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VERSION:2.0
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BEGIN:VEVENT
SUMMARY:Machine learning for optimizing plasma resource utilization on Mar
 s
DTSTART:20231129T140000Z
DTEND:20231129T160000Z
DTSTAMP:20260622T012928Z
UID:5c090edb-e6a4-4e01-b924-7627d2eacf74
SEQUENCE:1
CREATED:20231127T152710Z
DESCRIPTION: Abstract: On Mars\, the atmosphere plays a pivotal role in th
 e In-Situ Resource Utilization (ISRU) perspective\, mainly due to the abun
 dant atmospheric CO2. Plasma technologies\, especially the application of 
 low-temperature plasmas (LTPs)\, have been proposed to decompose the exist
 ing CO2\, facilitating the recovery of O2 and CO to support life\, fuel\, 
 and agriculture. However\, much remains to be done regarding accurate plas
 ma modeling\, which relies on the availability of precise reaction rate co
 efficients. Determining these constants is a non-trivial task\, primarily 
 addressed by scientists with extensive experience in the field.In this the
 sis\, we investigate the use of machine learning techniques to predict the
 se parameters. This is done with an automated and systematic approach\, ba
 sed on the heavy-species densities of the gas&#x27\;s final state. The tra
 ining data is generated using the Lisbon Kinetics simulation tool (LoKI).B
 oth Support Vector Regression (SVR) and Artificial Neural Network (ANN) mo
 dels were trained using an oxygen (O2) plasma kinetic scheme\, encompassin
 g 11 species and 53 heavy-species reaction processes. When evaluated on a 
 test dataset\, the top performing SVR and ANN models achieved mean relativ
 e error values of 0.10% and 0.22%\, respectively. Although both models exh
 ibited significant accuracy\, the SVR model emerged as superior\, offering
  both simplicity and heightened performance for our specific low-dimension
 al dataset. These two machine learning approaches serve as a successful pr
 eliminary step towards more comprehensive models to automate the predictio
 n of reaction rate coefficients.
LAST-MODIFIED:20231127T152710Z
LOCATION:Anfiteatro GA2\, Pavilhão Central\, 0\, Alameda
URL:http://df.vps.tecnico.ulisboa.pt/pt/eventos/machine-learning-for-optim
 izing-plasma-resource-utilization-on-mars/
X-ALT-DESC;FMTTYPE=text/html:<p data-block-key="bemh5"> <b>Abstract</b>: O
 n Mars\, the atmosphere plays a pivotal role in the <i>In-Situ</i> Resourc
 e Utilization (ISRU) perspective\, mainly due to the abundant atmospheric 
 CO2. Plasma technologies\, especially the application of low-temperature p
 lasmas (LTPs)\, have been proposed to decompose the existing CO2\, facilit
 ating the recovery of O2 and CO to support life\, fuel\, and agriculture. 
 However\, much remains to be done regarding accurate plasma modeling\, whi
 ch relies on the availability of precise reaction rate coefficients. Deter
 mining these constants is a non-trivial task\, primarily addressed by scie
 ntists with extensive experience in the field.<br/><br/></p><p data-block-
 key="1ffgt">In this thesis\, we investigate the use of machine learning te
 chniques to predict these parameters. This is done with an automated and s
 ystematic approach\, based on the heavy-species densities of the gas&#x27\
 ;s final state. The training data is generated using the Lisbon Kinetics s
 imulation tool (LoKI).<br/><br/></p><p data-block-key="5h4u3">Both Support
  Vector Regression (SVR) and Artificial Neural Network (ANN) models were t
 rained using an oxygen (O2) plasma kinetic scheme\, encompassing 11 specie
 s and 53 heavy-species reaction processes. When evaluated on a test datase
 t\, the top performing SVR and ANN models achieved mean relative error val
 ues of 0.10% and 0.22%\, respectively. Although both models exhibited sign
 ificant accuracy\, the SVR model emerged as superior\, offering both simpl
 icity and heightened performance for our specific low-dimensional dataset.
  These two machine learning approaches serve as a successful preliminary s
 tep towards more comprehensive models to automate the prediction of reacti
 on rate coefficients.</p>
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