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Journal articles on the topic 'Rosina'

Author: Grafiati

Published: 4 June 2021

Last updated: 19 February 2022

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1

Colaianni, Louis. "InterviewInterview with Rosina Lippy-Green." Voice and Speech Review 1, no. 1 (2000): 21–22. http://dx.doi.org/10.1080/23268263.2000.10761383.

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2

McLamore, Alyson. "Rosina: A Comic Opera (1782) (review)." Notes 57, no. 4 (2001): 993–97. http://dx.doi.org/10.1353/not.2001.0100.

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3

Beth, A., K. Altwegg, H. Balsiger, et al. "ROSINA ion zoo at Comet 67P." Astronomy & Astrophysics 642 (September 30, 2020): A27. http://dx.doi.org/10.1051/0004-6361/201936775.

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Context. The Rosetta spacecraft escorted Comet 67P/Churyumov-Gerasimenko for 2 yr along its journey through the Solar System between 3.8 and 1.24 au. Thanks to the high resolution mass spectrometer on board Rosetta, the detailed ion composition within a coma has been accurately assessed in situ for the very first time. Aims. Previous cometary missions, such as Giotto, did not have the instrumental capabilities to identify the exact nature of the plasma in a coma because the mass resolution of the spectrometers onboard was too low to separate ion species with similar masses. In contrast, the Double Focusing Mass Spectrometer (DFMS), part of the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis on board Rosetta (ROSINA), with its high mass resolution mode, outperformed all of them, revealing the diversity of cometary ions. Methods. We calibrated and analysed the set of spectra acquired by DFMS in ion mode from October 2014 to April 2016. In particular, we focused on the range from 13–39 u q−1. The high mass resolution of DFMS allows for accurate identifications of ions with quasi-similar masses, separating 13C+ from CH+, for instance. Results. We confirm the presence in situ of predicted cations at comets, such as CHm+ (m = 1−4), HnO+ (n = 1−3), O+, Na+, and several ionised and protonated molecules. Prior to Rosetta, only a fraction of them had been confirmed from Earth-based observations. In addition, we report for the first time the unambiguous presence of a molecular dication in the gas envelope of a Solar System body, namely CO2++.

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4

Barashkov, V. V. "DOCTOR ROSINA NEYMANN: SEMINARS OF INTERCULTURAL COMMUNICATION." Concept: philosophy, religion, culture 3 (2018): 192–94. http://dx.doi.org/10.24833/2541-8831-2018-3-7-192-194.

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5

Besharov, Douglas J. "Response to Deborah Daro and Rosina Becerra." Children and Youth Services Review 13, no. 4 (1991): 306–9. http://dx.doi.org/10.1016/0190-7409(91)90068-s.

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6

Lanne, Jean-Claude. "Rosina Neginsky Symbolism, its origins and its consequences." Revue des études slaves 84, no. 3-4 (2013): 570–75. http://dx.doi.org/10.4000/res.1198.

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7

Duarte, Rosina, and Dermeval Saviani. "Entrevista com Prof. Dermeval Savani a Rosina Duarte." ETD - Educação Temática Digital 2, no. 3 (2009): 143. http://dx.doi.org/10.20396/etd.v2i3.588.

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8

Weldon C. Matthews. "Arab Americans in Michigan by Rosina J. Hassoun." Michigan Historical Review 36, no. 1 (2010): 134–35. http://dx.doi.org/10.1353/mhr.2010.0018.

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9

Blain, Virginia. "Rosina Bulwer Lytton and the Rage of the Unheard." Huntington Library Quarterly 53, no. 3 (1990): 211–36. http://dx.doi.org/10.2307/3817439.

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10

Balsiger, H., K. Altwegg, E. Arijs, et al. "Rosetta Orbiter Spectrometer for Ion and Neutral Analysis—ROSINA." Advances in Space Research 21, no. 11 (1998): 1527–35. http://dx.doi.org/10.1016/s0273-1177(97)00945-9.

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11

Derosas, Renzo. "Reply to the note by Dalla-Zuanna and Rosina." Population Studies 64, no. 2 (2010): 197–98. http://dx.doi.org/10.1080/00324721003770815.

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12

MCDONELL, JENNIFER, and ROBERT DINGLEY. "L. E. L. AND ROSINA BULWER: AN UNPUBLISHED LETTER." Notes and Queries 44, no. 3 (1997): 332–33. http://dx.doi.org/10.1093/nq/44-3-332.

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13

MCDONELL, JENNIFER, and ROBERT DINGLEY. "L. E. L. AND ROSINA BULWER: AN UNPUBLISHED LETTER." Notes and Queries 44, no. 3 (1997): 332–33. http://dx.doi.org/10.1093/nq/44.3.332.

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14

Sypher, Francis. "The Collected Letters of Rosina Bulwer Lytton (3 vols.)." Women's Writing 16, no. 2 (2009): 348–52. http://dx.doi.org/10.1080/09699080903016748.

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15

De Keyser, J., F. Dhooghe, A. Gibbons, et al. "Correcting peak deformation in Rosetta's ROSINA/DFMS mass spectrometer." International Journal of Mass Spectrometry 393 (December 2015): 41–51. http://dx.doi.org/10.1016/j.ijms.2015.10.010.

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16

Balsiger, H., K. Altwegg, P. Bochsler, et al. "Rosina – Rosetta Orbiter Spectrometer for Ion and Neutral Analysis." Space Science Reviews 128, no. 1-4 (2007): 745–801. http://dx.doi.org/10.1007/s11214-006-8335-3.

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17

Sonnenschmidt, Rosina. "Niemand ist nur krank." Deutsche Heilpraktiker-Zeitschrift 12, no. 04 (2017): 24–28. http://dx.doi.org/10.1055/s-0043-112690.

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SummarySeit vielen Jahren begleitet Rosina Sonnenschmidt Patienten mit Krebs. Aus all den Erfahrungen, die sie dabei gewonnen hat, hat sie ein Behandlungskonzept abgeleitet. Neben der Miasmatik stellt sie dabei den Patienten mit seiner Individualität in den Mittelpunkt und aktiviert seine Potenziale. Sie fordert zudem Eigeninitiative von ihm, denn das eigene Tun und die Eigenverantwortung braucht es, um in den Heilungsprozess zu gelangen.

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18

Hoang, M., P. Garnier, J. Lasue, et al. "Investigating the Rosetta/RTOF observations of comet 67P/Churyumov-Gerasimenko using a comet nucleus model: influence of dust mantle and trapped CO." Astronomy & Astrophysics 638 (June 2020): A106. http://dx.doi.org/10.1051/0004-6361/201936655.

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Context. Cometary outgassing is induced by the sublimation of ices and the ejection of dust originating from the nucleus. Therefore measuring the composition and dynamics of the cometary gas provides information concerning the interior composition of the body. Nevertheless, the bulk composition differs from the coma composition, and numerical models are required to simulate the main physical processes induced by the illumination of the icy body. Aims. The objectives of this study are to bring new constraints on the interior composition of the nucleus of comet 67P/Churyumov-Gerasimenko (hereafter 67P) by comparing the results of a thermophysical model applied to the nucleus of 67P and the coma measurements made by the Reflectron-type Time-Of-Flight (RTOF) mass spectrometer. This last is one of the three instruments of the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA), used during the Rosetta mission. Methods. Using a thermophysical model of the comet nucleus, we studied the evolution of the stratigraphy (position of the sublimation and crystallisation fronts), the temperature of the surface and subsurface, and the dynamics and spatial distribution of the volatiles (H2O, CO2 and CO). We compared them with the in situ measurements from ROSINA/RTOF and an inverse coma model. Results. We observed the evolution of the surface and near surface temperature, and the deepening of sublimation fronts. The thickness of the dust layer covering the surface strongly influences the H2O outgassing but not the more volatiles species. The CO outgassing is highly sensitive to the initial CO/H2O ratio, as well as to the presence of trapped CO in the amorphous ice. Conclusions. The study of the influence of the initial parameters on the computed volatile fluxes and the comparison with ROSINA/RTOF measurements provide a range of values for an initial dust mantle thickness and a range of values for the volatile ratio. These imply the presence of trapped CO. Nevertheless, further studies are required to reproduce the strong change of behaviour observed in RTOF measurements between September 2014 and February 2015.

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19

NAIDITCH, FERNANDO. "Spanish PragmaticsEdited by MÁRQUEZ REITER, ROSINA, & MARÍA ELENA PLACENCIA." Modern Language Journal 91, no. 1 (2007): 143–44. http://dx.doi.org/10.1111/j.1540-4781.2007.00514_20.x.

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20

Bombara, Daniela. "L’'amour fou' tra spaesamento e straniamento in due scrittrici siciliane: Rosina Muzio Salvo e Cettina Natoli." Incontri. Rivista europea di studi italiani 36, no. 1 (2021): 75–90. http://dx.doi.org/10.18352/inc11008.

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Amour fou between displacement and estrangement in two Sicilian writers of the Nineteenth Century Rosina Muzio Salvo and Cettina Natoli This research aims at investigating the topos of love as deep and extreme passion, in opposition to social stereotypes, in two novels by two Sicilian female writers of the Nineteenth Century, Adelina (1845) by Rosina Muzio Salvo (1815-1866) and Margherita Royn (1886) by Cettina Natoli (1867-1913). In Adelina amour fou is in conflict with the patriotic needs and the moralism of the newborn middle-class society; in Margherita Royn, an overliterary, different kind of love clashes with the materialism and commercialization which dominate in late Nineteenth century. Adelina’s displacement is highlighted by the structure of the polyphonic epistolary novel, in which the protagonist’s ‘reasons of the heart’ are opposed to the opinions of all the other characters; according to a process of Verghian estrangement (Luperini, 1974), they convey a distorted picture of her passion and consider it a weird, unacceptable fact. Margherita is able to see reality only through an overly literary lens of extreme sentimentality; her isolation is manifest in the depiction of her body, consumed by an adulterous passion which contrasts with her husband’s rough physicality; overcome by jealousy, he will end up killing her.

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21

Meng, Ziye, Chaoliang Lei, Xiaoqin Chen, and Shihong Jiang. "Complete mitochondrial genome sequence of Heliconius melpomene rosina (Insecta: Lepidoptera: Nymphalidae)." Mitochondrial DNA Part A 27, no. 6 (2014): 3911–12. http://dx.doi.org/10.3109/19401736.2014.987261.

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22

Luspay-Kuti, A., M. Hässig, S. A. Fuselier, et al. "Composition-dependent outgassing of comet 67P/Churyumov-Gerasimenko from ROSINA/DFMS." Astronomy & Astrophysics 583 (October 30, 2015): A4. http://dx.doi.org/10.1051/0004-6361/201526205.

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23

Cruickshank, D. W. J. "Sir Ernest Gordon Cox, K.B.E. 24 April 1906 — 23 June 1996." Biographical Memoirs of Fellows of the Royal Society 46 (January 2000): 65–84. http://dx.doi.org/10.1098/rsbm.1999.0074.

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Gordon Cox, who died in 1996 at the age of 90, had two distinct careers. The first, as a crystallographer and structural chemist, lasted from 1927, when he joined Sir William Bragg's group at the Royal Institution, to 1960, when he left the University of Leeds. He was a pioneer of three-dimensional methods in X-ray structure analysis. From 1960 to 1971 he was the highly regarded secretary of the Agricultural Research Council. Cox was born on 24 April 1906 at Pretoria Cottage, Southdown, Twerton, in Somerset, where his father was a market gardener. Three years later his sister Christine was born. A third child, Kenneth, died in infancy. His father, Ernest Henry Cox, was born in 1884. He outlived two wives, married a third in 1941 and died in 1987 at the age of 103. Gordon's mother, Rosina Ring, was twelve years older than his father. They had married at Claverton, near Bath, on 29 April 1905. Rosina, one of many children of a chef, had been sent with two of her siblings to Canada to work on a farm in Ontario in the 1880s. She returned in 1895, and her son Herbert Moffat was born on her return to England. Gordon's family consisted of this elder half-brother, whom he worshipped, and the younger sister, with whom he often quarrelled. His mother often told him of the harsh life in Canada but she had also had some enjoyment there. She died in 1931.

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24

Carey, Christian. "Bennett - Bennett: Togetherness. Barbara Lueneburg (vln); Decibel, Daniele Rosina (cond). Diatribe, 2018." Tempo 72, no. 286 (2018): 91–93. http://dx.doi.org/10.1017/s0040298218000499.

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25

Rubin, Martin, Kathrin Altwegg, Annette Jäckel, and Hans Balsiger. "Development of a low energy ion source for ROSINA ion mode calibration." Review of Scientific Instruments 77, no. 10 (2006): 103302. http://dx.doi.org/10.1063/1.2358708.

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26

Chestang, Leon W. "Social Services and the Ethnic Community. Alfreda P. Iglehart , Rosina M. Becerra." Social Service Review 70, no. 3 (1996): 493–94. http://dx.doi.org/10.1086/604206.

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27

Schuhmann, M., K. Altwegg, H. Balsiger, et al. "Aliphatic and aromatic hydrocarbons in comet 67P/Churyumov-Gerasimenko seen by ROSINA." Astronomy & Astrophysics 630 (September 20, 2019): A31. http://dx.doi.org/10.1051/0004-6361/201834666.

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Context. Unlike all previous cometary space missions, the Rosetta spacecraft accompanied its target, comet 67P/Churyumov-Gerasimenko, for more than two years on its way around the Sun. Thereby, an unexpected diversity and complexity of the chemical composition was revealed. Aims. Our first step of decrypting the exact chemical composition of the gaseous phase is the identifying and quantifying the bulk composition of the pure aromatic and aliphatic hydrocarbons. Methods. For this study, data from ROSINA–Double Focusing Mass Spectrometer (DFMS) onboard the Rosetta spacecraft and the laboratory twin model were used. A joint campaign of laboratory calibration measurements and space data analysis was performed to derive the hydrocarbon bulk composition for the post-inbound equinox period at 1.52 AU in May 2015. Furthermore, several other mission phases were investigated to determine the dependencies of season, location, and heliocentric distance on the relative abundances of hydrocarbons. Results. It is shown that the bulk composition of the gaseous phase includes a high number of aliphatic compounds such as methane, ethane, and propane, as well as the aromatic compounds benzene and toluene. Butane and pentane were successfully identified in measurements at closer distance to the comet in May 2016. Furthermore, the presence of hexane and heptane in the coma is confirmed on rare occasions during the mission. Their presence in DFMS space data appears to be linked to days or periods of high dust activity. In addition to the saturated aliphatic and aromatic compounds, a high number of remaining unsaturated species is present, which cannot be explained by fragmentation of saturated species or contribution from other organic molecules in addition to pure hydrocarbons. This indicates the existence of unsaturated aliphatic and aromatic hydrocarbon molecules in the coma of comet 67P.

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28

Le Roy, Léna, Kathrin Altwegg, Hans Balsiger, et al. "Inventory of the volatiles on comet 67P/Churyumov-Gerasimenko from Rosetta/ROSINA." Astronomy & Astrophysics 583 (October 30, 2015): A1. http://dx.doi.org/10.1051/0004-6361/201526450.

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29

De Keyser, J., K. Altwegg, A. Gibbons, et al. "Position-dependent microchannel plate gain correction in Rosetta's ROSINA/DFMS mass spectrometer." International Journal of Mass Spectrometry 446 (December 2019): 116232. http://dx.doi.org/10.1016/j.ijms.2019.116232.

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30

Zamir, Sara. "Deciphering the Code Rosina: Gesture, Gender, Genre in Una voce poco fa." Studia Musicologica Norvegica 38, no. 01 (2012): 32–45. http://dx.doi.org/10.18261/issn1504-2960-2012-01-03.

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31

Zakharov, V. V., J. F. Crifo, A. V. Rodionov, M. Rubin, and K. Altwegg. "The near-nucleus gas coma of comet 67P/Churyumov-Gerasimenko prior to the descent of the surface lander PHILAE." Astronomy & Astrophysics 618 (October 2018): A71. http://dx.doi.org/10.1051/0004-6361/201832883.

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Context. The European Space Agency (ESA) Rosetta mission was the most comprehensive study of a comet ever performed. In particular, the Rosetta orbiter, which carried many instruments for monitoring the evolution of the dusty gas emitted by the cometary nucleus, returned an enormous volume of observational data collected from the close vicinity of the nucleus of comet 67P/Churyumov-Gerasimenko. Aims. Such data are expected to yield unique information on the physical processes of gas and dust emission, using current physical model fits to the data. We present such a model (the RZC model) and our procedure of adjustment of this model to the data. Methods. The RZC model consists of two components: (1) a numerical three-dimensional time-dependent code solving the Eulerian/Navier-Stokes equations governing the gas outflow, and a direct simulation Monte Carlo (DSMC) gaskinetic code with the same objective; and (2) an iterative procedure to adjust the assumed model parameters to best-fit the observational data at all times. Results. We demonstrate that our model is able to reproduce the overall features of the local neutral number density and composition measurements of Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) Comet Pressure Sensor (COPS) and Double Focusing Mass Spectrometer (DFMS) instruments in the period August 1–November 30, 2014. The results of numerical simulations show that illumination conditions on the nucleus are the main driver for the gas activity of the comet. We present the distribution of surface inhomogeneity best-fitted to the ROSINA COPS and DFMS in situ measurements.

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32

Luspay-Kuti, A., K. Altwegg, J. J. Berthelier, et al. "Comparison of neutral outgassing of comet 67P/Churyumov-Gerasimenko inbound and outbound beyond 3 AU from ROSINA/DFMS." Astronomy & Astrophysics 630 (September 20, 2019): A30. http://dx.doi.org/10.1051/0004-6361/201833536.

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Context. Pre-equinox measurements of comet 67P/Churyumov-Gerasimenko with the mass spectrometer ROSINA/DFMS on board the Rosetta spacecraft revealed a strongly heterogeneous coma. The abundances of major and various minor volatile species were found to depend on the latitude and longitude of the nadir point of the spacecraft. The observed time variability of coma species remained consistent for about three months up to equinox. The chemical variability could be generally interpreted in terms of surface temperature and seasonal effects superposed on some kind of chemical heterogeneity of the nucleus. Aims. We compare here pre-equinox (inbound) ROSINA/DFMS measurements from 2014 to measurements taken after the outbound equinox in 2016, both at heliocentric distances larger than 3 AU. For a direct comparison we limit our observations to the southern hemisphere. Methods. We report the similarities and differences in the concentrations and time variability of neutral species under similar insolation conditions (heliocentric distance and season) pre- and post-equinox, and interpret them in light of the previously published observations. In addition, we extend both the pre- and post-equinox analysis by comparing species concentrations with a mixture of CO2 and H2O. Results. Our results show significant changes in the abundances of neutral species in the coma from pre- to post-equinox that are indicative of seasonally driven nucleus heterogeneity. Conclusions. The observed pre- and post-equinox patterns can generally be explained by the strong erosion in the southern hemisphere that moves volatile-rich layers near the surface.

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33

Drozdovskaya, Maria N., Isaac R. H. G. Schroeder I, Martin Rubin, et al. "Prestellar grain-surface origins of deuterated methanol in comet 67P/Churyumov–Gerasimenko." Monthly Notices of the Royal Astronomical Society 500, no. 4 (2020): 4901–20. http://dx.doi.org/10.1093/mnras/staa3387.

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ABSTRACT Deuterated methanol is one of the most robust windows astrochemists have on the individual chemical reactions forming deuterium-bearing molecules and the physicochemical history of the regions where they reside. The first-time detection of mono- and di-deuterated methanol in a cometary coma is presented for comet 67P/Churyumov–Gerasimenko using Rosetta–ROSINA data. D-methanol (CH3OD and CH2DOH combined) and D2-methanol (CH2DOD and CHD2OH combined) have an abundance of 5.5 ± 0.46 and 0.00069 ± 0.00014 per cent relative to normal methanol. The data span a methanol deuteration fraction (D/H ratio) in the 0.71−6.6 per cent range, accounting for statistical corrections for the location of D in the molecule and including statistical error propagation in the ROSINA measurements. It is argued that cometary CH2DOH forms from CO hydrogenation to CH3OH and subsequent H–D substitution reactions in CH3–R. CHD2OH is likely produced from deuterated formaldehyde. Meanwhile, CH3OD and CH2DOD could form via H–D exchange reactions in OH–R in the presence of deuterated water ice. Methanol formation and deuteration is argued to occur at the same epoch as D2O formation from HDO, with formation of mono-deuterated water, hydrogen sulphide, and ammonia occurring prior to that. The cometary D-methanol/methanol ratio is demonstrated to agree most closely with that in prestellar cores and low-mass protostellar regions. The results suggest that cometary methanol stems from the innate cold (10–20 K) prestellar core that birthed our Solar system. Cometary volatiles individually reflect the evolutionary phases of star formation from cloud to core to protostar.

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34

Mora Ordóñez, Edith. "Cartas y viajes de ida y vuelta: diálogos bifronterizos en las novelas epistolares de Ana Castillo y Rosina Conde." Literatura y Lingüística, no. 38 (October 13, 2018): 103. http://dx.doi.org/10.29344/0717621x.38.1627.

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El presente estudio propone la comparación biborderlands o bifronteriza de dos novelas epistolares escritas desde ambos lados de la frontera México-Estados Unidos: Las cartas de Mixquiahuala (1986), de la chicana Ana Castillo, y La Genara (1998), de la mexicana Rosina Conde. El diálogo a través de las cartas en dichas obras constituye un encuentro especular que permite a las mujeres desdoblarse y mirarse a sí mismas. Desde las dos fronteras comparten experiencias de ruptura de las estructuras dominantes familiares, masculinas y patriarcales. La conversación epistolar incide en un proceso autoreflexivo, de reconocimiento y conformación de nuevas identidades y subjetividades femeninas.

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35

Rivilla, V. M., M. N. Drozdovskaya, K. Altwegg, et al. "ALMA and ROSINA detections of phosphorus-bearing molecules: the interstellar thread between star-forming regions and comets." Monthly Notices of the Royal Astronomical Society 492, no. 1 (2020): 1180–98. http://dx.doi.org/10.1093/mnras/stz3336.

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ABSTRACT To understand how phosphorus (P)-bearing molecules are formed in star-forming regions, we have analysed the Atacama Large Millimeter/Submillimeter Array (ALMA) observations of PN and PO towards the massive star-forming region AFGL 5142, combined with a new analysis of the data of the comet 67P/Churyumov–Gerasimenko taken with the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) instrument onboard Rosetta. The ALMA maps show that the emission of PN and PO arises from several spots associated with low-velocity gas with narrow linewidths in the cavity walls of a bipolar outflow. PO is more abundant than PN in most of the spots, with the PO/PN ratio increasing as a function of the distance to the protostar. Our data favour a formation scenario in which shocks sputter phosphorus from the surface of dust grains, and gas-phase photochemistry induced by UV photons from the protostar allows efficient formation of the two species in the cavity walls. Our analysis of the ROSINA data has revealed that PO is the main carrier of P in the comet, with PO/PN &gt; 10. Since comets may have delivered a significant amount of prebiotic material to the early Earth, this finding suggests that PO could contribute significantly to the phosphorus reservoir during the dawn of our planet. There is evidence that PO was already in the cometary ices prior to the birth of the Sun, so the chemical budget of the comet might be inherited from the natal environment of the Solar system, which is thought to be a stellar cluster including also massive stars.

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36

Khaldi, Boutheina. "Rosina-Fawzia al-Rawi,Midnight Tales: A Woman's Journey Through the Middle East." Journal of Middle East Women's Studies 3, no. 2 (2007): 118–19. http://dx.doi.org/10.2979/mew.2007.3.2.118.

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37

Guzmán Valerio, Luis. "Rosina Lozano. An American Language: The History of Spanish in the United States." Spanish in Context 16, no. 2 (2019): 314–21. http://dx.doi.org/10.1075/sic.00040.guz.

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38

Vélez-Ibáñez, Carlos G. "Rosina Lozano. An American Language: The History of Spanish in the United States." American Historical Review 125, no. 5 (2020): 1797–98. http://dx.doi.org/10.1093/ahr/rhz1273.

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39

Knowles, Scott C. "Embodied Consciousness: Performance Technologies ed. by Jade Rosina McCutcheon and Barbara Sellers-Young." Theatre History Studies 35, no. 1 (2016): 346–48. http://dx.doi.org/10.1353/ths.2016.0025.

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40

Гиппиус, Зинаида. "Письма к Софье Григорьевне Балашовской-Пети (Комментарии и подготовка к публикации Rosina Neginsky)". Russian Literature 37, № 1 (1995): 59–91. http://dx.doi.org/10.1016/0304-3479(95)91128-c.

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41

Ondruš, Ján, and Peter Hockicko. "Braking Deceleration Measurement Using the Video Analysis of Motions by Sw Tracker." Transport and Telecommunication Journal 16, no. 2 (2015): 127–37. http://dx.doi.org/10.1515/ttj-2015-0012.

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Abstract This contribution deals with the issue of car braking, particularly with the one of M1 category. Braking deceleration measurement of the vehicle Mazda 3 MPS was carried out by the declerograph XL MeterTM Pro. The main aim of the contribution is to perform comparison of the process of braking deceleration between the decelograph and the new alternative method of video analysis and to subsequently examine these processes. The test took place at the Rosina airfield, the airstrip in a small village nearby the town of Žilina. The last part of this paper presents the results, evlauation and comparison of the measurements carried out.

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42

Simon Wedlund, Cyril, Etienne Behar, Hans Nilsson, et al. "Solar wind charge exchange in cometary atmospheres." Astronomy & Astrophysics 630 (September 20, 2019): A37. http://dx.doi.org/10.1051/0004-6361/201834881.

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Context. Solar wind charge-changing reactions are of paramount importance to the physico-chemistry of the atmosphere of a comet. The ESA/Rosetta mission to comet 67P/Churyumov-Gerasimenko (67P) provides a unique opportunity to study charge-changing processes in situ. Aims. To understand the role of these reactions in the evolution of the solar wind plasma and interpret the complex in situ measurements made by Rosetta, numerical or analytical models are necessary. Methods. We used an extended analytical formalism describing solar wind charge-changing processes at comets along solar wind streamlines. The model is driven by solar wind ion measurements from the Rosetta Plasma Consortium-Ion Composition Analyser (RPC-ICA) and neutral density observations from the Rosetta Spectrometer for Ion and Neutral Analysis-Comet Pressure Sensor (ROSINA-COPS), as well as by charge-changing cross sections of hydrogen and helium particles in a water gas. Results. A mission-wide overview of charge-changing efficiencies at comet 67P is presented. Electron capture cross sections dominate and favor the production of He and H energetic neutral atoms (ENAs), with fluxes expected to rival those of H+ and He2+ ions. Conclusions. Neutral outgassing rates are retrieved from local RPC-ICA flux measurements and match ROSINA estimates very well throughout the mission. From the model, we find that solar wind charge exchange is unable to fully explain the magnitude of the sharp drop in solar wind ion fluxes observed by Rosetta for heliocentric distances below 2.5 AU. This is likely because the model does not take the relative ion dynamics into account and to a lesser extent because it ignores the formation of bow-shock-like structures upstream of the nucleus. This work also shows that the ionization by solar extreme-ultraviolet radiation and energetic electrons dominates the source of cometary ions, although solar wind contributions may be significant during isolated events.

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Burton, Robert S. "LINGUISTIC POLITENESS IN BRITAIN AND URUGUAY: A CONTRASTIVE STUDY OF REQUESTS AND APOLOGIES. Rosina Marquez Reiter. Amsterdam: Benjamins, 2001. Pp. xviii + 225. $95.00 cloth." Studies in Second Language Acquisition 25, no. 1 (2003): 166–67. http://dx.doi.org/10.1017/s0272263103230072.

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When asked by a group of toying aristocrats whether he has an opinion about certain events in world politics, Stevens, the British butler of Kazuo Ishiguro's award-winning novel, The remains of the day, replies to one of the gentlemen in the group, “I'm very sorry, sir; but I am unable to be of assistance on this matter” (p. 195). It is the kind of indirect apology that Rosina Marquez Reiter would find delicious and perfect proof of her working thesis that British speakers (especially when compared with Uruguayan speakers) try to maintain “face” as much as possible while at the same time trying to mitigate potential threats that might arise between speakers.

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Hässig, M., K. Altwegg, H. Balsiger, et al. "ROSINA/DFMS capabilities to measure isotopic ratios in water at comet 67P/Churyumov–Gerasimenko." Planetary and Space Science 84 (August 2013): 148–52. http://dx.doi.org/10.1016/j.pss.2013.05.014.

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Hässig, M., K. Altwegg, J. J. Berthelier, et al. "The capabilities of ROSINA/DFMS to measure argon isotopes at comet 67P/Churyumov–Gerasimenko." Planetary and Space Science 105 (January 2015): 175–78. http://dx.doi.org/10.1016/j.pss.2014.11.015.

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Kevin Blanton, Carlos. "An American Language: The History of Spanish in the United States by Rosina Lozano." Southwestern Historical Quarterly 122, no. 3 (2019): 340–42. http://dx.doi.org/10.1353/swh.2019.0023.

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Calmonte, U., K. Altwegg, H. Balsiger, et al. "Sulphur isotope mass-independent fractionation observed in comet 67P/Churyumov–Gerasimenko by Rosetta/ROSINA." Monthly Notices of the Royal Astronomical Society 469, Suppl_2 (2017): S787—S803. http://dx.doi.org/10.1093/mnras/stx2534.

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Lee, Ok Ran. "AmGAI-like interacts with ROSINA, a putative transcriptional regulator of DEFICIENS in Antirrhinum majus." Plant Science 178, no. 4 (2010): 366–73. http://dx.doi.org/10.1016/j.plantsci.2010.01.003.

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Pestoni, B., K. Altwegg, H. Balsiger, et al. "Detection of volatiles undergoing sublimation from 67P/Churyumov-Gerasimenko coma particles using ROSINA/COPS." Astronomy & Astrophysics 645 (January 2021): A38. http://dx.doi.org/10.1051/0004-6361/202039130.

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Context. The ESA Rosetta mission has allowed for an extensive in situ study of the comet 67P/Churyumov-Gerasimenko. In measurements performed by the ram gauge of the COmet Pressure Sensor (COPS), observed features are seen to deviate from the nominal ram gauge signal. This effect is attributable to the sublimation of the volatile fraction of cometary icy particles containing volatiles and refractories. Aims. The objective of this work is to investigate the volatile content of icy particles that enter the COPS ram gauge. Methods. We inspected the ram gauge measurements to search for features associated with the sublimation of the volatile component of cometary particles impacting the instrument. All the sublimation features with a high-enough signal-to-noise ratio were modelled by fitting one or more exponential decay functions. The parameters of these fits were used to categorise different compositions of the sublimating component. Results. Based on features that are attributable to ice sublimation, we infer the detection of 73 icy particles containing volatiles. Of these, 25 detections have enough volatile content for an in-depth study. From the values of the exponential decay constants, we classified the 25 inferred icy particles into three types, interpreted as different volatile compositions, which are possibly further complicated by their differing morphologies. The available data do not give any indication as to which molecules compose the different types. Nevertheless, we can estimate the total volume of volatiles, which is expressed as the diameter of an equivalent sphere of water (density of 1 g cm−3). This result was found to be on the order of hundreds of nanometres.

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Dorris, George. "The Metropolitan Opera Ballet, Fresh Starts: Rosina Galli and the Ballets Russes, 1912–1917." Dance Chronicle 35, no. 2 (2012): 173–207. http://dx.doi.org/10.1080/01472526.2012.685013.

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