dc.contributor.author |
Kondrat'eva E. |
|
dc.contributor.author |
Murav'eva I. |
|
dc.contributor.author |
Reznikov E. |
|
dc.date.accessioned |
2018-09-17T21:47:47Z |
|
dc.date.available |
2018-09-17T21:47:47Z |
|
dc.date.issued |
1997 |
|
dc.identifier.issn |
0038-0946 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/135447 |
|
dc.description.abstract |
The Leonid meteoric swarm, which was observed for the last time in 1966, is returning to the Sun, having a period of about 33 years. The increase of the swarm activity has already been noticed. By applying a numerical-simulation technique, an attempt is made to forecast the appearance of the compact portion of the swarm. This portion is related to the comet Tempel-Tuttle, whose orbital elements were used as a basis for calculations. © 1997 MAHK Hayka/Interperiodica Publishing. |
|
dc.relation.ispartofseries |
Solar System Research |
|
dc.title |
On the forthcoming return of the leonid meteoric swarm |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
6 |
|
dc.relation.ispartofseries-volume |
31 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
489 |
|
dc.source.id |
SCOPUS00380946-1997-31-6-SID27644547164 |
|