Academic literature on the topic 'Middle and low latitudes'

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Journal articles on the topic "Middle and low latitudes"

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Agnini, Claudia, Eliana Fornaciari, Isabella Raffi, Rita Catanzariti, Heiko Pälike, Jan Backman, and Domenico Rio. "Biozonation and biochronology of Paleogene calcareous nannofossils from low and middle latitudes." Newsletters on Stratigraphy 47, no. 2 (June 1, 2014): 131–81. http://dx.doi.org/10.1127/0078-0421/2014/0042.

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Chandran, A., and R. L. Collins. "Stratospheric sudden warming effects on winds and temperature in the middle atmosphere at middle and low latitudes: a study using WACCM." Annales Geophysicae 32, no. 7 (July 28, 2014): 859–74. http://dx.doi.org/10.5194/angeo-32-859-2014.

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Abstract. A stratospheric sudden warming (SSW) is a dynamical phenomenon of the wintertime stratosphere caused by the interaction between planetary Rossby waves propagating from the troposphere and the stratospheric zonal-mean flow. While the effects of SSW events are seen predominantly in high latitudes, they can also produce significant changes in middle and low latitude temperature and winds. In this study we quantify the middle and low latitude effects of SSW events on temperature and zonal-mean winds using a composite of SSW events between 1988 and 2010 simulated with the specified dynamics version of the Whole Atmosphere Community Climate Model (WACCM). The temperature and wind responses seen in the tropics also extend into the low latitudes in the other hemisphere. There is variability in observed zonal-mean winds and temperature depending on the observing location within the displaced or split polar vortex and propagation direction of the planetary waves. The propagation of planetary waves show that they originate in mid–high latitudes and propagate upward and equatorward into the mid-latitude middle atmosphere where they produce westward forcing reaching peak values of ~ 60–70 m s−1 day−1. These propagation paths in the lower latitude stratosphere appear to depend on the phase of the quasi-biennial oscillation (QBO). During the easterly phase of the QBO, waves originating at high latitudes propagate across the equator, while in the westerly phase of the QBO, the planetary waves break at ~ 20–25° N and there is no propagation across the equator. The propagation of planetary waves across the equator during the easterly phase of the QBO reduces the tropical upwelling and poleward flow in the upper stratosphere.
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Streltsov, A. V., and J. D. Huba. "Magnetospheric resonances at low and middle latitudes." Journal of Geophysical Research: Space Physics 120, no. 9 (September 2015): 7718–27. http://dx.doi.org/10.1002/2015ja021532.

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Haines, K. "Low-frequency variability in atmospheric middle latitudes." Surveys in Geophysics 15, no. 1 (January 1994): 1–61. http://dx.doi.org/10.1007/bf00665686.

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Jensen, J. W., and B. G. Fejer. "Longitudinal dependence of middle and low latitude zonal plasma drifts measured by DE-2." Annales Geophysicae 25, no. 12 (January 2, 2007): 2551–59. http://dx.doi.org/10.5194/angeo-25-2551-2007.

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Abstract. We used ion drift observations from the DE-2 satellite to study for the first time the longitudinal variations of middle and low latitude F region zonal plasma drifts during quiet and disturbed conditions. The quiet-time middle latitude drifts are predominantly westward; the low latitude drifts are westward during the day and eastward at night. The daytime quiet-time drifts do not change much with longitude; the nighttime drifts have strong season dependent longitudinal variations. In the dusk-premidnight period, the equinoctial middle latitude westward drifts are smallest in the European sector and the low latitude eastward drifts are largest in the American-Pacific sector. The longitudinal variations of the late night-early morning drifts during June and December solstice are anti-correlated. During geomagnetically active times, there are large westward perturbation drifts in the late afternoon-early night sector at upper middle latitudes, and in the midnight sector at low latitudes. The largest westward disturbed drifts during equinox occur in European sector, and the smallest in the Pacific region. These results suggest that during equinox SAPS events occur most often at European longitudes. The low latitude perturbation drifts do not show significant longitudinal
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Zhou, Yun-Liang, Li Wang, Chao Xiong, Hermann Lühr, and Shu-Ying Ma. "The solar activity dependence of nonmigrating tides in electron density at low and middle latitudes observed by CHAMP and GRACE." Annales Geophysicae 34, no. 4 (April 27, 2016): 463–72. http://dx.doi.org/10.5194/angeo-34-463-2016.

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Abstract. In this paper we use more than a decade of in situ electron density observations from CHAMP and GRACE satellites to investigate the solar activity dependence of nonmigrating tides at both low and middle latitudes. The results indicate that the longitudinal patterns of F region electron density vary with season and latitude, which are exhibiting a wavenumber 4 (WN4) pattern around September equinox at low latitudes and WN1/WN2 patterns during local summer at the southern/northern middle latitudes. These wave patterns in the F region ionosphere can clearly be seen during both solar maximum and minimum years. At low latitudes the absolute amplitudes of DE3 (contributing to the WN4 pattern) are found to be highly related to the solar activity, showing larger amplitudes during solar maximum years. Similarly a solar activity dependence can also be found for the absolute amplitudes of D0, DW2 and DE1 (contributing to the WN1 and WN2 pattern) at middle latitudes. The relative amplitudes (normalized by the zonal mean) of these nonmigrating tides at both low and middle altitudes show little dependence on solar activity. We further found a clear modulation by the quasi-biennial oscillation (QBO) of the relative DE3 amplitudes in both satellite observations, which is consistent with the QBO dependence as reported for the E region temperatures and zonal wind. It also supports the strong coupling of the low-latitude nonmigrating tidal activity between the E and F regions. However, the QBO dependence cannot be found for the relative amplitudes of the nonmigrating tides at middle latitudes, which implies that these tides are generated in situ at F region altitudes.
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Gulyaeva, T. L., S. Aggarwal, K. K. Mahajan, and S. Shastri. "Variability of foF2 at low and middle latitudes." Advances in Space Research 22, no. 6 (January 1998): 847–50. http://dx.doi.org/10.1016/s0273-1177(98)00110-0.

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Davies, K., and X. M. Liu. "Ionospheric slab thickness in middle and low latitudes." Radio Science 26, no. 4 (July 1991): 997–1005. http://dx.doi.org/10.1029/91rs00831.

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Backman, Jan, Isabella Raffi, Domenico Rio, Eliana Fornaciari, and Heiko Pälike. "Biozonation and biochronology of Miocene through Pleistocene calcareous nannofossils from low and middle latitudes." Newsletters on Stratigraphy 45, no. 3 (November 1, 2012): 221–44. http://dx.doi.org/10.1127/0078-0421/2012/0022.

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Andrioli, V. F., D. C. Fritts, P. P. Batista, B. R. Clemesha, and D. Janches. "Diurnal variation in gravity wave activity at low and middle latitudes." Annales Geophysicae 31, no. 11 (November 29, 2013): 2123–35. http://dx.doi.org/10.5194/angeo-31-2123-2013.

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Abstract. We employ a modified composite day extension of the Hocking (2005) analysis method to study gravity wave (GW) activity in the mesosphere and lower thermosphere using 4 meteor radars spanning latitudes from 7° S to 53.6° S. Diurnal and semidiurnal modulations were observed in GW variances over all sites. Semidiurnal modulation with downward phase propagation was observed at lower latitudes mainly near the equinoxes. Diurnal modulations occur mainly near solstice and, except for the zonal component at Cariri (7° S), do not exhibit downward phase propagation. At a higher latitude (SAAMER, 53.6° S) these modulations are only observed in the meridional component where we can observe diurnal variation from March to May, and semidiurnal, during January, February, October (above 88 km) and November. Some of these modulations with downward phase progression correlate well with wind shear. When the wind shear is well correlated with the maximum of the variances the diurnal tide has its largest amplitudes, i.e., near equinox. Correlations exhibiting variations with tidal phases suggest significant GW-tidal interactions that have different characters depending on the tidal components and possible mean wind shears. Modulations that do not exhibit phase variations could be indicative of diurnal variations in GW sources.
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Dissertations / Theses on the topic "Middle and low latitudes"

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Tsunomura, Satoru. "On the Contribution of Global Scale Polar-originating Ionospheric Current Systems to Geomagnetic Disturbances in Middle and Low Latitudes." 京都大学 (Kyoto University), 1999. http://hdl.handle.net/2433/182006.

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Adhikari, Binod. "HILDCAA-related effects recorded in middle-low latitude magnetometers." Instituto Nacional de Pesquisas Espaciais (INPE), 2015. http://urlib.net/sid.inpe.br/mtc-m21b/2015/02.27.16.58.

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Disturbances of the geomagnetic field are caused by enhanced solar windmagnetosphere electrodynamical coupling process. The principal cause of geomagnetic disturbance is the magnetic reconnection between the southward directed interplanetary magnetic field component and the northward directed magnetopause field, that establishes an electrodynamic coupling between the solar wind plasma and magnetosphere. In general, this coupling is controled by dominant structures emanating from the sun like sporadic coronal mass ejections (CMEs) and their interplanetary counterparts (ICMEs), around the solar maximum, and by corotating high-speed streams, including corotating interaction region (CIR), in the descending and minimum phases of solar cycle. These high speed streams are embedded with highly fluctuating Alfven waves, which produce phenomena called HILDCAA events (high-intensity, long duration, continuous AE activity). This study investigates magnetic records from middle-low latitude geomagnetic observatories during HILDCAA periods. To this purpose, three primary conditions of the interplanetary space are considered: HILDCAA (i) not preceded by magnetic storm, (ii) preceded by storm generated by CIR, and (iii) preceded by storm generated by ICME. A fourth case is considered as a background condition: a geomagnetically quiet interval. As methodology of analysis, wavelet techniques to study multi-scale features of the HILDCAA events were explored in this work. The signal analyses techniques are composed by continuous wavelet transform, discrete wavelet transform, cross correlation using wavelet, and the usual modulus cross correlation. Complementarly, an evaluation on the field aligned currents (FAC) are considered in the investigation. Besides this, we estimate the polar cap potential (PCP) and merging electric field (Ey), and examine the role of PCP and geomagnetic AL index to monitor geomagnetic activity generated by geoeffective solar wind parameters during HILDCAAs. Thus, this work contributes to extend the understanding of HILDCAA events at higher latitudes to disturbances occurring at middle-low latitudes. There are magnetic effects related to the occurrence of HILDCAA even at middle-low latitudes.
Perturbações do campo magnético da Terra são causadas por intensificação de um processo de acoplamento eletrodinâmico entre o vento solar e a magnetosfera. A causa principal das perturbações geomagnéticas é a reconexão magnética entre o campo magnético interplanetário com orientação para o sul e o campo magnético da Terra orientado para o norte, que estabelecem um acoplamento eletrodinâmico entre o plasma do vento solar e a magnetosfera. Em geral, esse acoplamento é controlado por estruturas dominantes emanadas do Sol como ejeções de matéria coronal (CMEs) e suas contrapartes interplanetárias (ICMES), em torno do máximo solar, e por feixes de alta velocidade corrotantes, incluindo regiões corrotantes de interação (CIR), nas fases descendente e de mínimo do ciclo solar. Esses feixes de alta velocidade portam ondas alfvênicas com intensa flutuação dos parâmetros físicos do plasma, que produzem os fenômenos de atividade AE continuada de alta intensidade e de longa duração, denominados eventos HILDCAA (high-intensity, long duration, continuous AE activity). Este estudo investiga os registros magnéticos obtidos de observatórios geomagnéticos durante períodos de HILDCAA. Para esse propósito, três condições fundamentais do espaço interplanetário são consideradas: HILDCAA (i) não precedida de tempestade geomagnética; (ii) precedida por tempestade gerada por CIR; e (iii) precedida por tempestade gerada por ICME. Um quarto caso é considerado como uma condição de ambiente de fundo: um intervalo geomagneticamente calmo. Como metodologia de análises, técnicas wavelets para estudar características multiescalas dos eventos HILDCAAs são exploradas neste trabalho. As técnicas de análises de sinais são compostas pela transformada wavelet contínua, transformada wavelet discreta, correlação cruzada usando wavelet, e a usual correlação cruzada das intensidades dos sinais. De maneira complementar, uma avaliação das correntes elétricas alinhadas com o campo geomagnético são consideradas na investigação. Além disso, estimamos o potencial na região polar (polar cap potential, PCP) e o campo elétrico resultante da reconexão magnética (Ey), e examinamos o papel do PCP e do índice geomagnético AL para monitorar a atividade geomagnética produzida pelos parâmetros solares geoefetivos durante os eventos HILDCAAs. Assim, este trabalho contribuiu para estender a compreensão dos eventos HILDCAAs de altas latitudes para distúrbios ocorrendo em médias e baixas latitudes. Há efeitos magnéticos relacionados a ocorrências de HILDCAAs mesmo em baixas e médias latitudes.
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Aoyama, Tadashi. "A study on the origin of small-scale field-aligned currents as observed in topside ionosphere at middle and low latitudes." 京都大学 (Kyoto University), 2017. http://hdl.handle.net/2433/225408.

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Jensen, John W. "Climatology of Middle and Low-Latitude F-Region Plasma Drifts from Satellite Measurements." DigitalCommons@USU, 2007. https://digitalcommons.usu.edu/etd/7444.

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We used ion drift observations from the DE-2 satellite to study for the first time the longitudinal variations of middle and low latitude F-region zonal plasma drifts during quiet and disturbed conditions. The daytime quiet-time drifts do not change much with longitude. In the dusk-premidnight period, the equinoctial middle latitude westward drifts are smallest in the European sector, and the low latitude eastward drifts are largest in the American-Pacific sector. The longitudinal variations of the late night-early morning drifts during June and December solstice are anti-correlated. During geomagnetically active time s, there are large westward perturbation drifts in the late afternoon-early night sector at upper middle latitudes and in the midnight sector at low latitudes. The largest westward disturbed drifts during equinox occur in the European sector and the smallest in the Pacific region. These results suggest that during equinox, Subauroral Polarization Streams (SAPS) events occur most often at European longitudes. The low latitude perturbation drifts do not show significant longitudinal dependence. We have used five years of measurements on board the ROCSA T-1 satellite to develop a detailed local-time, season, and longitude-dependent quiet-time global empirical model for equatorial F-region vertical plasma drifts. We show that the longitudinal dependence of the daytime and nighttime vertical drifts is much stronger than reported earlier, especially during December and June solstice. The late night downward drift velocities are larger in the eastern than in the western hemisphere at all seasons, the morning and afternoon December solstice drifts have significantly different longitudinal dependence, and the daytime upward drifts have strong wavenumber-four signatures during equinox and June solstice. The largest evening upward drifts occur during equinox and December solstice near the American sector. The longitudinal variations of the evening prereversal velocity peaks during December and June solstice are anti-correlated, which further indicates the importance of conductivity effects on the electrodynamics of the equatorial ionosphere. We have shown that disturbance dynamo largely does not affect daytime drifts. The upward perturbations during the nighttime are largely season independent, but near the prereversal enhancement, the downward perturbation drifts are largest during equinox and smallest during December.
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Shim, JA Soon. "Analysis of Total Electron Content (TEC) Variations in the Low- and Middle-Latitude Ionosphere." DigitalCommons@USU, 2009. https://digitalcommons.usu.edu/etd/403.

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Detailed study of the spatial correlations of day-to-day ionospheric TEC variations on a global scale was performed for four 30-day-long periods in 2004 (January, March/April, June/July, September/October) using observations from more than 1000 ground-based GPS receivers. In order to obtain the spatial correlations, initially, the day-to-day variability was calculated by first mapping the observed slant TEC values for each 5-minute GPS ground receiver-satellite pair to the vertical and then differencing it with its corresponding value from the previous day. This resulted in more than 150 million values of day-to-day change in TEC (delta TEC). Next, statistics were performed on the delta TEC values. The study indicates strong correlationsbetween geomagnetic conjugate points, and these correlations are larger at low latitudes than at middle latitudes. Typical correlation lengths, defined as the angular separation at which the correlation coefficient drops to 0.7, were found to be larger at middle latitudes than at low latitudes. The correlation lengths are larger during daytime than during nighttime. The results indicate that the spatial correlation is largely independent of season. These spatial correlations are important for understanding the physical mechanisms that cause ionospheric weather variability and are also relevant to data assimilation. In an effort to better understand the effects of neutral wind and electric field on the TEC variability, a physics-based numerical Ionosphere/Plasmasphere Model (IPM) was used. The model solves the transport equations for the six ions, O+, NO+, O2+, N2+, H+, and He+, on convecting flux tubes that realistically follow the geomagnetic field. Two of the inputs required by the IPM are the thermospheric neutral wind and the low-latitude electric field, which can be given by existing empirical model or externally specified by the user. To study the relative importance of the neutral wind and the electric field for the TEC variations, these two model inputs were externally modified and the resulting variations in TEC were compared. Neutral wind and electric field modifications were introduced at three different local times in order to investigate the effect of different start times of the imposed perturbations on TEC. This study focused on modeled low- and middlelatitude TEC variations in the afternoon and post-sunset at three different longitude sectors for medium solar activity and low geomagnetic activity. The largest changes in TEC were found predominantly in the equatorial anomaly, and a significant longitudinal dependence was observed. The results indicate that the perturbation effect on the TEC at 2100 LT varied nonlinearly with the elapsed time after the imposed neutral wind and electric field perturbations. An important outcome of this study is that daytime neutral wind and/or electric field modifications will lead to essentially identical TEC changes in the 2100 local time sector.
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Mohd, Ali Aiffah. "GNSS in aviation : ionospheric threats at low latitudes." Thesis, University of Bath, 2018. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.761026.

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Radio signals propagating through the ionised upper atmosphere (the ionosphere) in low latitude regions of the world can experience amplitude scintillation. This could threaten safety-critical applications of satellite navigation such as aviation. The research presented here studied the effects of amplitude scintillation on a Septentrio PolaRxS geodetic receiver and a Garmin 480 aviation receiver by means of a Spirent GNSS constellation simulator. Different types of fade profiles showed that an abrupt drop in signal strength caused a loss of lock on the signal more often than a profile with a slow, gradual fade. A performance comparison of the two receivers demonstrated that the aviation receiver was more vulnerable than the geodetic receiver. An unexpected loss of lock at a specific fade duration and depth was seen with the Garmin receiver and was not explained. A single fade with a long fade duration was more likely to cause a loss of signal lock compared to rapid multiple fades. Scintillation on signals from low elevation satellites can significantly degrade the precision and integrity of the navigation solution in an aviation receiver; especially if the satellites are within the best geometrical set. RAIM was observed to be no longer available during the critical landing approach phase of the scenario, in the case when all satellites in view were affected by the scintillation-induced signal perturbations. A technique was also developed to simulate L5 scintillation based on real scintillation events of L1, in the absence of real captured data for L5. This was done to enable future investigations on aviation receiver performance when both L1 and L5 frequencies experience scintillation. Analysis indicated that L5 signal can be more vulnerable to the scintillation compared to the L1 signal, which may have important implications for aviation safety.
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Hoch, David M. "Passive and low energy building design for high latitudes." Thesis, University of Cambridge, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.279588.

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Hood, L. L., B. E. Soukharev, M. Fromm, and J. P. McCormack. "Origin of extreme ozone minima at middle to high northern latitudes." AMER GEOPHYSICAL UNION, 2001. http://hdl.handle.net/10150/624004.

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Extreme ozone minima represent localized and temporally brief (several days) reductions in column ozone amounts below some chosen absolute level. Although such minima at middle to high northern latitudes are known to be primarily dynamical in origin, a remaining issue is whether heterogeneous chemical loss processes may also contribute significantly to their formation. A case in point is the record low 165 Dobson units (DU) minimum occurring on November 30, 1999, when temperatures near 30 hPa at the location of the minimum were lower than the threshold for the formation of type I polar stratospheric clouds (PSC). An examination of Polar Ozone and Aerosol Measurement III data for times surrounding the event shows that PSCs were indeed present in the vicinity where the ozone minimum was observed. However, archived data show that a similar extreme minimum of 167 DU with characteristics comparable to those of the November 30, 1999, minimum occurred on October 30, 1985, when no PSCs were present. An ensemble of 71 extreme ozone minima with amplitudes under 215 DU exhibit a nearly linear relationship between ozone minimum deviations from the zonal mean and corresponding 30-hPa temperature deviations. Such a relationship is predicted by analytic transport models which assume that vertical motions (i.e., upwelling) are responsible for the ozone minima. Temperature deviations near 30-hPa were unusually large for both the November 30, 1999, and the October 30, 1985, events, implying unusually rapid upward transport for these events. All 71 minima occur in regions where deviations from the zonal mean of 330 K potential vorticity are negative, implying an additional contribution to their formation by quasi-horizontal transport. The timescale for column ozone reductions during extreme ozone minima events is also determined and found to be at least 20 times more rapid than expected from known chemical loss processes. The data are therefore most consistent with a purely dynamical origin for extreme ozone minima in general and the November 30, 1999, event in particular. As was shown by earlier work, the basic dynamical process involves a combination of isentropic transport of ozone-poor air from the tropical upper troposphere and rapid upwelling over upper tropospheric anticyclonic disturbances resulting from poleward Rossby wave breaking events.
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Drexler, Josef. "Determining the properties of low-frequency Farley-Buneman waves at high latitudes." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2000. http://www.collectionscanada.ca/obj/s4/f2/dsk2/ftp03/MQ58028.pdf.

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Akuetevi, Cataria Quam Cyrille. "Dynamics of turbulent western boundary currents at low latitudes, a numerical study." Thesis, Grenoble, 2014. http://www.theses.fr/2014GRENU002/document.

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Les courants turbulents de bord ouest sont l'un des phénomènes les plus dominants des océans, il en existe aux faibles latitudes aussi. Ils sont caractérisés par une dynamique très turbulente avec une forte production d'énergie cinétique, et une forte variabilité interne. Plusieurs régions existent où les courants de bord ouest se rétrofléchissent (décollage de la côte) pour former des structures cohérentes: des anticyclones, des bursts (arrachements) et des dipoles. Circulant le long de la côte, les courants de bord ouest interagissent très fortement avec le bord ouest et la bathymétrie et sont donc un problème de couche limite. Cependant aucune étude du point de vue de la théorie de couche limite n'a été jamais été faite. Cette thèse aborde le problème d'un point de vue de couche limite par l'utilisation d'un modèle idéalisé "shallow water" à très haute résolution (2.5km) afin d'isoler et de comprendre les processus. Les résultats sont ensuite appliqués à des sorties de modèle réaliste Drakkar (~10km) basé sur le code NEMO. Le courant de Somali est ensuite pris pour cette application
Strong western boundary currents are one of dominant features of the world oceans, also at low latitudes. They exhibit a turbulent dynamics and their region is a source of strong kinetic energy production and internal variability of the worlds oceans. Several places exists where the western boundary currents retrofect (i.e separation from the coast) and generate coherent structures as anticyclonic eddies, bursts and dipoles. The dynamics of turbulent western boundary currents has so far not been extensively studied in the viewpoint of turbulent boundary-layer theory. The approach followed in this thesis is to use a fine resolution (2.5km) reduced-gravity shallow water model to understand the turbulent boundary-layer processes and then apply these findings to the Ocean General Circulation Model NEMO in the Drakkar configuration (~10km). The case of the Somali Currentis considered for this application
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Books on the topic "Middle and low latitudes"

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S, Nieuwolt, ed. Tropical climatology: An introduction to the climates of the low latitudes. 2nd ed. New York: Wiley, 1998.

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P, Kharin E., Semenov V. I͡U︡, and Rossiĭskai͡a︡ akademii͡a︡ nauk. Nat͡s︡ionalʹnyĭ geofizicheskiĭ komitet, eds. Hourly indices of geomagnetic activity for the middle latitudes: Catalogue 1964-1991. Moscow: Geophysical Committee, Russian Academy of Sciences, 1992.

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Geomorphology in the tropics: A study of weathering and denudation in low latitudes. Chichester [England]: Wiley, 1994.

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Rajan, S. Irudaya, and Prem Saxena, eds. India's Low-Skilled Migration to the Middle East. Singapore: Springer Singapore, 2019. http://dx.doi.org/10.1007/978-981-13-9224-5.

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Institute of Medicine (U.S.). Committee on Cancer Control in Low- and Middle-Income Countries. Cancer control opportunities in low- and middle-income countries. Edited by Sloan Frank A and Gelband Hellen. Washington, DC: National Academies Press, 2006.

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Marquez, Lani Rice, ed. Improving Health Care in Low- and Middle-Income Countries. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-43112-9.

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Neal, Cassidy, ed. Secrets of healthy Middle Eastern cuisine. New York: Interlink Books, 2000.

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Abourezk, Sanaa. Secrets of healthy Middle Eastern cuisine. London: Stacey International, 2003.

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Abourezk, Sanaa. Secrets of healthy Middle Eastern cuisine. New York: Interlink Books, 2003.

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Institution, Brookings, ed. Impact of health insurance in low- and middle-income countries. Washington, D.C: Brookings Institution Press, 2010.

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Book chapters on the topic "Middle and low latitudes"

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Prölss, Gerd W. "Space Weather Effects in the Upper Atmosphere: Low and Middle Latitudes." In Lecture Notes in Physics, 193–214. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-31534-6_6.

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Crowley, Geoff, and R. R. Meier. "Disturbed O/N2 ratios and their transport to middle and low latitudes." In Midlatitude Ionospheric Dynamics and Disturbances, 221–34. Washington, D. C.: American Geophysical Union, 2008. http://dx.doi.org/10.1029/181gm20.

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Fejer, B. G., M. Blanc, and A. D. Richmond. "Post-Storm Middle and Low-Latitude Ionospheric Electric Fields Effects." In Earth's Magnetic Field, 415–37. Dordrecht: Springer Netherlands, 2017. http://dx.doi.org/10.1007/978-94-024-1225-3_13.

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Heelis, R. A. "Low- and middle-latitude ionospheric dynamics associated with magnetic storms." In Midlatitude Ionospheric Dynamics and Disturbances, 51–61. Washington, D. C.: American Geophysical Union, 2008. http://dx.doi.org/10.1029/181gm06.

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Hauchecorne, Alain, Sergey Khaykin, Philippe Keckhut, Nahoudha Mzé, Guillaume Angot, and Chantal Claud. "Recent Dynamic Studies on the Middle Atmosphere at Mid- and Low-Latitudes Using Rayleigh Lidar and Other Technologies." In Infrasound Monitoring for Atmospheric Studies, 757–76. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-75140-5_24.

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Raffi, Isabella, Claudia Agnini, Jan Backman, Eliana Fornaciari, Domenico Rio, and Heiko Pälike. "A New Low- to Middle-Latitude Biozonation and Revised Biochronology of Palaeogene Calcareous Nannofossils." In Springer Geology, 137–41. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-04364-7_28.

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Pfaff, Robert F., Carmen Liebrecht, Jean-Jacques Berthelier, Michel Malingre, Michel Parrot, and Jean-Pierre Lebreton. "DEMETER satellite observations of plasma irregularities in the topside ionosphere at low, middle, and sub-auroral latitudes and their dependence on magnetic storms." In Midlatitude Ionospheric Dynamics and Disturbances, 297–310. Washington, D. C.: American Geophysical Union, 2008. http://dx.doi.org/10.1029/181gm27.

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Sarnthein, Michael, and Kyaw Winn. "Reconstruction of Low and Middle Latitude Export Productivity, 30,000 Years BP to Present: Implications for Global Carbon Reservoirs." In Climate-Ocean Interaction, 319–42. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-2093-4_16.

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Jackson, John E. "Apple Production at Low Latitudes." In Temperate Fruit Crops in Warm Climates, 305–42. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-017-3215-4_11.

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Bashkuev, Yu B., V. B. Haptanov, D. G. Buyanova, and E. M. Mitkinov. "Schumann Resonances in Middle Latitudes of Asia." In Environmental and Space Electromagnetics, 607. Tokyo: Springer Japan, 1991. http://dx.doi.org/10.1007/978-4-431-68162-5_66.

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Conference papers on the topic "Middle and low latitudes"

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J. O. Werneck de Carvalho, Vinicius, Luiz Benyosef, and Angelo De Santis. "A Comparative Study of Pc’s 5-6 Geomagnetic Pulsations at Low and Middle Latitudes." In II PAN AMERICAN WORKSHOP ON GEOMAGNETISM – II PANGEO. Recife, Brazil: Even3, 2018. http://dx.doi.org/10.29327/2pangeo.a34.

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McDermid, I. S., Thierry Leblanc, Philippe Keckhut, Alain Hauchecorne, Chiao Y. She, and David A. Krueger. "Climatology of the middle-atmosphere temperature from long-term lidar measurements at mid and low latitudes." In Asia-Pacific Symposium on Remote Sensing of the Atmosphere, Environment, and Space, edited by Upendra N. Singh, Huanling Hu, and Gengchen Wang. SPIE, 1998. http://dx.doi.org/10.1117/12.319557.

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Ning, Wang, Guo Li-xin, Ding Zong-hua, Zhao Zhen-wei, and Lin Le-ke. "The difference in variation characteristics of the F2-peak height hmF2 at the low and middle latitudes." In 2016 11th International Symposium on Antennas, Propagation and EM Theory (ISAPE). IEEE, 2016. http://dx.doi.org/10.1109/isape.2016.7834101.

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Sergeev, I. Yu. "Evolution of low frequency electromagnetic fluctuations in low- and middle-latitude ionosphere." In 2011 XXXth URSI General Assembly and Scientific Symposium. IEEE, 2011. http://dx.doi.org/10.1109/ursigass.2011.6051174.

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Akhtemov, Z. S., Y. T. Tsap, and V. I. Haneychuk. "ON THE RELATIONSHIP OF CORONAL HOLES OF MIDDLE AND LOW LATITUDES WITH THE GENERAL MAGNETIC FIELD OF THE SUN." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2019. http://dx.doi.org/10.31725/0552-5829-2019-23-26.

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Liu, Ruoxiao, and Yuhua Zou. "Daytime Low and Middle Latitudes Plasma Density Enhancements Observed by Swarm Constellation during the 7–8 September 2017 Geomagnetic Storm." In 2019 6th International Conference on Space Science and Communication (IconSpace). IEEE, 2019. http://dx.doi.org/10.1109/iconspace.2019.8905978.

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Bakhmetieva, Nataliya V., Savely M. Grach, Evgeny N. Sergeev, and Alexei V. Shindin. "Results of Diagnostics of the Earth Lower Ionosphere by the Creation of Artificial Periodic Irregularities in High, Middle and Low Latitudes." In 2019 Russian Open Conference on Radio Wave Propagation (RWP). IEEE, 2019. http://dx.doi.org/10.1109/rwp.2019.8810203.

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Samanes, Jorge, and Fernanda Florez. "Analysis of the nighttime lower ionosphere for equatorial, low and middle latitudes over a region from 30°E and 60°E." In 2020 XXXIIIrd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS). IEEE, 2020. http://dx.doi.org/10.23919/ursigass49373.2020.9232313.

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V., Deepa, Geetha Ramkumar, Maria Antonita, and B. V. Krishnamurthy. "Estimation of gravity wave energy in the low latitude middle atmosphere using lidar." In Asia-Pacific Remote Sensing Symposium, edited by Upendra N. Singh, Toshikazu Itabe, and D. Narayana Rao. SPIE, 2006. http://dx.doi.org/10.1117/12.694341.

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Calle, A., D. Mateos, V. Cachorro, C. Toledano, C. Velasco, A. Benito, R. Gonzalez, A. M. De Frutos, J. C. Antuna Sanchez, and R. Roman. "Aerosol Optical Depth Characterization in Middle and Polar Latitudes." In IGARSS 2018 - 2018 IEEE International Geoscience and Remote Sensing Symposium. IEEE, 2018. http://dx.doi.org/10.1109/igarss.2018.8518625.

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Reports on the topic "Middle and low latitudes"

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Sanchez-Ayendez, Melba M. Mammogram Compliance Among Low-Income Middle-Women in Puerto Rico. Fort Belvoir, VA: Defense Technical Information Center, September 2001. http://dx.doi.org/10.21236/ada400641.

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Abay, Kibrom A., Hosam Ibrahim, and Clemens Breisinger. Food policies and obesity in low and middle income countries. Washington, DC: International Food Policy Research Institute, 2020. http://dx.doi.org/10.2499/p15738coll2.133679.

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McBurnie, Chris, Taskeen Adam, Thomas Kaye, and Björn Haßler. Zero-rating educational content in low- and middle-income countries. EdTech Hub, May 2020. http://dx.doi.org/10.53832/edtechhub.0004.

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Makela, Jonathan. Studies of Ionospheric Plasma Structuring at Low Latitudes from Space and Ground, Their Modeling and Relationship to Scintillations. Fort Belvoir, VA: Defense Technical Information Center, January 2009. http://dx.doi.org/10.21236/ada531096.

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Xie, Julian, and Kelly Brownell. Nutritious food procurement in cities in low and middle income countries. Global Alliance for Improved Nutrition (GAIN), June 2019. http://dx.doi.org/10.36072/wp.7.

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Sanchez-Ayendez, Melba M. Mammogram Compliance Among Low-Income Middle-Aged Women in Puerto Rico. Fort Belvoir, VA: Defense Technical Information Center, September 2002. http://dx.doi.org/10.21236/ada411452.

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Kreidenweis, S. M., and W. R. Cotton. Development and testing of an aerosol/stratus cloud parameterization scheme for middle and high latitudes. Final technical progress report, November 1, 1994--October 31, 1998. Office of Scientific and Technical Information (OSTI), May 1999. http://dx.doi.org/10.2172/355040.

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Bulat, Jennae, Anne Hayes, Wykia Macon, Renata Ticha, and Brian Abery. School and Classroom Disabilities Inclusion Guide for Low- and Middle-Income Countries. RTI Press, January 2017. http://dx.doi.org/10.3768/rtipress.2017.op.0031.1701.

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Hayes, Anne M., Eileen Dombrowski, Allison H. Shefcyk, and Jennae Bult. Learning Disabilities Screening and Evaluation Guide for Low- and Middle-Income Countries. RTI Press, April 2018. http://dx.doi.org/10.3768/rtipress.2018.op.0052.1804.

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Abstract:
Learning disabilities are among the most common disabilities experienced in childhood and adulthood. Although identifying learning disabilities in a school setting is a complex process, it is particularly challenging in low- and middle-income countries that lack the appropriate resources, tools, and supports. This guide provides an introduction to learning disabilities and describes the processes and practices that are necessary for the identification process. It also describes a phased approach that countries can use to assess their current screening and evaluation services, as well as determine the steps needed to develop, strengthen, and build systems that support students with learning disabilities. This guide also provides intervention recommendations that teachers and school administrators can implement at each phase of system development. Although this guide primarily addresses learning disabilities, the practices, processes, and systems described may be also used to improve the identification of other disabilities commonly encountered in schools.
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Sitabkhan, Yasmin, and Linda M. Platas. Early Mathematics Counts: Promising Instructional Strategies from Low- and Middle-Income Countries. RTI Press, July 2018. http://dx.doi.org/10.3768/rtipress.2018.op.0055.1807.

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This occasional paper examines common instructional strategies in early-grade mathematics interventions through a review of studies in classrooms in low- and middle-income countries. Twenty-four studies met the criteria for inclusion, and analyses reveal four sets of instructional strategies for which there is evidence from multiple contexts. Of the 24 studies, 16 involved the use of multiple representations, 10 involved the use of developmental progressions, 6 included supporting student use of explanation and justification, and 5 included integration of informal mathematics. Based on the review, we provide conclusions and recommendations for future research and policy.
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