Photometric investigation of the short period eclipsing binary star V719 Her

The Behlen observatory 0.76 m telescope CCD photometer is used to obtain 347 observations of the short period (P0^d.4) eclipsing binary star V719 Her. The observations done withV andR bandpass filters were made on 6 nights in 1993. Previously published light elements and the present five timings of minimum provide a new epoch and a more accurate orbital period of 0.4009828 days. Our analyses show that the period of the system appears to decrease. We recommend future monitoring of the eclipse minima for this system. No published spectral classification for V719 Her exists. From the color,V-R=0.391, we estimate it to be about F5.The 1993 version of the Wilson Devinney model gave the photometric solutions. The adopted solution indicates that V719 Her is a W UMa type contact binary. The mass ratio,q=(m ₂/m ₁, where star 1 eclipse at the primary minimum)=0.296 suggests that V719 Her is a WUMa system with type-A (transit during primary eclipse) configuration. The secondary minimum shows a total eclipse. V719 Her with period less than 0.5 and spectral class F5, is probably a zero-age contact system. Since our photometric solution shows that the luminosity difference between the components is very large, we suspect that V719 Her is most likely a single line spectroscopic binary. We recommend spectroscopic study of this system.     

SWAN: A study of Solar Wind Anisotropies on SOHO with Lyman alpha sky mapping

On board the SOHO spacecraft poised at L1 Lagrange point, the SWAN instrument is mainly devoted to the measurement of large scale structures of the solar wind, and in particular the distribution with heliographic latitude of the solar wind mass flux. This is obtained from an intensity map of the sky Lyman emission, which reflects the shape of the ionization cavity carved in the flow of interstellar H atoms by the solar wind. The methodology, inversion procedure and related complications are described. The subject of latitude variation of the solar wind is shortly reviewed: earlier Lyman results from Prognoz in 1976 are confirmed by Ulysses. The importance of the actual value of the solar wind mass flux for the equation of dynamics in a polar coronal hole is stressed. The instrument is composed of one electronic unit commanding two identical Sensor Units, each of them allowing to map a full hemisphere with a resolution of 1°, thanks to a two-mirrors periscope system. The design is described in some details, and the rationale for choice between several variants are discussed. A hydrogen absorption cell is used to measure the shape of the interplanetary Lyman line and other Lyman emissions. Other types of observations are also discussed : the geocorona, comets (old and new), the solar corona, and a possible signature of the heliopause. The connexion with some other SOHO instruments, in particular LASCO, UVCS, SUMER, is briefly discussed.     

A Spatial Data Infrastructure Approach for the Characterization of New Zealand's Groundwater Systems

The future information needs of stakeholders for hydrogeological and hydro‐climate data management and assessment in New Zealand may be met with an Open Geospatial Consortium (OGC) standards‐compliant publicly accessible web services framework which aims to provide integrated use of groundwater information and environmental observation data in general. The stages of the framework development described in this article are search and discovery as well as data collection and access with (meta)data services, which are developed in a community process. The concept and prototype implementation of OGC‐compliant web services for groundwater and hydro‐climate data include demonstration data services that present multiple distributed datasets of environmental observations. The results also iterate over the stakeholder community process and the refined profile of OGC services for environmental observation data sharing within the New Zealand Spatial Data Infrastructure (SDI) landscape, including datasets from the National Groundwater Monitoring Program and the New Zealand Climate Database along with datasets from affiliated regional councils at regional‐ and sub‐regional scales. With the definition of the New Zealand observation data profile we show that current state‐of‐the‐art standards do not necessarily need to be improved, but that the community has to agree upon how to use these standards in an iterative process.     

Hacked Landscapes: Tensions,Borders, and Positionality in Spatial Literacy

By focusing on critical geographies, landscape, and spatial literacy, this article evaluates a semester-long spatial justice project conducted in a preservice teacher education program. The analysis recognizes the limitations of reading the products literally as a means of comprehending spatial representation. It expands the analysis by hacking the products and producing new landscapes to read against or up against the products as sociospatial texts. It considers the deployment of landscape concepts—borders, the representation of tension, and the gaze and subjectivity of the reader-authors—as central elements of spatial literacy that is of consequence.     

Zur Tektonik des nördlichen Hegaus

Ohne Zusammenfassung     

Tagung der Deutschen Quartärvereinigung in Hannover vom 7. bis 11. Oktober 1948

Ohne Zusammenfassung     

A comment on “Calcic amphibole equilibria and a new amphibole — plagioclase geothermometer” by J.D. Blundy and T.J.B. Holland (Contrib Mineral Petrol (1990) 104: 208–224)

Conclusions The calibration by Blundy and Holland is not a calibration of the reaction albite + tremolite = edenite + 4quartz, because the Al^IV content of amphiboles is a combined result of substitutions.The requirements for a calibration of any of these substitutions are: (1) an amphibole-activity model unequivocally accounting for each substitution and (2) a data-set, wherein all amphiboles are buffered by the same assemblages.     

The tectonic history of the Pre-Saharan depression (Morocco) a geomorphological interpretation

During the Cretaceous and Tertiary periods the Pre-Saharan depression between Ouarzazate and Errachidia was an area of deposition in a spatially and chronologically highly differentiated pattern. The variable structural and tectonic history of this region in also reflected in its denudational development. Until the late Pliocene/early Pleistocene the western part (Ouarzazate basin) was a depositional basin for lacustrine and alluvial sediments. Pediment formation did not start before the Pleistocene period. In the central part of the depression (between Boumalne and Tinerhir) denudational activity on cuesta scarps started already in the late Miocene to early Pliocene as can be deduced from a new dating of the Foum el Kous volcano (2.9 my) and from Djebl Sarhro gravels on the crest of the Paleogene scarp. In the easternmost part of the depression (between Goulmima and Errachidia) there are no Neogene sediments, and the calculations of rates of scarp retreat demonstrate that scarp backwearing must have begun in the late Eocene. Thus the shift from depositional to erosional activity in the Pre-Saharan depression ranges from the late Eocene to the Pleistocene. This is at the same time an expression of its complex tectonic history.

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Zusammenfassung Die präsaharische Senke zwischen Ouarzazate und Errachidia war während der Kreide und des Tertiärs ein Sedimentationsgebiet mit zeitlich und räumlich hoch differenzierten Fazies- und Mächtigkeitsabfolgen. Die variable strukturelle und tektonische Entwicklung dieser Zeit spiegelt sich wider in der nachfolgenden Abtragungsgeschichte. Der westliche Teil der Senke, das Becken von Ouarzazate, war bis zum späten Pliozän/frühen Pleistozän ein Ablagerungsbecken für limnische und alluviale Sedimente, bis im frühen Pleistozän die Genese von Pedimenten einsetzte. Im zentralen Teil der präsaharischen Senke zwischen Boumalne und Tinerhir begann die erosive Reliefentwicklung an Stufenhängen bereits im späten Miozän bis frühen Pliozän, wie sich aus einer absoluten Datierung des Ankaratrits des Foum el Kous (2,9 my) ableiten läßt, der sich in die zu dieser Zeit bereits existente Stufenvorlandzone ergoß. Eine untere Zeitmarke für die Entstehung der Schichtstufe stellen die von Süden vom Djebl Sarhro in die Senke hereintransportierten Schotter von Timadriouine dar. Im Ostteil der präsaharischen Senke zwischen Goulmima und Errachidia fehlen neogene Sedimente, und die Ermittlung von Stufenrückwanderungsraten für die Hamada de Meski zeigt, daß die Abtragung hier schon im späten Eozän eingesetzt haben muß. Der Wechsel von Sedimentations- zu subaerischen Abtragungsbedingungen reicht in der präsaharischen Senke vom frühen Pleistozän im Westen bis zum Eozän im Osten. Das ist auf geomorphologischer Grundlage ein Hinweis auf die komplexe strukturelle und tektonische Entwicklung dieser Region.

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Résumé Au cours du Crétacé et du Tertiaire, la dépression présaharienne entre Ouarzazate et Errachidia a été un domaine de sédimentation marqué par de fortes variations de faciès et d'épaisseurs dans le temps et dans l'espace. L'histoire structurale et tectonique mouvementée de cette période se reflète également dans la dénudation qui a suivi. La partie ouest de la dépression (bassin d'Ouarzazate) a constitué jusqu'à la limite Plio-Pléistocène une aire de dépôt de sédiments lacustres et alluviaux; la formation de pédiments n'y a débuté qu'au Pléistocène. Dans la partie centrale de la dépression, entre Boumalne et Tinerhir, l'érosion en cuestas a débuté dès le Miocène supérieur/Pliocène inférieur, comme l'indique une datation récente à 2,9 Ma de l'ankaratrite du volcan Foum el Kous qui s'est écoulée en avant d'une cuesta qui existait déjà à ce moment. Une limite inférieure pour la formation des cuestas est fournie par les graviers de Timadriouine transportés dans la dépression depuis le sud à partir du Djebel Sarhro.Dans la partie orientale de la dépression présaharienne, entre Goulmina et Errachidia, les sédiments néogènes font défaut et l'évaluation de la vitesse de recul des fronts de cuestas montre que ce processus a dû commencer à l'Eocène supérieur. Ainsi, le passage de la sédimentation à l'activité érosive dans la dépression pré-saharienne varie du Pléistocène inférieur à l'ouest, à l'Eocène à l'est. C'est là, à partir de données géomorphologiques, une indication de l'histoire structurale et tectonique complexe de cette région.

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- Ouarzazate Errachidia , , , . . , Ouarzazate / ; . Boumalne Tinerhir () , , Foum el Kous (2,9 Ma), . Timadriouine Djebl Sarhro . Goulmina Errachidia Hamada de Meski , , , . , . .