A Possible Origin of Tektites by Soil Fusion at Impact Sites-Reference-Cited by-同舟云学术

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A Possible Origin of Tektites by Soil Fusion at Impact Sites

Published:1962-04 Issue:4823 Volume:194 Page:8-10
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

SCHWARCZ HENRY P.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/194008a0.pdf

Reference26 articles.

1. Cohen, A. J., Impact Crater Glasses: a Systematization, Program, Forty-second Annual Meeting, Amer. Geophys. Union (1961).

2. Chao, E. C. T., Science, 135, 97 (1961).

3. Viste, E., and Anders, E., J. Geophys. Res. (in the press).

4. Spencer, L. J., Mineralog. Mag., 23, 387 (1933).

5. Urey, H. C., Nature, 179, 556 (1957).

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1. Magnetite in Muong Nong‐Type Australasian Tektites From South China;Geochemistry, Geophysics, Geosystems;2023-10

2. Magnetic Properties of Australasian Tektites From South China;Journal of Geophysical Research: Solid Earth;2023-03

3. Chemistry of Tertiary sediments in the surroundings of the Ries impact structure and moldavite formation revisited;Geochimica et Cosmochimica Acta;2016-04

4. A review of volatile compounds in tektites, and carbon content and isotopic composition of moldavite glass;Meteoritics & Planetary Science;2012-06

5. The history of tektites;Geological Society, London, Special Publications;2006

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