alexa Determination Of Meteoroid Characteristics, Exploded In Khakassia 06.12.2016 According To Seismic And Video Data
ISSN: 2168-9792

Journal of Aeronautics & Aerospace Engineering
Open Access

OMICS International organises 3000+ Global Conferenceseries Events every year across USA, Europe & Asia with support from 1000 more scientific Societies and Publishes 700+ Open Access Journals which contains over 50000 eminent personalities, reputed scientists as editorial board members.

Open Access Journals gaining more Readers and Citations

700 Journals and 15,000,000 Readers Each Journal is getting 25,000+ Readers

This Readership is 10 times more when compared to other Subscription Journals (Source: Google Analytics)

Share This Page

Additional Info

Loading Please wait..

3rd International Conference and Exhibition on Satellite & Space Missions
May 11-13, 2017 Barcelona, Spain

Aleksei Vladimirovich Liseikin, Victor S Seleznev and Ivan I Amelin
Geophysical Survey of Russian Academy of Sciences, Russia
Institute of Computational Mathematics and Mathematical Geophysics SB-RAS, Russia
Posters & Accepted Abstracts: J Aeronaut Aerospace Eng
DOI: 10.4172/2168-9792-C1-017
6.12.2016 at 18:36 local time (18-36 UTC) on the territory of the Republic of Khakassia, there was a rare astronomical phenomenon that thousands of people could see–it was a fall of large enough astronomical body. In spite of the fact that this fall didn’t cause damage it was necessary to say that the most powerful impact wave was near high-security objects–Maina and Sayano-Shushenskaya HPP. The last one was equipped with the local seismological net which the explosion impact wave was recorded on (Figure 1). The analysis of data from surveillance cameras and dashboard cameras showed that the azimuth of meteoroid trajectory was 1350±100, and the luminous trace finished over the seismological net surrounding Sayano-Shushenskaya HPP. The interpretation of seismologic data let us specify in a substantial way the trajectory of bolide flight and determine the territory of potential falling out of meteor body fragments. At the moment of explosion, there was a surface seismic wave, amplitude was incomparably lower than same of Chelyabinsk meteoroid explosion and it was recorded only by seismic stations situated at the distance of 10 km from the epicentrum.

Email: [email protected]

image PDF   |   image HTML

Relevant Topics

Peer Reviewed Journals
Make the best use of Scientific Research and information from our 700 + peer reviewed, Open Access Journals
International Conferences 2017-18
Meet Inspiring Speakers and Experts at our 3000+ Global Annual Meetings

Contact Us

© 2008-2017 OMICS International - Open Access Publisher. Best viewed in Mozilla Firefox | Google Chrome | Above IE 7.0 version