bibtype A - Abstract
ARLID 0585405
utime 20240514140057.9
mtime 20240422235959.9
DOI 10.5194/egusphere-egu24-3075
title (primary) (eng) Estimation of unknown source term based on radioxenon observations with the presence of background signal
specification
page_count 1 s.
media_type E
serial
ARLID cav_un_epca*0585420
title EGU General Assembly 2024 Abstracts
publisher
place Munich
name European Geosciences Union
year 2024
keyword radioxenon observations
keyword nuclear test
keyword International Monitoring Stations
author (primary)
ARLID cav_un_auth*0267768
name1 Tichý
name2 Ondřej
institution UTIA-B
full_dept (cz) Adaptivní systémy
full_dept (eng) Department of Adaptive Systems
department (cz) AS
department (eng) AS
full_dept Department of Adaptive Systems
fullinstit Ústav teorie informace a automatizace AV ČR, v. v. i.
author
ARLID cav_un_auth*0101207
name1 Šmídl
name2 Václav
institution UTIA-B
full_dept (cz) Adaptivní systémy
full_dept Department of Adaptive Systems
department (cz) AS
department AS
full_dept Department of Adaptive Systems
fullinstit Ústav teorie informace a automatizace AV ČR, v. v. i.
author
ARLID cav_un_auth*0387255
name1 Mácha
name2 Václav
institution UTIA-B
full_dept (cz) Adaptivní systémy
full_dept Adaptive Systems
department (cz) AS
department AS
country CZ
fullinstit Ústav teorie informace a automatizace AV ČR, v. v. i.
author
ARLID cav_un_auth*0466450
name1 Kuśmierczyk-Michulec
name2 J.
country AT
author
ARLID cav_un_auth*0466451
name1 Sommerer
name2 W.
country AT
author
ARLID cav_un_auth*0466452
name1 Tipka
name2 A.
country AT
source
url http://library.utia.cas.cz/separaty/2024/AS/tichy-0585405.pdf
cas_special
project
project_id GA24-10400S
agency GA ČR
country CZ
ARLID cav_un_auth*0464279
abstract (eng) The identification of a sample associated with a nuclear test is a challenging task for the CTBTO because of the presence of a noble gas background in the constant evolving atmosphere. This background is caused by nuclear power plants, nuclear research reactors, and medical isotope production facilities and contributes to samples collected by the noble gas systems of the International Monitoring Stations (IMS). Because of that background, standard linear inverse model applied to Xe-133 measurements is prone to substantial errors. To address this problem, we investigate possible methods for separation of the background signal and any signal from a nuclear explosion, which is further processed for estimation of the Xe-133 source term. We assume that the observed unknown point release of Xe-133 can be modeled as a linear model y=Mx, where y is the vector of observations, M is source-receptor sensitivity (SRS) matrix,\nand x is the temporal profile of the unknown release from a nuclear explosion, i.e. its source term. Since the signal in the observation vector is most probably mixed with civilian emitters, we test methods for separation of the contributions from the unknown signal and the background. We compare various approaches, ranging from simple model calibration, to simulated background term and their combinations with anomaly detection. The results are demonstrated on the data from the 1st Nuclear Explosion Signal Screening Open Inter-Comparison Exercise 2021 where advantages and disadvantages of studied methods are discussed and results are evaluated with the use of ground truth information on temporal and spatial location of the Xe-133 source.
action
ARLID cav_un_auth*0466498
name EGU General Assembly 2024
dates 20240414
mrcbC20-s 20240419
place Vienna / Online
url https://www.egu24.eu/home.html
country AT
RIV BD
FORD0 10000
FORD1 10100
FORD2 10102
reportyear 2025
num_of_auth 6
presentation_type PR
inst_support RVO:67985556
permalink https://hdl.handle.net/11104/0353494
confidential S
article_num EGU24-3075
arlyear 2024
mrcbU14 SCOPUS
mrcbU24 PUBMED
mrcbU34 WOS
mrcbU63 cav_un_epca*0585420 EGU General Assembly 2024 Abstracts European Geosciences Union 2024 Munich