File:IDPmajorelements.png
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Summary[edit]
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The largest data set for major elements (Schramm et al., 1989) comes from the analyses of 200 stratospheric interplanetary dust particles. Brownlee (1997) gives electron microprobe data for 500 cosmic spherules in the 1 micrometer to 1 millimeter size range but the compositions of these melted particles only partly reflect that of their precursors because of effects related to hypervelocity entry into the atmosphere (Love and Brownlee, 1991; Kornblum, 1969). The author of the figure is Thomas Stephan, Institut für Planetologie, Münster, Germany. This file is licensed under Creative Commons Attribution 2.5 License: https://creativecommons.org/licenses/by/2.5/ See the (Jessberger chapter in Grün, E., Gustafson, B.A.S., Dermott, S.F., Fechtig, H. (Eds.) Interplanetary Dust book for more details on the analyses of elemental abundances in interplanetary dust particles.
ReferencesBrownlee D. E. (1997). "The elemental composition of cosmic spherules". Meteoritics Planet. Sci. 32: 157–176. Bibcode:1997M&PS...32..157B. doi:10.1111/j.1945-5100.1997.tb01257.x. E. K. Jessberger, T. Stephan, D. Rost, P. Arndt, M. Maetz, F. J. Stadermann, D. E. Brownlee, J. P. Bradley, G. Kurat (2001). Properties of Interplanetary Dust: Information from Collected Samples, in Grün, E., Gustafson, B.A.S., Dermott, S.F., Fechtig, H. (Eds.) Interplanetary Dust, pp. 253–294, Springer-Verlag. Kornblum J.J. (1969). "Micrometeoroid interaction with the atmosphere". J. Geophys. Res. 74: 1893–1906. Bibcode:1969JGR....74.1893K. doi:10.1029/JB074i008p01893. Love S. G.; Brownlee D. E. (1991). "Heating and thermal transformation of micrometeorites entering the Earth's atmosphere". Icarus. 89: 26–43. Bibcode:1991Icar...89...26L. doi:10.1016/0019-1035(91)90085-8. Schramm L. S.; Brownlee D. E.; Wheelock M. M. (1989). "Major element composition of stratospheric micrometeorites". Meteoritics. 24: 99–112. Bibcode:1989Metic..24...99S. doi:10.1111/j.1945-5100.1989.tb00950.x. | ||
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History of Image:IDPmajorelements.jpg[edit]
- 2006-03-24T19:42:38Z Babbage (Talk | contribs) (/* Summary */ typo)
- 2006-03-20T22:11:51Z Bkell (Talk | contribs) ({{badJPEG}})
- 2006-02-16T17:09:26Z Ligulembot (Talk | contribs) ([[WP:AWB|AWB assisted]] migrate {{[[template:journal reference|journal reference]]}} to {{[[template:cite journal|cite journal]]}})
- 2005-09-29T23:12:28Z Amara (Talk | contribs) (Changed figure attribute to Thomas Stephan (29-09-05 2005 Dust Meeting))
- 2005-09-21T10:31:55Z Amara (Talk | contribs) (Added more references.)
- 2005-09-21T10:11:16Z Amara (Talk | contribs) (The largest data set for major elements (Schramm et al., 1989) comes from the analyses of 200 stratospheric interplanetary dust particles. Brownlee (1997) gives electron microprobe data for 500 cosmic spherules in the 1 micrometer to 1 milimeter size ran)
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| current | 21:58, 21 July 2008 | | 814 × 563 (101 KB) | 718 Bot (talk | contribs) | == Summary == The largest data set for major elements (Schramm et al., 1989) comes from the analyses of 200 stratospheric interplanetary dust particles. Brownlee (1997) gives electron microprobe data for 500 cosmic spherules in the 1 micrometer to 1 mill |
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