bibtype |
J -
Journal Article
|
ARLID |
0482893 |
utime |
20240103215130.8 |
mtime |
20171208235959.9 |
SCOPUS |
85035799138 |
WOS |
000417176700003 |
DOI |
10.1007/s11038-017-9511-z |
title
(primary) (eng) |
Automated Meteor Detection by All-Sky Digital Camera Systems |
specification |
page_count |
27 s. |
media_type |
P |
|
serial |
ARLID |
cav_un_epca*0256505 |
ISSN |
0167-9295 |
title
|
Earth, Moon, and Planets |
volume_id |
120 |
volume |
3 (2017) |
page_num |
189-215 |
|
keyword |
meteor detection |
keyword |
autonomous fireball observatories |
keyword |
fish-eye camera |
keyword |
Hough transformation |
author
(primary) |
ARLID |
cav_un_auth*0101203 |
name1 |
Suk |
name2 |
Tomáš |
full_dept (cz) |
Zpracování obrazové informace |
full_dept (eng) |
Department of Image Processing |
department (cz) |
ZOI |
department (eng) |
ZOI |
institution |
UTIA-B |
full_dept |
Department of Image Processing |
garant |
K |
fullinstit |
Ústav teorie informace a automatizace AV ČR, v. v. i. |
|
author
|
ARLID |
cav_un_auth*0100099 |
name1 |
Šimberová |
name2 |
Stanislava |
full_dept (cz) |
Sluneční oddělení |
full_dept |
Department of Solar Physics |
institution |
ASU-R |
full_dept |
Department of Solar Physics - Team 1 |
fullinstit |
Astronomický ústav AV ČR, v. v. i. |
|
cas_special |
project |
ARLID |
cav_un_auth*0314467 |
project_id |
GA15-16928S |
agency |
GA ČR |
|
abstract
(eng) |
We have developed a set of methods to detect meteor light traces captured by all-sky CCD cameras. Operating at small automatic observatories (stations), these cameras create a network spread over a large territory. Image data coming from these stations are merged in one central node. Since a vast amount of data is collected by the stations in a single night, robotic storage and analysis are essential to processing.\nThe proposed methodology is adapted to data from a network of automatic stations equipped with digital fish-eye cameras and includes data capturing, preparation, pre-processing, analysis, and finally recognition of objects in time sequences. In our experiments we utilized real observed data from two stations.\n |
RIV |
IN |
FORD0 |
10000 |
FORD1 |
10200 |
FORD2 |
10201 |
reportyear |
2018 |
num_of_auth |
2 |
mrcbC47 |
ASU-R 10000 10300 10308 |
mrcbC55 |
ASU-R BN |
inst_support |
RVO:67985815 |
inst_support |
RVO:67985556 |
permalink |
http://hdl.handle.net/11104/0278694 |
confidential |
S |
mrcbC86 |
3+4 Article Astronomy Astrophysics|Geosciences Multidisciplinary |
mrcbC86 |
3+4 Article Astronomy Astrophysics|Geosciences Multidisciplinary |
mrcbC86 |
3+4 Article Astronomy Astrophysics|Geosciences Multidisciplinary |
mrcbT16-e |
ASTRONOMYASTROPHYSICS|GEOSCIENCESMULTIDISCIPLINARY |
mrcbT16-j |
0.364 |
mrcbT16-s |
0.630 |
mrcbT16-B |
12.473 |
mrcbT16-D |
Q4 |
mrcbT16-E |
Q3 |
arlyear |
2017 |
mrcbU14 |
85035799138 SCOPUS |
mrcbU24 |
PUBMED |
mrcbU34 |
000417176700003 WOS |
mrcbU63 |
cav_un_epca*0256505 Earth, Moon, and Planets 0167-9295 1573-0794 Roč. 120 č. 3 2017 189 215 |
|