Heterogeneous chemical processes as a source of persistent meteor trains-Reference-Cited by-同舟云学术

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Heterogeneous chemical processes as a source of persistent meteor trains

Published:2001-09 Issue:9 Volume:36 Page:1217-1224
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:

Author:

MURAD Edmond

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1111/j.1945-5100.2001.tb01955.x/fullpdf

Reference67 articles.

1. Surface-mediated chemiluminescent reaction of O and NO;Arnold;Chem. Phys. Lett.,1991

2. Sodium emission from long enduring meteor trains;Baggaley;Nature,1975

3. The chemical reduction of meteoric metal oxides as a source of meteor train emission;Baggaley;Bull. Astron. Inst. Czech.,1976

4. Hollow meteor trains;Baggaley;Nature,1977

5. The red afterglows in meteor wakes;Baggaley;Bull. Astron. Inst. Czech.,1977

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3. Color and spectral characteristics of long-lived meteor trail formed by the Tunka bolide;Solnechno-Zemnaya Fizika;2022-09-30

4. Nanoparticles in the inner solar system;Planetary and Space Science;2007-06

5. INTERPLANETARY DUST AND CARBONACEOUS METEORITES: CONSTRAINTS ON POROSITY, MINERALOGY AND CHEMISTRY OF METEORS FROM RUBBLE-PILE PLANETESIMALS;Earth, Moon, and Planets;2005-07-30

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