Das „Randcenoman“ der Nördlichen Kalkalpen und seine Bedeutung für den Ablauf der ostalpinen Deckenüberschiebungen und ihrer Schubweiten

Zusammenfassung Das Randcenoman erstreckt sich über 220 km als ein der Cenoman-Serie zugehöriger Grenzbereich gegen die Flyschzone am Nordrand der Kalkalpen vom Chiemsee bis in das Große Walsertal.An einer Anzahl durchgehender Profile wurden stratigraphische und sedimentologische Untersuchungen durchgeführt.Nach Mikrofaunen konnten neue stratigraphische Belege für eine örtliche Sedimentationsfortsetzung ohne erkennbare Schichtunterbrechung vom Alb bis in das Cenoman gefunden werden. Hinweise auf unterturones Alter ergaben sich an zwei Stellen. Die alttertiären Tratenbachschichten sind tektonisch von Randcenoman und Flysch abgegrenzt.Trotz eines heterogenen Gesteinsaufbaus in vertikaler und horizontaler Ausdehnung mit einer differenzierten Wechsellagerung von Peliten, Psammiten und Psephiten zeigt die Cenoman-Serie petrographische Konstanz in Gefüge und Mineralzusammensetzung, besonders im Geröllspektrum und der Schwermineralassoziation (Chromit-SpinellPicotit).Die Gesteine des Randcenoman sind in einem einheitlichen Ablagerungsraum sedimentiert worden. Das gilt auch für ihre Anteile in der Arosa-Zone im Allgäu und im Bregenzer Wald.Faziesbeziehungen zur Flyschzone gibt es nicht.Auf das Ablagerungsmilieu deuten Flachwasserbildungen hin, die im flachen Randbereich der Geosynklinale während langdauernder Ruhigwasserfazies mit episodischen Unterbrechungen abgelagert wurden.Die petrographische Zusammensetzung der allothigenen Gerölle, ihr Rundungsgrad, ihre metamorphe Beanspruchung und ihr Erhaltungszustand lassen Analogieschlüsse mit Gesteinen vom Verrucano-Typ zu. Im Zusammenhang mit der Tonmineralführung der Pelite (Kaolinit) und der typischen Chromit-Spinell-Beteiligung kann auf ein breites Festland geschlossen werden. An der Detritusanlieferung sind neben dem mesozoischen kalkalpinen Untergrund und Gesteinen vom Verrucano-Typ Unterostalpin und Südpenninikum beteiligt. Damit sind die nördlichen Kalkalpen im Süden der Tauern beheimatet.Der Zeitraum der Überschiebung über das Penninikum liegt nicht vor Unterturon.Mittelkretazische Bewegungen werden in der Cenoman-Serie nur untergeordnet wirksam, wo sich Konglomerate und Geröllpsammite an der Wende Alb-Cenoman horizontieren lassen.

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The Randcenoman extends over a distance of 220 km as a boundary part of the Cenomanian Series along the alpine Flysch at the northern margin of the Limestone Alps from Chiem-See to the Grosses Walsertal.Series of continuous profiles have been investigated by stratigraphic and sedimentologic methods.By use of microfossils it could be proved that sedimentation lasted from Albian up to Cenomanian without visible interruption. At two different localities it was possible to find references to Turonian age.The Tratenbach layers of Tertiary age are separated tectonically from the Randcenoman and the Flysch.The rocks of Randcenoman show a very constant texture and association of minerals, especially in boulders and heavy minerals (chromite-spinel-picotite).These rocks must have been sedimented into an uniform trough. Same may be said concerning their contents within the Arosa-Zone in the Algovian region and in the Woods of Bregenz. There are no connections possible with facies of the Flysch series.Sediments of low water type show that these series have been deposed along the margin of the Alpine Geosyncline during long times of stagnant waters with episodical interruptions.The petrographic composition of the allothigenic boulders, their roundness, metamorphic stress and their state of conversation allows comparisons with rocks of the series of the Verrucano.The existance of a vast continent may be derived from the clay contents of the pelites (kaolinite) and the typical appearance of chromite-spinel minerals. The detritus has been delivered partly by the Lower Austroalpine unit and southern Penninicum, and by Mesozoic series of the Limestone Alps and rocks of Verrucano type.Concluding the origin of the Northern Limestone Alps has to be located south of the Tauern window.The movement of the Austroalpine nappes over the Penninicum cannot have happened before Lower Turonian age. The movements of Middle Cretaceous time are only of small efficiency on the series of Cenomanian where conglomerates and psammites containing boulders could be dated to be of Albanian-Cenomanian age.

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Résumé Le «Randcenomanien» s'étend sur 220 Km comme un ensemble-limite appartenant au Cénomanien, au contact de la zone du Flysch à la bordure Nord des Alpes calcaires, depuis le Lac de Chiem jusqu'à la «Grosse Walsertal»,L'auteur a effectué, le long d'un certain nombre de profils, des recherches stratigraphiques et sédimentologiques.A partir des microfaunes, on peut trouver de nouvelles preuves stratigraphiques en faveur d'une continuité de la sédimentation de l'Albien jusqu'au Cénomanien, sans aucune interruption reconnaissable. A deux endroits l'auteur a trouvé des indications concernant la présence du Turonien inférieur. Les couches du «Tratenbach» appartenant au Tertiaire inférieur sont séparées par voie tectonique du «Randcenomanien» et du Flysch.Malgré une constitution lithologique hétérogène, tant suivant la verticale que l'horizontale, avec des alternances bien marquées de pélites, psammites et pséphites, la série du Cénomanien montre une constance pétrographique quant à la texture et la composition minéralogique, spécialement dans la gamme des galets et l'association des minéraux lourds (Chromite-Spinelle-Picotite).Les roches du «Randcenomanien» ont été sédimentées dans un bassin uniforme; c'est aussi le cas dans la zone d'Arosa dans l'Allgäu et de la forêt de Bregenz.Il n'y a aucune connection avec les facies de la zone du Flysch.Quant au milieu de sédimentation, is est donné par les formations d'eaux profondes qui ont été déposées dans la région de bordure peu profonde du géosynclinal au cours de périodes de longue durée, en eau calme, avec seulement quelques interruptions épisodiques.La composition pétrographique des galets allothigènes, leur degré d'arrondi, leur degré de métamorphisme et leur état de conservation permettent de faire des analogies avec des roches du type Verrucano. Compte tenu aussi des minéraux argileux intervenant dans la constitution des pélites (kaolinite) et à la participation typique de la Chromite et du spinelle, on en arrive à la conclusion que le continent fournisseur de ces sédiments a été assez vaste. Aux apports détritiques du Mésozoïque inférieur des Alpes calcaires et des roches du type «Verrucano», sont venus s'ajouter ceux en provenance de l'Austroalpin inférieur et du Pennique méridional. C'est pourquoi le lieu d'origine des «Alpes calcaires» du Nord doit se trouver au sud des Tauern.Le chevauchement sur le Penninicum n'a pas eu lieu avant le Turonien inférieur.Les mouvements Crétacé inférieur dans le Cénomanien n'ont été que peu actifs, là où des conglomérats et des psammites à galets se sont épandus entre l'Albien et le Cénomanien.

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Erweiterte Fassung eines am 25. Februar 1972 auf der 62. Jahrestagung der Geologischen Vereinigung in Frankfurt gehaltenen Vortrages.     

Oxide minerals in lithic fragments from Luna 20 fines

One hundred and seventy-six oxide mineral grains in the Luna 20 samples were analyzed by electron microprobe. Spinel is the most abundant oxide, occurring in troctolite fragments. Next most abundant is ilmenite, which occurs in all rock types except those containing spinel. Chromite also occurs in all rock types except those containing spinel. Minor amounts of ulvöspinel, armalcolite, zirkelite, baddeleyite and an unidentified TiO₂-rich phase were also found.Spinel grains are predominantly spinel-hercynite solid solutions, commonly with very minor chromite. The $\text{Fe}\text{(Fe + Mg)}$ ratio is generally lower than in spinel from Apollo 14 rocks. Chromites in non-mare rocks are similar to those from mare rocks. Ilmenite of mare origin is Mg-poor and Zr-rich compared to non-mare ilmenite; these elements may therefore be useful in determining the origin of ilmenite grains.Phase equilibria considerations suggest that spinel troctolite crystallized from a melt high in alumina; a likely candidate is the high-alumina basalt of Prinzet al. (1973a).Sub-micron wide rods of metallic Fe occur in plagioclase grains and may have formed by sub-solidus reduction processes.     

Ferroan anorthosite: A widespread and distinctive lunar rock type

Eight of eleven Apollo 16 rake-sample anorthosites are very similar to each other, to hand-specimen Apollo 16 anorthosites, and to Apollo 15 anorthosites. They have feldspar An_96.6, both high- and low-Ca pyroxene with a restricted range of (low-magnesium) composition, minor olivine (～ Fo₆₀), traces of ilmenite and chromite, and originally coarse-grained, but now cataclastic texture. Such ferroan anorthosite is evidently a coherent, distinctive and widespread lunar rock type of cumulate origin which may not necessarily be very closely related genetically to other highland rock types.     

A Ca ii H&K survey of γ Doradus candidates

In an investigation of the starspot hypothesis as it applies to the 'slowly variable' F-type dwarfs, we spectroscopically observed eight promising γ Doradus candidates to search for Ca  ii H&K emission. We found that there are no significant emission reversals in the cores of these resonance lines. Based on the ceiling flux calculations of the Ca  ii K line and on calculations of the Rossby number, we conclude that there is no support for the presence of strong magnetic activity and the starspot hypothesis in these objects.     

Late Cretaceous reactivation of major crustal shear zones in northern Namibia: constraints from apatite fission track analysis

Namibia's passive continental margin records a long history of tectonic activity since the Proterozoic. The orogenic belt produced during the collision of the Congo and Kalahari Cratons in the Early Proterozoic led to a zone of crustal weakness, which became the preferred location for tectonism during the Phanerozoic. The Pan-African Damara mobile belt forms this intraplate boundary in Namibia and its tectonostratigraphic zones are defined by ductile shear zones, where the most prominent is described as the Omaruru Lineament–Waterberg Thrust (OML–WT). The prominance of the continental margin escarpment is diminished in the area of the Central and Northern Zone of the Damara belt where the shear zones are located. This area has been targeted with a set of 66 outcrop samples over a 550-km-long, 60-km-broad coast-parallel transect from the top of the escarpment in the south across the Damara sector to the Kamanjab Inlier in the north. Apatite fission track age and length data from all samples reveal a regionally consistent cooling event. Thermal histories derived by forward modelling bracket this phase of accelerated cooling in the Late Cretaceous. Maximum palaeotemperatures immediately prior to the onset of cooling range from ca. 120 to ca. 60 °C with the maximum occurring directly south of the Omaruru Lineament. Because different palaeotemperatures indicate different burial depth at a given time, the amount of denudation can be estimated and used to constrain vertical displacements of the continental crust. We interpret this cooling pattern as the geomorphic response to reactivation of basement structures caused by a change in spreading geometry in the South Atlantic and South West Indian Oceans.     

Extremely low temperatures in the stratosphore and very low total ozone amount above northern and central Europe during winter 1989

On 1 February 1989, -83.5°C was recorded in 27.8 hPa over Hohenpeißenberg, the lowest temperature in the 22-year series. This was measured together with a very low total ozone amount of 266 DU. This may be compared with nearly twice this amount on 27 February 1989. The situation was very unusual: following an extremely cold winter in the Arctic stratosphere, the stratospheric cold pole was located over southern Scandinavia on 1 February in a very southerly position. The analyzed temperatures of -92 °C in 30 hPa were also unusual. Even though the low ozone amounts over Hohenpeißenberg were probably dynamically caused, an additional very small ozone decrease due to heterogeneous reactions in altitudes from 23–28 km, where the temperatures lie below -80 °C, cannot be ruled out. Extinction measurements by the orbitting SAGE II instrument indeed show polar stratospheric clouds over Europe near 50° N during the period 31 January–2 February. Also, polar stratospheric clouds were previously observed over Kiruna at similarly low temperatures and signs of a corresponding small ozone decrease were noted there.     

On the spectral dissipation of ocean waves due to white capping

Summary The effect of white capping on the spectral energy balance of surface waves is investigated by expressing the white-cap interactions in terms of an equivalent ensemble of random pressure pulses. It is shown first that the source function for any non-expansible interaction process which is weak-in-the-mean is quasi-linear. In the case of white capping, the damping coefficient is then shown to be proportional to the square of the frequency, provided the wave scales are large compared with the white-cap dimensions. The remaining free factor is determined indirectly from consideration of the spectral energy balance. The proposed white-capping dissipation function is consistent with the structure of the energy balance derived from JONSWAP, and the existence of a ^–5 spectrum governed by a non-local energy balance between the atmospheric input, the nonlinear energy transfer and dissipation. However, closure of the energy balance involves hypotheses regarding the structure of the atmospheric input function which need to be tested by further measurements. The proposed set of source functions may nevertheless be useful for numerical wave-prediction. According to the model, nearly all the momentum transferred across the air-sea interface enters the wave field. For fetchlimited and fully developed spectra in a stationary, uniform wind field, the drag coefficient remains approximately constant. However, for more general wind conditions, this will not be the case and the wave spectrum should be included in an accurate parameterisation of the air-sea momentum transfer.Contribution from the Sonderforschungsbereich Meeresforschung Hamburg of the Deutsche Forschungsgemeinschaft.     

Ingella Station,a New Chondrite Find from the Tenham Strewnfield,Queensland, Australia

Abstract— Based on optical microscopy and electron microprobe analysis of mafic minerals, Ingella Station, a new meteorite find from the area of the Tenham strewnfield, Queensland, Australia, is classified as an H5a chondrite.     

The Deformational Response of a Viscoelastic Solid Earth Model Coupled to a Thermomechanical Ice Sheet Model

We apply a coupled thermomechanical ice sheet—self-gravitating viscoelastic solid Earth model (SGVEM), allowing for the dynamic exchange of ice thickness and bedrock deformation, in order to investigate the effect of viscoelastic deformation on ice dynamics and vice versa. In a synthetic glaciation scenario, we investigate the interaction between the ice sheet and the solid Earth deformation, the glacial-isostatic adjustment (GIA), accounting for an atmospheric forcing depending on the ice sheet surface altitude. We compare the results from the coupled model to runs with the common elastic lithosphere/relaxing asthenosphere (ELRA) model, where the lithosphere is represented by a thin plate and the mantle relaxes with one characteristic relaxation time, as well as to a rigid Earth without any deformation. We find that the deformational behaviour of the SGVEM on ice dynamics (i.e. stored ice volume, ice thickness and velocity field) is comparable to the ELRA for an optimal choice of the parameters in steady state, but exhibits differences in the transient behaviour. Beyond the ice sheet, in the region of peripheral forebulge, the differences in the transient surface deformation between ELRA and SGVEM are substantial, demonstrating the inadequacy of the ELRA model for interpreting constraints on GIA in the periphery of the ice sheet, such as sea-level indicators and GPS uplift rates.