- Atmospheric Ozone and Climate
- Optical Polarization and Ellipsometry
- Stellar, planetary, and galactic studies
- Calibration and Measurement Techniques
- Solar and Space Plasma Dynamics
- Impact of Light on Environment and Health
- Lightning and Electromagnetic Phenomena
- Air Quality Monitoring and Forecasting
- Natural product bioactivities and synthesis
- Intraocular Surgery and Lenses
- Remote Sensing in Agriculture
- Ophthalmology and Visual Impairment Studies
- Astrophysics and Cosmic Phenomena
- Astronomy and Astrophysical Research
- Optical and Acousto-Optic Technologies
- solar cell performance optimization
- Electromagnetic Compatibility and Noise Suppression
- Ocular Surface and Contact Lens
- Adaptive optics and wavefront sensing
- Herpesvirus Infections and Treatments
- Light effects on plants
- Power Line Communications and Noise
- Infrared Target Detection Methodologies
- Pharmacological Effects of Natural Compounds
- Leaf Properties and Growth Measurement
Croatian Academic and Research Network
2021
Laboratoire d’études spatiales et d’instrumentation en astrophysique
2018-2020
Université Paris Sciences et Lettres
2018-2020
Université de Versailles Saint-Quentin-en-Yvelines
2018-2020
Sorbonne Université
2018-2020
Université Paris Cité
2018-2020
Observatoire de Paris
2018-2020
Centre National de la Recherche Scientifique
2018-2020
Institut Technique de l'Aviculture
2020
Janssen (France)
2019
The SITELLE Imaging Fourier Transform Spectrometer was successfully commissioned at the Canada France Hawaii Telescope starting in July 2015. Here we discuss commissioning process, outcome of early tests on-sky as well ensuing work to optimize modulation efficiency large optical path difference and image quality instrument.
Views Icon Article contents Figures & tables Video Audio Supplementary Data Peer Review Share Twitter Facebook Reddit LinkedIn Tools Reprints and Permissions Cite Search Site Citation P. R. Barker, M. Crofts, Gal; A superior ''superior'' mirage. Am. J. Phys. 1 October 1989; 57 (10): 953–954. https://doi.org/10.1119/1.16138 Download citation file: Ris (Zotero) Reference Manager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Dropdown Menu input auto suggest filter your...
Traditional transmissive polarimetric methods can be used for wavelengths above 123 nm where birefringent materials transmit light and create significant birefringence. Below nm, no suitable solution is known to measure the four Stokes parameters on a large wavelength range. Therefore, we study here an innovative reflective (rather than transmissive) polarimeter working in far ultraviolet (FUV) range from 90 130 nm. We take advantage of phase shift created by reflections as well different...
POLLUX is a project of high-resolution UV spectropolarimeter for the prospective LUVOIR space observatory. It will work in range 90-400 nm with R ≥ 120000. The baseline design consists 3 channels representing echelle spectrographs dedicated polarimeters, customized echelles and freeform-based concave holographic gratings. We study requirements manufacturing assembly precision. consider three performance criteria related to spectral resolving power, calibration stability, gratings diffraction...
High-resolution spectropolarimetry is a useful astronomical technique, in particular to study stellar magnetic fields. It has been extensively used the past but mostly visible range. Space missions equipped with high-resolution spectropolarimeters working ultra-violet (UV) are now being studied. We propose concept of polarimeter temporal modulation and allowing perform Stokes IQUV measurements over full UV + Visible The purpose this article describe concept, two prototypes bench developed on...
The ultra-violet (UV) high-resolution spectropolarimeter Pollux is being studied in Europe under CNES leadership for the LUVOIR space mission. a projected 15-m telescope equipped with suite of instruments proposed to NASA. will perform spectropolarimetric measurements from 90 400 nm resolution 120000. spectrograph be divided three channels, each its own polarimeter: far UV (FUV, 90-124.5 nm), mid (MUV, 118.5-195 and near (NUV, 190-390 nm). We present here our FUV prototype investigation...
The ultra-violet (UV) high-resolution spectropolarimeter Pollux is being studied in Europe under CNES leadership for the LUVOIR space mission. a projected 15−m telescope equipped with suite of instruments proposed to NASA. will perform spectropolarimetric measurements from 90 400 nm resolution 120000. spectrograph be divided three channels, each its own polarimeter: far UV (FUV, 90−124.5 nm), mid (MUV, 118.5−195 and near (NUV, 190-390 nm). We present here our FUV prototype investigation...
High-resolution spectropolarimetry is a useful astronomical technique, in particular to study stellar magnetic fields. It has been extensively used the past but mostly visible range. Space missions equipped with high-resolution spectropolarimeters working ultra-violet (UV) are now being studied. We propose concept of polarimeter temporal modulation and allowing perform Stokes IQUV measurements over full UV + Visible The purpose this article describe concept, two prototypes bench developed on...
High-resolution spectropolarimetry is a technique used to study many astronomical objects including stellar magnetic fields. It has mainly been on ground for optical and, more recently, infrared (IR) observations. Space mission projects ultra-violet (UV) high-resolution spectropolarimetry, such as Pollux onboard LUVOIR proposed NASA, are being studied in Europe under CNES leadership. Bringing spectropolarimeter into space means that the instrument should be prepared environment temperatures....
Digital subscriber line (DSL) is a technology that widely used for bringing high-speed Internet access to the users' premises.Unfortunately, use of DSL over existing copper telecommunication networks can result in radiation cause interference radio systems operating same frequency range.To restrict such disturbances various limits wire-line have been proposed.However, differ significantly from each other which makes it difficult adopt common protection criteria.In this paper, comparison...