The micrometeoroid mass flux into the upper atmosphere: Arecibo results and a comparison with prior estimates

By J. D. Mathews, D. Janches, David D. Meisel, Qihou Zhou. 2001

151 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/d8969c850ecc56bac9ef447ef494cc52830e78b6

How researchers see this paper

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

In Astronomy and Astrophysics

1. D. Nesvorný
2. William Bottke
3. David Vokrouhlický
4. A. Morbidelli
5. Harold Levison
6. P. Jenniskens
7. M. Gounelle
8. Kevin J. Walsh

In Atmospheric Science

1. William Bottke
2. D. Nesvorný
3. David Vokrouhlický
4. Harold Levison
5. A. Morbidelli
6. Kevin J. Walsh
7. D. Rubincam

Citations in the corpus

• COMETARY ORIGIN OF THE ZODIACAL CLOUD AND CARBONACEOUS MICROMETEORITES. IMPLICATIONS FOR HOT DEBRIS DISKS (2009, background): “The more recent high-gain antenna observations show that smaller meteoroids appear to show a weaker helion/ antihelion source of eccentric short-period orbits (Mathews et al. 2001; Hunt et al. 2004; Galligan & Baggaley 2004).”
• DYNAMICAL MODEL FOR THE ZODIACAL CLOUD AND SPORADIC METEORS (2011, background): “As pointed out by Mathews et al. (2001), the difference between the AO and LDEF measurements could be resolved if LDEF data were recalibrated to v ∼ 50 km s−1, which is the prevailing meteor speed as seen at Arecibo (see Janches et al. 2003, 2006, Fentzke et al. 2009).”