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- Corpolongo, A., et al.
(författare)
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SHERLOC Raman Mineral Class Detections of the Mars 2020 Crater Floor Campaign
- 2023
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Ingår i: Journal of Geophysical Research - Planets. - : John Wiley and Sons Inc. - 2169-9097 .- 2169-9100. ; 128:3
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Tidskriftsartikel (refereegranskat)abstract
- The goals of NASA's Mars 2020 mission include searching for evidence of ancient life on Mars, studying the geology of Jezero crater, understanding Mars' current and past climate, and preparing for human exploration of Mars. During the mission's first science campaign, the Perseverance rover's SHERLOC deep UV Raman and fluorescence instrument collected microscale, two-dimensional Raman and fluorescence images on 10 natural (unabraded) and abraded targets on two different Jezero crater floor units: Séítah and Máaz. We report SHERLOC Raman measurements collected during the Crater Floor Campaign and discuss their implications regarding the origin and history of Séítah and Máaz. The data support the conclusion that Séítah and Máaz are mineralogically distinct igneous units with complex aqueous alteration histories and suggest that the Jezero crater floor once hosted an environment capable of supporting microbial life and preserving evidence of that life, if it existed.
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- Neff, Curtis W., et al.
(författare)
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Coupled resonator optical waveguide structures with highly dispersive media
- 2006
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Ingår i: Optoeletronic Materials and Devices, Pts 1 and 2. - BELLINGHAM, WA : SPIE-INT SOC OPTICAL ENGINEERING. - 0819464473 ; , s. U316-U324
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Konferensbidrag (refereegranskat)abstract
- Enhanced slow light propagation is predicted in a coupled resonator optical waveguide structure possessing highly dispersive elements using the finite-difference time-domain method. The group velocity is shown to be below 0.01c(0).
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- Edgeman, Rick, et al.
(författare)
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On Leaders and Leadership
- 1999
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Ingår i: Quality Progress. ; :October issue, s. 49-54
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Tidskriftsartikel (refereegranskat)
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- Way, Michael J., et al.
(författare)
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Large-scale Volcanism and the Heat Death of Terrestrial Worlds
- 2022
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Ingår i: The Planetary Science Journal. - : Institute of Physics (IOP). - 2632-3338. ; 3:4
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Tidskriftsartikel (refereegranskat)abstract
- Large-scale volcanism has played a critical role in the long-term habitability of Earth. Contrary to widely held belief, volcanism, rather than impactors, has had the greatest influence on and bears most of the responsibility for large-scale mass extinction events throughout Earth's history. We examine the timing of large igneous provinces (LIPs) throughout Earth's history to estimate the likelihood of nearly simultaneous events that could drive a planet into an extreme moist or runaway greenhouse, leading to the end of volatile cycling and causing the heat death of formerly temperate terrestrial worlds. In one approach, we make a conservative estimate of the rate at which sets of near-simultaneous LIPs (pairs, triplets, and quartets) occur in a random history statistically the same as Earth's. We find that LIPs closer in time than 0.1-1 million yr are likely; significantly, this is less than the time over which terrestrial LIP environmental effects are known to persist. In another approach, we assess the cumulative effects with simulated time series consisting of randomly occurring LIP events with realistic time profiles. Both approaches support the conjecture that environmental impacts of LIPs, while narrowly avoiding grave effects on the climate history of Earth, could have been responsible for the heat death of our sister world Venus.
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- Bjereld, Ylva, 1984, et al.
(författare)
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The association between self-reported psychosomatic complaints and bullying victimisation and disability among adolescents in Finland and Sweden
- 2023
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Ingår i: Scandinavian Journal of Public Health. - : SAGE Publications. - 1403-4948 .- 1651-1905. ; 51:8, s. 1136-1143
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Tidskriftsartikel (refereegranskat)abstract
- Aim: To analyse the associations between bullying victimisation, disability, and self-reported psychosomatic complaints in adolescents, and to investigate the role of support from parents and teachers in such associations. Methods: The study was based on Finnish and Swedish data from two waves (2013/2014 and 2017/2018) of the Health Behaviour in School-aged Children survey (n=16,057). Descriptive statistics were produced for four groups of adolescents: (a) bullied with disabilities; (b) not bullied with disabilities; (c) bullied without disabilities; and (d) not bullied without disabilities (reference group). Two multilevel multinomial logistic regression models were performed for the Finnish and Swedish samples separately. The first model analysed associations between psychosomatic complaints and bullying victimisation, controlling for a range of confounders. The second model analysed associations between psychosomatic complaints and social support from parents and teachers. Results: Across both countries, bullied adolescents with disabilities were more likely to self-report psychosomatic complaints than the reference group, even after adjusting for other potential confounders. Teacher support was identified as a potential protective factor as the odds ratio for psychosomatic complaints decreased when including teacher support as a factor in the model. The association with parent support showed mixed findings in Finland and Sweden. Conclusions: Disability in combination with bullying victimisation generated the highest levels of self-reported psychosomatic complaints compared to adolescents that were not bullied nor had disabilities. High teacher support may be a protective factor against psychosomatic complaints for bullied and/or disabled adolescents.
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- Bonfanti, A., et al.
(författare)
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CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii
- 2021
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 646
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Tidskriftsartikel (refereegranskat)abstract
- Context. The detection of a super-Earth and three mini-Neptunes transiting the bright (V = 9.2 mag) star HD 108236 (also known as TOI-1233) was recently reported on the basis of TESS and ground-based light curves. Aims. We perform a first characterisation of the HD 108236 planetary system through high-precision CHEOPS photometry and improve the transit ephemerides and system parameters. Methods. We characterise the host star through spectroscopic analysis and derive the radius with the infrared flux method. We constrain the stellar mass and age by combining the results obtained from two sets of stellar evolutionary tracks. We analyse the available TESS light curves and one CHEOPS transit light curve for each known planet in the system. Results. We find that HD 108236 is a Sun-like star with R? = 0.877 ± 0.008 R? , M? = 0.869-0.048+0.050 M? , and an age of 6.7-5.1+4.0 Gyr. We report the serendipitous detection of an additional planet, HD 108236 f, in one of the CHEOPS light curves. For this planet, the combined analysis of the TESS and CHEOPS light curves leads to a tentative orbital period of about 29.5 days. From the light curve analysis, we obtain radii of 1.615 ± 0.051, 2.071 ± 0.052, 2.539-0.065+0.062, 3.083 ± 0.052, and 2.017-0.057+0.052 R? for planets HD 108236 b to HD 108236 f, respectively. These values are in agreement with previous TESS-based estimates, but with an improved precision of about a factor of two. We perform a stability analysis of the system, concluding that the planetary orbits most likely have eccentricities smaller than 0.1. We also employ a planetary atmospheric evolution framework to constrain the masses of the five planets, concluding that HD 108236 b and HD 108236 c should have an Earth-like density, while the outer planets should host a low mean molecular weight envelope. Conclusions. The detection of the fifth planet makes HD 108236 the third system brighter than V = 10 mag to host more than four transiting planets. The longer time span enables us to significantly improve the orbital ephemerides such that the uncertainty on the transit times will be of the order of minutes for the years to come. A comparison of the results obtained from the TESS and CHEOPS light curves indicates that for a V - 9 mag solar-like star and a transit signal of -500 ppm, one CHEOPS transit light curve ensures the same level of photometric precision as eight TESS transits combined, although this conclusion depends on the length and position of the gaps in the light curve.
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