Policy concerns in Bulgarian food distribution

The Bulgarian food distribution system, like those of its Central and East European neighbours, lags behind the West in critical performance areas. Previous research quantified Central and East European food distribution deficiencies on the basis of a five factor model. This study investigates the attitudes of 250 Bulgarian consumers using these same five factors: food processing, quality, cost, availability and retailing. The findings show that the Bulgarian food distribution system does not satisfy consumer wants as well as do systems in other former communist countries in four of the five factors. At the same time, Bulgarian consumers are more satisfied than UK and US consumers in the system's ability to make some foods available. The study also shows that Bulgarian consumers who use privatised shops perceive the system more positively than those who use state and cooperative outlets. The implications of these and other findings are discussed in terms of critical policy concerns for government and industry stakeholders.     

A low plain between arcadia and agronomy: Ippolito Nievo and the Friulan landscape

An analysis of the historical and cultural context of a large number of literary works illuminates the concept of landscape, a recurrent theme in contemporary humanistic geography. In this context, the works of Ippolito Nievo present an opportunity to look closer at the socio-economic circumstances of his time while also offering suggestive interpretative elements about the attitudes held concerning the wetlands of the lower Friulan plain.     

Origin and implications of mafic xenoliths associated with Cenozoic extension-related volcanism in the Válencia Trough, NE Spain

Summary The Válencia Trough of northeastern Spain represents a poorly understood region of Cenozoic extension-related magmatism in western Europe. We present chemical data on mafic xenoliths and their host basalt from the Roca Negra cinder cone in the Catalán Volcanic Zone in the Válencia Trough. The xenoliths consist of augite+hornblende+ oxides±plagioclase±apatite±olivine::Lbiotitelorthopyroxene, and range from clinopyroxenites and hornblendites to gabbroic rocks. The major and trace element compositions of the xenoliths are compatible with formation as cumulates from a range of olivine tholeiitic to strongly alkaline magmas, and show a strong affinity to the Middle Miocene to Recent rift-related magmatism in the Cátalan Volcanic Zone. The xenoliths formed at temperatures of 1110–1180 °C, pressures of 2–7 kb (with 10 kb as the upper limit), and oxygen fugacities corresponding to 1–2 log units above the NNO oxygen buffer. The estimated pressure range implies formation in magma chambers within the crust, possibly also near the crust/mantle boundary (underplating). The presence of crustal cumulates indicates that the total volume of magmas emplaced into the crust in the Cátalan Volcanic Zone may be significantly larger than indicated by surface exposures. Isotopic compositions of the xenoliths are⁸⁷Sr/⁸⁶Sr: 0.703537–0.703647,¹⁴³Nd/¹⁴⁴Nd: 0.512732–0.512766,²⁰⁶Pb/²⁰⁴Pb: 18.097–19.106,²⁰⁷Pb/²⁰⁴Pb: 15.522–15.579, and²⁰⁸Pb/²⁰⁴Pb: 37.850–38.794. This range suggests the involvement of two mantle source components. One of these may be the low-velocity component recognized in Cenozoic magmatism in the eastern Atlantic Ocean to central Europe and western Mediterranean. The other component, which differs from those involved in other domains of Cenozoic volcanism in Europe and adjacent areas, may be located in the lithospheric mantle underlying NE Spain, which was metasomatized during late Variscan to early Alpine deformation.

---

Herkunft und Bedeutung mafischer Xenolithe aus känozoiscben Extensions-bezogenen Vulkaniten aus dem Valencia Trog, Nordost-Spanien

Zusammenfassung Der Válencia Trog in Nordost-Spanien stellt eine noch wenig verstandene Region mit känozoischen Extensions-bezogenern Magmatismus in Westeuropa dar. Wir geben hier chemische Daten über mafische Xenolithe und ihre basaltischen Muttergesteine aus dem Roca Negra Kegei in der vulkanischen Zone von Catalan im Valencia Trog. Die Xenolithe bestehen aus Augit+Hornblende+Oxiden±Plagioklas±Apatit±Olivin±Biotit±Orthopyroxen und reichen in ihrer Zusammensetzung von Klinopyroxeniten und Homblenditen his zu gabbroischen Gesteinen. Die Haupt- und Spurenelementzusammensetzung der Xenolithe entspricht einer Kumulatbildung aus Olivin-tholéitischen bis stark alkalischen Magmen and zeigt eine deutliche Affinität mit dem mittelmiozanen bis rezenten Rift-bezogenen Magmatismus in der vulkanischen Zone von Catalan. Die Xenolithe bildeten sich bei Temperaturen von 1.110 bis 1.180 °C und bei Drucken von 2–7 kb (mit 10 kb als Obergrenze) und bei Sauerstoff-Fugazitäten, die 1 bis 2 log Einheiten über dem NNO Sauerstoff-Puffer liegen. Die abgeschätzten Drucke weisen auf Bildung in Magmakammern innerhalb der Kruste bin, womölich auch in der Nähe der Kruste-Mantelgrenze (Underplating). Das Vorkommen von krustalen Kumulaten zeigt, daß das gesamte Volumen von Magma, das in die Kruste der vulkanischen Zone von Catalan eingedrungen ist, wesentlich größer ist als das, das man aus Oberflächen-Ausbissen entnehmen k6nnte. Die Isotopen-Zusammensetzung der Xenolithe sind⁸⁷Sr/⁸⁶Sr: 0.703537–0.703647,¹⁴³Nd/¹⁴⁴Nd: 0.512732–0.512766,²⁰⁶Pb/204 Pb: 18.097–19.106,²⁰⁷Pb/²⁰⁴Pb: 15.522–15.579, and²⁰⁸Pb/²⁰⁴Pb: 37.850–38.794. Dies läßt erkennen, daß es sich bier um zwei verschiedene Mantel-Quellen handelt. Eine davon könnte die Niedrig-Geschwindigkeitskomponente sein, die man in känozoiscben Magmatiten des östlichen Atlantischen Ozeans, sowie in Zentraleuropa und im westlichen Mittelmeer erkannt hat. Die andere Komponete unterscheidet sich von jenen, die in anderen Bereichen von känozoischem Vulkanismus in Europa und benachbarten Gebieten vorkommen. Sie könnte im lithosphärischen Mantel unterhalb von Nordost-Spanien liegen, der während der variszischen bis zur frühalpidischen Deformation metasomatisch beeinflußt wurde.

---

---

With 10 Figures     

Isotopic,mineralogical, and thermobarometric variations of Al-Wahbah crater (Maklaa Tameya), Kishb area,Saudi Arabia

The Cenozoic volcanism of western Saudi Arabia extends from southern Yemen to Jordan northward. They cover an area of nearly 180,000 km². The rocks are dominated by alkali olivine basalts and olivine basalts. Al-Wahbah crater, a part of Harrat Kishb, represents a model occurrence to study the gneisses of these rocks. New mineral chemistry and isotopic data are presented. It aims to follow the isotopic, mineralogical, and thermobarometry variations among these volcanics. Amphiboles of the studied volcanics belong to the monoclinic calcic group. The chemistry of the amphibole crystals shows two ranges of pressure. They are 3.6–5.6 and 0.38–0.78 kbar. The Al_iv values of the amphiboles are in the range of 1.202 and 1.407, indicating corresponding temperature condition of 820–920 and 620–720 °C, respectively. The feldspar of the studied samples has the composition of plagioclase, though some grains have sanidine composition. They are formed in temperature range of 975 and 400 °C. The coexisting amphiboles and plagioclases indicate two sets of pressure and temperature. They are 540–575 °C (3.5–4 kbar) and 510–525 °C (~2 kbar), respectively. Rb–Sr isochron of the whole rock yields an age of 0.867 ± 0.160 Ma with initial Sr⁸⁷/Sr⁸⁶ of 0.702 ± 0.00086. The low initial ratio of Sr⁸⁷/Sr⁸⁶ together with positive values of εNd today implies that the studied volcanics have mantle source. Meanwhile, the present isotopic data suggest extraction of juvenile magma from asthenosphere source. The present study shows that the Al-Wahbah crater rocks belong to Cenozoic basalts and indicate EM-I-like signature.     

Plio-pleistocene volcanism in the Andean Cordillera of Central Chile (33∘ – 40∘ S. L.)

Recent field studies in the Andean Cordillera of Central Chile (33–40 S. L.) have shown a widespread distribution around the Chile-Argentina border of pliopleistocene volcanic and pyroclastic flow (5-1 m. y. K/Ar). The older ages are found in Rio Blanco (Santiago) area and the younger in the Cola de Zorro area. They cover horizontal to sub-horizontally, with strong unconformity their meso-cenozoic basement.In the Rio Blanco area the most silicic rocks are dactic and rhyolitic ignimbrites and lava flows. They are similar to the Rhyolitic Formation (Zeil andPichler, 1967) of northern Chile.South of 36 S. L. most of the rocks are calcalkaline basalts and andesites except for the samples from the Pino Hachado area, which plot nearRittman's alkaline field. Chemical inhomogenety of the plio-pleistocene volcanic rocks is thus present in the Andes of Central Chile.

---

Zusammenfassung Neue Arbeiten über die Geologie der Cordillera de los Andes im zentralen Abschnitt Chiles (33–40 S) haben eine enorme Verbreitung von plio/pleistozänen Vulkaniten (5-1 m. a.) vor allem in der Grenzregion mit Argentinien ergeben. Die höheren Alter fand man im Gebiet von Rio Blanco (Santiago) und die jüngsten im Gebiet von Cola de Zorro.Die Vulkanite bedecken mit einer horizontalen bis subhorizontalen Verbreitung und mit einer scharfen Diskordanz alle Gesteinsserien des Mesozoikums und Känozoikums.Im Gebiet von Rio Blanco handelt es sich um Ignimbrite rhyolitischer und dacitischer Zusammensetzung. Die kieselsäurereichsten Proben sind ähnlich den Gesteinen der Rhyolit-Formation vonZeil &Pichler (1967) in Nordchile.Südlich von 36 S hat die Mehrheit der Proben eine andesitische und basaltische Zusammensetzung. Es sind kalkalkaline Gesteine mit Ausnahme der Proben von Pino Hachado, die einen starken alkalinen Trend nach dem Diagramm vonRittmann haben. Auf diese Weise ergibt sich eine chemische Inhomogenität bei den plio/pleistozänen Vulkaniten von Zentralchile.

---

Resumen Los más recientes trabajos de geología de campo en la Cordillera de los Andes de Chile Central (33–40 L. S.) han evidenciado enormes extensiones de rocas volcánicas pliopleistocénicas (5-1 m. a.) sobre todo en el área limítrofe con Argentina. Las mayores edades fueron encontradas en el area de Rio Blanco (Santiago) y las más jóvenes en el area de Cola de Zorro.Las rocas volcánicas plio-pleistocénicas cubren con disposición horizontal a subhorizontal y con fuerte discordancia a todas las rocas subyacentes del Meso y Cenozoico.En el area de Río Blanco las rocas son ignimbritas de composición riolítica a dacítica y corresponden a las muestras más silícicas similar a rocas de la Formación Riolítica del norte de Chile deZeil yPichler (1967).Al sur del paralelo 36 S la mayoría de las muestras son de composición andesítica y basáltica de naturaleza calcoalcalina excepto las muestras de Pino Hachado que presentan fuerte afînidad alcalina según el diagrama deRittmann. De esta manera se muestra que existe inhomogeneidad química en las rocas volcánicas plios-pleistocénicas de Chile Central.

---

Cordillera de los Andes (33°–40° S) , . - (), --. , , . - . 36° . - , . . . , - .

     

Damage of topaz and other minerals in the electron microscope

Summary Hydroxyl bearing topaz suffers beam-damage in the electron microscope. Irradiation by the beam rapidly produces contrast from strain fields around small needle-shaped pores about 2–5 nm wide and 30–120 nm long, produced by the loss of hydrogen as water and/or hydrogen fluoride. In the majority of cases the damage ceases after a short period of time, and the topaz electron diffraction pattern remains apparently unchanged. In a few cases complete breakdown of the topaz occurs to produce mullite and/or fine-grained -alumina, the latter usually being sputtered onto the carbon support film. The different degrees of breakdown which are found in the electron beam are similar to reactions which occur on heating in air. Although the main factor which determines the degree of beam-induced damage which occurs is believed to be temperature, the heating effect of the beam is alone unlikely to cause the reactions. The lowering of reaction temperature is attributed to mechanically induced enhancement of diffusion in the electron beam and to the weakening of chemical bonds by ionisation effects. The strain fields found in topaz were also produced in samples of humite and apatite observed in the electron microscope, and the formation of fine-grained metal oxides was found in several silicates and phosphates.

---

Zerstörung von Topas und anderen Mineralen im Elektronenmikroskop

Zusammenfassung Hydroxil-hältige Topase unterliegen im Elektronenmikroskop einer Zerstörung durch den Elektronenstrahl. Durch die Bestrahlung entstehen rasch Kontraste von gestörten Bereichen rund um kleine nadelförmige Poren von etwa 2–5 nm Durchmesser und 30–120 nm Länge, die durch den Verlust von Wasserstoff als Wasser und/oder Hydrogenfluorid verursacht werden. Meist hört die Zerstörung nach kurzer Zeit auf und das Elektronen-Beugungsbild des Topases bleibt anscheinend unverändert. In wenigen Fällen kommt es zu einem kompletten Zusammenbruch des Topases und es entsteht Mullit und/oder feinkörniges -Al₂O₃. Die unterschiedlichen Grade des Zusammenbruchs, die im Elektronenstrahl beobachtet werden, sind Reaktionen ähnlich, die beim Erhitzen in Luft auftreten. Obwohl als Hauptfaktor, der den Grad der Strahlinduzierten Zerstörung bestimmt, die Temperatur angenommen werden kann, ist es unwahrscheinlich, daß der Hitzeeffekt des Strahls allein die Reaktionen verursacht. Die Erniedrigung der Reaktionstemperatur wird der mechanisch bedingten Erhöhung der Durchdringungsfähigkeit des Elektronenstrahls und der Schwächung der chemischen Bindung durch Ionisierungseffekte zugeschrieben. Die im Elektronenmikroskop in Topas gefundenen gestörten Bereiche wurden auch in Proben von Humit und Apatit beobachtet; in verschiedenen Silikaten und Phosphaten wurde die Bildung feinkörniger Metalloxide gefunden.

---

---

With 3 Figures

---

Dedicated to Professor Dr.Josef Zemann on the occasion of his 6oth birthday.     

Das Amazonas-Entwässerungssystem in Zeit und Raum

The history of the Amazon river system is fixed by two geologic main events: the development of the Atlantic Ocean caused by the break up of the Gondwana continent, and the evolution of the Andean orogenesis. On the other hand the direction of the drainage flow is caused by the Amazon Graben in the subsoil. Also the pleistocene glaciation influenced the Amazon drainage system by lowering the sea level as result of ice fixing in polar regions.     

On the formation of the vein-type uranium „Yellow Ores“ from the Schwarzach Area (NE-Bavaria,Germany) and on the behaviour of P,As, V and Se during supergene processes

Most of the U occurrences situated at the western edge of the Bohemian Massif show in their upper parts secondary U minerals. The immigration (P, V, As and Se) from the country rocks and the ore body, via saprolite and paleosoils into the secondary ore minerals is investigated. The P content is suggested to be closely related to hydromorphic paleosoils. From those intermediate stages it may have been brought into the upper parts of the vein structures. No laterogenic impoverishment in the wall rocks with respect to phosphorus or apatite could be determined. The arsenic distributions is also governed as at other sulfide deposits by underlying sulfides and reducing conditions of a primary hypogene ore zone, whereas vanadium content in U secondary minerals is closely related to the enclosing country rocks. Granites, on account of their low content in mafic minerals, have low V contents in U secondary minerals. Besides the Schwarzach Area, U ore mineralisations from other U occurrences have been investigated. Some of the U deposits are certainly of “per ascensum” origin and their secondary U mineralisation can well be interpreted as having been derived from the underlying primary “black ores”. However, some mineralisations cannot be classified with certainty as being “per ascensum”. They include some properties pointing to “per ascensum” (e. g. sulfide association) as well as characteristics typical for “per descensum” (small depth, large amounts of U-VI minerals). The mode of formation may in some cases be as follows: Variscan or Alpine ore mineralisations of no economic significance may have formed a reducing environment and caused U to be concentrated. Younger redistribution processes influenced by modern tectonics (uplifting) and the fluviatile drainage pattern have taken place and in some cases destroyed the primary deposits or enhanced the ore mineralisation. These processes roughly resemble those described from sandstone — hosted roll front deposits.     

Scientific objectives of the Monsoon Experiment (MONEX)

The Monsoon Experiment is the core of the GARP Monsoon Subprogramme, which is a major international effort to achieve a better understanding of the Planetary monsoon circulation, the major seasonal perturbation of the general circulation of the atmosphere and the influence of the annual cycle of precipitation associated with the monsoon on the agriculture of the many populous nations of the region.This is a summary report of the International MONEX Planning Meetings, which were held in Yerevan, USSR, March 1973; Singapore, November 1974; New Delhi, March 1977; and Kuala Lumpur, February 1978.MONEX represents a group of observational studies during the First GARP Global Experiment (FGGE) over the South China Sea (December 1978), Arabian Sea (May–June 1979), and Bay of Bengal (July–August 1979). These periods will permit study of most of the significant aspects of the winter and summer monsoons. This is elaborated on in Sections 2 and 3.     

The Triassic in Thailand

The tectonic movements which occurred in Thailand between the Permian and the Jurassic (Indosinian Orogeny) caused the uplifting and subsidence of areas which were dominant paleogeographic features during the Triassic. The strong orogenic movements during the Norian caused an alteration of the paleogeographic conditions.The two sedimentation cycles of the Triassic comprised a marine facies development from the Skythian to the early Norian and a terrestrial one from the later Norian to the Rhaetian/Liassic.The development of the facies and structure of the Triassic sediments, as well as the intrusion and effusion of igneous rocks, are due to the subduction of oceanic crust beginning in the Carboniferous and to the collision of the Eurasian with the Indochina Plate during the Norian.

---

Zusammenfassung Die zwischen Perm und Jura in Thailand auftretenden tektonischen Bewegungen (Indosinische Orogenese) führten zur Bildung von Hebungs- und Senkungsgebieten, die die Paläogeographie in der Trias beherrschten. Die starken orogenen Bewegungen im Nor führten zu einer Umgestaltung der paläogeographischen Verhältnisse.Die beiden während der Trias auftretenden Sedimentationszyklen bestehen aus einer marinen Faziesentwicklung vom Skyth bis zum unteren Nor und einer terrestrischen vom oberen Nor bis zum Rhät/Lias.Die fazielle und strukturelle Entwicklung der Triassedimente sowie die Intrusion bzw. Effusion von Eruptivgesteinen sind auf die seit dem Karbon erfolgende Subduktion ozeanischer Kruste und die Kollision der Eurasiatischen Platte mit der Indochinesischen Platte im Nor zurückzuführen.

---

Résumé Les mouvements tectoniques («Orogenèse Indosinienne») intervenus entre le Permien et le Trias en Thaïlande se sont traduits en soulèvements et affaissements qui ont dominé la paléogéographie du Trias. Les forts mouvements orogéniques du Norien ont conduit à transformer les rapports paléogéographiques.Les deux cycles sédimentaires du Trias consistent dans le développement d'un faciès marin du Scythien au Norien inférieur, et d'un faciès continental du Norien supérieur au Rhétien/Lias. L'évolution du faciès et de la structure des sédiments du Trias, l'intrusion et l'effusion des roches ignées sont attribuées à la subduction de la croute océanique consécutive au Carbonifère, et à la collision de la «Plaque Euroasiatique» avec la «Plaque Indochinoise» au Norien.

---

— — , . . - , - — . , , , , .