Rosario Sanz

ORCID: 0000-0002-7109-9349
Publications
Citations
Views
---
Saved
---
About
Contact & Profiles
Research Areas
  • Planetary Science and Exploration
  • Space Exploration and Technology
  • Atmospheric Ozone and Climate
  • Astro and Planetary Science
  • Optical and Acousto-Optic Technologies
  • Calibration and Measurement Techniques
  • Semiconductor Lasers and Optical Devices
  • Atmospheric and Environmental Gas Dynamics
  • Solar and Space Plasma Dynamics
  • Space Science and Extraterrestrial Life
  • Spacecraft Design and Technology
  • Optical Network Technologies
  • Photonic and Optical Devices
  • Aging, Health, and Disability
  • Gamma-ray bursts and supernovae
  • Astronomy and Astrophysical Research
  • Geography and Environmental Studies in Latin America
  • Stellar, planetary, and galactic studies
  • Scientific Research and Discoveries
  • Spectroscopy and Laser Applications

Instituto de Astrofísica de Andalucía
2015-2024

Consejo Superior de Investigaciones Científicas
2024

Universidad Carlos III de Madrid
2006

NOMAD is a spectrometer suite on board ESA's ExoMars trace gas orbiter due for launch in January 2016. consists of two infrared channels and one ultraviolet visible channel allowing the instrument to perform observations quasi-constantly, by taking nadir measurements at dayside nightside, during solar occultations. In this paper, design, manufacturing, testing are described. We focus upon optical working principle these channels, where an echelle grating, used as diffractive element,...

10.1364/ao.54.008494 article EN Applied Optics 2015-09-29

NOMAD is a spectrometer suite on board the ESA/Roscosmos ExoMars Trace Gas Orbiter, which launched in March 2016. consists of two infrared channels and one ultraviolet visible channel, allowing instrument to perform observations quasi-constantly, by taking nadir measurements at day- night-side, during solar occultations. Here, part 2 linked study, we describe design, manufacturing, testing channel called UVIS. We focus upon optical design working principle where telescopes are coupled single...

10.1364/ao.56.002771 article EN cc-by Applied Optics 2017-03-23

NOMAD [1] (Nadir and Occultation for MArs Discovery) is a multi-channel spectrometer onboard the ExoMars 2016 Trace Gas Orbiter (TGO), operating from Martian orbit since April 2018. Among other two, Solar (SO) channel covers infrared (IR) spectrum 2.3 to 4.3 µm (2320 4350 cm−1). The design of SO allows vertical sampling typically 1 km. Its high spectral resolution (λ/∆λ∼17000) its relatively signal noise ratio (∼2500), make...

10.5194/egusphere-egu25-11667 preprint EN 2025-03-14

Suspended aerosols may have a direct impact in atmospheric processes, such as photochemical reactions and radiative balance dynamics. On Mars, the most common are composed of mineral dust particles and/or water ice. This last one is known to affect both [2] cycle [1], whereas suspended prevalent aerosol component on planet.The instrument Nadir Occultation for Mars Discovery (NOMAD) suite three spectrometers board Trace Gas Orbiter (TGO) which has been observing Martian atmosphere routinely...

10.5194/egusphere-egu25-12204 preprint EN 2025-03-15

The ExoMars Trace Gas Orbiter (TGO) mission is a joint venture of the space agencies ESA and ROSCOSMOS which was launched in 2016 carries onboard instruments dedicated to studying trace gas compositions Martian atmosphere. NOMAD (Nadir Occultation for MArs Discovery) one such instrument that housed three observing channels named UVIS (the Ultra Violet Visible Spectrometer), LNO (Limb Nadir Occultation) SO (Solar scan atmosphere nadir limb geometries [1]. channel operates IR (Infra-Red)...

10.5194/epsc2024-1120 preprint EN 2024-07-03

NOMAD [1] (Nadir and Occultation for MArs Discovery) is a multi-channel spectrometer onboard the ExoMars 2016 Trace Gas Orbiter (TGO), which began its observations in April 2018. Among other two (LNO UVIS), Solar (SO) channel covers infrared (IR) spectrum from 2.3 to 4.3 µm (2320 4350 cm-1). Composed of an echelle grating Litrow configuration, total 6 diffraction orders (with typical width 20 35 cm-1) are selected during each solar occultation using Acousto-Optical Tunable Filter...

10.5194/epsc2024-1125 preprint EN 2024-07-03

The characterization of the thermal structure Martian atmosphere with unprecendented vertical resolution is one goals ESA and Roscosmos Exomars Trace Gas Orbiter (TGO) [1]. This can be achieved two solar occultation instruments, NOMAD [2] ACS [3], whose ultimate goal to sound temperature density from Mars' lowermost atmospheric layers up thermosphere. Both instrumetns are synergistic complementary, in particular, SO channel NIR MIR spectrometers instrument exploit a number strong CO2...

10.5194/epsc2024-1033 preprint EN 2024-07-03

 1.     The importance of studying lunar dust particlesInternational scientific and commercial interests in exploration missions to solar system bodies such as the Moon, asteroids comets have increased significantly during last two decades will continue increase future. One major environmental constraint is presence charged dust-like particles. They can be a threat for both human robotic missions.The effects on Extra-Vehicular Activity systems...

10.5194/epsc2024-923 preprint EN 2024-07-03

NOMAD [1] (Nadir and Occultation for MArs Discovery) is a multi-channel spectrometer onboard the ExoMars 2016 Trace Gas Orbiter (TGO), which began its observations in April 2018. Among other two (LNO UVIS), Solar (SO) channel covers infrared (IR) spectrum from 2.3 to 4.3 µm (2320 4350 cm-1). Composed of an echelle grating Litrow configuration, total 6 diffraction orders (with typical width 20 35 cm-1) are selected during each solar occultation using Acousto-Optical Tunable Filter...

10.5194/epsc2024-1018 preprint EN 2024-07-03

Our knowledge of the temperature structure in upper atmosphere Mars (understood here as mesosphere/thermosphere, layers between ~80 and 200 km altitude from surface) has significantly improved last decade thanks to data provided by MAVEN/NASA, Express/ESA, ExoMars-TGO/ESA missions [e.g. 1, 2, 3]. However, aspects such variation temperatures with local time or latitude are still poorly characterized due sampling limitation different instruments, rely mostly on information Global Climate...

10.5194/epsc2024-955 preprint EN 2024-07-03

The Spacecraft INterface and control Board for NomAD (SINBAD) is an electronic interface designed by the Instituto de Astroffisica Andalucfia (IAA-CSIC). It part of Nadir Occultation MArs Discovery instrument (NOMAD) on board in ESAs ExoMars Trace Gas Orbiter mission. This mission was launched March 2016. SINBAD Flight Software (SFS) software embedded SINBAD. charge managing interfaces, devices, data, observing sequences, patching contingencies NOMAD. presented this paper most remarkable...

10.1117/12.2230760 article EN Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE 2016-07-26

NOMAD is a spectrometer suite: UV-visible-IR spectral ranges. part of the payload ESA ExoMars Trace Gas Orbiter Mission. SINBAD boards are in charge communication and management power control between spacecraft instrument channels. development took four years, while entire test required five very short time to develop an devoted space mission. The hardware shown attached poster: developed boards, prototype final models. models were delivered order testing integration with spacecraft.

10.1117/12.2233353 article EN Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE 2016-07-29

Short pulsed laser sources have recently been under investigation for applications in high speed optical communications systems. Studies concerning short pulse based on Gain Switching techniques and compression devices made. Nonlinear Optical Loop Mirrors (NOLM) provide both reshaping of the pulses. As achieved widths become shorter, timing jitter becomes crucial. The present work turns attention to influence performance NOLM device. results obtained will be basis design a compact quality...

10.1117/12.652306 article EN Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE 2006-02-09
Coming Soon ...