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A superspace method for discrete-time bilinear model identification by interaction matrices
KTH, School of Information and Communication Technology (ICT), Communication Systems, CoS, Radio Systems Laboratory (RS Lab). Thayer School of Engineering, United States .ORCID iD: 0000-0003-2948-1082
2011 (English)In: KYLE T. ALFRIEND ASTRODYNAMICS SYMPOSIUM, 2011, 445-464 p.Conference paper, Published paper (Refereed)
Abstract [en]

This paper presents a method for discrete-time bilinear state-space model identification from a single set of input-output data. The initial state can be unknown. By extending the interaction matrix formulation from linear to bilinear state-space models, the bilinear system state is expressed in terms of input-output measurements. This relationship is used to convert the bilinear model to an Equivalent Linear Model (ELM) which can be identified by any linear identification method such as a superspace method presented here. The bilinear state-space model is then extracted from the identified ELM. A companion paper deals with the identification of nonlinear input-output models instead of state-space models for a bilinear system using the same interaction matrix approach.

Place, publisher, year, edition, pages
2011. 445-464 p.
Series
Advances in the Astronautical Sciences, ISSN 1081-6003 ; 139
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-170101ISI: 000309482700028Scopus ID: 2-s2.0-80053418231ISBN: 978-0-87703-565-7 (print)OAI: oai:DiVA.org:kth-170101DiVA: diva2:827187
Conference
American-Astronautical-Society Kyle T Alfriend Astrodynamics Symposium, MAY 17-19, 2010, Monterey, CA
Note

QC 20150626

Available from: 2015-06-26 Created: 2015-06-26 Last updated: 2015-06-26Bibliographically approved

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Čelik, Hans

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Citation style
  • apa
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  • vancouver
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More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
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  • text
  • asciidoc
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