Anti-Semitism in German geography 1900–1945

The number of Anti-Semitic opinions found in geographical and geopolitical literature gives evidence of a wide-spread hostility towards Jews before 1945. Only very few critical dissidents branded Anti-Semitism as propaganda of political rightists. The extent to which Anti-Semitism served as an ideological bridge between geography and geopolitics in Germany till 1945 must be established. But independent from geopolitics, there are lots of proof for an autochthonously developed Anti-Semitism among German university geographers long before geopolitics was created. All in all geopolitics had no innovative effect on the research and the theory of political geography in Germany till 1945. Its main topics, epistemological premises and methodological apparatus grew on the substratum of authochthonous traditions created in the 19th century. Geopolitics only takes up basic reflections that already exist.     

The observability of topological defects with ground-based interferometers

Topological defect theories lead to non-Gaussian features on maps of fluctuations of the cosmic microwave background radiation (CMBR), which enable us to distinguish them from maps predicted by standard inflationary models. We have recently presented a maximum entropy method (MEM) which simultaneously deconvolves interferometer maps of CMBR fluctuations, and separates out foreground contaminants. By applying this method to simulated observations using a realistic ground-based interferometer, we demonstrate that it is possible to recover the prominent hotspots in the CMBR maps which delineate individual defects, even in the presence of a significant Galactic foreground.     

Visualization of three-dimensional datasets

The effective visualization of three-dimensional (3d) datasets, both observationally and computationally derived, is an increasing problem in solar physics. We present here plots of computational data derived from the 3d reconstruction of the magnetic field of a loop system, rendered as anaglyphs. By combining images of the same 3d object from two slightly different angles a realistic and useful 3d effect is obtained, aiding data visualization. The application of the same technique to real solar data (such as from the Coronal Diagnostic Spectrometer (CDS) on board the Solar and Heliospheric Observatory (SOHO)) is discussed.     

Clast sizes of ejecta from explosive eruptions on asteroids: implications for the fate of the basaltic products of differentiation

We use a simple model of the formation, growth, coalescence and migration of veins of basaltic melt generated by partial melting in chondritic asteroids to deduce the sizes of, and pressures within, the fluid-filled dikes reaching the surfaces of such bodies. The gas contents ( 1000 ppm of mainly CO and N₂) of the asteroids were high enough that bubbles of free gas trapped in the melt veins gave the basaltic melts significant buoyancy; expansion of these gases as a dike opened to the vacuum at the surface led to fragmentation of the melts into liquid droplets which were transported upwards by the accelerating gases to the surface. The sizes of these droplets and, hence, of the pyroclastic glass beads into which they cooled, are calculated to lie in the range 30 μm to 4 mm; this range is essentially independent of the size or gas content of the asteroid parent and only weakly dependent on the internal pressure of the erupting fluid. The fate of the pyroclasts, however, does depend on all of these factors. At very low internal pressures, significant separation of the gas and liquid in a rising dike may take place and not all of the liquid will be expelled from the dike when it opens to the surface. For relatively large ( 100 km radius) asteroids with relatively low ( 300 ppm) gas contents, the larger clasts are too heavy to be lifted from the level at which magma fragmentation takes place by the gas flow and so would also remain behind to form basaltic veins. The apparent absence of basaltic veins in meteorites then implies both that internal pressures in near-surface dikes were generally greater than 0.3 MPa and that low gas contents were not common. Finally, as long as pyroclasts are lofted from the magma fragmentation level, they will be accelerated to at least 90% of the final gas speed. If this speed exceeds the escape speed from the asteroid (as happens readily for high gas contents and small asteroids), the pyroclasts will be expelled into space and lost from the meteorite record. Otherwise (low gas contents or large asteroids), they will eventually fall back to be incorporated into the surface regolith, modifying the chemical and physical properties of meteorites subsequently derived from it.     

Analysis of microtremors within the Provadia region near a salt leaching mine

By analysis of microtremors recorded with digital seismological monitoring equipment near the Provadia salt diapir (Bulgaria), two groups of events showing different characteristics have been detected in the vicinity of the salt production area. The first group of events has low magnitudes and is located at a distance of about 1 km from the top of the salt diapir. These events show low stress drops. The second group of tremors is located outside the salt diapir. The corresponding magnitudes and stress drops are larger. The first class of events seems to be related to processes at the contour of the salt leaching caverns, whereas the origin of the second group seems to be connected with stress redistribution processes around the salt body. Based on this analysis, the tectonic model of the Provadia salt diapir has been modified.     

K－Ar测年法在确定沉积岩成岩时代中的应用——以鄂尔多斯盆地为例

根据伊利石Ｋ－Ａｒ测年法研究，确定鄂尔多斯盆地存在两期与构造运动有关的成岩作用事件：即与早期燕山运动有关的侏罗纪（１７０—１６０Ｍａ）和与晚期加里东运动有关的志留－泥盆纪（４２０－３７０Ｍａ）成岩作用时代。为了揭示碎屑物质对Ｋ－Ａｒ年龄的影响和伊利石成岩作用的机制，本文提出了一个通过观察Ｋ－Ａｒ年龄随深度变化的趋势来进行判断的模式。在Ｋ－Ａｒ年龄小于地层时代的条件下，Ｋ－Ａｒ年龄与深度呈正相关，或者很相近的Ｋ－Ａｒ年龄与深度变化无关均标志着没有或很少有碎屑物质的影响；同时，前者指示逐渐埋藏条件下的成岩作用，而后者则反映短暂的热事件引起的成岩作用事件。     

IGU study group on “famine research and food production systems”

The International Geographical Union Reports

IGU study group on famine research and food production systemsNewletter No. I, November 1988     

Trondhjemites,tonalites and diorites in the South Portuguese Zone and their relations to the vulcanites and mineral deposits of the Iberian Pyrite Belt

In the South Portuguese Zone close associations of diorites, tonalites and trondhjemites occur north of the Pyrite Belt. The period of their emplacement is Pre-Carboniferous and not, as has generally been assumed, Variscanpostorogen. The trondhjemitic intrusive suite and the Lower Carboniferous spilite-keratophyre association are related through their comagmatic derivation. Both series share sodium dominance, low concentrations of large-ion lithophile elements, indicators of a water-rich original magma and a deficient scorification of the element potential, which was acummulated in the sulphide and manganese deposits of the Pyrite Belt through post-volcanic hydrothermal processes. The mineralogically and geochemically primitive composition of both plutomtes and vulcanites, their mode of eruption from acid to basic facies as well as their position in the orogenic process indicate that they represent products of a successively proceeding partial melting of subducting oceanic crust. The trondhjemitic intrusives are the initialites in the magmatic-orogenic development.

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Zusammenfassung In der Südportugiesischen Zone treten nördlich des Pyritgürtels enge Vergesellschaftungen von Dioriten, Tonaliten und Trondhjemiten auf. Der Zeitraum ihrer Platznahme ist päkarbonisch und nicht, wie bisher allgemein angenommen, variszisch-postorogen. Die trondhjemitische Intrusivsequenz und die unterkarbonische Spilit-Keratophyr-Assoziation sind in weiten Bereichen durch komagmatische Herkunft verbunden. Gemeinsamkeiten beider Abfolgen sind ihre Na-Dominanz, die niedrigen Gehalte an gro\ionigen Elementen, die Anzeichen für ein wasserreiches Ausgangsmagma und die mangelhafte Verschlackung des Elementpotentials, das in den Sulfid- und Manganlagerstätten des Pyritgürtels während postvulkanischer, hydrothermaler Proze\e angereichert wurde. Die mineralogisch wie geochemisch primitive Zusammensetzung sowohl der Plutonite wie der Vulkanite, ihr Eruptionsmodus von saurer zu basischer Fazies sowie ihre Position im orogenen Ablauf deuten darauf hin, da\ sie die Produkte einer sukzessiv fortschreitenden Aufschmelzung subduzierender, ozeanischer Kruste darstellen. Die trondhjemitischen Intrusiva sind die Initialite innerhalb der magmatisch-orogenen Entwicklung.

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Résumé Dans la zone sud du Portugal, il existe, au nord de la ceinture pyriteuse, des associations étroites de diorites, de tonalites et de trondhjémites. Leur mise en place date de la période pré-carbonifère et non, comme on l'avait généralement admis jusqu'à présent, de la période varisque post-orogénique. Le faisceau intrusif trondhjémitique et l'association spilite-kératophyre du Carbonifère inférieur sont liés par une origine comagmatique. Les points communs des deux successions sont leur dominante sodique, les faibles teneurs en éléments à gros ions, les indices d'un magma de départ aquifère et la scorification réduite du potentiel d'éléments qui, dans les gisements de sulfure et de manganèse de la ceinture pyriteuse a été enrichi par des processus post-volcaniques et hydrothermaux. La composition primitive, tant minéralogique que géochimique, de la plutonite comme de la vulcanite, leur mode d'éruption qui va du type acide au type basique, ainsi que leur position dans le processus orogénique indiquent qu'il s'agit de produits successifs de la fusion partielle d'une croûte océanique en voie de subduction. Les intrusions trondhjémitiques représentent le stade initial dans l'évolution orogéno-magmatique.

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Matrix material in type 3 chondrites—occurrence,heterogeneity and relationship with chondrules

Matrix material in type 3 chondrites forms rims on chondrules, metal-sulfide aggregates, Ca,Al-rich inclusions and chondritic clasts; it also forms lumps up to a millimeter in size, which may contain coarser silicates. Chondrules of all types were found with internal matrix lumps that appear to have entered the chondrules before the latter had crystallized. Mean concentrations of Mg, Na, Al and Ca in matrix occurrences show up to fivefold variations in a single chondrite. Variations between mean matrix compositions of individual type 3 ordinary chondrites are almost as large and partly reflect systematic differences between H, L and LL matrices. Such variations are probably a result of nebular separation of feldspathic material and ferromagnesian silicates.Compositions of chondrules and their matrix rims are normally unrelated, although rim compositions are correlated with those of matrix lumps inside chondrules. A single chondrule was found with a composition nearly identical to that of its internal matrix lump, suggesting that some chondrules may have formed from matrix material. Matrix lumps are as heterogeneous as chondrules, but mean chondrule and matrix compositions differ, even allowing for possible loss of metallic Fe,Ni during chondrule formation. Since bulk compositions of matrix lumps and rims have probably not changed significantly since their formation except for Fe-Mg exchange, our matrix samples cannot represent typical chondrule precursor materials.