The survival of solar flare tracks in interplanetary dust silicates on deceleration in the Earth's atmosphere

P. Fraundorf; T. Lyons; P. Schubert

doi:10.1029/JB087iS01p0A409

The survival of solar flare tracks in interplanetary dust silicates on deceleration in the Earth's atmosphere

P. Fraundorf, T. Lyons, P. Schubert

University of Missouri-St. Louis

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

Original language	American English
Journal	Journal of Geophysical Research
Volume	87
DOIs	https://doi.org/10.1029/JB087iS01p0A409
State	Published - Jan 1 1982

Disciplines

Geology
Astrophysics and Astronomy
Geophysics and Seismology

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10.1029/JB087iS01p0A409License: Unspecified

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title = "The survival of solar flare tracks in interplanetary dust silicates on deceleration in the Earth's atmosphere",

author = "P. Fraundorf and T. Lyons and P. Schubert",

note = "Pulse heating experiments on magnesium-rich olivine and pyroxene, two silicates often found in micrometeorites collected in the stratosphere, show that iron ion tracks remain detectable in the transmission electron microscope for temperature maxima up to approximately 600 C.",

year = "1982",

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doi = "10.1029/JB087iS01p0A409",

language = "American English",

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T1 - The survival of solar flare tracks in interplanetary dust silicates on deceleration in the Earth's atmosphere

AU - Fraundorf, P.

AU - Lyons, T.

AU - Schubert, P.

N1 - Pulse heating experiments on magnesium-rich olivine and pyroxene, two silicates often found in micrometeorites collected in the stratosphere, show that iron ion tracks remain detectable in the transmission electron microscope for temperature maxima up to approximately 600 C.

PY - 1982/1/1

Y1 - 1982/1/1

UR - https://ntrs.nasa.gov/search.jsp?R=19830034149

U2 - 10.1029/JB087iS01p0A409

DO - 10.1029/JB087iS01p0A409

M3 - Article

VL - 87

JO - Journal of Geophysical Research

JF - Journal of Geophysical Research

ER -

The survival of solar flare tracks in interplanetary dust silicates on deceleration in the Earth's atmosphere

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