The distribution of temperature maxima for micrometeorites decelerated in the Earth's atmosphere without melting

P. Fraundorf

doi:10.1029/GL007i010p00765

The distribution of temperature maxima for micrometeorites decelerated in the Earth's atmosphere without melting

University of Missouri-St. Louis

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	Geophysical Research Letters
Volume	7
DOIs	https://doi.org/10.1029/GL007i010p00765
State	Published - Jan 10 1980

Disciplines

Geology
Geophysics and Seismology
Atmospheric Sciences

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10.1029/GL007i010p00765License: Unspecified

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title = "The distribution of temperature maxima for micrometeorites decelerated in the Earth's atmosphere without melting",

author = "P. Fraundorf",

note = "A simple model for the statistics of heating of micrometeorites decelerated in the earth's atmosphere without melting predicts that for 10 micron particles with thermal emissivity near 1, roughly half of those with density 1 g/cc are heated above 550 C, while half of those with density 3 g/cc are heated above 800 C.",

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doi = "10.1029/GL007i010p00765",

language = "American English",

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journal = "Geophysical Research Letters",

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T1 - The distribution of temperature maxima for micrometeorites decelerated in the Earth's atmosphere without melting

AU - Fraundorf, P.

N1 - A simple model for the statistics of heating of micrometeorites decelerated in the earth's atmosphere without melting predicts that for 10 micron particles with thermal emissivity near 1, roughly half of those with density 1 g/cc are heated above 550 C, while half of those with density 3 g/cc are heated above 800 C.

PY - 1980/1/10

Y1 - 1980/1/10

UR - https://ntrs.nasa.gov/search.jsp?R=19810025878

U2 - 10.1029/GL007i010p00765

DO - 10.1029/GL007i010p00765

M3 - Article

VL - 7

JO - Geophysical Research Letters

JF - Geophysical Research Letters

ER -

The distribution of temperature maxima for micrometeorites decelerated in the Earth's atmosphere without melting

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