Towards a new model of the interplanetary meteoroid environment

Advances in Space Research

Volumn 29, Issue 8, 2002, Pages 1171-1175

  Dikarev, Valeri ^a,c   Jehn, Rüdiger ^b   Grün, Eberhard ^a  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b ESA ESOC   (Germany)

^c ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

COLLISION AVOIDANCE; RISK ASSESSMENT; SPACECRAFT INSTRUMENTS;

DUST RESEARCHERS;

METEORITES;

METEORITE;

EID: 0036072268     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(02)00134-5     Document Type: Article

References (20)

1. Radar studies of the orbits of small meteoroids
2. Steady-state space distribution of meteoric particles under the operation of the Poynting-Robertson effect
3. The out-of-plane distribution of zodiacal dust near the earth
4. Five populations of interplanetary meteoroids
5. A new approach to dynamical evolution of interplanetary dust
6. Structure of the zodiacal cloud: New analytical and numerical solutions
7. Physikalische und Chemische Eigenschaften des Interplanetaren Stabes - Messungen des Mikrometeoritenexperimentes auf Helios
8. Collisional balance of the meteoritic complex
9. South-north and radial traverses through the interplanetary dust cloud
10. Collisional evolution and the resulting mass distribution of interplanetary dust
11. Modeling the number density distribution of interplanetary dust on the ecliptic plane within 5AU of the sun
12. Modeling the particle mass distribution within 1 AU of the sun
13. Micrometeor observations using the Arecibo 430 MHz radar
14. How to maintain the spatial distribution of interplanetary dust
15. Physical and dynamical studies of meteors: Meteor fragmentation and stream-distribution studies
16. The harvard radio meteor project velocity distribution reappraised
17. The Poynting-Robertson effect on meteor orbits