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1.
Pole-to-pole moisture conditions for the IGY 总被引：1，自引：0，他引：1
Summary A study of the mean atmospheric humidity conditions on a planetary scale during the IGY covering the calendar year 1958 is presented. The fields of mean precipitable water content and of the zonal and meridional transports of water vapor are analyzed for the entire globe. Zonally averaged values of the various quantities at several levels are presented in tabular form and compared whenever possible with previous results or indirectly are analyzed on the basis of information obtained from different sources. The structure of these fields is studied and the corresponding implications for the general circulations of the atmosphere are discussed. Finally the zonal water balance for all the globe is discussed and its implications analyzed. 相似文献
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Four co-ignimbrite plumes were generated along the flow path of the pyroclastic flow of 7 August 1980 at Mount St. Helens.
Three of the plumes were generated in discrete pulses which can be linked to changes in slope along the channel. One plume
was generated at the mouth of the channel where the flow decelerated markedly as it moved onto the lower slopes of the pumice
plain. Plume generation here may be triggered by enhanced mixing due to a hydraulic jump associated with an abrupt slope change.
Measurements of plume ascent velocity and width show that the co-ignimbrite plumes increased in velocity with height. The
plumes have initial velocities of 1–2 m/s. Two of the plumes reached a velocity maximum (4.6 and 8.8 m/s, respectively, at
heights of 270 and 315 m above the flow) and thereafter decelerated. The other plumes reached velocities of 6.2 and 13 m/s.
The four plumes become systematically less energetic downstream as measured by their ascent rates, which can be interpreted
as a consequence of decreasing interaction of the pyroclastic flow front with the atmosphere. Theoretical models of both co-ignimbrite
plumes and discrete co-ignimbrite clouds assume that there is no initial momentum, and both are able to predict the observed
acceleration stage. The rising plumes mix with and heat air and sediment out particles causing their buoyancy to increase.
Theoretical models agree well with observations and suggest that the initial motion of the ascending material is best described
as a discrete thermal cloud which expands as it entrains air, whereas the subsequent motion of the head may become influenced
by material supplied from the following plume. The models agree well with observations for an initial temperature of the ash
and air mixture in the range of 500–600 K, which is in turn consistent with the measured initial ash temperature of around
920 K. Ash masses of 3.4×105 to 1.8×106 kg are estimated.
Received: 11 January 1996 / Accepted: 7 October 1996 相似文献
4.
Murray Close Phil Abraham Judith Webber Eliza Cowey Bronwyn Humphries Graham Fenwick Simon Howard Kimberly Huynh Travis Grace Pierre-Yves Dupont Louise Weaver 《Ground water》2020,58(6):901-912
The vast majority of microorganisms in aquifers live as biofilms on sediment surfaces, which presents significant challenges for sampling as only the suspended microbes will be sampled through normal pumping. The use of a down-well low frequency sonicator has been suggested as a method of detaching microbes from the biofilm and allowing rapid sampling of this community. We developed a portable, easy to use, low-frequency electric sonicator and evaluated its performance for a range of well depths (tested up to 42 m below ground level) and casing types. Three sonicators were characterized in laboratory experiments using a 1 m long tank filled with pea gravel. These included a commercially available pneumatic sonicator, a rotating flexible shaft sonicator, and the prototype electric sonicator. The electric sonicator detached between 56 and 74% of microbes grown on gravel-containing biobags at distances ranging between 2 and 50 cm from the sonicator. The field testing comprises of a total of 55 sampling events from 48 wells located in 4 regions throughout New Zealand. Pre- and post-sonication samples showed an average 33 times increase in bacterial counts. Microbial sequence data showed that the same classes are present in pre- and post-sonicated samples and only slight differences were seen in the proportions present. The sampling process was rapid and the significant increases in bacterial counts mean that microbial samples can be quickly obtained from wells, which permits more detailed analysis than previously possible. 相似文献
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Karolina MOSTOWIK Damian KRZYCZMAN Eliza PACZKOWSKA Bartomiej RZONCA Janusz SIWEK Patryk WACAWCZYK 《山地科学学报》2021,(4):819-833
Flysch-type aquifers in the Eastern Carpathians usually feed periodic and low-discharge springs.However,in some areas,such as in the upper part of the Po(l)onin... 相似文献
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Summary By analogy with the calculation from data of angular momentum flow across latitude surfaces in the earth's atmosphere, the corresponding calculation is proposed for the case of our galaxy and possibly other spiral nebulae. A cylindrical wall of constant radius is used to replace the latitude wall, and the subject is developed through consideration of an ideal model. Gravitational torques enter the problem in addition to advective effects and possible other torques in actual systems. The relation of gravitational torques to the structure of ordinary spirals is discussed, and certain more special effects for the case of barred spirals are introduced and discussed. The connection of the subject with the classical theory of tidal evolution is pointed out.
Zusammenfassung Analog mit der Berechnung von Daten des Flusses des Momentes der Bewegungsgrösse über Breiten-Oberflächen in der Erd-Atmosphäre wird eine korrespondierende Berechnung für den Fall unseres Sternsystems und eventuell anderer spiraler Himmelskörper vorgeschlagen. Eine zylindrische Wand mit konstantem Radius wird benutzt, um die Breitenwand zu ersetzen, und dieses Problem wird entwickelt durch die Betrachtung eines idealen Modelles. Drehmomente der Schwerkraft kommen bei diesen Problem hinzu, zusätzlich der Wirkungen von Advektion und in aller Wahrscheinlichkeit anderer Drehmomente in den vorhandenen Systemen. Die Beziehung der Drehmomente der Schwerkraft in Bezug auf gewöhnliche Spiralen ist besprochen, und gewisse mehr spezialisierte Wirkungen für den Fall von Stangen-Spiralen werden eingeführt und besprochen. Der Zusammenhang dieses Problems mit der klassischen Theorie von Drehmomenten der Gezeiten ist nachgewiesen.
Sommario In analogia ai calcoli che, partendo da dati sperimentali, vengono fatti sul trasferimento del momento angolare fra zone dell'atmosfera a diverse latitudini, vengono qui proposti corrispondenti calcoli per la nostra galassia e possibilmente per altre nebulose a spirale. Viene usata una superficie cilindrica a raggio costante in sostituzione della superficie conica a latitudine costante; l'argomento è sviluppato secondo un modello ideale. La coppia gravitazionale viene presa in considerazione insieme agli effetti convettivi e ad altre possibili coppie. Viene discussa la relazione fra la coppia gravitazionale e la struttura di una spirale ordinaria; sono quindi introdotti e discussi certi effetti nel caso di spirali a sbarra. Infine viene messo in luce la relazione del presente argomento con la teoria classica della coppia dovuta alle marce.相似文献
7.
Peixoto Filho Flávio Tito Vargas Junior Euripedes do Amaral Santos Erick Slis Raggio Ferreira Francisco Henriques 《Geotechnical and Geological Engineering》2021,39(6):4127-4142
Geotechnical and Geological Engineering - In coring operations, core jamming is a permanent concern, taking place when the rock core sample becomes stuck within the inner core barrel, thus... 相似文献
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Summary General harmonic analysis (FFT) and maximum entropy spectral analysis (MEM) are used in order to study annual and monthly values of air temperature, precipitation and insolation in a number of weather stations in Duero Hydrographic Basin. The corresponding spectra estimates were prepared and compared. MEM estimates show better power resolution and a better spectral definition than FFT estimates. Based on the similarity behavior of the spectra, four main climatic zones were clearly defined. Finally, physical interpretation of the main features of the most representative spectra for the four regions was attempted.With 9 Figures 相似文献
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Summary Harmonic analyses along latitudes 30°, 45° and 60° of the mean northern hemisphere water vapor field are presented. The seasonal variations of these spectra are investigated and the relative contributions of the various scales of mean eddies to the meridional transport of water vapor are calculated. Of special interest is the finding that perturbations of wave number 2, corresponding to the great continents and oceans, are dominant at all three latitudes and of primary importance in effecting the northward transport of water vapor.The research reported in this article was sponsored by the Geophysics Research Directorate, Air Force Cambridge Research Center, under Contract No. AF 19 (604)-2242. 相似文献
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We use N-body experiments to study the survival of power-law density cusps in mergers of spherical galaxy models. Steep cusps (e.g.
ρ∝r
-2) are preserved during mergers of equal-mass models; this may be viewed as a general consequence of the incomplete violent
relaxation observed in such mergers. Progenitor profile has a strong effect on remnant shape; steep cusps produce oblate remnants.
If bright ellipticals form by hierarchical mergers of faint ones, the lack of steep cusps in these galaxies is somewhat surprising.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献