE version 2.0.0
SPASE version 1.2.0
Coordinated Data Analysis Web (CDAWeb) supports not only interactive plotting of variables from multiple instruments on multiple investigations simultaneously on arbitrary, user-defined time-scales. It also supports data retrieval in various formats using its interactive web interface or ftp service.
Coordinated Data Analysis Web (CDAWeb) home page at Space Physics Data Facility of the NASA Goddard Space Flight Center.
| Role | Person | |
|---|---|---|
| 1. | Project scientist | Dr. Robert E. McGuire |