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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 4 ALTRI PRODOTTI SCIENTIFICI (Other scientific products)
  4. 4.03 Rapporti di progetto
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/33668
DC FieldValueLanguage
dc.contributor.authorMASCIADRI, Elenaen_US
dc.contributor.authorTURCHI, Alessioen_US
dc.date.accessioned2023-02-21T13:47:23Z-
dc.date.available2023-02-21T13:47:23Z-
dc.date.issued2021en_US
dc.identifier.urihttp://hdl.handle.net/20.500.12386/33668-
dc.description.abstractThe H2020 SOLARNET project includes a study to investigate the possibility to set-up systems for the forecast of the optical turbulence (OT) in the day-time regimes at the two sites of Roque de los Muchachos Observatory (ORM, La Palma) and Teide Observatory (TO, Tenerife), with a particular attention to the site that will be selected for the European Solar Telescope (EST). More precisely the study aims to upgrade to day-time conditions the method to forecast the OT (C N2 profiles and integrated astroclimatic parameters) that was developed by the INAF partner for night-time ground-based astronomy. The technique implies the use of a mesoscale model (Meso-Nh) [RF1, RF2, RF3, RF4]. Seeing measurements at the ORM and TO are presented in [RF5, RF6]. This document presents the global atmospheric model configuration. This includes the set-up of the orography and the sequence of initialisation. Besides, we analysed also measurements taken by the Stockholm University (SU) partner at the SST with the WF-WFS method in the past years in perspective of using such measurements as a reference to calibrate and/or validate forecasts. In [RF6] measurements taken with a SHABAR by the Istituto de Astrofisica de Canarias (IAC) partner during past years have been analysed with the same philosophy and goal. The analysis of WF-WFS measurements has to be seen as an integration of the [RF6]. We remind that measurements are relevant in this process as they represent the reference with respect to which we can provide an analysis of the forecasts.en_US
dc.language.isoengen_US
dc.titleTURBULENCE PREDICTION: REPORT ON MODEL GEOMETRYen_US
dc.typeResearch report-
dc.relation.mediumELETTRONICOen_US
dc.relation.numberofpages20en_US
dc.type.refereeREF_0en_US
dc.description.numberofauthors2en_US
dc.description.internationalnoen_US
dc.contributor.countryITAen_US
dc.relation.scientificsectorFIS/05 - ASTRONOMIA E ASTROFISICAen_US
dc.identifier.classificationD7.12en_US
dc.type.miur298 Altro-
dc.relation.fundH2020en_US
dc.relation.projectSOLARNET (Integrating High Resolution Solar Physics)en_US
dc.relation.ercsectorERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentationen_US
dc.relation.versioning1.0en_US
dc.description.oa1 – prodotto con file in versione Open Access (allegare il file al passo  5-Carica)en_US
item.openairetypeResearch report-
item.grantfulltextopen-
item.languageiso639-1en-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
item.cerifentitytypePublications-
crisitem.project.grantno824135-
crisitem.author.deptO.A. Arcetri-
crisitem.author.deptO.A. Arcetri-
crisitem.author.orcid0000-0002-0450-4092-
crisitem.author.orcid0000-0003-3439-8005-
Appears in Collections:4.03 Rapporti di progetto
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