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TAPAS, a web-based service of atmospheric transmission computation for astronomy
- Source :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 564, pp.A46. ⟨10.1051/0004-6361/201322383⟩, Astronomy and Astrophysics-A&A, 2014, 564, pp.A46. ⟨10.1051/0004-6361/201322383⟩
- Publication Year :
- 2014
- Publisher :
- HAL CCSD, 2014.
-
Abstract
- Spectra of astronomical targets acquired from ground-based instruments are affected by the atmospheric transmission. The authors and their institutes are developing a web-based service, TAPAS (Transmissions of the AtmosPhere for AStromomical data). This service, freely available, is developed and maintained within the atmospheric ETHER data center. TAPAS computes the atmospheric transmission in the line-of-sight to the target indicated by the user. The user files a request indicating the time, ground location, and either the equatorial coordinates of the target or the Zenith Angle of the line-of sight (LOS). The actual atmospheric profile (temperature, pressure, humidity, ozone content) at that time and place is retrieved from the ETHER atmospheric data base (from a combination of ECMWF meteorological field and other informations), and the atmospheric transmission is computed from LBLRTM software and HITRAN data base for a number of gases: O2, H2O, O3, CO2, and Rayleigh extinction. The first purpose of TAPAS output is to allow identification of observed spectral features as being from atmospheric or astrophysical origin. The returned transmission may also serve for characterizing the spectrometer in wavelength scale and Instrument Line Spectral Function (ILSF) by comparing one observed spectrum of an atmospheric feature to the transmission. Finally, the TOA (Top Of Atmosphere) spectrum may be obtained either by division of the observed spectrum by the computed transmission or other techniques developed on purpose. The obtention of transmissions for individual species allows more potentialities and better adjustments to the data. In this paper, we describe briefly the mechanism of computation of the atmospheric transmissions, and we show some results for O2 and H2O atmospheric absorption. The wavelength range is presently 500-2500 nm. The address is http://ether.ipsl.jussieu.fr/tapas/<br />Comment: 12 pages, 10 figures, submitted to Astronomy and Astrophysics
- Subjects :
- Physics
spectroscopy
Spectrometer
transmission
FOS: Physical sciences
Astronomy and Astrophysics
Context (language use)
Astrophysics
Spectral line
[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
symbols.namesake
telluric
Transmission (telecommunications)
Space and Planetary Science
Extinction (optical mineralogy)
atmosphere
symbols
HITRAN
spectrometer
Rayleigh scattering
Astrophysics - Instrumentation and Methods for Astrophysics
Instrumentation and Methods for Astrophysics (astro-ph.IM)
Zenith
Remote sensing
Subjects
Details
- Language :
- English
- ISSN :
- 00046361
- Database :
- OpenAIRE
- Journal :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 564, pp.A46. ⟨10.1051/0004-6361/201322383⟩, Astronomy and Astrophysics-A&A, 2014, 564, pp.A46. ⟨10.1051/0004-6361/201322383⟩
- Accession number :
- edsair.doi.dedup.....b7efd782f1283322b91a73823c31a2bb
- Full Text :
- https://doi.org/10.1051/0004-6361/201322383⟩