26Al and the partial ionization of the solar nebula

Guy J. Consolmagno; J. R. Jokipii

doi:10.1007/BF00896999

²⁶Al and the partial ionization of the solar nebula

Guy J. Consolmagno, J. R. Jokipii

Lunar and Planetary Lab

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25 Scopus citations

Abstract

Calculation of the ionization state and consequent magnetic Reynolds number for the solar nebula shows that the presence of²⁶Al will result in strong coupling of the gas to magnetic fields. In the absence of²⁶Al,⁴⁰K will still result in substantial ionization, but the degree of magnetic coupling is much more model dependent.

Original language	English (US)
Pages (from-to)	253-259
Number of pages	7
Journal	The Moon and the Planets
Volume	19
Issue number	2
DOIs	https://doi.org/10.1007/BF00896999
State	Published - Oct 1978

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science
Earth and Planetary Sciences (miscellaneous)

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title = "26Al and the partial ionization of the solar nebula",

abstract = "Calculation of the ionization state and consequent magnetic Reynolds number for the solar nebula shows that the presence of26Al will result in strong coupling of the gas to magnetic fields. In the absence of26Al,40K will still result in substantial ionization, but the degree of magnetic coupling is much more model dependent.",

author = "Consolmagno, {Guy J.} and Jokipii, {J. R.}",

year = "1978",

month = oct,

doi = "10.1007/BF00896999",

language = "English (US)",

volume = "19",

pages = "253--259",

journal = "The Moon and the Planets",

issn = "0165-0807",

number = "2",

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T1 - 26Al and the partial ionization of the solar nebula

AU - Consolmagno, Guy J.

AU - Jokipii, J. R.

PY - 1978/10

Y1 - 1978/10

N2 - Calculation of the ionization state and consequent magnetic Reynolds number for the solar nebula shows that the presence of26Al will result in strong coupling of the gas to magnetic fields. In the absence of26Al,40K will still result in substantial ionization, but the degree of magnetic coupling is much more model dependent.

AB - Calculation of the ionization state and consequent magnetic Reynolds number for the solar nebula shows that the presence of26Al will result in strong coupling of the gas to magnetic fields. In the absence of26Al,40K will still result in substantial ionization, but the degree of magnetic coupling is much more model dependent.

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U2 - 10.1007/BF00896999

DO - 10.1007/BF00896999

M3 - Article

AN - SCOPUS:0011047762

SN - 0165-0807

VL - 19

SP - 253

EP - 259

JO - The Moon and the Planets

JF - The Moon and the Planets

IS - 2

ER -

²⁶Al and the partial ionization of the solar nebula

Abstract

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