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91.
The various lobes and segments of the southern periphery of the Laurentide ice sheet reached their maximum extension at different times between 21,000 and 14,000 yr ago, but the CLIMAP date of 18,000 yr ago is taken as a reference level to review the distribution of major vegetational formations in central and eastern United States. Tundra was apparently confined to a narrow belt peripheral to the ice margin only in the Minnesota area and from northern Pennsylvania to New England, with extensions down the crest of the Appalachian Highlands at least as far as Maryland. Some areas south of the Great Lakes may later have been marked by treeless vegetation briefly as the ice retreated. The boreal forest to the south in the central United States was dominated by spruce; the jack pine that had prevailed during previous times was apparently eliminated by the time the ice reached its maximum. In the Appalachian Highlands and the Atlantic Coastal Plain, however, jack pine occurred along with spruce, which decreased in importance southward. The southern limit of the boreal forest in the Southeast was perhaps somewhere in southern Georgia and Alabama. Oak and other temperate deciduous trees were minor components of the boreal coniferous forests especially in the southern Appalacchians, but there is no evidence yet in the southeastern states for a relic mixed mesophytic forest 18,000 yr ago similar to the rich modern deciduous forests of the region, except possibly in the Lower Mississippi Valley. The climate in much of the Southeast was apparently dry as well as cool at that time; in Florida oak/pine scrub and prairie-like openings prevailed, and all but the deepest lakes dried up.  相似文献   
92.
Explosive eruptions of this large Quaternary rhyolitic volcano have produced voluminous pumice fall deposits and ignimbrites. A stratigraphie study reveals more than 30 fall deposits, totalling more than 90 km3, which have come from many different vents. Some are of plinian type, and one is among the largest known in the world. The main ignimbrite (Rio Caliente) is of intra-plinian type. In all, 140 km3 of rhyolitic material were erupted during the past 105 years, of which 50 km5 are dispersed well outside the volcano. The dense rock equivalent volume is 60 km3, of which fall deposits, ignimbrites and lava bodies comprise 45 %, 25 % and 30 % respectively. The average output rate of 0.06 km3 per century is nearly an order of magnitude less than for the most productive rhyolitic volcanoes known. A circular area 10 km across in the centre of La Primavera contains updomed lacustrine ashes and associated sediments, including a remarkable giant pumice bed, which probably accumulated in a caldera lake. La Primavera has no record of historical eruptions, and hot springs are the only signs of present activity, but the updoming is thought to be due to the uprise of a new acid pluton beneath the volcano and future eruptions are probable.
Zusammenfassung Explosionsartige Eruptionen des gro\en quartÄren Rhyolith-Vulkans La Primavera haben mÄchtige Bimstuffe und Ignimbrite aufgehÄuft. Eine stratigraphische Untersuchung hat über 30 Aschelagen erkennen lassen, die aus verschiedenen Schloten stammen und insgesamt mehr als 90 km3 an Volumen ausmachen. Einige davon gehören zum plimanischen Typ, von denen eine sogar die grö\te bisher bekannte Lage der Erde ist. Der Haupt-Ignimbrit (Rio Caliente) gehört zum intraplimanischen Typ. Insgesamt wurden in den letzten 100 000 Jahren 140 km3 rhyolithisches Material ausgeworfen, von denen 50 km3 deutlich au\erhalb des eigentlichen Vulkans liegen. Das Äquivalentvolumen des dichten Gesteins betrÄgt 60 km3, von dem 45 % auf Tuffe, 25 % auf Ignimbrite und 30 % auf Lavakörper entfallen. Die durchschnittliche Auswurfrate von 0,06 km3 pro Jahrhundert liegt fast eine Grö\enordnung unter den meisten bekannten aktiven Rhyolith-Vulkanen. Ein kreisrundes Gebiet von 10 km Durchmesser im Zentrum des La Primavera zeigt aufgewölbte lakustrine Aschen und damit assoziierte Sedimente, darunter eine bemerkenswerte riesige Bimslage, die wahrscheinlich in einem Caldera-See abgelagert wurde. Der Vulkan La Primavera ist in historischer Zeit nicht ausgebrochen und hei\e Quellen sind die einzigen Anzeichen heutiger AktivitÄt, aber die Aufwölbung wird als Hinweis auf das Hochdringen eines neuen sauren Plutons unter dem Vulkan angesehen, so da\ zukünftige Eruptionen wahrscheinlich sind.

Résumé Des éruptions explosives de ce grand volcan rhyolitique quaternaire ont produit de volumineux dépÔts de ponces et d'ignimbrites. Une étude stratigraphique fait apparaÎtre plus de 30 dépÔts totalisant plus de 90 km3 provenant de nombreuses bouches volcaniques différentes. Certaines sont du type plinien, dont l'une est parmi les plus grandes connues au monde. L'ignimbrite principale (Rio Caliente) est du type intraplinien. En tout 140 km3 de matériaux rhyolitiques ont été rejetés au cours des 105 dernières années, dont 50 km3 ont été dispersés bien au delà du volcan. Le volume de roche compact équivalent est de 60 km3, parmi lequel les tuffs, les ignimbrites et les laves occupent respectivement 45%, 25% et 30%. L'émission moyenne, de 0,06 km3 par siècle, est d'un ordre de grandeur moindre que pour la plupart des volcans rhyolitiques les plus productifs actuellement connus. Une région circulaire de 10 km de diamètre dans le centre de La Primavera contient des domes de cendres lacustres et autres sédiments associés, et parmi eux une couche géante de ponce remarquable, qui s'est probablement accumulée dans un lac-caldère. On ne connaÎt pas d'éruptions historiques de la Primavera, et seules des sources chaudes témoignent d'une activité actuelle; toutefois on pense que l'allure en dome est due à la poussée d'un nouveau pluton acide sous le volcan, et que des éruptions sont probables dans le futur.

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93.
The Iforas (60 000 km2) falls within the Pan-African mobile belt bordering the West-African craton in north-eastern Mali Republic. It is characterized by major N-S shear belts parallel to the edge of the craton which delimit longitudinal blocks some of which have undergone considerable horizontal displacements. The central core of the Iforas which consists largely of reactivated pre-Pan-African basement injected by Pan-African syn- and post-tectonic intermediate and acid plutonic rocks, has behaved as a relatively rigid blocks during the Pan-African dividing the orogenic belt into a western Iforas and an eastern Iforas.Western Iforas displays W to E zonation: an ophiolitic suture (Timetrine); trench volcano-sedimentary deposits cut by gabbros diorites and acid granitoids (Tilemsi); and a late orogenic composite »coastal range batholith intruding the pre-Pan-African basement of Central Iforas and its overlying volcano-sedimentary deposits which here display a littoral facies and a tillite.Central Iforas consists of two major units: a polycyclic pre-Pan-African basement metamorphosed under high amphibolite facies conditions of presumed Eburnean age and the Iforas granulite block bound to the W, N and E by shear zones.Eastern Iforas was totally separated during metamorphism and deformation from the Iforas granulite block. From West to East, three lithological assemblages have been recognised separed by shear belts: a Quartzite Group, a Gneissic Group and a Pelitic Group the latter representing the southern prolongation of the central Hoggar Pharusian province.Shear zones are an essential feature of Pan-African tectonism East of the West-African craton. The superimposed stress fields have been recognised producing: early N20° trending sinistral shear zones, a north-south dextral shear zone (Andjour-Tamaradant shear zone) and late conjugating sinistral NNW and dextral ENE wrench faults.Late Pan-African events reflect the uplift and unroofing of the Pan-African composite batholith, the intrusion of circular granite plutons often located close to shear zones and alternating episodes of distension and compression.Lastly the simple model proposed for the closing stages of the Pan-African in the Iforas is that of an active continental plate margin separated from the West African craton by an oceanic domain. Subsequent continental collision to the South with a promotory of the West African craton led to the formation of the Dahomeyan thrust front and modified the stress field. Closure of the oceanic domain of western Iforas is thought to have taken place by continued eastward subduction of the oceanic plate and sinistral movement along an inferred north westerly trending transform fault coinciding with the future Cretaceous Gao trough and an alignement of strong positive gravity anomalies. It was accompanied by the northerly migration of central and western Iforas along the conjugating dextral N-S Andjour-Tamaradant shear zone. Further shortening led to folding of the arcuate Timetrine-Ydouban-Gourma fold belt overlying the deformed margin of the West African craton.
Zusammenfassung Das Iforas-Gebiet (60 000 km2) gehört zur pan-afrikanischen Bewegungszone, die in Mali an das westafrikanische Kraton grenzt. Diese Zone wird von N-S Scherbewegungen parallel zum Kraton durchzogen, wobei größere horizontale Versetzungsbeträge langgestreckte Blöcke herausgetrennt haben. Der zentrale Teil von Iforas besteht im wesentlichen aus reaktiviertem prae-panafrikanischem Basement, das in pan-afrikanischer Zeit von syn- und posttektonischen, intermediären und sauren Plutoniten intrudiert wurde. Dieses Gebiet wirkt als relativ starrer Block, der während der pan-afrikanischen Orogenese den Orogengürtel in einen westlichen und einen östlichen Ast teilt. Das westliche Iforas-Gebiet zeigt eine E-W Zonierung: eine Ophiolith-Sutur, einen vulkano-sedimentären Gürtel und einen Rand-Batholithen.Zentral-Iforas wird aus zwei Einheiten aufgebaut: ein mehrfach metamorphisiertes Basement und einen Granitblock.In den überregionalen Scherzonen lassen sich drei Stress-Felder erkennen: eine ältere 20° streichende sinistrale Scherzone, eine N-S dextrale Scherzone und jüngere NNW und dextrale ENE Bruchzonen.Spät-pan-afrikanische Ereignisse sind durch Heraushebung und Abtrag, Granitintrusionen und wechselnden Dehnungs- und Kompressionsbewegungen gekennzeichnet.

Résumé L'Adrar des Iforas (60 000 km2) fait partie de la zone mobile pan-africaine en marge du craton ouest-africain au Nord-Est de la République du Mali. La région est caractérisée par d'importants accidents mylonitiques parallèles à la bordure du craton qui délimitent des compartiments longitudinaux dont certains ont subi des déplacements horizontaux considérables. La zone dorsale des Iforas qui consiste essentiellement en un socle pré-pan-africain réactivé et injecté au Pan-Africain par des roches plutoniques intermédiaires et acides, syn- et post-tectoniques, s'est comportée en compartiments relativement rigides au cours du Pan-Africain, divisant la chaîne en un rameau occidental et un rameau oriental.Le rameau occidental présente une zonation d'Ouest en Est: une suture ophiolitique (Timetrine); des dépôts volcano-sédimentaires de fosse recoupés par des gabbros et des diorites; et un vaste batholite composite tardi-orogénique qui recoupe le socle pré-pan-africain de la zone dorsale des Iforas et sa couverture de dépôts volcanosédimentaires ici à faciès littoral.La zone dorsale des Iforas comprend deux unités majeures: un socle prépan-africain polycyclique métamorphisé dans le faciès amphibolite, d'âge éburnéen présumé et le môle granulitique des Iforas, délimité à l'W, au N et à l'E par des accidents mylonitiques.Le rameau oriental était séparé du môle granulitique des Iforas lors du métamorphisme et de la déformation. D'W en E, on trouve trois unités séparées par des zones mylonitiques: un Groupe de Quartzites, un Groupe de Gneiss et un Groupe de Pélites. Ce dernier représente le prolongement vers le Sud de la province pharusienne du centre Hoggar.Les grands accidents de cisaillement sont un fait marquant du tectonisme pan-africain à l'Est du craton ouest-africain. Trois champs de contraintes superposées ont produit des accidents précoces sénestres de direction N20, un accident N-S dextre (Andjour-Tamaradant), et des failles cisaillantes tardives conjuguées d'orientation NNW sénestres et ENE dextres.Les événements pan-africains tardifs sont marqués par la surrection et l'érosion des batholites pan-africains, la mise en place de plutons granitiques souvent à proximité des grands accidents et par des alternances de distensions et de compressions.Enfin un modèle simple est proposé pour les stades ultimes du Pan-Africain dans l'Adrar des Iforas: une marge continentale active séparée du craton ouest-africain par un domaine océanique; suite à une collision au Sud avec un promontoire du craton ouestafricain qui aurait produit le front de chevauchement dahomeyen et modifié le champ de contraintes, la fermeture du domaine océanique de l'Ouest Iforas se serait produite par subduction à l'E de la plaque océanique et une translation sénestre le long d'une faille transformante orientée NW et coincidant avec le fossé crétacé de Gao et un alignement d'anomalies gravimétriques positives. Elle aurait été accompagnée par le déplacement vers le N de l'Iforas occidental et central le long de l'accident cisaillant dextre d'Andjour-Tamaradant. Cette fermeture aurait provoqué les plissements de la chaîne du Timetrine-Ydouban-Gourma qui repose sur la bordure déformée du craton ouestafricain.

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94.
Feedback occurs between many components of the climate system, and makes the study of climate very difficult. A modeling approach is presented in which feedbacks are represented specifically. Analysis of very simple models shows how feedback between two components affects their behavior; positive feedback increases persistence, and can produce climatic changes even without changes in external forcing. In any quantitative study, the magnitudes of all relevant feedbacks must be known accurately. As an example, it is shown how the effect of CO2 on global temperature must depend greatly on the feedback between global temperature and ice extent.  相似文献   
95.
The behavior of electric and magnetic field variations over the eastern coastal region of North America is studied using a scaled laboratory electromagnetic analogue model. The model source frequency used simulates a period of 1 h in the geophysical scale. The results indicate that deflection and conductive channelling of induced electric current is important for both the E-polarization (northeast-southwest direction of the electric field of the source) and the H-polarization (northwest-southeast) of the source field. In the model, conductive channelling occurs through the Strait of Belle Isle, Cabot Strait, and in the St. Lawrence River. Current deflection is particularly prevalent around the southeast coast of Newfoundland for both E- and H-polarization, and around the northeast coastline of Nova Scotia for E-polarization. The model results also show current deflection by cape and bay coastal features, as well as by ocean depth contours.A comparison of model measurements for the cases of a uniform source field and a line current source indicate that the nature of the source field has a measurable but surprisingly small effect on the vertical to horizontal magnetic field ratio for both E- and H-polarizations, and negligible effect on the magnetotelluric ratio for coastal regions.The model fields in coastal regions were found to be strongly influenced by induced currents, deflected and channelled by the coastline and ocean bathymetry, and were dependent on the nature and particularly the polarization of the source field. Thus, along the complex coastline of eastern North America, a wide range of electric and magnetic field values should be expected. In some regions the coast effect, measured by the vertical to horizontal magnetic field ratio at the coast, could be expected to be extremely small or absent, while in other regions the ratio could approach a value as large as unity for variations of 1 h period.  相似文献   
96.
Radial velocity anomalies in the lower mantle that give rise to triplications in the travel-time curve for short-periodP waves will produce arrivals havingdT/d values that differe by roughly 0.2–0.5 s/deg. The first two arrivals associated with such triplications will be separated by less than one second over a distance range of 4°–10° they may not, therefore, be separable visually on single seismograms, so that their presence can only be inferred from some measurable property that depends on their mutual interference. If there are lateral variations in the regions of anomalous velocity gradients, the interfering signals will also have different azimuths of arrival. Using two synthetic wavelets we have investigated the effect of interference on bothdT/d and azimuth measurements at the Yellowknife Array. We found that if the interfering pulses have a dominant frequencyv, there is a range of time separations (0.30/v0.55/v) over which the measureddT/d and azimuth values may fluctuate by much more than the differences indT/d and azimuth between the interfering signals. We have evaluated the following empirically defined functions for three different primary signals, and for three different relative amplitudes of the interfering signals:f (t), the drift function, which expresses how the measured slownesses,p, and azimuths, , differ from the slownesses and azimuths of the primary wavelets; f(), the range function, which describes the behaviour of the upper and lower bounds ofp and as a function of the difference in arrival times of the signals, andf , studied the properties of these functions, and have outlined how these properties provide criteria based on the numerical and statistical characteristics of the arrival vectors, and on the waveform of the signal that will enable small radial velocity anomalies to be more clearly delineated.Contribution No. 863 from the Earth Physics Branch.  相似文献   
97.
A 2-year study of sedimentation in Lake Biel reveals that three major factors can account for the spatial and temporal patterns of tripton sedimentation. Allochthonous inputs of particulate matter mostly derived from the Aare river during spring snowmelt and other high-water periods, provide about 50% of the carbonate and 50% of the siliceous matter collected in sediment traps. Phytoplankton activity in this eutrophic, hard-water lake accounts for the rest of the carbonate and siliceous matter, the latter being mostly diatom frustules. Sedimentation rates are thus highest during periods of maximum river flooding, maximum phytoplankton activity and following the breakdown of the thermocline, at which time trapped particles settle out. Resuspension of sediment is important in at least one basin. Resolution of carbonate appears to be minor.  相似文献   
98.
Repeated electronic distance measurements across Kilauea Caldera with Tellurometers and Geodimeter show definite horizontal expansion related to the vertical uplift and outward tilting of the summit prior to an eruption, and contraction during and after a flank eruption. Measurements started in October 1964, along a 3098 meter line between Uwekahuna and Keanakakoi, indicate a relatively uniform lengthening of 12 centimeters during the interval October 22, 1964 to March 1, 1965. Rapid shortening of the line by 28 centimeters was measured 4 days after the beginning of a flank eruption which involved emission of approximately 29 million cubic meters of lava during the period March 5 to March 15, 1965. During the expansion, the standard deviation of 10 Tellurometer measurements from a least-squares srtaight line solution is ± 2.0 centimeters (6.5 ppm) whereas 9 Geodimeter measurements have a standard deviation of ± 1.1 (3.6 ppm) centimeters. Absolute distance readings between the two instruments differ by 4 centimeters (13 ppm), but relative changes in distance were the same on both instruments. Changes in distance across Kilauea Caldera can, therefore, be easily measured to accuracies of 4 to 7 parts per million with standard electronic distance measuring systems. On active volcanoes where ground surface deformation exceeds 10–100 parts per million with changes in subsurface magma pressure or volume, repeated horizontal distance measurements can be a most useful technique.  相似文献   
99.
Short gravity-capillary waves, the predominant radar scatterers under many oceanic and radar-viewing conditions, are modulated in amplitude, velocity and orientation by the larger-scale motions of the ocean surface. These modulations render the larger scales observable to microwave radar. The high data rate and advanced technology of modern radar systems make it possible to measure these modulations and, in some cases, to display them as images of the ocean surface. While the modulation of orientation and velocity are straightforward to understand, the amplitude modulation is a dynamic response of the equilibrium short gravity-capillary waves to larger scale driving forces including straining by orbital velocities of large waves. Microwave studies of the growth and equilibrium of short wind-generated waves are reviewed. It is shown that the response of these waves to straining can produce modulations in radar cross-section greater than those due to tilting but which are wind-speed dependent. The net modulation depends strongly on the direction as well as the magnitude of the wind speed. Quantitative determination of ocean wave-height spectra from measured modulations will therefore be a complicated procedure. Measurements of ocean waves with CW Doppler and Synthetic Aperture radars are discussed in the light of these findings.  相似文献   
100.
Summary. In 1984, the Australian Bureau of Mineral Resources and the Geological Survey of Queensland recorded a regional seismic reflection profile of over 800 km length from the eastern part of the Eromanga Basin to the Beenleigh Block east of the Clarence Moreton Basin. A relatively transparent upper crustal basement with an underlying, more reflective lower crust is characteristic of much of the region. Prominent westerly dipping reflectors occur well below the sediments of the eastern margin of the Clarence Moreton Basin and the adjacent Beenleigh Block, and provide some of the most interesting features of the entire survey. A wide angle reflection/refraction survey of 192 km length and an expanding reflection spread of 25 km length were recorded across the Nebine Ridge. The only clear deep reflectors are interpreted as P-to-SV or SV-to-P converted reflections from a mid-crustal boundary at a depth of about 17 km. The combined Nebine Ridge data provide well-constrained P and S wave velocity models of the upper crust, and suggest a crustal structure quite different from that beneath the adjacent Mesozoic basins.  相似文献   
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