2.7.1
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spase://NASA/NumericalData/ISEE3/IsotAbun
NASA
NumericalData
ISEE 3 Isotopic Abundance Ratios
https://doi.org/10.48322/b049-ja74
2026-02-18T18:12:09Z
2025-05-15T18:39:11Z
Only known prior ReleaseDate of the metadata
2025-11-14T16:02:25Z
Added PublicationInfo. Added ResourceType and NamingAuthority. ZCB
2025-12-04T13:29:38Z
Added MetadataRightsList and RightsList(s). Updated to 2.7.1. ZCB
2026-02-18T18:12:09Z
Added DOI. tlk
This data product consists of a single ASCII file
containing values and their uncertainties for 32 abundance ratios of
various pairs of isotopes of 13 chemical elements (C, O, Ne, Mg, Al,
Si, Ti, V, Cr, Mn, Fe, Co, Ni). Between this data product and a
companion catalog with isotopic fractions, isotopic composition
information is given for 21 chemical elements. The ratios are based
on 1978-1981 observations of ~50-500 MeV/n cosmic rays by the U.
Chicago cosmic ray experiment on ISEE 3. Each of the ratios is
linked in the ASCII file to the publication where its derivation is
discussed.
Please acknowledge the author(s) of the relevant
publication(s) as mentioned above, and acknowledge Mark Wiedenbeck, the
ISEE 3 instrument Principal Investigator.
Wiedenbeck, Mark E.
2025-11-14T16:02:25Z
Space Physics Data Facility
spase://SMWG/Person/Mark.E.Wiedenbeck
PrincipalInvestigator
subdirectory holding ISEE 3 cosmic ray data
https://spdf.gsfc.nasa.gov/pub/data/isee/isee3/energetic_particles_cr/cr_composition/
spase://VEPO/NumericalData/ISEE3/IsotAbun
spase://VSPO/NumericalData/ISEE3/IsotAbun
spase://SMWG/Repository/NASA/GSFC/SPDF
Online
Open
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CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products
FTPS from SPDF (not with most browsers)
ftps://spdf.gsfc.nasa.gov/pub/data/isee/isee3/energetic_particles_cr/cr_composition/table3.txt
HTTPS from SPDF
https://spdf.gsfc.nasa.gov/pub/data/isee/isee3/energetic_particles_cr/cr_composition/table3.txt
In CDF via HTTP from SPDF
Text
3
KB
Please acknowledge the author(s) of the relevant
publication(s) as mentioned above, and acknowledge Mark Wiedenbeck, the
ISEE 3 instrument Principal Investigator.
spase://SMWG/Instrument/ISEE3/HECR
EnergeticParticles
IonComposition
1978-08-18T00:00:00
1981-04-30T00:00:00
This is span of data used in deriving 32-month averaged ratios
P32M
Heliosphere.NearEarth