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991.
Zusammenfassung An vier verschiedenen Arten der GattungOscillatoria konnte nach Anf?rbung mit Acridinorange im Fluoreszenzmikroskop die Feinstruktur des Centroplasmas beobachtet werden. Besonders deutlich liessenO. animalis undO. terebriformis feine L?ngsstrukturen erkennen, die schr?g zur Trichomachse ausgerichtet waren und auf einen spiraligen Bau des gesamten Protoplasten schliessen liessen. Voraussetzung für diese Versuche waren junge Algen aus 3–4 Tage alten Kulturen. Die Anordnung der nukleins?urehaltigen Strukturen in den Zellen stimmte mit der Drehrichtung der lebenden Algen überein. Es wird angenommen, dass die Windungsrichtung der Oscillatorien artspezifisch ist.
Summary It was possible, after staining with acridin orange, to observe in the fluoromicroscope the fine structure of the centroplasm of four different species of the genusOscillatoria. Especially in the case ofO. animalis andO. terebriformis, fine longitudinal structures could be distinguished; they run obliquely towards the trichome axis and could be a sign of spiral structure of the whole protoplast. Such structures can be observed only on young algae taken from cultures 3 or 4 days old. The arrangement of the nucleinate structures in the cells corresponds to the twisting movement of the live algae. It can be supposed that the twisting direction taken by the Oscillatoria is characteristic of the species.
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992.
Summary The present paper contains studies of the nocturnal radiation at some Indian Stations (Madras, Waltair, Nagpur, New Delhi and Poona) with the help of the Ångström compensation Pyrgeometer. The technique of measurement is also described briefly. A study of the mean monthly variation of sky radiation during clear as well as all nights has been discussed. A comparitive study of mean monthly values of sky and other nocturnal radiation components at these stations is also presented. Ångström, [4]2) expressed the dependence of sky radiationS—on water vapour pressuree (mm of mercury) at the earth's surface and air temperatureT (degrees absolute), near the instrument to be given byS=T 4 (0.75–0.32×10–0.069e ) cal/cm2/min. According to this semi-empirical relationship, the calculated values of sky radiation for clear nights are smaller than the observed values of sky radiation at all the above stations. It is for this reason the authors obtained a new formula with different constants using nine years observed data at all the stations. To investigate the value of the constant, the mean annual observations presented for nine years from clear skies were analysed for correlations betweenB (black body radiation) versesS (sky radiation),N (net radiation) andE (absolute error) and obtained a good correlation co-efficients 0.90, 1 and 0.98 respectively. The new suggested formula isS=T 4 (0.88–0.32×10–0.069e ) cal/cm2/min, 267° A<T<313° A. It is also verified using with observed data of different years of the stations. The agreement between the computed values with the new formula of sky radiation and observed sky radiation is found to be good.  相似文献   
993.
Zusammenfassung Am Südostrand des Münsterländer Kreidebeckens fließen alle größeren Wasserläufe im Bereich der Turonkalke nach NNE oder NE, obwohl das allgemeine Gelände- und Schichtengefälle nach NNW gerichtet ist. Die Ursachen für diese Abweichung sind im Mechanismus der Felserosion zu suchen, der im wesentlichen durch die Eigentümlichkeiten der Karstgerinne und durch die Gesteinszerklüftung bestimmt wird. Bei den Detailuntersuchungen geben sich komplexe Beziehungen zwischen Fließrichtung und Kluftrichtungen zu erkennen.Besonders bedeutend für die Entstehung der NNE gerichteten Täler sind die 170°- und 30°-streichenden Klüfte.
On the south-east border of the Cretaceous basin of Munster, Westfalia, the current directions of streams in the area of Turon-limestone go to NNE or NE, although the main dipping of land surface as well as bedding planes points towards NNW. This divergence is caused by the mechanism of rock erosion, which is determined by peculiarities of subterranean stream channels and joints in limestone. The investigations show complex relations between flow direction and direction of joints.The 170°- and 30°-striking joints are significant of the origin of the NNE direction of the valleys.

Résumé Dans le Turonien au bord sud-est du bassin Crétacé de Münster (Westphalie) toutes les rivières coulent en direction nord-nord-est ou nord-est, quoique la surface morphologique générale et les couches soient penchées en direction nord-nord-ouest. Cette divergence est expliquée par le mécanisme de l'érosion qui dépend principalement des fentes et du caractère des ruisseaux karstiques. Pendant ces études on a pu observer des relations complexes entre la direction des courants et la direction des fentes.Les fentes en direction nord-nord-est (30°) et sud-sud-est (170°) ont considérablement influencé l'origine des vallées.

- - , -. . . , NNE, , 170° 30°.


Herrn Professor Dr.Roland Brinkmann zum 70. Geburtstag gewidmet.  相似文献   
994.
Sudoite, muscovite, and quartz are authigenic minerals of the Cornberger Sandstein, the youngest eolian member of the uppermost Lower Permian. The sudoite is to a great extent similar to the material from the Kesselberg area (Black Forest, Germany).
$$\begin{gathered} n_z \approx n_z = 1.572 \pm 0.002 \hfill \\ \underline {{\text{ }}n_x = 1.568 \pm 0.003} \hfill \\ {\text{ }}\Theta \Delta = 0.004 \pm 0.003 \hfill \\ \end{gathered} $$  相似文献   
995.
Summary Echo records from the Atlantic west of the Faroe Islands are presented which, for the first time, give evidence of the influence exerted by day on the vertical movement of pelagic fishes by a considerable reduction of luminous intensity (solar eclipse). This phenomenon corresponds with the fact well known since some years from investigations in the North Sea which prove that by night pelagic fishes move in a vertical direction according to the variation in luminous intensity.
Sur des enregistrements ultra-sonores caractérisant le comportement des poissons pélagiques pendant l'éclipsé de soleil au 30 juin 1954
Résumé On présente des enregistrements ultra-sonores faits en océan Atlantique à l'ouest de l'archipel de Færoé. Ces enregistrements font, pour la première fois, preuve de l'influence exercée de jour sur le mouvement vertical des poissons pélagiques par une réduction sensible de l'intensité lumineuse (éclipse de soleil). Ce phénomène correspond avec le fait bien connu depuis quelques ans par des recherches dans la mer du Nord. Suivant ces recherches, les poissons pélagiques se meuvent nuitamment dans la direction verticale suivant la variation de l'intensité lumineuse.
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996.
Zusammenfassung Feintektonische Untersuchungen, ergänzt durch stratigraphische Profilaufnahme, erbrachten den Nachweis eines Hönningen-Seifener-Sattels aus Schichten des Unteren Siegen, Im NW wie SE wird dieser Sattel von flachwelligen Muldenzonen begleitet, deren südöstliche in Richtung auf die Siegerländer Hauptüberschiebung einen zunehmenden Schuppenbau zeigt.  相似文献   
997.
Zusammenfassung Der Verwitterungsmantel (Laterit s. l.) der südlichen Goldküste besteht aus Horizonten, die sowohl verschiedene Entstehungsart als verschiedenes Alter haben. Brekzien oder Steinschichten sind unter aridem Klima als Wüstenpflaster entstanden. Zonen chemisch verwitterten Felses, Horizonte von lehmigem Sand (an deren Aufbau Termiten wesentlich beteiligt sind) und Konkretionen haben sich unter feuchtem Klima gebildet. Harte limonitische Oberflächen-Krusten deuten auf progressive Austrocknung hin. Unter diesen drei klimatischen Bedingungen gebildete Horizonte wiederholen sich mehrfach im Verwitterungsmantel der Goldküste. Ein junger, unvollständiger Zyklus ist weit verbreitet, ein älterer Zyklus tritt nur in begrenzten Vorkommen auf, und ein dritter Zyklus ist fast nur noch in aufgearbeiteten, limonitisierten Bruchstücken erhalten. Die wiederholten Klimaschwankungen machen es wahrscheinlich, daß der Verwitterungsmantel zeitlich dem größeren Teil des Quartärs entspricht. Wahrscheinlich können die Ergebnisse auf weit größere Gebiete angewandt werden.  相似文献   
998.
Ohne Zusammenfassung  相似文献   
999.
Thirty-two weather diaries written in astronomical calendars in central Europe in the late fifteenth and sixteenth centuries are presented and discussed. Systematic weather observations were promoted by the rise of planetary astronomy and its application in astro-meteorology. The practice of keeping weather diaries spread from Cracow (Poland) to Ingolstadt (Germany) and from there to other universities. The data obtained from these sources provided the backbone for setting up series of precipitation indices for Poland, Germany and Switzerland. Monthly statistics of days with precipitation, snowfall and frost were computed by counting the relevant entries in the most important diaries. The results were compared with either those obtained from instrumental measurements in the same place or with those from modern instrumental measurements in a neighbouring place. The final results show that autumn was considerably colder in the early sixteenth century. April was considerably drier and July was wetter during the period 1508-1531 than during 1901-1960. In order to highlight the impact of weather patterns on grain prices in a year of crisis, the timing of wet and dry spells in southern Poland and southern Germany is compared for the year 1529. Winters became 1.7°C colder from 1564 to 1576 and the month of July tended to be wetter than in 1901-1960. Details noted in the diaries kept between 1585 and 1600 by the astronomers Brahe (near Copenhagen) and Fabricius (in the Ostfriesland region of northwestern Germany) closely agree. It rained more often in June and July and temperatures dropped. The winter months were more frequently dominated by winds from easterly directions, the frequency of snowfall was higher and a deficit occurred in precipitation. This points to a higher frequency of high pressure in the Fennoscandian area with cold air advection from the east or northeast.  相似文献   
1000.
The column amounts of nitrogen dioxide (NO2) and ozone (O3) were measured using a visible spectrometer based on the twilight zenith-sky technique at two observatories located at similar latitudes in the northern part of Japan separated by a distance of 150 km. The measurements began in April 1991 at the Moshiri Observatory (44.4°N, 142.3°E) and in April 1994 at the Rikubetsu Observatory (43.5°N, 143.8°E). Since weather conditions and the possible influence from tropospheric pollution were not always identical at these two observatories, the overall accuracy of the measurements was studied comparing these data sets. The first year data obtained at a solar zenith angle of 90 degrees indicated that the NO2 slant column values at sunrise and sunset agreed within 0.36 and 0.54 × 1016 cm-2, respectively, corresponding to 5 % (June) and to 12 % (December) of the columns. The O3 values agreed within 0.76 × 1019 cm-2, corresponding to 4 % (March) 6 % (August) of the columns, although a part of the difference was systematic. The O3 column amounts were also compared to those obtained by the Dobson spectrometer at Sapporo (43.5°N, 143.8°E), whose latitude is similar to these observatories. When an air mass factor of 17.5 was used, the two-year Moshiri vertical column values agreed with the Dobson direct sun values to within 15 Dobson Units, or 3 6 % of the column. The difference between the two values was found to be due partly to the change in the air mass factor caused by seasonal and day-to-day changes in the shape of the O3 vertical profiles. These results confirm the reliability of the NO2 and O3 measurements by visible spectrometers at these sites for the Network for the Detection of Stratospheric Change (NDSC).  相似文献   
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