Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/33668
DC Field | Value | Language |
---|---|---|
dc.contributor.author | MASCIADRI, Elena | en_US |
dc.contributor.author | TURCHI, Alessio | en_US |
dc.date.accessioned | 2023-02-21T13:47:23Z | - |
dc.date.available | 2023-02-21T13:47:23Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/33668 | - |
dc.description.abstract | The 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.iso | eng | en_US |
dc.title | TURBULENCE PREDICTION: REPORT ON MODEL GEOMETRY | en_US |
dc.type | Research report | - |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.numberofpages | 20 | en_US |
dc.type.referee | REF_0 | 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 | D7.12 | en_US |
dc.type.miur | 298 Altro | - |
dc.relation.fund | H2020 | en_US |
dc.relation.project | SOLARNET (Integrating High Resolution Solar Physics) | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.relation.versioning | 1.0 | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairetype | Research report | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
crisitem.project.grantno | 824135 | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-0450-4092 | - |
crisitem.author.orcid | 0000-0003-3439-8005 | - |
Appears in Collections: | 4.03 Rapporti di progetto |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
SOLARNET-D7.12_v3.pdf | 10.18 MB | Adobe PDF | View/Open |
Page view(s)
21
checked on Sep 22, 2023
Download(s)
3
checked on Sep 22, 2023
Google ScholarTM
Check
Items in DSpace are published in Open Access, unless otherwise indicated.