Shift the photometric center of the gegenschein

The latitude component of the deviation of the photometric centre of the gegenschein from the antisolar point was considered. It was concluded that the centre of the gegenschein is shifted towards the northern hemisphere the respect to ecliptic. Using the catalogues of individual meteor orbits based...

Full description

Bibliographic Details
Main Authors: Yu. M. Gorbanev, A. V. Golubaev
Format: Article
Language:English
Published: National Aviation University 2004-12-01
Series:Вісник Астрономічної школи
Online Access:http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/126.html
_version_ 1819206206308220928
author Yu. M. Gorbanev
A. V. Golubaev
author_facet Yu. M. Gorbanev
A. V. Golubaev
author_sort Yu. M. Gorbanev
collection DOAJ
description The latitude component of the deviation of the photometric centre of the gegenschein from the antisolar point was considered. It was concluded that the centre of the gegenschein is shifted towards the northern hemisphere the respect to ecliptic. Using the catalogues of individual meteor orbits based on photographic, television and radar observations (the materials of the Meteor Data Centre in Lund), the optical theory of the gegenschein was tested. Using the distribution of meteor orbits as a function of the five elements f(i, a, e, Ω, ω), the spatial distribution of the meteor matter is determined. The shift of the maximum density in distribution of the interplanetary dust towards to north from ecliptic is obtained. The deviation of the centre of the gegenschein north of the ecliptic is explained by this result.
first_indexed 2024-12-23T05:03:55Z
format Article
id doaj.art-cfc52e3557c242c1aefb764d0c321ed1
institution Directory Open Access Journal
issn 1607-2855
2411-6602
language English
last_indexed 2024-12-23T05:03:55Z
publishDate 2004-12-01
publisher National Aviation University
record_format Article
series Вісник Астрономічної школи
spelling doaj.art-cfc52e3557c242c1aefb764d0c321ed12022-12-21T17:59:09ZengNational Aviation UniversityВісник Астрономічної школи1607-28552411-66022004-12-0151-212613410.18372/2411-6602.05.11262411-6602.05.1126Shift the photometric center of the gegenscheinYu. M. Gorbanev0A. V. Golubaev1Astronomical Observatory, Odessa National University, UkraineAstronomical Observatory, Odessa National University, UkraineThe latitude component of the deviation of the photometric centre of the gegenschein from the antisolar point was considered. It was concluded that the centre of the gegenschein is shifted towards the northern hemisphere the respect to ecliptic. Using the catalogues of individual meteor orbits based on photographic, television and radar observations (the materials of the Meteor Data Centre in Lund), the optical theory of the gegenschein was tested. Using the distribution of meteor orbits as a function of the five elements f(i, a, e, Ω, ω), the spatial distribution of the meteor matter is determined. The shift of the maximum density in distribution of the interplanetary dust towards to north from ecliptic is obtained. The deviation of the centre of the gegenschein north of the ecliptic is explained by this result.http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/126.html
spellingShingle Yu. M. Gorbanev
A. V. Golubaev
Shift the photometric center of the gegenschein
Вісник Астрономічної школи
title Shift the photometric center of the gegenschein
title_full Shift the photometric center of the gegenschein
title_fullStr Shift the photometric center of the gegenschein
title_full_unstemmed Shift the photometric center of the gegenschein
title_short Shift the photometric center of the gegenschein
title_sort shift the photometric center of the gegenschein
url http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/126.html
work_keys_str_mv AT yumgorbanev shiftthephotometriccenterofthegegenschein
AT avgolubaev shiftthephotometriccenterofthegegenschein