A new method for determining the transfer function of an Acousto optical tunable filter
dc.contributor.author | Mahieux, A. | |
dc.contributor.author | Wilquet, V. | |
dc.contributor.author | Drummond, R. | |
dc.contributor.author | Belyaev, D. | |
dc.contributor.author | Federova, A. | |
dc.contributor.author | Vandaele, A.C. | |
dc.date | 2009 | |
dc.date.accessioned | 2016-04-05T13:47:15Z | |
dc.date.available | 2016-04-05T13:47:15Z | |
dc.identifier.uri | https://orfeo.belnet.be/handle/internal/3307 | |
dc.description | The current study describes the determination of the transfer function of an Acousto Optical Tunable Filter from the in-flight solar observations of the SOIR instrument on board Venus Express. An approach is proposed in order to reconstruct the transfer function profile from the analysis of various solar lines. Moreover this technique allows the determination of the evolution of the transfer function as a function of the AOTF radio frequency. © 2009 Optical Society of America. | |
dc.language | eng | |
dc.title | A new method for determining the transfer function of an Acousto optical tunable filter | |
dc.type | Article | |
dc.subject.frascati | Physical sciences | |
dc.audience | Scientific | |
dc.subject.free | Functions | |
dc.subject.free | Optical filters | |
dc.subject.free | Probability density function | |
dc.subject.free | Acousto-optical tunable filters | |
dc.subject.free | Analysis of various | |
dc.subject.free | Radio frequencies | |
dc.subject.free | Solar lines | |
dc.subject.free | Solar observations | |
dc.subject.free | Venus express | |
dc.subject.free | Transfer functions | |
dc.source.title | Optics Express | |
dc.source.volume | 17 | |
dc.source.issue | 3 | |
dc.source.page | 2005-2014 | |
Orfeo.peerreviewed | Yes | |
dc.identifier.doi | 10.1364/OE.17.002005 | |
dc.identifier.scopus | 2-s2.0-59749093453 |