<abstract xmlns="http://www.w3.org/1999/xhtml"><p>Space debris of millimeter dimensions is almost not detectable by normal methods of observation from Earth. However, particles of such sizes can cause damage to the spacecraft. and even eliminate it. Estimating the status of impurity of near-Earth space mainly based on mathematical models, which are confirmed only for large particles. The millimetric fractions of space debris elements remain unexplored. In case of invasion of debris particles into the planet’s atmosphere, they burn down as well as meteoric particles of natural origin. In this work, the observation technique of separation of debris particles and particles of natural origin is described. Also, the results of the detection of particles from space debris received during the TV observations on the wide-angle camera patrol camera FAVOR (Russia, Northern Caucasus).</p></abstract>

Space debris of millimeter dimensions is almost not detectable by normal methods of observation from Earth. However, particles of such sizes can cause damage to the spacecraft. and even eliminate it. Estimating the status of impurity of near-Earth space mainly based on mathematical models, which are confirmed only for large particles. The millimetric fractions of space debris elements remain unexplored. In case of invasion of debris particles into the planet’s atmosphere, they burn down as well as meteoric particles of natural origin. In this work, the observation technique of separation of debris particles and particles of natural origin is described. Also, the results of the detection of particles from space debris received during the TV observations on the wide-angle camera patrol camera FAVOR (Russia, Northern Caucasus).

Study the combustion processes of space debris in the Earth’s atmosphere by meteoric TV camera

Applied Mathematics and Nonlinear Sciences

This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License.

Space debris of millimeter dimensions is almost not detectable by normal methods of observation from Earth. However, particles of such sizes can cause damage...

Case	Meteor	Elongation(Degrees)	angular velocity (deg/s)	Linear velocity (km/s)
1	2006-08-31=00h41m28s	86	2.1 (± 0.35)	3.4
2	2006-09-13=22h00m46s	74	2.8 (± 0.35)	4.7
3	2006-09-18=19h59m54s	78	2.7 (± 0.35)	4.5
4	2006-10-14=22h24m04s	90	2.2 (± 0.35)	3.5
5	2006-10-20=17h21m04s	89	1.9 (± 0.35)	3.0
6	2007-10-12=20h08m06s	79	2.4 (± 0.35)	3.9
7	2007-10-18=23h36m45s	70	2.0 (± 0.35)	3.2

Study the combustion processes of space debris in the Earth’s atmosphere by meteoric TV camera

Publicado en línea: 15 nov 2017

Páginas: 473 - 478

Recibido: 05 jul 2017

Aceptado: 15 nov 2017

DOI: https://doi.org/10.21042/AMNS.2017.2.00038

Palabras clave
Space debris, observation methods, TV observation

© 2017 V.A. Leonov, A.V. Bagrov, G.F. Attia, A.M. Abdelaziz, R. Ghoneim, published by Sciendo

This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License.

Fig. 1

Fig. 2

Characteristics of meteors from space debris.

Study the combustion processes of space debris in the Earth’s atmosphere by meteoric TV camera

Publicado en línea: 15 nov 2017

Páginas: 473 - 478

Recibido: 05 jul 2017

Aceptado: 15 nov 2017

DOI: https://doi.org/10.21042/AMNS.2017.2.00038

Palabras claveSpace debris, observation methods, TV observation

© 2017 V.A. Leonov, A.V. Bagrov, G.F. Attia, A.M. Abdelaziz, R. Ghoneim, published by Sciendo

This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License.

Fig. 1

Fig. 2

Characteristics of meteors from space debris.

Palabras clave
Space debris, observation methods, TV observation