Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Djelloul Djafer"'
Autor:
Mohamed Zaiani, Abdanour Irbah, Djelloul Djafer, Constantino Listowski, Julien Delanoe, Dimitris Kaskaoutis, Sabrina Belaid Boualit, Fatima Chouireb, Mohamed Mimouni
Publikováno v:
Remote Sensing, Vol 13, Iss 12, p 2271 (2021)
Radiative transfer in the Earth’s atmosphere under clear-sky conditions strongly depends on turbidity due to aerosols and hydrometeors. It is therefore important to know its temporal radiative properties for a given site when the objective is to op
Externí odkaz:
https://doaj.org/article/c77a97a0d6e7406fb163511a4d50c12f
Autor:
Abdanour Irbah, Fatima Chouireb, Julien Delanoë, Mohamed Mimouni, Mohamed Zaiani, Djelloul Djafer, Dimitris Kaskaoutis, Sabrina Belaid Boualit, Constantino Listowski
Publikováno v:
Remote Sensing, Vol 13, Iss 2271, p 2271 (2021)
Remote Sensing
Remote Sensing, MDPI, 2021, 13, pp.2271. ⟨10.3390/rs13122271⟩
Remote Sensing; Volume 13; Issue 12; Pages: 2271
Remote Sensing
Remote Sensing, MDPI, 2021, 13, pp.2271. ⟨10.3390/rs13122271⟩
Remote Sensing; Volume 13; Issue 12; Pages: 2271
Radiative transfer in the Earth’s atmosphere under clear-sky conditions strongly depends on turbidity due to aerosols and hydrometeors. It is therefore important to know its temporal radiative properties for a given site when the objective is to op
Publikováno v:
Leonardo Electronic Journal of Practices and Technologies, Vol 14, Iss 27, Pp 177-184 (2015)
For many developing countries, solar radiation measurements are only available for selected stations due to the cost of the measurement equipment and techniques involved. In this study, a simple model based on Radial Basis Function neural networks is
Autor:
Slimane Bekki, Mustapha Meftah, David Bolsée, Gaël Cessateur, Dominique Sluse, Alain Sarkissian, Alain Hauchecorne, Abdanour Irbah, Nuno Pereira, Luc Damé, Djelloul Djafer
Publikováno v:
Solar Physics
Solar Physics, Springer Verlag, 2017, 292 (art. 101), ⟨10.1007/s11207-017-1115-2⟩
Solar Physics, 2017, 292 (art. 101), ⟨10.1007/s11207-017-1115-2⟩
Solar Physics, Springer Verlag, 2017, 292 (art. 101), ⟨10.1007/s11207-017-1115-2⟩
Solar Physics, 2017, 292 (art. 101), ⟨10.1007/s11207-017-1115-2⟩
The solar spectrum is a key parameter for different scientific disciplines such as solar physics, climate research, and atmospheric physics. The SOLar SPECtrometer (SOLSPEC) instrument of the Solar Monitoring Observatory (SOLAR) payload onboard the I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9571d0309bf319d50433d2bc2dc4fb80
https://hal-insu.archives-ouvertes.fr/insu-01571600
https://hal-insu.archives-ouvertes.fr/insu-01571600
Publikováno v:
Renewable Energy
Renewable Energy, 2017, 101, pp.347-355. ⟨10.1016/j.renene.2016.08.038⟩
Renewable Energy, Elsevier, 2017, 101, pp.347-355. ⟨10.1016/j.renene.2016.08.038⟩
Renewable Energy, 2017, 101, pp.347-355. ⟨10.1016/j.renene.2016.08.038⟩
Renewable Energy, Elsevier, 2017, 101, pp.347-355. ⟨10.1016/j.renene.2016.08.038⟩
International audience; A new method using the wavelet transform properties is developed to determine clear days of solar irradiance. These days are needed to model the solar radiation and to compare the existing empirical models. We use this method
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8f3910bc7c23160fa9c6a990cc85a1fc
https://insu.hal.science/insu-01394851/document
https://insu.hal.science/insu-01394851/document
Publikováno v:
The Astrophysical Journal. 875:L26
The solar oblateness results from distortion processes due to several phenomena inside the Sun but also induced by the centrifugal potential of the surface rotation. This fundamental parameter is therefore of great scientific interest, but its measur
Autor:
Djelloul Djafer, Jean-François Hochedez, Mickael Crepel, Mustapha Meftah, Thierry Corbard, Alain Hauchecorne, Abdanour Irbah
Publikováno v:
Solar Physics
Solar Physics, Springer Verlag, 2014, 289 (1), pp.1-10. ⟨10.1007/s11207-013-0347-z⟩
Solar Physics, 2014, 289 (1), pp.1-10. ⟨10.1007/s11207-013-0347-z⟩
Solar Physics, Springer Verlag, 2014, 289 (1), pp.1-10. ⟨10.1007/s11207-013-0347-z⟩
Solar Physics, 2014, 289 (1), pp.1-10. ⟨10.1007/s11207-013-0347-z⟩
International audience; Knowledge of the Solar Diameter Imager and Surface Mapper (SODISM) plate scale is a fundamental parameter for obtaining the solar radius. We have determined the plate scale of the telescope on the ground and in flight onboard
Publikováno v:
Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave
Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, Jun 2016, Edinburgh, United Kingdom. pp.99044G, ⟨10.1117/12.2232028⟩
Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, Jun 2016, Edinburgh, United Kingdom. pp.99044G, ⟨10.1117/12.2232028⟩
International audience; The scientific objectives of a space mission translate into instrumental developments and satellites operations to observe the astronomical objects of interest. The payload in its space environment is however subject to import
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47f16ff324769b9a0ae38ffa219c2fb8
https://hal-insu.archives-ouvertes.fr/insu-01345786
https://hal-insu.archives-ouvertes.fr/insu-01345786
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 591, A150 (11p.). ⟨10.1051/0004-6361/201527914⟩
Astronomy and Astrophysics-A&A, 2016, 591, A150 (11p.). ⟨10.1051/0004-6361/201527914⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 591, A150 (11p.). ⟨10.1051/0004-6361/201527914⟩
Astronomy and Astrophysics-A&A, 2016, 591, A150 (11p.). ⟨10.1051/0004-6361/201527914⟩
International audience; Daily observation conditions are needed when observing the Sun at high angular resolution. MISOLFA is a daytime seeing monitor developed for this purpose that allows the estimation of the spatial and temporal parameters of atm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b5b19d2e594bee74dec861d5f028d518
https://hal-insu.archives-ouvertes.fr/insu-01322842/file/aa27914-15.pdf
https://hal-insu.archives-ouvertes.fr/insu-01322842/file/aa27914-15.pdf
Publikováno v:
Solar Physics
Solar Physics, Springer Verlag, 2012, 281 (2), pp.863-875. ⟨10.1007/s11207-012-0109-3⟩
Solar Physics, 2012, 281 (2), pp.863-875. ⟨10.1007/s11207-012-0109-3⟩
Solar Physics, Springer Verlag, 2012, 281 (2), pp.863-875. ⟨10.1007/s11207-012-0109-3⟩
Solar Physics, 2012, 281 (2), pp.863-875. ⟨10.1007/s11207-012-0109-3⟩
International audience; A new method to detect sunspots on full-disk solar images, recorded in an optical wide spectral band and in the line of Ca ii K1, is presented. It is based on the compact wavelet transform and a process that automatically iden