Terrestrial Heat and the Generation of Magmas || Erratum: Some Consequences of Solar Wind Induction...
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Erratum: Some Consequences of Solar Wind Induction in the Moon Source: Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, Vol. 288, No. 1355, Terrestrial Heat and the Generation of Magmas (Apr. 17, 1978), p. 644 Published by: The Royal Society Stable URL: http://www.jstor.org/stable/74949 . Accessed: 07/05/2014 17:38 Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at . http://www.jstor.org/page/info/about/policies/terms.jsp . JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. . The Royal Society is collaborating with JSTOR to digitize, preserve and extend access to Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences. http://www.jstor.org This content downloaded from 169.229.32.136 on Wed, 7 May 2014 17:38:18 PM All use subject to JSTOR Terms and Conditions
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Transcript of Terrestrial Heat and the Generation of Magmas || Erratum: Some Consequences of Solar Wind Induction...
Erratum: Some Consequences of Solar Wind Induction in the MoonSource: Philosophical Transactions of the Royal Society of London. Series A, Mathematical andPhysical Sciences, Vol. 288, No. 1355, Terrestrial Heat and the Generation of Magmas (Apr. 17,1978), p. 644Published by: The Royal SocietyStable URL: http://www.jstor.org/stable/74949 .
Accessed: 07/05/2014 17:38
Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at .http://www.jstor.org/page/info/about/policies/terms.jsp
.JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range ofcontent in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new formsof scholarship. For more information about JSTOR, please contact [email protected].
.
The Royal Society is collaborating with JSTOR to digitize, preserve and extend access to PhilosophicalTransactions of the Royal Society of London. Series A, Mathematical and Physical Sciences.
http://www.jstor.org
This content downloaded from 169.229.32.136 on Wed, 7 May 2014 17:38:18 PMAll use subject to JSTOR Terms and Conditions
[ 644 ]
ERRATUM
Phil. Trans. R. Soc. Lond. A 285, 537-547 (1977)
Some consequences of solar wind induction in the Moon
BY C. P. SONETT
Figure 6 and its description on page 545 should consist of the following:
100 high conductivity - ' core radius
-1000 km
boD o1 m max Fe/FeS
- 500km
3 .~, //> three-layer U- / // core-free moon -
3 10'2 3Okm max Fe core
: ~ 1off scale o0 Gina (E-W)- j?off scale Gi (NSV
10-3 . . . ,,,1 , .. ......1 ,i I t I 10 102 10 104
frequency/gHz
FIGURE 6. Transfer functions based upon s.s.p. theory for a 3L Moon with a superimposed core of varying conductivity. Cores of 1000, 700, 500 and 300 km are shown. The heavy boundary lines for each core size encompass a suite of conductivities ranging from 10-2 to 102 S/m. The perfect reflectivity of 102 S/m cores is indicated by the asymptotic response at very low frequency. A revised version of the data shown in this figure is given in Wiskerschen & Sonett, A lunar metal core?, Proc. 8th Lunar Sci. Conf., p. 515, I977.
This content downloaded from 169.229.32.136 on Wed, 7 May 2014 17:38:18 PMAll use subject to JSTOR Terms and Conditions
