Finding meteor cluster candidates in series of astronomical images
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F25%3A00385750" target="_blank" >RIV/68407700:21230/25:00385750 - isvavai.cz</a>
Result on the web
<a href="https://ui.adsabs.harvard.edu/abs/2025JIMO...53..167K/abstract" target="_blank" >https://ui.adsabs.harvard.edu/abs/2025JIMO...53..167K/abstract</a>
DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Finding meteor cluster candidates in series of astronomical images
Original language description
Each night, astronomical systems record a significant amount of image data and indicate a variety of meteor events. In recent years, specific phenomena of parallel meteor occurrences or even meteor clusters have also been reported. These phenomena are typically identified through a process of post-evaluation of meteor trajectories. However, astronomical systems usually do not focus so much on such phenomena, and thus automatic real-time identification or post-identification is rather rare. This presents an opportunity for the development of novel approaches to signal and identify candidate meteors that are related to each other (they have disintegrated from the same parental object). In light of this, we have proposed an approach to indicate these events in astronomical image sequences. The proposed method employs multiple meteor detection based on Probabilistic Hough Transform with further utilization of its output parameters. The detected events are evaluated according to their temporal sequence and proximity. Finally, the similarity of the detected events is evaluated in a specific feature space, where the parallelism and velocity of the detected events are evaluated. The results of this algorithm were tested on data of recent September epsilon Perseid (SPE) meteor showers recorded by the MAIA (Meteor Automatic Imager and Analyzer), and also on data of one simulated cluster.
Czech name
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Czech description
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Classification
Type
J<sub>ost</sub> - Miscellaneous article in a specialist periodical
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA20-10907S" target="_blank" >GA20-10907S: Meteor clusters: An evidence for fragmentation of meteoroids in interplanetary space</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2025
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
WGN, Journal of the International Meteor Organization
ISSN
1016-3115
e-ISSN
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Volume of the periodical
53
Issue of the periodical within the volume
4
Country of publishing house
BE - BELGIUM
Number of pages
6
Pages from-to
167-172
UT code for WoS article
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EID of the result in the Scopus database
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