CaltechAUTHORS
  A Caltech Library Service

Feasibility of Iodine and Bromine Analysis in Genesis Solar Wind Collectors

Pravdivtseva, O. and Meshik, A. and Hohenberg, C. M. and Burnett, D. S. (2011) Feasibility of Iodine and Bromine Analysis in Genesis Solar Wind Collectors. Meteoritics and Planetary Science, 46 (S1). A192-A192. ISSN 1086-9379. https://resolver.caltech.edu/CaltechAUTHORS:20130128-142650955

[img]
Preview
PDF - Published Version
See Usage Policy.

80Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20130128-142650955

Abstract

Comparison of elemental abundances in sun, meteorites and earth provides understanding of the formation and evolution of the solar system. Yet, the majority of the solar system abundances are based on meteoritic values [1–6]. Here we report an attempt to estimate a feasibility of direct measurements of iodine and bromine in the GENESIS solar wind Aluminum on Sapphire collector (AloS) using neutron induced conversions: ^(127)I(n,γβ)^(128)Xe, ^(79)Br(n,γβ)^(80)Kr and ^(81)Br(n,γβ)^(82)Kr.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1111/j.1945-5100.2011.01221.xDOIUNSPECIFIED
http://onlinelibrary.wiley.com/doi/10.1111/j.1945-5100.2011.01221.x/abstractPublisherUNSPECIFIED
Additional Information:© 2011 The Meteoritical Society. Article first published online: 25 Jul. 2011. This work is supported by NASA grant NNX07AM76G.
Funders:
Funding AgencyGrant Number
NASANNX07AM76G
Issue or Number:S1
Record Number:CaltechAUTHORS:20130128-142650955
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130128-142650955
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:36631
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:29 Jan 2013 00:03
Last Modified:03 Oct 2019 04:39

Repository Staff Only: item control page