Motion of a fragmented meteoroid through the planetary atmosphere

By N. Artemieva, V. Shuvalov. 2001

140 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/8ba016f9d2ffe4791173fc7b940a27ef6fbb6e7b

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Aerospace Engineering

1. B. Ivanov
2. W. Hartmann
3. S. Byrne
4. A. S. McEwen
5. Gerhard Neukum
6. S. Werner
7. Mark A. Wieczorek
8. James W. Head III

In Astronomy and Astrophysics

1. W. Hartmann
2. B. Ivanov
3. A. S. McEwen
4. S. Byrne
5. S. Werner
6. Ingrid Daubar
7. C. Dundas
8. M. Kennedy

Citations in the corpus

• Very low strengths of interplanetary meteoroids and small asteroids (2011, background): “It has not been proven that these values hold for meteorite strength, though it is commonly assumed in meteoroid fragmentation theories (e.g., Baldwin and Sheaffer 1971; Nemtchinov and Popova 1997; Borovička et al. 1998; Artemieva and Shuvalov 2001; Bland and Artemieva 2006).”
• The current martian cratering rate (2010, background): “In addition, the vertical impact velocity is reduced by atmospheric breakup, due to the addition of some amount of transverse velocity (Artemieva and Shuvalov, 2001), although this is probably a very small effect.”
• Cratering History and Lunar Chronology (2006, background): “In particular, the amount and velocity of ricochet are strong functions of impact angle (Schultz and Gault 1990; Pierazzo and Melosh 2000c; Artemieva and Shuvalov 2001).”