The dynamics of the zodiacal dust cloud on account of optical and infrared observations

Title:

The dynamics of the zodiacal dust cloud on account of optical and infrared observations

Creator:

Kneißel, B. and Giese, R. H.

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:ab517180-aec1-4111-a830-7459dbb92ace
uuid:ab517180-aec1-4111-a830-7459dbb92ace

Subject:

optical and infrared observations, zodiacal dust cloud, and collisions

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

The method to determine the inclination distribution of zodiacal particle orbits according to 3D-density models of zodiacal dust presented by Giese and Kneißel (1987, this volume) is briefly discussed. The results show that models with additional bulges at the solar poles bear an isotropic component of the inclination distribution amounting up to 20% of all orbits, whereas infrared models show almost no isotropic component. The existence of an isotropic component for zodiacal dust orbits is questioned by comparison with the orbital elements of meteoroidal particles which serve as a source for the zodiacal dust by mutual collisions

Language:

Czech

Rights:

http://creativecommons.org/publicdomain/mark/1.0/
policy:public

Coverage:

241-244

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:67

Harvested from:

CDK

Metadata only:

false