The Corals of Steeple Ashton (English Upper Oxfordian), Wiltshire     

P.E. Negus  Louise Beauvais 《Proceedings of the Geologists' Association. Geologists' Association》1979,90(4):213-227

  相似文献   

Fine-grained rocks: Shales or physilites     

Charles E. Weaver 《Sedimentary Geology》1980,27(4):301-313

Fine-grained sediments and rocks containing a high percentage of phyllosilicate minerals have never been satisfactorily classified. Rocks names are poorly defined. The definition of many terms such as clay, clay mineral and shale are logically inconsistent. The major problems are caused by the assumption that there is a fixed relation between grain size and mineralogy and that structure is a basic parameter.Shallow-buried recent and ancient marine sediments with a high content of phyllosilicates commonly contain 60–80% clay and 20–40% silt. Phyllosilicates are present in approximately the same amounts as the clay-size material. Many fine-grained sediments that have been deeply buried commonly contain 30–40% clay; the phyllosilicate mineral content is in the range of 60–80%.In most fine-grained sediments, as deposited, the majority of the material is in the clay size. With burial and diagenesis, much of the clay-sized material grows to silt size. Thus, claystones are converted to siltstones.The term physil, an abbreviated form of phyllosilicate, is proposed to describe all sheet silicate minerals regardless of grain size. Physilites are rocks with a high content of physils. A simple classification is proposed in which size, mineralogy and structure are treated as independent variables.  相似文献   

Microwave remote sensing of sea ice in the AIDJEX Main Experiment     

W. J. Campbell  J. Wayenberg  J. B. Ramseyer  R. O. Ramseier  M. R. Vant  R. Weaver  A. Redmond  L. Arsenaul  P. Gloersen  H. J. Zwally  T. T. Wilheit  T. C. Chang  D. Hall  L. Gray  D. C. Meeks  M. L. Bryan  F. T. Barath  C. Elachi  F. Leberl  T. Farr 《Boundary-Layer Meteorology》1978,13(1-4):309-337

During the AIDJEX Main Experiment, April 1975 through May 1976, a comprehensive microwave sensing program was performed on the sea ice of the Beaufort Sea. Surface and aircraft measurements were obtained during all seasons using a wide variety of active and passive microwave sensors. The surface program obtained passive microwave measurements of various ice types using four antennas mounted on a tracked vehicle. In three test regions, each with an area of approximately 1.5 × 10⁴ m², detailed ice crystallographic, dielectric properties, and brightness temperatures of first-year, multiyear, and first-year/multiyear mixtures were measured. A NASA aircraft obtained passive microwave measurements of the entire area of the AIDJEX manned station array (triangle) during each of 18 flights. This verified the earlier reported ability to distinguish first-year and multiyear ice types and concentration and gave new information on ways to observe ice mixtures and thin ice types. The active microwave measurements from aircraft included those from an X- and L-band radar and from a scatterometer. The former is used to study a wide variety of ice features and to estimate deformations, while both are equally usable to observe ice types. With the present data, only the scatterometer can be used to distinguish positively multiyear from first-year and various types of thin ice. This is best done using coupled active and passive microwave sensing.We dedicate this work to our beloved friend William NordbergHe pioneered in microwave ice observations, and his brilliance and enthusiasm inspired all of us.  相似文献   

An analysis of Apollo lunar soil samples 12070,889, 12030,187, and 12070,891: Basaltic diversity at the Apollo 12 landing site and implications for classification of small‐sized lunar samples          下载免费PDF全文

Louise Alexander  Joshua F. Snape  Katherine H. Joy  Hilary Downes  Ian A. Crawford 《Meteoritics & planetary science》2016,51(9):1654-1677

Lunar mare basalts provide insights into the compositional diversity of the Moon's interior. Basalt fragments from the lunar regolith can potentially sample lava flows from regions of the Moon not previously visited, thus, increasing our understanding of lunar geological evolution. As part of a study of basaltic diversity at the Apollo 12 landing site, detailed petrological and geochemical data are provided here for 13 basaltic chips. In addition to bulk chemistry, we have analyzed the major, minor, and trace element chemistry of mineral phases which highlight differences between basalt groups. Where samples contain olivine, the equilibrium parent melt magnesium number (Mg#; atomic Mg/[Mg + Fe]) can be calculated to estimate parent melt composition. Ilmenite and plagioclase chemistry can also determine differences between basalt groups. We conclude that samples of approximately 1–2 mm in size can be categorized provided that appropriate mineral phases (olivine, plagioclase, and ilmenite) are present. Where samples are fine‐grained (grain size <0.3 mm), a “paired samples t‐test” can provide a statistical comparison between a particular sample and known lunar basalts. Of the fragments analyzed here, three are found to belong to each of the previously identified olivine and ilmenite basalt suites, four to the pigeonite basalt suite, one is an olivine cumulate, and two could not be categorized because of their coarse grain sizes and lack of appropriate mineral phases. Our approach introduces methods that can be used to investigate small sample sizes (i.e., fines) from future sample return missions to investigate lava flow diversity and petrological significance.  相似文献   

Response of a climate model to tidal mixing parameterization under present day and last glacial maximum conditions     

lvaro Montenegro  Michael Eby  Andrew J. Weaver  Steven R. Jayne 《Ocean Modelling》2007,19(3-4):125-137

Experiments with a climate model were conducted under present day and last glacial maximum conditions in order to examine the model’s response to a vertical mixing scheme based on internal tide energy dissipation. The increase in internal tide energy flux caused by a 120 m reduction in sea level had the expected effect on diffusivity values, which were higher under lower sea level conditions. The impact of this vertical diffusivity change on the Atlantic meridional overturning is not straightforward and no clear relationship between diffusivity and overturning is found. There exists a weak positive correlation between overturning and changes to the power consumed by vertical mixing. Most of the climatic response generated by sea level change was not related to alterations in the internal tide energy flux but rather to the direct change in sea level itself.  相似文献   

Observations of photometric profiles of two planetary nebulae     

R. Louise  A. Kherous 《Astrophysics and Space Science》1991,176(1):149-162

It is noted that the Abel integral of a Gaussian function is a Gaussian function. This special property is used in order to develop an analytic method for studying photometric profile in Planetary Nebulae. Monochromatic observations have been made at the Haute-Provence Observatory using the RCA-CCD (320×512 pixels) mounted at theF/6 Newtonian focus of the 1.2 m telescope. Among the observed nebulae, two of them (NGC 6778 and NGC 7354) are regular enough to test the photometric profile method. The nebular emissivity per volume unit is then obtained for H⁺ and O⁺⁺ ions.  相似文献   

Quantified,multi-scale X-ray fluorescence element mapping using the Maia detector array: application to mineral deposit studies     

Louise A. Fisher  Denis Fougerouse  James S. Cleverley  Christopher G. Ryan  Steven Micklethwaite  Angela Halfpenny  Robert M. Hough  Mary Gee  David Paterson  Daryl L. Howard  Kathryn Spiers 《Mineralium Deposita》2015,50(6):665-674

  相似文献   

Correspondence: Comment on “a parametrization of solar energy disposition in the climate system” (Wang et al., 2004)     

Andrew J. Weaver  Michael Eby 《大气与海洋》2013,51(4):293-294

  相似文献   

Diagnostics of subseasonal prediction biases of the Asian summer monsoon by the NCEP climate forecast system   总被引：1，自引：0，他引：1  

Xiangwen Liu  Song Yang  Arun Kumar  Scott Weaver  Xingwen Jiang 《Climate Dynamics》2013,41(5-6):1453-1474

Biases of subseasonal prediction of the Asian summer monsoon are diagnosed using daily data from the hindcasts of 45-day integrations by the National Centers for Environmental Prediction Climate Forecast System version 2. The retrospective forecasts often show apparent systematic biases, which are mostly represented by the underestimation of the whole Asian monsoon. Biases depend not only on lead time, but also on the stage of monsoon evolution. An abrupt turning point of bias development appears around late June and early July, when ensemble spread and bias growth of winds and precipitation show a significant change over the northwestern Pacific (NWP) and the South Asian summer monsoon (SASM) region. The abrupt turning of bias development of winds, precipitation, and surface temperature is also captured by the first two modes of multivariate empirical orthogonal function analysis. Several features appear associated with the abrupt change in bias development: the western Pacific subtropical high (WPSH) begins its first northward jump and the surface temperature over the Tibetan Plateau commences a transition from warm bias to cold bias, and a reversal of surface temperature biases occurs in the eastern tropical Indian Ocean and the SASM region. The shift of WPSH position and the transition of surface thermal bias show close relationships with the formation of bias centers in winds and precipitation. The rapid growth in bias due to the strong internal atmospheric variability during short leads seems to mainly account for the weak WPSH and SASM in the model. However, at certain stages, particularly for longer-lead predictions, the biases of slowly varying components may also play an important role in bias development of winds and precipitation.  相似文献   

What causes solar active region loops to exist at transition region temperatures?     

Louise K. Harra  Cristine H. Mandrini  Sarah A. Matthews 《Solar physics》2004,223(1):57-76

High-lying, dynamic loops have been observed at transition region temperatures since Skylab observations. The nature of these loops has been debated for many years with several explanations having been put forward. These include that the loops are merely cooling from hotter coronal loops, that they are produced from siphon flows, or that they are loops heated only to transition region temperatures. In this paper we will make use of combined SOHO-MDI (Michelson-Doppler Imager), SOHO-CDS (Coronal Diagnostic Spectrometer) and Yohkoh SXT (Soft X-ray Telescope) datasets in order to determine whether the appearance of transition region loops is related to small-scale flaring in the corona, and to estimate the magnetic configuration of the loops. The latter allows us to determine the direction of plasma flows in the transition region loops. We find that the appearance of the transition region loops is often related to small-scale flaring in the corona and in this case the transition region loops appear to be cooling with material draining down from the loop top.  相似文献