vai_a_storia   vai_a_organizzazione   vai_a_sedi   vai_a_personale   Area Riservata
    English English Version  

Far infrared radiative properties of water vapor and clouds in Antarctica

  Articoli su Riviste JCR/ISI  (anno 2015)

Autori:  Palchetti L., Bianchini G., Di Natale G., Del Guasta M

Affiliazione Autori:  Consiglio Nazionale delle Ricerche, Istituto Nazionale di Ottica, Via Madonna del Piano 10, Sesto Fiorentino, 50019, Italy

Riassunto:  Water vapor and clouds are among the most important greenhouse components whose radiative features cover all the broad spectral range of the thermal emission of the atmosphere. Typically more than 40% of the total thermal emission of Earth occurs in the far-infrared (FIR) spectral region from 100 to 667 cm(-1) (wavelengths from 100 to 15 mu m). Nevertheless, this spectral region has not ever been fully covered down to 100 cm(-1) by space missions, and only a few ground-based experiments exist because of the difficulty of performing measurements from high altitude and very dry locations where the atmosphere is sufficiently transparent to observe the FIR emission features. To cover this lack of observations, the Italian experiment Radiative Properties of Water Vapor and Clouds in Antarctica has collected a 2-yr dataset of spectral measurements of the radiance emitted by the atmosphere and by clouds, such as cirrus and polar stratospheric clouds, from 100 to 1,400 cm(-1) (100-7 mu m of wavelength), including the underexplored FIR region, along with polarization-sensitive lidar observations, daily radiosondes, and other ancillary information to characterize the atmosphere above the site. Measurements have been performed almost continuously with a duty cycle of 6 out of 9 h, from the Italian-French base of Concordia at Dome C over the Antarctic Plateau at 3,230 m MSL, in all-sky conditions since 2012. Because of the uniqueness of the observations, this dataset will be extremely valuable for evaluating the accuracy of atmospheric absorption models (both gas and clouds) in the underexplored FIR and to detect possible daily, seasonal, and annual climate signatures.

Volume n.:  96 (9)      Pagine da: 1505  a: 1518
Ulteriori informazioni:  This research was supported by the Italian PNRA (Programma Nazionale di Ricerche in Antartide) and the Institut polaire francais Paul Emile Victor (IPEV). More specifically it was developed as a part of the Subproject PRANA (Proprieta Radiative dell\'Atmosfera e delle Nubi in Antartide). Data and information on radio sounding measurements were obtained from the IPEV/PNRA Project \"Routine Meteorological Observation at Station Concordia\" (www.climantartide .it/index.php?lang=en). We thank all of the institutions and their associates listed in Table 3 for supplying information about other measurements available at Concordia station. L\'articolo ha ottenuto la copertina del fascicolo Volume 96 Issue 9 (September 2015.
DOI: 10.1175/BAMS-D-13-00286.1

*Impact Factor della Rivista: (2015) 7.929   *Citazioni: 13
data tratti da "WEB OF SCIENCE" (marchio registrato di Thomson Reuters) ed aggiornati a:  14/07/2019

Riferimenti visionabili in IsiWeb of Knowledge: (solo per sottoscrittori)
Per visualizzare la scheda dell'articolo su IsiWeb: Clicca qui
Per visualizzare la scheda delle Citazioni dell'articolo su IsiWeb: Clicca qui

INO © Istituto Nazionale di Ottica - Largo Fermi 6, 50125 Firenze | Tel. 05523081 Fax 0552337755 - P.IVA 02118311006     P.E.C.    Info