Consumer Acculturation in Situ: The Continuing Legacy of French Colonization in North Africa

Author(s):  
Elizabeth C. Hirschman ◽  
Mourad Touzani
2020 ◽  
Vol 13 (7) ◽  
pp. 4009-4033
Author(s):  
Anteneh Getachew Mengistu ◽  
Gizaw Mengistu Tsidu

Abstract. Africa is one of the most data-scarce regions as satellite observation at the Equator is limited by cloud cover and there is a very limited number of ground-based measurements. As a result, the use of simulations from models is mandatory to fill this data gap. A comparison of satellite observation with model and available in situ observations will be useful to estimate the performance of satellites in the region. In this study, GOSAT column-averaged carbon dioxide dry-air mole fraction (XCO2) is compared with the NOAA CT2016 and six flask observations over Africa using 5 years of data covering the period from May 2009 to April 2014. Ditto for OCO-2 XCO2 against NOAA CT16NRT17 and eight flask observations over Africa using 2 years of data covering the period from January 2015 to December 2016. The analysis shows that the XCO2 from GOSAT is higher than XCO2 simulated by CT2016 by 0.28±1.05 ppm, whereas OCO-2 XCO2 is lower than CT16NRT17 by 0.34±0.9 ppm on the African land mass on average. The mean correlations of 0.83±1.12 and 0.60±1.41 and average root mean square deviation (RMSD) of 2.30±1.45 and 2.57±0.89 ppm are found between the model and the respective datasets from GOSAT and OCO-2, implying the existence of a reasonably good agreement between CT and the two satellites over Africa's land region. However, significant variations were observed in some regions. For example, OCO-2 XCO2 are lower than that of CT16NRT17 by up to 3 ppm over some regions in North Africa (e.g. Egypt, Libya, and Mali), whereas it exceeds CT16NRT17 XCO2 by 2 ppm over Equatorial Africa (10∘ S–10∘ N). This regional difference is also noted in the comparison of model simulations and satellite observations with flask observations over the continent. For example, CT shows a better sensitivity in capturing flask observations over sites located in North Africa. In contrast, satellite observations have better sensitivity in capturing flask observations in lower-altitude island sites. CT2016 shows a high spatial mean of seasonal mean RMSD of 1.91 ppm during DJF with respect to GOSAT, while CT16NRT17 shows 1.75 ppm during MAM with respect to OCO-2. On the other hand, low RMSDs of 1.00 and 1.07 ppm during SON in the model XCO2 with respect to GOSAT and OCO-2 are respectively determined, indicating better agreement during autumn. The model simulation and satellite observations exhibit similar seasonal cycles of XCO2 with a small discrepancy over Southern Africa (35–10∘ S) and during wet seasons over all regions.


2015 ◽  
Vol 170 ◽  
pp. 280-289 ◽  
Author(s):  
Nazzareno Pierdicca ◽  
Fabio Fascetti ◽  
Luca Pulvirenti ◽  
Raffaele Crapolicchio ◽  
Joaquin Muñoz-Sabater

2018 ◽  
Vol 3 (2) ◽  
pp. 191-206 ◽  
Author(s):  
Andrea Rodríguez-Antón ◽  
A. César González-García ◽  
Juan Antonio Belmonte

Digital tools are increasingly used in cultural astronomy, so that it is now more important than ever to assess their precision and reliability, and to identify what uncertainties they may introduce. The present work aims to address these issues by comparing a dataset of orientations of Roman cities in the Iberian Peninsula measured in situ with measurements of the same structures obtained through different digital tools. By this, it is possible to estimate the errors that using these techniques introduce and to establish precision limits to data in future work. The results of this preliminary study are then implemented in an archaeoastronomical research project in North Africa, where some on-site measurements had been made in previous fieldwork campaigns by members of the group prior to the current political unrest that now prevents work at some sites in the region. In these instances, Google Earth Pro (2017) and HeyWhatsThat (Kosowsky 2012) have been key tools that have allowed us to complete a survey stretching from present-day Morocco to Libya, as well as to extract a preliminary outline of orientation trends in Roman Africa.


Bothalia ◽  
1983 ◽  
Vol 14 (3/4) ◽  
pp. 411-416 ◽  
Author(s):  
P. Quézel

PRESENT VEGETATION AND FLORA OF NORTHERN AFRICA, THEIR MEANING IN RELATION TO THEIR ORIGIN, EVOLUTION AND MIGRATIONS OF FLORAS AND THE STRUCTURES OF PAST VEGETATION In the light of recent works and biogeographic synthesis, the Mediterranean flora appears more and more as a heterogeneous entity, reflecting, to a great extent, the palaeogeographic and palaeoclimatic history of the region. In particular, the co-existence of elements of southern stock and of northerly elements, presently points to the possibilities of exchange which occurred very early in the Tertiary between the Gondwanian type of floras or the less  tropical types and the Laurasian floras.The tropical elements are numerous and can be linked to various entities according to their age; a pantropical entity comprising in particular, Tetraclinis and Warionia, but also various families, is common to all the tropical regions and, without any doubt, contemporary with the dismemberment of Gondwana; a north-tropical entity peculiarly common to California and the Mediterranean region; a palaeotropical entity strongly heterogeneous and complex. One finds there: —  thermophilous sclerophyll types often linked to the African rainforest species, — old xerophilous types, distributed in South Africa and north of the Equator (randflora), — endemic taxa of high African mountains, showing affinities with Ethiopian species or of the high African mountains, —  taxa more recently arrived or even common sahelian species settled during the last pluvial. The elements of extratropical stock are composed of autochthonal or Mediterraneo-Tertiary elements, and of northern elements. The Mediterraneo-Tertiary elements are the remnants of differentiated floras generally in situ on the banks of the Tethys and on the micro-plates which occur there. The role of the Iberian micro-plate is particularly important in the western Magreb. It is advisable to associate them with various species belonging to the Irano-touranian and Saharo-Arab stocks, whose settlement is often recent. An oro-Mesogean entity is particularly important and brings together the endemo-vicariant taxa generally occurring from the Atlas to the western Himalayas. The northern elements bring together a mesothermal entity, a remnant o f the pre-glacial Lauresian floras, poorly represented in north Africa, a microthermal northern entity generally comprising species recently established and a north-alpine entity contemporary with the last glaciations, extremely localized on the high Atlas mountains. Finally, the origin of the main characteristic formations of the Mediterranean stages is examined and discussed.


2020 ◽  
Author(s):  
Yahia Mehdi Seddik Cherifi ◽  
Selma Amrani

AbstractObjectiveWe assessed DNA conservation using a range of archaeological skeletal samples from Sudan (Missiminia in Upper Nubia, 350 B.C.E to 1400 C.E) from the unfavorable conditions of the Saharan milieu and humidity of the Nile valley by tracking maternal lineage on the ‘X-Group’ (Ballaneans).MethodWe were able to extract, amplify, and sequence mt-DNA HVS-I (Sanger sequencing method) from 11 petrous bone samples, eight for the X-Group set and three for the reference set (one Christian, one Late Meroitic, and one Meroitic).ResultsIt was possible to find the haplogroups (L1b, L2, L3, H2, N, T1a, X and W) and to carry out comparative data analysis in relation to haplogroup data cited in the literature. This investigation into the maternal lineage of X-Group (350 to 500 C.E.) origins allowed us to validate the efficiency of petrous bone sampling from ancient human remains from the Nile-Saharan milieu and established that the Ballaneans experienced an in-situ development with more admixture from the Levant region and North Africa.ConclusionsOur study used mt-DNA (HVS-I) to look for the biological origins of the X-Group from Upper-Nubia and demonstrated the feasibility of ancient DNA research on skeletons from the Nile-Saharan environment. The use of Next Sequencing Generation (NGS) should optimize and improve the detection of shorter DNA strands and their sequencing in complete genomes from ancient skeletal remains (petrous bones) from hot and humid environments.


1984 ◽  
Vol 75 ◽  
pp. 743-759 ◽  
Author(s):  
Kerry T. Nock

ABSTRACTA mission to rendezvous with the rings of Saturn is studied with regard to science rationale and instrumentation and engineering feasibility and design. Future detailedin situexploration of the rings of Saturn will require spacecraft systems with enormous propulsive capability. NASA is currently studying the critical technologies for just such a system, called Nuclear Electric Propulsion (NEP). Electric propulsion is the only technology which can effectively provide the required total impulse for this demanding mission. Furthermore, the power source must be nuclear because the solar energy reaching Saturn is only 1% of that at the Earth. An important aspect of this mission is the ability of the low thrust propulsion system to continuously boost the spacecraft above the ring plane as it spirals in toward Saturn, thus enabling scientific measurements of ring particles from only a few kilometers.


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