Submarine Groundwater Discharge-Derived Nutrient Loads to San Francisco Bay: Implications to Future Ecosystem Changes

Submarine groundwater discharge (SGD) was quantified at select sites in San Francisco Bay (SFB) from radium (²²³Ra and ²²⁴Ra) and radon (²²²Rn) activities measured in groundwater and surface water using simple mass balance box models. Based on these models, discharge rates in South and Central Bays were 0.3?C7.4?m³?day^?1?m^?1. Although SGD fluxes at the two regions (Central and South Bays) of SFB were of the same order of magnitude, the dissolved inorganic nitrogen (DIN) species associated with SGD were different. In the South Bay, ammonium (NH ₄ ⁺ ) concentrations in groundwater were three-fold higher than in open bay waters, and NH ₄ ⁺ was the primary DIN form discharged by SGD. At the Central Bay site, the primary DIN form in groundwater and associated discharge was nitrate (NO ₃ ^? ). The stable isotope signatures (??¹⁵N_NO3 and ??¹⁸O_NO3) of NO ₃ ^? in the South Bay groundwater and surface waters were both consistent with NO ₃ ^? derived from NH ₄ ⁺ that was isotopically enriched in ¹⁵N by NH ₄ ⁺ volatilization. Based on the calculated SGD fluxes and groundwater nutrient concentrations, nutrient fluxes associated with SGD can account for up to 16?% of DIN and 22?% of DIP in South and Central Bays. The form of DIN contributed to surface waters from SGD may impact the ratio of NO ₃ ^? to NH ₄ ⁺ available to phytoplankton with implications to bay productivity, phytoplankton species distribution, and nutrient uptake rates. This assessment of nutrient delivery via groundwater discharge in SFB may provide vital information for future bay ecological wellbeing and sensitivity to future environmental stressors.     

Petrological evidence for the development of refolded folds during a single deformational event

The Pelona Schist, which forms the lower plate of the Vincent thrust in the San Gabriel Mountains of southern California, has undergone a complex history of folding. The youngest folds in the schist (style 2 folds) range in shape from open to tight and fold both compositional layering and schistosity. These are superposed upon isoclinal folds with axial-plane schistosity (style 1 folds) that, in turn, overprint older isoclinal folds (also called style 1 folds). Samples from the hinges of style 2 folds contain two generations of muscovite. Muscovites of the older generation are parallel to the folded (style 1) schistosity. The newer muscovites recrystallized during and/or after style 2 folding. Microprobe analysis indicates that the two generations of muscovite are very similar in composition, although the new muscovites tend to have slightly higher paragonite and celadonite contents than the old muscovites. From the gross similarity of the two groups of muscovite, it is concluded that the style 1 and style 2 folds were produced during a single progressive deformation. The slightly higher paragonite and celadonite contents of the new muscovites are thought to indicate that both pressure and temperature were increasing during the deformation. This is consistent with the deformation being due to underthrusting of the Pelona Schist beneath the upper plate of the Vincent thrust.     

Noble metals in the insoluble carbonaceous substance of black shales and ores: Direct atomic emission data

The way of extraction of insoluble carbonaceous substance (ICS) from black shales and technique of determination of noble metals (NM) in it by direct arc atomic emission analysis (AEA) were developed. The first results are reported on the determination of mineral-bound noble metals in ICS concentrates, which were extracted from the rocks and ores of the Sukhoi Log, Vernyi, Vasil’evskoe, Kuranakh, Daugyztau, Bakyrchik, Kamennoe, El’dorado, and other deposits.     

Liquefaction Identification Using IRS-1D Temporal Indices Data

One of the major after effect of Bhuj Earthquake which occurred on January 26, 2001 was wide spread appearance of liquefaction of soil in the Rann of Kachchh and the coastal areas of Kandla port covering an area of more than tens of thousands of kilometers. Remote sensing data products allow us to explore the land surface parameters at different spatial scales. In this work, an attempt has been made to identify the liquefied soil area using conventional indices from IRS-1D temporal images. The same has been investigated and compared with Class Based Sensor Independent (CBSI) spectral indices, while applying fuzzy based noise classification as soft computing approach using supervised classification. Seven spectral indices have been investigated to identify liquefied soil areas using temporal multi-spectral images. The result shows that the temporal variations can be accounted by using appropriate remote sensing based spectral indices. It is found that CBSI based TNDVI using temporal data yields the best results for identification of liquefied soil areas, while CBSI based SR gives best results for water body identification.     

Bericht über die Versammlung der Geologischen Vereinigung am 24.–26. Sept. 1924 in Innsbruck

Ohne Zusammenfassung     

Geodynamic evolution of the lithosphere of the Sea of Okhotsk region from geophysical data

The tectonic structure and anomalous distributions of geophysical fields of the Sea of Okhotsk region are considered; the lack of reliable data on the age of the lithosphere beneath basins of various origins in the Sea of Okhotsk is noted. Model calculations based on geological and geophysical data yielded an age of 65 Ma (the Cretaceous-Paleocene boundary) for the Central Okhotsk rise underlain by the continental lithosphere. This estimate agrees with the age (the end of the Cretaceous) derived from seismostratigraphic data. A comparative analysis of theoretical and measured heat fluxes in the Akademii Nauk Rise, underlain by a thinned continental crust, is performed. The analysis points to a higher (by 20%) value of the measured thermal background of the rise, which is consistent with a high negative gradient of gravity anomalies in this area. Calculations yielded an age of 36 Ma (the Early Oligocene) and a lithosphere thickness of 50 km for the South Okhotsk depression, whose seafloor was formed by processes of backarc spreading. The estimated age of the depression is supported by kinematic data on the region; the calculated thickness of the lithosphere coincides with the value estimated from data of magnetotelluric sounding here. This indicates that the formation time (36 Ma) of the South Okhotsk depression was estimated correctly. Numerical modeling performed for the determination of the basement age of rifting basins in the Sea of Okhotsk gave the following estimates: 18 Ma (the Early Miocene) for the Deryugin basin, 12 Ma (the Middle Miocene) for the TINRO basin, and 23 Ma (the Late Oligocene) for the West Kamchatka trough. These estimates agree with the formation time (Oligocene-Quaternary) of the sedimentary cover in rifting basins of the Sea of Okhotsk derived from geological and geophysical data. Model temperature estimates are obtained for lithologic and stratigraphic boundaries of the sedimentary cover in the Deryugin and TINRO basins and the West Kamchatka trough; the temperature analysis indicates that the latter two structures are promising for oil and hydrocarbon gas generation; the West Kamchatka trough possesses better reservoir properties compared to the TINRO and Deryugin basins. The latter is promising for the generation of hydrocarbon gas. Paleogeodynamic reconstructions of the Sea of Okhotsk region evolution are obtained for times of 90, 66, and 36 Ma on the basis of kinematic, geomagnetic, structural, tectonic, geothermal, and other geological and geophysical data.     

An investigation of earthquake induced pounding between adjacent buildings

The response of adjacent buildings in city blocks to several strong earthquakes is analysed, taking into account the mutual collisions, or pounding, resulting from insufficient or non-existing separation distances. The buildings are idealized as lumped-mass, shear beam type, multi-degree-of-freedom (MDOF) systems with bilinear force-deformation characteristics and with bases supported on translational and rocking spring-dashpots. Collisions between adjacent masses can occur at any level and are simulated by means of viscoelastic impact elements. Using five real earthquake motions the effects of the following factors are investigated: building configuration and relative size, seismic separation distance and impact element properties. It is found that pounding can cause high overstresses, mainly when the colliding buildings have significantly different heights, periods or masses. This suggests a possibility for introducing a set of conditions into the codes, combined with some special measures, as an alternative to the seismic separation requirement.     

Unusual spatial-temporal dynamics of geomagnetic disturbances during the main phase of the extremely strong magnetic storm of November 7–8, 2004

The spatial dynamics of geomagnetic variations and pulsations, auroras, and riometer absorption during the development of the main phase of the extremely strong magnetic storm of November 7–8, 2004, has been studied. It has been indicated that intense disturbances were observed in the early morning sector of auroral latitudes rather than in the nighttime sector, as usually takes place during magnetic storms. The unusual spatial dynamics was revealed at the beginning of the storm main phase. A rapid poleward expansion of disturbances from geomagnetic latitudes of 65°–66° to 74°–75° and the development of the so-called polar cap substorm with a negative bay amplitude of up to 2500 nT, accompanied by precipitation of energetic electrons (riometer absorption) and generation of Pi2–Pi3 pulsations, were observed when IMF B _z was about ?45 nT. The geomagnetic activity maximum subsequently sharply shifted equatorward to 60°–61°. The spatial dynamics of the westward electrojet, Pi2–Pi3 geomagnetic pulsations, and riometer absorption was similar, which can indicate that the source of these phenomena is common.     

Further investigations of the fog in the photo-electric condensation nucleus counter

Summary The effect on extinction of isothermal distillation, shrinking of the droplets by evaporation without recondensation of the liberated water vapour, coagulation and differential settling of the fog droplets which take place in the fog of a photo-electric nucleus counter and which can produce a small additional extinction («creep») in the first seconds after its formation, were numerically examined. The relative contribution of each process to the total creep observed is assessed. It is found that isothermal distillation can produce amounts of creep (up to 1.70%) which exceed considerably those caused by evaporation or coagulation. The results of these computations explain the occurrence of creep with concentrations greater than approx. 25 000 nuclei/cm³ in fog-tubes of 3.85 cm air-column diameter.That the disappearance of creep in fog-tubes of diameters 2.5 cm and less is due to the accelerated heat-flow from the walls of the narrow fog-tube was previously proved by reducing appropriately the diameter of the light pencil through the fog. In order to meet the objection that by restricting the cross section of the light pencil the fine structure of the fog comes into play, the increase in the travel time of the heat from the walls was achieved this time by using a photo-electric counter with a fog-tube of 8 cm diameter and a light beam of 2.8 cm diameter as in the «Standard Counter 1946». As expected, creep was found in every single measurement up to readings of 53%. Typical examples of the galvanometer pointer-movement and photographic records of the extinction during fog formation in such a wide fog-tube for readings between approx. 10 and 76% are given and their peculiarities discussed.The extinction over the range from 175 000 to 20 000 nuclei/cm³ was also measured with a red and a blue monochromatic interference filter and the results contrasted against the computed extinctions for these two wave lengths. It was ascertained that for the same number of nuclei the extinction for red light is in general larger than that for blue; the difference between the observed extinctions varies considerably, becoming zero or even negative. The most striking feature, however, is the different course of the extinction for the two wave lengths as a function of the number or size of the droplets.The size of the fog droplets in the counter was deduced from the extinction measurements for these two wave lengths and by collecting the falling droplets on coated slides. The radius of the droplets obtained by the optical method varies from 1.81 to 3.19 when the extinction decreases from 86 to 56%. The radius of the droplets as deduced from gelatine coated slides dyed with Naphtol Green B increases from 1.44 at 67.4% extinction (42 400 nuclei/cm³) to 6.30 at 15.6% (858 nuclei/cm³).

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Zusammenfassung Der Einflus der isothermalen Destillation, des Einschrumpfens der Tröpfchen durch Verdunstung ohne Wiederkondensation des freiwerdenden Wasserdampfes, des Zusammenfliessens und Absetzens der Nebeltröpfchen auf die Extinktion, welche im Nebel des photo-elektrischen Kernzählers stattfinden und die in den ersten Sekunden nach seiner Bildung eine kleine zusätzliche Extinktion (im folgenden Kriechen genannt) erzeugen können, wurde numerisch geprüft. Der entsprechende Beitrag jedes einzelnen der oben genannten Prozesse zum Gesamtbetrag des beobachteten Kriechens wurde abgeschätzt. Es wurde gefunden, dass isothermale Destillation zusätzliche Extinktions-Beträge (bis zu 1.70%) erzeugen kann, welche jene durch Verdunstung oder Zusammenfliessen der Tröpfchen verursachten, beträchtlich übersteigen. Die Resultate dieser Berechnungen erklären das Auftreten des Kriechens bei Konzentrationen grösser als ca. 25 000 Kerne per cm³ in Nebelrohren von 3.85 cm Luftsäulen-Durchmesser.Dass das Verschwinden des Kriechens in Nebelrohren mit einem Durchmesser von 2.5 cm und weniger dem beschleunigten Wärmefluss von den Wänden des engen Nebelrohres zuzuschreiben ist, wurde früher durch eine entsprechende Verengung des Lichtbündels, welches zur Durchleuchtung des Nebels verwendet wird, bewiesen. Um dem Einwand zu begegnen, dass bei so starker Verkleinerung des Querschnittes des Lichtbündels, wie sie benützt wurde, schon die Feinstruktur des Nebels eine Rolle spielt, wurde diesmal die Verlängerung der Laufzeit der Wärme von den Wänden durch Erweiterung des Nebelrohres auf 8 cm Durchmesser erzielt, während der Durchmesser des Lichtbündels mit 2.8 cm — wie im «Standard photo-elektrischen Kernzähler 1946» — unverändert belassen wurde. Entsprechend den Erwartungen wurde bei jeder einzelnen Messung bis zu Lesungen von 53% Kriechen festgestellt. Typische Beispiele der Bewegung des Galvanometer-Zeigers und photographische Aufzeichnungen der Extinktion während der Nebelbildung in einem solchen weiten Nebelrohr werden für Lesungen zsischen ca. 10 und 76% gegeben und ihre Eigentümlichkeiten besprochen.Die Extinktion für Konzentrationen zwischen 175 000 und 20 000 Kernen per cm³ wurde auch mit einem roten und blauen Interferenz-Filter gemessen und die Resultate den für diese zwei Wellenlängen berechneten Extinktionen gegenübergestellt. Es wurde festgestellt, dass bei der gleichen Kernzahl die Extinktion für rotes Licht im allgemeinen grösser ist als jene für blaues; die Differenz zwischen den beobachteten Extinktionen schwankt beträchtlich, wird null oder sogar negativ. Am auffallendsten ist jedoch der verschiedene Verlauf der Extinktion für die zwei Wellenlängen als Funktion der Zahl oder Grösse der Tröpfchen.Die Grösse der Nebeltröpfchen im Nebelrohr des photo-elektrischen Kernzählers wurde aus den Extinktions-Messungen in diesen zwei Wellenlängen und durch Auffangen der fallenden Tröpfchen auf Mikroskop-Objektträgern und Deckgläsern, welche mit gefärbter Gelatine überzogen waren, bestimmt. Der Radius der Tröpfchen, welcher mittels der optischen Methode ermittelt wurde, liegt zwischen 1.81 und 3.19 , wenn die Extinktion von 86 auf 56% abnimmt.Der Tröpfchenradius, wie er aus den Flecken auf den Mikroskopgläschen, deren Gelatineüberzug mit Naphtol Grün B eingefärbt war, bestimmt wurde, wächst von 1.44 bei 67.4% Extinktion (42 400 Kerne per cm³) auf 6.30 bei 15.6% (858 Kerne per cm³).

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The research reported in this article has been sponsored and supported in part by the Geophysics Research Directorate of the Air Force Cambridge Research Center, Air Research and Development Command, United States Air Force, under Contract AF 61(052)-26, through the European Office, ARDC in Brussels.