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Dive into the research topics where Enrico Tessarolo is active.

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Featured researches published by Enrico Tessarolo.


Optical Materials Express | 2015

Effects of helium ion bombardment on metallic gold and iridium thin films

Sara Zuccon; E. Napolitani; Enrico Tessarolo; Paola Zuppella; Alain Jody Corso; Francesca Gerlin; Marco Nardello; M. G. Pelizzo

Single layer mirrors have been prepared by evaporating gold and iridium on silicon substrates. The samples have been exposed to 4 keV He + ion flux at different total fluences, simulating the effect of solar wind ions on optical coatings. We show that the ion implantation significantly affects the optical characteristics of the metallic films. The phenomena are explained and modeled also considering the related material modifications observed with chemical and morphological analysis.


Proceedings of SPIE | 2016

Optical components in harsh space environment

M. G. Pelizzo; Alain Jody Corso; Enrico Tessarolo; P. Zuppella; Roman Böttger; Rene Huebner; Vincenzo Della Corte; P. Palumbo; G. Taglioni; G. Preti; L. Foggetta; Paolo Valente; Piergiorgio Rancoita; Alessandro Martucci; E. Napolitani

Space exploration is linked to the development of increasingly innovative instrumentation, able to withstand the operation environment, rich in ion particles and characterized by high temperatures. Future space missions such as JUICE and SOLAR ORBITER will operate in a very harsh and extreme environment-. Electrons and ions are considered among the causes of potential damage of the optical instrumentation and components. Development of hard coatings capable to preserve their optical properties is pivotal. Different coating materials have been exposed to ion irradiation in particle accelerators. Change in optical performances has been observed in the extreme ultraviolet and visible spectral region and structural properties have been analyzed by different techniques. The knowledge of the damage mechanisms and thresholds allows the selection of more promising candidate materials to realize the optical components for the new frontiers space missions.


Journal of Astronomical Telescopes, Instruments, and Systems | 2015

Study of optical materials to be used on Multi Element Telescope for Imaging and Spectroscopy instrument

Marco Nardello; Sara Zuccon; A. J. Corso; P. Zuppella; Francesca Gerlin; Enrico Tessarolo; Maria Guglielmina Pelizzo

Abstract. The European Space Agency mission Solar Orbiter (SOLO) is dedicated to the study of the solar atmosphere and heliosphere. As a part of the payload, the instrument METIS (Multi Element Telescope for Imaging and Spectroscopy) will provide images of the corona, both in the visible range and at the hydrogen Lyman-α emission line (121.6 nm). The realization of optical coatings, based on Al and MgF2, able to reflect/transmit such spectral components is, therefore, necessary. Since optical characteristics of materials in the vacuum ultraviolet range are not well studied and vary greatly with the realization process, we implemented a study of their properties in different deposition conditions. This is aimed to the realization of a custom designed filter able to transmit the 121.6 nm wavelength while reflecting visible light, and thus separating visible from ultraviolet light paths in the METIS instrument.


Proceedings of SPIE | 2014

Phase delay characterization of multilayer coatings for FEL applications

Alain Jody Corso; Enrico Tessarolo; Paola Zuppella; Sara Zuccon; Marco Nardello; M. G. Pelizzo

The phase delay induced by multilayer (ML) mirrors is an important feature in many fields such as attosecond pulses compression, photolithography or in pump and probe experiments performed with Free Electron Laser (FEL) pulses. The experimental characterization of the ML phase delay can be obtained by the standing wave distribution measurement (by using Total Electron Yield (TEY) signal) combined to reflectance measurement. In this work, a ML structure with aperiodic capping-layers was designed and deposited for FEL applications and their reflectance and phase delay was characterized. The method adopted allows to retrieve the ML phase delay by using the TEY signals taken at different working configurations and it doesn’t require the comparison with a bulk reference sample. The results obtained are presented and discussed.


Proceedings of SPIE | 2017

Continuous palladium-based thin films for hydrogen detection

Alain Jody Corso; Marco Angiola; Enrico Tessarolo; Martino Guidolin; Alberto Donazzan; Alessandro Martucci; M. G. Pelizzo

Metallic films of palladium (Pd) and palladium-tin (Pd-Sn) have been deposited by evaporation technique. They were used as sensitive material for optical sensor by measuring the variation of absorbance. All samples were then oxidized by annealing at 500°C in low vacuum atmosphere. All the films were investigated by X-Ray Diffraction (XRD), Atomic Force Microscopy (AFM) to observe the influence of the structure and morphology on the optical properties of the films, carrying useful information for the sensing properties of the different sensing materials. Furthermore, the sensing performances were tested by monitoring the variation on the optical absorbance induced during the absorption / desorption of hydrogen gas. While the use of Pd for gas sensing has been widely covered for electrical and SPR sensors, this work aims to extend our comprehension of the optical sensing behavior, especially in absorbance-mode, of the thin films of PdO, Pd-Sn and PdO-SnO2.


Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems | 2017

Systematic investigation of the optical coatings damages induced in harsh space environment

Alain Jody Corso; Enrico Tessarolo; Alessandro Martucci; Maria Guglielmina Pelizzo

The scientific goals required to the next-generation space missions lead the development of innovative instrumentation, conceived to operate in increasingly harsh environments. Optical coatings are among the sub-systems which can highly suffer the agents in such environments. In particular, as recently demonstrated, the accelerated ions and particles can potentially jeopardize the coatings optical performances, with a consequent degradation of the overall functionality of an instrument. Despite its importance, this issue is still poorly investigated. In fact, the fragmentary knowledge of the space environments and the low number of previous ground testing experiments complicates the definition of clear procedures to investigate the behavior of the optical coatings in space. A systematic approach devoted to identify a methodology for the validation of optical coatings under ions irradiation is presented. Monte Carlo simulations are used to evaluate the effects induced by different ion species and energies on both layers and multilayers of different materials, getting an accurate overview of the main criticalities. Such results are then used to plan representative irradiation experiments and the subsequent analysis procedures needed for a proper characterization of the exposed samples. In this paper, a summary of the experiments performed so far is presented. Thanks to these studies we have identified three main damage mechanisms which can be used to explain most of the degradation effects observed when an optical coating is irradiated with low energy particles. A brief discussion of such mechanisms is reported.


Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems | 2017

Ions irradiation on bi-layer coatings

Enrico Tessarolo; Alain Jody Corso; Alessandro Martucci; Maria Guglielmina Pelizzo; Roman Böttger

Future space missions will operate in very harsh and extreme environments. Optical and electronics components need to be optimized and qualified in view of such operational challenges. This work focuses on the effect of low alpha particles irradiation on coatings. Low energy He+ (4 keV and 16 keV) ions have been considered in order to simulate in laboratory the irradiation of solar wind (slow and fast components) alpha particles. Mono- and proper bi-layers coatings have been investigated. The experimental tests have been carried out changing doses as well as fluxes during the irradiation sessions. Optical characterization in the UV-VIS spectral range and superficial morphological analysis have performed prior and after irradiation.


Proceedings of SPIE | 2015

Graphene-like coatings for biosensors devices

P. Zuppella; Francesca Gerlin; Sara Zuccon; Alain Jody Corso; Enrico Tessarolo; Marco Nardello; Davide Bacco; M. G. Pelizzo

The interest in graphene–like materials involves many research areas, including the development of biosensors devices. We have recently studied the use of graphene/metal bilayer for surface plasmon resonance (SPR) equipment devoted to detection of chemical processes and biomolecules recognition. The dual role of graphene is to protect the metal layer underneath and to enhance the bioaffinity by adsorbing biomolecules with carbon–based ring structures. Depending on the application, it may be necessary laser and chemical treatments of graphene to improve the performances of the whole device. The processing effects will be investigated by near edge X-ray absorption fine structure (NEXAFS) spectroscopy. The use of synchrotron light is mandatory for NEXAFS analysis since a continuous EUV source of selected polarization is required. The ideas, the analysis and the results are the subjects of this work.


Proceedings of SPIE | 2015

He+ ions damage on optical coatings for solar missions

Davide Bacco; Alain Jody Corso; P. Zuppella; Francesca Gerlin; Roman Böttger; E. Napolitani; Enrico Tessarolo; Marco Nardello; Sara Zuccon; M. G. Pelizzo

Single layer thin films have been exposed to low energy alpha particles (4keV). Implanted doses are equivalent to those accumulated in 1, 2, 4 and 6 years of ESA Solar Orbiter mission operation. Two ions fluences have been considered. In order to change the total dose accumulated, for each ion flux the time of exposure was varied. Reflectance in the visible spectral range has been measured prior and after implantation. Results show no significant change in performances in gold and palladium, while a small decrease in performances is observed in iridium. The implantation rate does not seem to affect the experiment.


Proceedings of SPIE | 2015

Radiometric modelling of a space optical instrument: an example of application to PHEBUS

Alain Jody Corso; Paola Zuppella; Jean Francois Mariscal; Nicolas Rouanet; Eric Quémerais; Marco Nardello; P. Nicolosi; Enrico Tessarolo; Davide Bacco; Francesca Gerlin; Sara Zuccon; Maria Guglielmina Pelizzo

Probing of Hermean Exosphere By Ultraviolet Spectroscopy (PHEBUS) is a dual channels spectrometer working in the Extreme UltraViolet (EUV) and Far UltraViolet (FUV) range. It will be on board of ESA BepiColombo cornerstone mission and it will be devoted to investigate the composition, the dynamic, the formation and the feeding mechanisms of Mercury’s exosphere system. A consistent interpretation of the observational data collected by PHEBUS requires a deeply knowledge of its radiometric behavior. The Mueller’s matrix formalism can be adopted to derive an accurate radiometric model able to takes into account also the polarization state of the source observed by PHEBUS. Moreover, this theoretical model can be further verified and refined during an experimental ground calibration campaign. In this work we present the radiometric model derived for PHEBUS spectrometer together with some results obtained during the Flight Model (FM) ground calibration which is still ongoing. In particular, the obtained results employing this approach show that this is a complete and versatile method to perform the radiometric calibration of a generic space instrument.

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Paola Zuppella

National Research Council

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Roman Böttger

Helmholtz-Zentrum Dresden-Rossendorf

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