36 research outputs found
Analysis of factors influencing the ultrasonic fetal weight estimation
Objective: The aim of our study was the evaluation of sonographic fetal weight estimation taking into consideration 9 of the most important factors of influence on the precision of the estimation. Methods: We analyzed 820 singleton pregnancies from 22 to 42 weeks of gestational age. We evaluated 9 different factors that potentially influence the precision of sonographic weight estimation ( time interval between estimation and delivery, experts vs. less experienced investigator, fetal gender, gestational age, fetal weight, maternal BMI, amniotic fluid index, presentation of the fetus, location of the placenta). Finally, we compared the results of the fetal weight estimation of the fetuses with poor scanning conditions to those presenting good scanning conditions. Results: Of the 9 evaluated factors that may influence accuracy of fetal weight estimation, only a short interval between sonographic weight estimation and delivery (0-7 vs. 8-14 days) had a statistically significant impact. Conclusion: Of all known factors of influence, only a time interval of more than 7 days between estimation and delivery had a negative impact on the estimation
Anomalous accelerations in spacecraft flybys of the Earth
[EN] The flyby anomaly is a persistent riddle in astrodynamics.
Orbital analysis in several flybys of the Earth
since the Galileo spacecraft flyby of the Earth in 1990 have
shown that the asymptotic post-encounter velocity exhibits
a difference with the initial velocity that cannot be attributed
to conventional effects. To elucidate its origin, we have developed
an orbital program for analyzing the trajectory of
the spacecraft in the vicinity of the perigee, including both
the Sun and the MoonÂżs tidal perturbations and the geopotential
zonal, tesseral and sectorial harmonics provided by
the EGM96 model. The magnitude and direction of the
anomalous acceleration acting upon the spacecraft can be
estimated from the orbital determination program by comparing
with the trajectories fitted to telemetry data as provided
by the mission teams. This acceleration amounts to a
fraction of a mm/s2 and decays very fast with altitude. The
possibility of some new physics of gravity in the altitude
range for spacecraft flybys is discussed.Acedo RodrĂguez, L. (2017). Anomalous accelerations in spacecraft flybys of the Earth. Astrophysics and Space Science. 362(12):1-15. doi:10.1007/s10509-017-3205-xS11536212Acedo, L.: Galaxies 3, 113 (2015)Acedo, L.: Mon. Not. R. Astron. Soc. 463(2), 2119 (2016)Acedo, L.: Adv. Space Res. 59(7), 1715 (2017). 1701.06939Acedo, L., Bel, L.: Astron. Nachr. 338(1), 117 (2017). 1602.03669Adler, S.L.: Int. J. Mod. Phys. A 25, 4577 (2010). 0908.2414 . doi: 10.1142/S0217751X10050706Adler, S.L.: In: Proceedings of the Conference in Honour of Murray Gellimannâs 80th Birthday, p. 352 (2011). doi: 10.1142/9789814335614_0032Anderson, J.D., Nieto, M.M.: In: Klioner, S.A., Seidelmann, P.K., Soffel, M.H. (eds.) Relativity in Fundamental Astronomy: Dynamics, Reference Frames, and Data Analysis. IAU Symposium, vol. 261, p. 189 (2010). doi: 10.1017/S1743921309990378Anderson, J.D., Laing, P.A., Lau, E.L., Liu, A.S., Nieto, M.M., Turyshev, S.G.: Phys. Rev. Lett. 81(14), 2858 (1998). gr-qc/0104064 . doi: 10.1103/PhysRevLett.81.2858Anderson, J.D., Laing, P.A., Lau, E.L., Liu, A.S., Nieto, M.M., Turyshev, S.G.: Phys. Rev. D 65(8), 082004 (2002). gr-qc/0104064 . doi: 10.1103/PhysRevD.65.082004Anderson, J.D., Campbell, J.K., Ekelund, J.E., Ellis, J., Jordan, J.F.: Phys. Rev. Lett. 100(9), 091102 (2008). doi: 10.1103/PhysRevLett.100.091102Atchison, J.A., Peck, M.A.: J. Guid. Control Dyn. 33, 1115 (2010). doi: 10.2514/1.47413Bertolami, O., Francisco, F., Gil, P.J.S.: Class. Quantum Gravity 33(12), 125021 (2016). 1507.08457 . doi: 10.1088/0264-9381/33/12/125021Bolton, S.J., Adriani, A., Adumitroaie, V., Allison, M., Anderson, J., Atreya, S., Bloxham, J., Brown, S., Connerney, J.E.P., DeJong, E., Folkner, W., Gautier, D., Grassi, D., Gulkis, S., Guillot, T., Hansen, C., Hubbard, W.B., Iess, L., Ingersoll, A., Janssen, M., Jorgensen, J., Kaspi, Y., Levin, S.M., Li, C., Lunine, J., Miguel, Y., Mura, A., Orton, G., Owen, T., Ravine, M., Smith, E., Steffes, P., Stone, E., Stevenson, D., Thorne, R., Waite, J., Durante, D., Ebert, R.W., Greathouse, T.K., Hue, V., Parisi, M., Szalay, J.R., Wilson, R.: Science 356, 821 (2017). doi: 10.1126/science.aal2108Cahill, R.T.: ArXiv e-prints (2008). 0804.0039Chamberlin, A., Yeomans, D., Giorgini, J., Chodas, P.: Horizons Ephemeris System (2016). http://ssd.jpl.nasa.gov/horizons.cgi . Accessed: 2016-10-27Chao, B.F.: C. R. GĂ©osci. 338, 1123 (2006). doi: 10.1016/j.crte.2006.09.014Coddington, E., Levinson, N.: McGraw-Hill, New York (1955)Debono, I., Smoot, G.F.: Universe 2(4), 23 (2016). doi: 10.3390/universe2040023Desai, S.D.: J. Geophys. Res., Oceans 107(C11), 7 (2002). 3186. doi: 10.1029/2001JC001224Dickey, J.O., Bender, P.L., Faller, J.E., Newhall, X.X., Ricklefs, R.L., Ries, J.G., Shelus, P.J., Veillet, C., Whipple, A.L., Wiant, J.R., Williams, J.G., Yoder, C.F.: Science 265, 482 (1994). doi: 10.1126/science.265.5171.482Dyson, F.W., Eddington, A.S., Davidson, C.: Philos. Trans. R. Soc. Lond., Ser. A 220, 291 (1920). doi: 10.1098/rsta.1920.0009Everitt, C.W.F., et al.: Phys. Rev. Lett. 221101(106) (2011)Feng, J.L., Fornal, B., Galon, I., Gardner, S., Smolinsky, J., Tait, T.M.P., Tanedo, P.: Phys. Rev. Lett. 117, 071803 (2016). 1604.07411 . doi: 10.1103/PhysRevLett.117.071803Folkner, W.M., Williams, J.G., Boggs, D.H., Park, R.S., Kuchynka, P.: IPN Prog. Rep. 42(196) (2014)Fornberg, B.: Math. Comput. 51(184), 699 (1988). doi: 10.1090/S0025-5718-1988-0935077-0Franklin, A., Fischback, E.: The Rise and Fall of the Fifth Force. Discovery, Pursuit, and Justification in Modern Physics, second edition. Springer, New York (2016)Giorgini, J.D.: Personal communication (2015)Hackmann, E., Laemmerzahl, C.: In: 38th COSPAR Scientific Assembly. COSPAR Meeting, vol. 38, p. 3 (2010)Hafele, J.C.: ArXiv e-prints (2009). 0904.0383ICGEM: International Center for Global Gravity Field Models. http://icgem.gfz-potsdam.de/tom_longtimeIERS: In: Petit, G., Luzum, B. (eds.) IERS Conventions (2010), p. 1. Verlag des Bundesamts fĂŒr Kartographie und GeodĂ€sie, Frankfurt am Main (2010)Iess, L., Asmar, S.: Int. J. Mod. Phys. D 16, 2117 (2007). doi: 10.1142/S0218271807011449Iess, L., Asmar, S., Tortora, P.: Acta Astronaut. 65, 666 (2009). doi: 10.1016/j.actaastro.2009.01.049Iess, L., Di Benedetto, M., James, M., Mercolino, M., Simone, L., Tortora, P.: Acta Astronaut. 94, 699 (2014). doi: 10.1016/j.actaastro.2013.06.011Iorio, L.: Sch. Res. Exch. (2009). 0811.3924 . doi: 10.3814/2009/807695Iorio, L.: Astron. J. 142, 68 (2011a). 1102.4572 . doi: 10.1088/0004-6256/142/3/68Iorio, L.: Mon. Not. R. Astron. Soc. 415, 1266 (2011b). 1102.0212Iorio, L.: Europhys. Lett. (2011c). 1105.4145 . doi: 10.1209/0295-5075/96/30001Iorio, L.: Adv. Space Res. 54(11), 2441 (2014a). 1311.4218 . doi: 10.1016/j.asr.2014.06.035Iorio, L.: Galaxies 2, 259 (2014b). 1404.6537 . doi: 10.3390/galaxies2020259Iorio, L.: Universe 1(1), 38 (2015a). doi: 10.3390/universe1010038Iorio, L.: Int. J. Mod. Phys. D 24, 1530015 (2015b). 1412.7673Iorio, L., Giudice, G.: New Astron. 11, 600 (2006). gr-qc/0601055Iorio, L., Lichtenegger, H.I.M., Ruggiero, M.L., Corda, C.: Astrophys. Space Sci. 331, 351 (2011). 1009.3225 . doi: 10.1007/s10509-010-0489-5Jouannic, B., Noomen, R., van den IJSel, J.A.A.: In: Proceedings of the 25th International Symposium on Space Flight Dynamics ISSFD, Munich, Germany (2015)Kennefick, D.: Phys. Today 62, 37 (2009). doi: 10.1063/1.3099578King-Hele, D.: Satellite Orbits in an Atmosphere. Theory and Applications. Blackie and Son Ltd., Glasgow (1987)LĂ€mmerzahl, C., Preuss, O., Dittus, H.: In: Dittus, H., Lammerzahl, C., Turyshev, S.G. (eds.) Lasers, Clocks and Drag-Free Control: Exploration of Relativistic Gravity in Space. Astrophysics and Space Science Library, vol. 349, p. 75 (2008). doi: 10.1007/978-3-540-34377-6_3Le Verrier, U.: C. R. Hebd. Acad. Sci. 49, 379 (1859)Lemoine, F.G.E.A.: NASA/TP-1998-206861 (1998)Lewis, R.A.: In: Robertson, G.A. (ed.) American Institute of Physics Conference Series. American Institute of Physics Conference Series, vol. 1103, p. 226 (2009). doi: 10.1063/1.3115499Longair, M.: Philos. Trans. R. Soc., Math. Phys. Eng. Sci. (2015). doi: 10.1098/rsta.2014.0287McCulloch, M.E.: Mon. Not. R. Astron. Soc. 389, 57 (2008). 0806.4159 . doi: 10.1111/j.1745-3933.2008.00523.xMoe, M.M., Wallace, S.D., Moe, K.: In: Washington DC American Geophysical Union Geophysical Monograph Series, vol. 87, p. 349 (1995). doi: 10.1029/GM087p0349Murphy, E.M.: Phys. Rev. Lett. 83, 1890 (1998). doi: 10.1103/PhysRevLett.83.1890Naval Observatory: Dept. of the Navy, USA (2009)Newcomb, S.: Tables of the Four Inner Planets. Government Printing Office, Washington (1895)Nyambuya, G.G.: ArXiv e-prints (2008). 0803.1370Nyambuya, G.G.: New Astron. 57, 22 (2017). doi: 10.1016/j.newast.2017.06.001PĂĄramos, J., Hechenblaikner, G.: Adv. Space Res. 79â80(7), 76 (2013). 1210.7333v1Peskin, M.E., Schroeder, D.V.: An Introduction to Quantum Field Theory. Westview Press, Perseus Books Group, London (1995)Pinheiro, M.J.: Phys. Lett. A 378, 3007 (2014). 1404.1101Pinheiro, M.J.: Mon. Not. R. Astron. Soc. 461(4), 3948 (2016)Renzetti, G.: Cent. Eur. J. Phys. 11, 531 (2013). doi: 10.2478/s11534-013-0189-1Rievers, B., LĂ€mmerzahl, C.: Ann. Phys. 523, 439 (2011). 1104.3985 . doi: 10.1002/andp.201100081Roseveare, N.T.: Mercuryâs Perihelion, from Le Verrier to Einstein. Clarendon Press, Wotton-under-Edge (1982)Rubincam, D.P.: Icarus 148, 2 (2000). doi: 10.1006/icar.2000.6485Standish, E.M.: In: Macias, A., LĂ€mmerzahl, C., Camacho, A. (eds.) Recent Developments in Gravitation and Cosmology. American Institute of Physics Conference Series, vol. 977, p. 254 (2008). doi: 10.1063/1.2902789Standish, E.M.: In: Klioner, S.A., Seidelmann, P.K., Soffel, M.H. (eds.) Relativity in Fundamental Astronomy: Dynamics, Reference Frames, and Data Analysis. IAU Symposium, vol. 261, p. 179 (2010). doi: 10.1017/S1743921309990354Thompson, P.F., Abrahamson, M., Ardalan, S., Bordi, J.: In: 24th AAS/AIAA Space Flight Mechanics Meeting, Santa Fe, New Mexico, January 26â30, 2014 (2014). http://hdl.handle.net/2014/45519Turyshev, S.G., Toth, V.T.: Living Rev. Relativ. (2010). 1001.3686 . doi: 10.12942/lrr-2010-4Turyshev, S.G., Toth, V.T., Kinsella, G., Lee, S.-C., Lok, S.M., Ellis, J.: Phys. Rev. Lett. 108(24), 241101 (2012). 1204.2507 . doi: 10.1103/PhysRevLett.108.241101Varieschi, G.U.: Gen. Relativ. Gravit. 46, 1741 (2014). 1401.6503 . doi: 10.1007/s10714-014-1741-zWilhelm, K., Dwivedi, B.N.: Astrophys. Space Sci. 358, 18 (2015). doi: 10.1007/s10509-015-2413-5Will, C.M.: Living Rev. Relativ. 3(9) (2006)Will, C.M.: Class. Quantum Gravity (2015). doi: 10.1098/rsta.2014.0287Will, C.M.: In: Peron, R., Colpi, M., Gorini, V., Moschella, U. (eds.) Gravity: Where Do We Stand? Astrophysics and Space Science Library, vol. 349, p. 9 (2016). doi: 10.1007/978-3-319-20224-2_2Williams, J.G., Boggs, D.H.: Celest. Mech. Dyn. Astron. 126, 89 (2016). doi: 10.1007/s10569-016-9702-3Williams, J.G., Dickey, J.O.: In: Noomen, R., Klosko, S., Noll, C., Pearlman, M. (eds.) Proceedings of 13th International Workshop on Laser Ranging, p. 75 (2003). http://cddisa.gsfc.nasa.gov/lw13/lw_proceedings.htmlWilliams, J.G., Newhall, X.X., Dickey, J.O.: Phys. Rev. D 53, 6730 (1996). doi: 10.1103/PhysRevD.53.6730Williams, J.G., Turyshev, S.G., Boggs, D.H.: Phys. Rev. Lett. 93(26), 261101 (2004). gr-qc/0411113 . doi: 10.1103/PhysRevLett.93.261101Williams, J.G., Turyshev, S.G., Boggs, D.H.: Planet. Sci. 3, 2 (2014). doi: 10.1186/s13535-014-0002-5Williams, J.G., Boggs, D.H., Yoder, C.F., Ratcliff, J.T., Dickey, J.O.: J. Geophys. Res. 106, 27933 (2001). doi: 10.1029/2000JE001396Wolfram, S.: The Mathematica Book, fifth edition. Wolfram Media, Champaign (2003
Formation of gullies on Mars by debris flows triggered by CO_2 sublimation
Martian gully landforms resemble terrestrial debris flows formed by the action of liquid water and have thus been interpreted as evidence for potential habitable environments on Mars within the past few millennia. However, ongoing gully formation has been detected under surface conditions much too cold for liquid water, but at times in the martian year when a thin layer of seasonal CO_2 frost is present and defrosting above the regolith. These observations suggest that the CO_2 condensationâsublimation cycle could play a role in gully formation. Here we use a thermo-physical numerical model of the martian regolith underlying a CO_2 ice layer and atmosphere to show that the pores beneath the ice layer can be filled with CO_2 ice and subjected to extreme pressure variations during the defrosting season. The subsequent gas fluxes can destabilize the regolith material and induce gas-lubricated debris flows with geomorphic characteristics similar to martian gullies. Moreover, we find that subsurface CO_2 ice condensation, sublimation and pressurization occurs at conditions found at latitudes and slope orientations where gullies are observed. We conclude that martian gullies can result from geologic dry ice processes that have no terrestrial analogues and do not require liquid water. Such dry ice processes may have helped shape the evolution of landforms elsewhere on the martian surface
Prise en charge alcoologique des malades hospitalises aux urgences pour intoxication ethylique aigue
Aspects mĂ©dico-Ă©conomiques du dĂ©pistage Ă©chographique des malformations fĆtales : revue de la littĂ©rature
Objectives: The systematic use of ultrasound during pregnancy aims at birth defect detection. Our objective was to assess the economic efficiency of prenatal ultrasound screening for fetal malformations. Methods: We carried out a literature review on Medline via PubMed between 1985 and 2015, from the economic perspective of the prenatal ultrasound screening for fetal malformations. Results: The literature on this subject was sparse and we selected only twelve articles presenting relevant economic data, of which only eight were proper medico-economic studies. We found arguments for the economic effectiveness of ultrasound screening for fetal malformation detection, which is largely linked to the terminations of pregnancies and to the cost of the handicaps "avoided". However, none of the reviewed articles could reach medico-economic conclusions. Additionally, we highlighted various elements making economic analyses more complex in this field: the choice of the method, the uncertainty around two essential parameters (the efficiency of ultrasound and the costs of procedures) and the difficulties to compare or to generalize results. We also noticed important methodological heterogeneity among the studies and the absence of French study. Conclusions: Previously published data are insufficient to assess the economic efficiency of prenatal ultrasound screening for fetal malformations.Objectifs: Lâun des objectifs majeurs de lâutilisation systĂ©matique de lâĂ©chographie obstĂ©tricale pendant la grossesse est le dĂ©pistage des malformations fĆtales. Notre objectif Ă©tait dâanalyser lâefficience mĂ©dico-Ă©conomique de ce dĂ©pistage. MĂ©thodes: Nous avons rĂ©alisĂ© une revue de la littĂ©rature Ă partir de Medline via PubMed, entre 1985 et 2015, sur lâaspect mĂ©dico-Ă©conomique du dĂ©pistage par Ă©chographie des malformations fĆtales. RĂ©sultats: La littĂ©rature Ă©tait trĂšs pauvre sur le sujet et nous nâavons pu retenir et analyser que 12 articles prĂ©sentant des donnĂ©es intĂ©ressantes pour notre revue, dont huit vĂ©ritables Ă©tudes mĂ©dico-Ă©conomiques. Nous avons identifiĂ© des arguments en faveur du caractĂšre Ă©conomiquement pertinent dâun programme de dĂ©pistage des malformations, ceci Ă©tant en grande partie liĂ© Ă la pratique des interruptions mĂ©dicales de grossesse et aux coĂ»ts des handicaps « Ă©vitĂ©s », mais sans pouvoir conclure dâun point de vue mĂ©dico-Ă©conomique. Nous avons surtout pu mettre en Ă©vidence plusieurs Ă©lĂ©ments compliquant lâapplication de ces analyses dans ce domaine : le choix du type dâĂ©tude, la forte incertitude sur deux paramĂštres essentiels (lâefficacitĂ© de lâĂ©chographie et le coĂ»t des procĂ©dures), la difficultĂ© Ă comparer ou gĂ©nĂ©raliser les rĂ©sultats. Nous avons aussi constatĂ© lâhĂ©tĂ©rogĂ©nĂ©itĂ© mĂ©thodologique des Ă©tudes et lâabsence dâĂ©tude française. Conclusion: Les donnĂ©es existantes de la littĂ©rature sont actuellement insuffisantes pour Ă©valuer lâefficience mĂ©dico-Ă©conomique du dĂ©pistage des malformations par Ă©chographie
Gene expression profiling of reproductive meristem types in early rice inflorescences by laser microdissection
In rice, inflorescence architecture is established at early stages of reproductive development and contributes directly to grain yield potential. After induction of flowering, the complexity of branching, and therefore the number of seeds on the panicle, is determined by the activity of different meristem types and the timing of transitions between them. Although some of the genes involved in these transitions have been identified, an understanding of the network of transcriptional regulators controlling this process is lacking. To address this we used a precise laser microdissection and RNA-sequencing approach in Oryza sativa ssp. japonica cv. Nipponbare to produce quantitative data that describe the landscape of gene expression in four different meristem types: the rachis meristem, the primary branch meristem, the elongating primary branch meristem (including axillary meristems), and the spikelet meristem. A switch in expression profile between apical and axillary meristem types followed by more gradual changes during transitions in axillary meristem identity was observed, and several genes potentially involved in branching were identified. This resource will be vital for a mechanistic understanding of the link between inflorescence development and grain yield