[
    {
        "id": "authors:wns4n-q8s48",
        "collection": "authors",
        "collection_id": "wns4n-q8s48",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140617-164044646",
        "type": "book_section",
        "title": "The Cosmic Ray \u00b3He/\u2074He Ratio from 0.2 to 3.6 GeV/nucleon",
        "author": [
            {
                "family_name": "Reimer",
                "given_name": "O.",
                "clpid": "Reimer-O"
            },
            {
                "family_name": "Barbier",
                "given_name": "L. M.",
                "clpid": "Barbier-L-M"
            },
            {
                "family_name": "Christian",
                "given_name": "E. R.",
                "orcid": "0000-0003-2134-3937",
                "clpid": "Christian-Eric-R"
            },
            {
                "family_name": "Davis",
                "given_name": "A. J.",
                "orcid": "0000-0002-9922-8915",
                "clpid": "Davis-Andrew-J"
            },
            {
                "family_name": "Golden",
                "given_name": "R. L.",
                "clpid": "Golden-R-L"
            },
            {
                "family_name": "Hof",
                "given_name": "M.",
                "orcid": "0000-0003-2884-3037",
                "clpid": "Hof-Martin"
            },
            {
                "family_name": "Krombel",
                "given_name": "K. E.",
                "clpid": "Krombel-K-E"
            },
            {
                "family_name": "Labrador",
                "given_name": "A. W.",
                "orcid": "0000-0001-9178-5349",
                "clpid": "Labrador-Allan-W"
            },
            {
                "family_name": "Menn",
                "given_name": "W.",
                "clpid": "Menn-W"
            },
            {
                "family_name": "Mewaldt",
                "given_name": "R. A.",
                "orcid": "0000-0003-2178-9111",
                "clpid": "Mewaldt-R-A"
            },
            {
                "family_name": "Mitchell",
                "given_name": "J. W.",
                "clpid": "Mitchell-J-W"
            },
            {
                "family_name": "Ormes",
                "given_name": "J. F.",
                "clpid": "Ormes-J-F"
            },
            {
                "family_name": "Rasmussen",
                "given_name": "I. L.",
                "clpid": "Rasmussen-I-L"
            },
            {
                "family_name": "Schindler",
                "given_name": "S. M.",
                "clpid": "Schindler-Stephen-M"
            },
            {
                "family_name": "Simon",
                "given_name": "M. I.",
                "clpid": "Simon-M-I-Astro"
            },
            {
                "family_name": "Stochaj",
                "given_name": "S. J.",
                "clpid": "Stochaj-S-J"
            },
            {
                "family_name": "Stone",
                "given_name": "E. C.",
                "orcid": "0000-0002-2010-5462",
                "clpid": "Stone-E-C"
            },
            {
                "family_name": "Streitmatter",
                "given_name": "R. E.",
                "clpid": "Streitmatter-R-E"
            },
            {
                "family_name": "Webber",
                "given_name": "W. R.",
                "orcid": "0000-0001-9238-9145",
                "clpid": "Webber-William-R"
            }
        ],
        "contributor": [
            {
                "family_name": "Iucci",
                "given_name": "M.",
                "clpid": "Iucci-M"
            },
            {
                "family_name": "Lamanna",
                "given_name": "E.",
                "clpid": "Lamanna-E"
            }
        ],
        "abstract": "The abundances of cosmic ray helium isotopes between 0.2 and 3.6 GeV/n were measured by the IMAX balloon-borne magnet spectrometer during a flight in Canada in July, 1992. A high-resolution time-of-flight system and two silica-aerogel Cherenkov counters were used in conjunction with a drift chamber/MWPC-tracking system to determine mass by means of the velocity vs. magnetic rigidity technique.",
        "publisher": "Caltech Library",
        "publication_date": "1995-09"
    }
]