A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron

<p>We have measured the isotopic composition of galactic cosmic ray iron in the energy interval ~1550-2200 MeV/nucleon using a balloon-borne mass spectrometer. The instrument was flown from Palestine, Texas, in May 1984 for &gt;35 hours at an atmospheric depth of ~6 g/cm². Masses were deri...

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Main Author: Grove, Jon Eric
Format: Others
Language:en
Published: 1989
Online Access:https://thesis.library.caltech.edu/2338/3/grove_JE_1989.pdf
Grove, Jon Eric (1989) A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/3cr8-jv31. https://resolver.caltech.edu/CaltechETD:etd-05312007-121425 <https://resolver.caltech.edu/CaltechETD:etd-05312007-121425>
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spelling ndltd-CALTECH-oai-thesis.library.caltech.edu-23382021-07-16T05:01:26Z https://thesis.library.caltech.edu/2338/ A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron Grove, Jon Eric <p>We have measured the isotopic composition of galactic cosmic ray iron in the energy interval ~1550-2200 MeV/nucleon using a balloon-borne mass spectrometer. The instrument was flown from Palestine, Texas, in May 1984 for &gt;35 hours at an atmospheric depth of ~6 g/cm². Masses were derived by the Cerenkov-Energy technique. The Cerenkov counter employed a silica aerogel radiator with index of refraction n = 1.1. Particle energies were measured in a stack of NaI(Tl) scintillators, which also provided particle trajectories. The calibration of the detectors is discussed, along with the algorithms we have used to calculate velocities, energies, and masses. The limitations of aerogels as Cerenkov radiators, particularly the stability of their light yield, are considered. A detailed discussion of the sources of mass uncertainty is presented, including an analytic model of the contribution from fluctuations in the Cerenkov yield from knock-on electrons. The achieved mass resolution is ~0.65 amu, which is consistent with the theoretical estimate. We report an ⁵⁴Fe/⁵⁶Fe abundance ratio of 0.14<sup>+0.18</sup><sub>-0.11</sub> and an 84% confidence upper limit of ⁵⁸Fe/⁵⁶Fe ≤ 0.07 at the top of the atmosphere. Combining our data with those of previous measurements of the composition of iron at lower energies, and using a model of the galactic propagation, we derive cosmic-ray source abundance ratios of ⁵⁴Fe/⁵⁶Fe = 0.064<sup>+0.032</sup><sub>-0.027</sub> and ⁵⁸Fe/⁵⁶Fe ≤ 0.062. These values are consistent with the composition of solar-system iron and place restrictions on the conditions under which cosmic-ray iron is synthesized.</p> 1989 Thesis NonPeerReviewed application/pdf en other https://thesis.library.caltech.edu/2338/3/grove_JE_1989.pdf Grove, Jon Eric (1989) A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/3cr8-jv31. https://resolver.caltech.edu/CaltechETD:etd-05312007-121425 <https://resolver.caltech.edu/CaltechETD:etd-05312007-121425> https://resolver.caltech.edu/CaltechETD:etd-05312007-121425 CaltechETD:etd-05312007-121425 10.7907/3cr8-jv31
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language en
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sources NDLTD
description <p>We have measured the isotopic composition of galactic cosmic ray iron in the energy interval ~1550-2200 MeV/nucleon using a balloon-borne mass spectrometer. The instrument was flown from Palestine, Texas, in May 1984 for &gt;35 hours at an atmospheric depth of ~6 g/cm². Masses were derived by the Cerenkov-Energy technique. The Cerenkov counter employed a silica aerogel radiator with index of refraction n = 1.1. Particle energies were measured in a stack of NaI(Tl) scintillators, which also provided particle trajectories. The calibration of the detectors is discussed, along with the algorithms we have used to calculate velocities, energies, and masses. The limitations of aerogels as Cerenkov radiators, particularly the stability of their light yield, are considered. A detailed discussion of the sources of mass uncertainty is presented, including an analytic model of the contribution from fluctuations in the Cerenkov yield from knock-on electrons. The achieved mass resolution is ~0.65 amu, which is consistent with the theoretical estimate. We report an ⁵⁴Fe/⁵⁶Fe abundance ratio of 0.14<sup>+0.18</sup><sub>-0.11</sub> and an 84% confidence upper limit of ⁵⁸Fe/⁵⁶Fe ≤ 0.07 at the top of the atmosphere. Combining our data with those of previous measurements of the composition of iron at lower energies, and using a model of the galactic propagation, we derive cosmic-ray source abundance ratios of ⁵⁴Fe/⁵⁶Fe = 0.064<sup>+0.032</sup><sub>-0.027</sub> and ⁵⁸Fe/⁵⁶Fe ≤ 0.062. These values are consistent with the composition of solar-system iron and place restrictions on the conditions under which cosmic-ray iron is synthesized.</p>
author Grove, Jon Eric
spellingShingle Grove, Jon Eric
A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron
author_facet Grove, Jon Eric
author_sort Grove, Jon Eric
title A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron
title_short A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron
title_full A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron
title_fullStr A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron
title_full_unstemmed A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron
title_sort balloon measurement of the isotopic composition of galactic cosmic ray iron
publishDate 1989
url https://thesis.library.caltech.edu/2338/3/grove_JE_1989.pdf
Grove, Jon Eric (1989) A Balloon Measurement of the Isotopic Composition of Galactic Cosmic Ray Iron. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/3cr8-jv31. https://resolver.caltech.edu/CaltechETD:etd-05312007-121425 <https://resolver.caltech.edu/CaltechETD:etd-05312007-121425>
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