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1.
Life Sci Space Res (Amst) ; 39: 26-42, 2023 Nov.
Artigo em Inglês | MEDLINE | ID: mdl-37945086

RESUMO

The Light Ion Detector for ALTEA (LIDAL) is a new instrument designed to measure flux, energy spectra and Time of Flight of ions in a space habitat. It was installed in the International Space Station (Columbus) on January 19, 2020 and it is still operating. This paper presents the results of LIDAL measurements in the first 17 months of operation (01/2020-05/2022). Particle flux, dose rate, Time of Flight and spectra are presented and studied in the three ISS orthogonal directions and in the different geomagnetic regions (high latitude, low latitude, and South Atlantic Anomaly, SAA). The results are consistent with previous measurements. Dose rates range between 1.8 nGy/s and 2.4 nGy/s, flux between 0.21 particles/(sr cm2 s) and 0.32 particles/(sr cm2 s) as measured across time and directions during the full orbit. These data offer insights concerning the radiation measurements in the ISS and demonstrate the capabilities of LIDAL as a unique tool for the measurement of space radiation in space habitats, also providing novel information relevant to assess radiation risks for astronauts.


Assuntos
Radiação Cósmica , Monitoramento de Radiação , Voo Espacial , Astronave , Atividade Solar , Monitoramento de Radiação/métodos , Doses de Radiação , Íons
2.
Phys Rev Lett ; 104(24): 241601, 2010 Jun 18.
Artigo em Inglês | MEDLINE | ID: mdl-20867292

RESUMO

The possibility of anisotropies in the speed of light relative to the limiting speed of electrons is considered. The absence of sidereal variations in the energy of Compton-edge photons at the European Synchrotron Radiation Facility's GRAAL facility constrains such anisotropies representing the first nonthreshold collision-kinematics study of Lorentz violation. When interpreted within the minimal standard-model extension, this result yields the two-sided limit of 1.6×10(-14) at 95% confidence level on a combination of the parity-violating photon and electron coefficients (κ(o+))(YZ), (κ(o+))(ZX), c(TX), and c(TY). This new constraint provides an improvement over previous bounds by 1 order of magnitude.

3.
Phys Rev B Condens Matter ; 36(16): 8285-8287, 1987 Dec 01.
Artigo em Inglês | MEDLINE | ID: mdl-9942639
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