Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/33633
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | MARIS, Michele | en_US |
dc.contributor.author | Tomasi. Maurizio | en_US |
dc.date.accessioned | 2023-02-20T15:46:35Z | - |
dc.date.available | 2023-02-20T15:46:35Z | - |
dc.date.issued | 2009 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/33633 | - |
dc.description.abstract | This document reports an analysis of the differences among the REBA parameters optimazion in CSL and in Flight. Such differences arise from 1. presence of a sky signal, in particular the cosmological dipole; 2. different operative conditions; 3. 4K cooler fluctuations; 4. additive constraints to the maximum acceptable processing error which where not considered in CSL. Among the possible additive constrains the most important are: 1. to limit the processing error in total power; 2. to limit the impact of onboard processing on the r deterermination. All of these effects asks to improve the OCA2 optimization procedures in order to have a program adapted to flight conditions. This does not require large modification of OCA2, in most cases it is a matter to add more tests at the output of the application or to use OCA2 in a different manner. However, this could have an impact on the overall speed of the optimization procedure. In the following we will denote with OCA2@CSL the version of OCA2 operated at CSL, and with OCA2@FLIGHT the OCA2 optimizzation algorithm updated for Flight. | en_US |
dc.language.iso | eng | en_US |
dc.title | Planck/LFI: Flight Effects on the REBA Parameters Optimization | en_US |
dc.type | Research report | - |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | PL-LFI-OAT-TN-063 | en_US |
dc.relation.numberofpages | 35 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.note | Questo documento rappresenta la versione finale del report. This document represents the final version of this report. | en_US |
dc.description.numberofauthors | 2 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.identifier.classification | PL-LFI-OAT-TN-063 | en_US |
dc.type.miur | 298 Altro | - |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | en_US |
dc.relation.versioning | 0.2 | en_US |
dc.contributor.reviewer | M. Bersanelli, C.R.Butler | en_US |
dc.contributor.approved | N. Mandolesi | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Research report | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.orcid | 0000-0001-9442-2754 | - |
È visualizzato nelle collezioni: | 4.03 Rapporti di progetto |
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File | Descrizione | Dimensioni | Formato | |
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PL_LFI_OAT_TN_063.pdf | Planck Report | 1.95 MB | Adobe PDF | Visualizza/apri |
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