First Lunar Flashes Observed from Morocco (ILIAD Network): Implications for Lunar Seismology     

Mamoun Ait Moulay Larbi  Ahmed Daassou  David Baratoux  Sylvain Bouley  Zouhair Benkhaldoun  Mohamed Lazrek  Raphael Garcia  Francois Colas 《Earth, Moon, and Planets》2015,115(1-4):1-21

  相似文献   

Mineral grain availability and pupal-case building by lotic caddisflies: Effects on case architecture, stability and building expenses     

Bernhard Statzner  Sylvain Dolédec 《Limnologica》2011,41(3):266-280

The retreat-making larvae of many lotic caddisflies build entirely new pupal cases with fine gravel and sand that they collect in the neighbourhood of the building place to fix it with silk to cobbles in swift flow (where finer sediments are generally rare). Previous field observations on Hydropsyche siltalai pupal cases illustrate that natural local resource limitations of the preferred grain fraction (2.5–3.15 mm) produced chained effects across other grain fractions, as the alternative use of more grains in the 1.6–2 mm fraction (an unlimited resource) induced an increased use of more grains in the 0.315–0.5 mm fraction (another unlimited resource). To examine the implications of these observations for H. siltalai, we used (1) mesocosms to created minor deviations in the availability of the natural grain size composition of the building material of pupal cases at otherwise carefully replicated natural stream habitat conditions and (2) recently developed technologies to assess many case characteristics so far ignored in studies of caddisfly cases. When the preferred coarser grains (2.5–3.15 mm) were unavailable, more grains with intermediate size (1.25–2.0 mm) were used (and not other, still available coarse grains) and fewer larvae built cases in groups, thereby not only loosing the benefits (lower costs for grain transport and silk) but also avoiding potential disadvantages associated with grouped cases (more aggressive encounters with conspecifics for rare building material, less flow exposure and thus reduced water renewal in the pupal chamber). Unavailability of 2.5–3.15-mm and 0.315–0.5-mm grains caused a reduction of larvae building in groups, more use of grains with intermediate size, changes of several other grain characteristics (e.g. number, circularity) and considerable investment into silk to maintain the case resistance. Finally, grain availability deviating most from that observed in nature (no grains of 2.5–3.15 mm and 1.6–2.0 mm) caused dramatic responses, as mortality increased so that fewer pupal cases were built, using typically more coarse grains so that many cases had an elevated resistance against crushing forces; in addition, many males had a retarded development, whereas female development was unaffected. Thus, the response of H. siltalai to any of the three types of grain limitations differed, illustrating an immense diversity to respond to grain-size shortage.  相似文献   

A new slope mass rating in mountainous terrain, Jammu and Kashmir Himalayas: application of geophysical technique in slope stability studies     

R. P. Singh  C. S. Dubey  S. K. Singh  D. P. Shukla  B. K. Mishra  M. Tajbakhsh  P. S. Ningthoujam  M. Sharma  N. Singh 《Landslides》2013,10(3):255-265

The slopes of western Lesser Himalaya (at Sangaldhan Block of Udhampur near Ramban, Jammu and Kashmir India) are being severely affected by tectonic and erosional activities. These activities result in deposit of a thick cover of rock fragments and overburden just above the hard rock. The thickness of overburden cover has directly affected the stability of slope in the study area, though the traditional stability estimation techniques, rock mass rating and slope mass rating, rate this area as moderately stable which does not represent the real stability condition. In this research work, the geotechnical and geophysical surveys have been carried out to reckon the slope stability conditions more accurately as compared to traditional slope stability estimation techniques. A new rating, new slope mass rating, is developed, which gives a better picture of the stability of slopes. It incorporates a new parameter of overburden thickness profile, along with slope angle and other associated factors on the slopes of the mountainous terrains. The vertical electrical sounding surveys were conducted for the demarcation of rock–overburden interface and for determining the overburden cover. This new classification depicts an increase of 12.84 % in unstable slope areas giving a better assessment and factual picture of slope stability in our study area. This study also enumerates the importance of geophysical applications in slope stability studies. The research work is applicable in mountainous terrains such as Himalaya, and the major component of the application is the orientation of overburden or the profile of thickness in relation with slope of surface.  相似文献   

Opaque minerals,magnetic properties,and paleomagnetism of the Tissint Martian meteorite     

Jérôme Gattacceca  Roger H. Hewins  Jean‐Pierre Lorand  Pierre Rochette  France Lagroix  Cécile Cournède  Minoru Uehara  Sylvain Pont  Violaine Sautter  Rosa. B. Scorzelli  Chrystel Hombourger  Pablo Munayco  Brigitte Zanda  Hasnaa Chennaoui  Ludovic Ferrière 《Meteoritics & planetary science》2013,48(10):1919-1936

  相似文献   

Volatile transport on inhomogeneous surfaces: I – Analytic expressions,with application to Pluto’s day     

Olivier Mousis  Jonathan I. Lunine  Eric Chassefière  Franck Montmessin  Azzedine Lakhlifi  Sylvain Picaud  Jean-Marc Petit  Daniel Cordier 《Icarus》2012,218(1):80-87

The two orders of magnitude drop between the measured atmospheric abundances of non-radiogenic argon, krypton and xenon in Earth versus Mars is striking. Here, in order to account for this difference, we explore the hypothesis that clathrate deposits incorporated into the current martian cryosphere have sequestered significant amounts of these noble gases assuming they were initially present in the paleoatmosphere in quantities similar to those measured on Earth (in mass of noble gas per unit mass of the planet). To do so, we use a statistical-thermodynamic model that predicts the clathrate composition formed from a carbon dioxide-dominated paleoatmosphere whose surface pressure ranges up to 3 bars. The influence of the presence of atmospheric sulfur dioxide on clathrate composition is investigated and we find that it does not alter the trapping efficiencies of other minor species. Assuming nominal structural parameters for the clathrate cages, we find that a carbon dioxide equivalent pressure of 0.03 and 0.9 bar is sufficient to trap masses of xenon and krypton, respectively, equivalent to those found on Earth in the clathrate deposits of the cryosphere. In this case, the amount of trapped argon is not sufficient to explain the measured Earth/Mars argon abundance ratio in the considered pressure range. In contrast, with a 2% contraction of the clathrate cages, masses of xenon, krypton and argon at least equivalent to those found on Earth can be incorporated into clathrates if one assumes the trapping of carbon dioxide at equivalent atmospheric pressures of ～2.3 bar. The proposed clathrate trapping mechanism could have then played an important role in the shaping of the current martian atmosphere.  相似文献   

Large-Scale Mapping of Hard-Rock Aquifer Properties Applied to Burkina Faso     

Nathalie Courtois  Patrick Lachassagne  Robert Wyns  Raymonde Blanchin  Francis D. Bougaïré  Sylvain Somé  Aïssata Tapsoba 《Ground water》2010,48(2):269-283

A country-scale (1:1,000,000) methodology has been developed for hydrogeologic mapping of hard-rock aquifers (granitic and metamorphic rocks) of the type that underlie a large part of the African continent. The method is based on quantifying the “useful thickness” and hydrodynamic properties of such aquifers and uses a recent conceptual model developed for this hydrogeologic context. This model links hydrodynamic parameters (transmissivity, storativity) to lithology and the geometry of the various layers constituting a weathering profile. The country-scale hydrogeological mapping was implemented in Burkina Faso, where a recent 1:1,000,000-scale digital geological map and a database of some 16,000 water wells were used to evaluate the methodology.  相似文献   

Fate and tidal transport of butyltin and mercury compounds in the waters of the tropical Bach Dang Estuary (Haiphong, Vietnam)     

Navarro P  Amouroux D  Thanh ND  Rochelle-Newall E  Ouillon S  Arfi R  Van TC  Mari X  Torréton JP 《Marine pollution bulletin》2012,64(9):1789-1798

In this work, two field campaigns were performed in July 2008 (wet season) and March 2009 (dry season) to produce original data on the concentration, partition and distribution of mercury and butyltin compounds along the tropical Bach Dang Estuary located in North Vietnam (Haiphong, Red River Delta). The results demonstrate that mercury and butyltin speciation in the surface waters of this type of tropical estuary is greatly affected by the drastic changes in the seasonal conditions. During high river discharge in the wet season, there was a large estuarine input of total Hg and tributyltin, while the longer residence time of the waters during the dry season promotes increasing MMHg formation and TBT degradation. Although most of the Hg and TBT is transported into the estuary from upstream sources, tidal cycle measurements demonstrate that this estuary is a significant source of TBT and MMHg during the wet (～3kgTBT/day) and dry (～3gMMHg/day) seasons.  相似文献   

The geological evolution of Merapi volcano, Central Java, Indonesia   总被引：1，自引：0，他引：1  

Ralf Gertisser  Sylvain J. Charbonnier  J?rg Keller  Xavier Quidelleur 《Bulletin of Volcanology》2012,74(5):1213-1233

Merapi is an almost persistently active basalt to basaltic andesite volcanic complex in Central Java (Indonesia) and often referred to as the type volcano for small-volume pyroclastic flows generated by gravitational lava dome failures (Merapi-type nuées ardentes). Stratigraphic field data, published and new radiocarbon ages in conjunction with a new set of ⁴⁰K–⁴⁰Ar and ⁴⁰Ar–³⁹Ar ages, and whole-rock geochemical data allow a reassessment of the geological and geochemical evolution of the volcanic complex. An adapted version of the published geological map of Merapi [(Wirakusumah et al. 1989), Peta Geologi Gunungapi Merapi, Jawa Tengah (Geologic map of Merapi volcano, Central Java), 1:50,000] is presented, in which eight main volcano stratigraphic units are distinguished, linked to three main evolutionary stages of the volcanic complex—Proto-Merapi, Old Merapi and New Merapi. Construction of the Merapi volcanic complex began after 170?ka. The two earliest (Proto-Merapi) volcanic edifices, Gunung Bibi (109?±?60?ka), a small basaltic andesite volcanic structure on Merapi’s north-east flank, and Gunung Turgo and Gunung Plawangan (138?±?3?ka; 135?±?3?ka), two basaltic hills in the southern sector of the volcano, predate the Merapi cone sensu stricto. Old Merapi started to grow at ~30?ka, building a stratovolcano of basaltic andesite lavas and intercalated pyroclastic rocks. This older Merapi edifice was destroyed by one or, possibly, several flank failures, the latest of which occurred after 4.8?±?1.5?ka and marks the end of the Old Merapi stage. The construction of the recent Merapi cone (New Merapi) began afterwards. Mostly basaltic andesite pyroclastic and epiclastic deposits of both Old and New Merapi (<11,792?±?90 ¹⁴C years BP) cover the lower flanks of the edifice. A shift from medium-K to high-K character of the eruptive products occurred at ~1,900 ¹⁴C years BP, with all younger products having high-K affinity. The radiocarbon record points towards an almost continuous activity of Merapi since this time, with periods of high eruption frequency interrupted by shorter intervals of apparently lower eruption rates, which is reflected in the geochemical composition of the eruptive products. The Holocene stratigraphic record reveals that fountain collapse pyroclastic flows are a common phenomenon at Merapi. The distribution and run-out distances of these flows have frequently exceeded those of the classic Merapi-type nuées ardentes of the recent activity. Widespread pumiceous fallout deposits testify the occurrence of moderate to large (subplinian) eruptions (VEI 3–4) during the mid to late Holocene. VEI 4 eruptions, as identified in the stratigraphic record, are an order of magnitude larger than any recorded historical eruption of Merapi, except for the 1872?AD and, possibly, the October–November 2010 events. Both types of eruptive and volcanic phenomena require careful consideration in long-term hazard assessment at Merapi.  相似文献   

Sampling strategies based on sets of behavioural parameters. Application to a simple pesticide fate model     

Thierry Leviandier  Stéphanie Madier  Sylvain Payraudeau 《Stochastic Environmental Research and Risk Assessment (SERRA)》2012,26(4):557-568

Sampling strategies are necessary to minimise the cost of data acquisition. We consider the case when several samples must be analysed at the same time, knowing rainfall data, optionally discharge data. We assume also that a rainfall-runoff and pesticide transfer model is available. Three methods are presented based on behavioural sets calculated on prior events, which provide optimal sampling times with respect to different statistical criteria, for a fixed number of samples. A methodology to compare these strategies, adapted to a context of data scarcity is proposed for proper validation. We consider that the combination of a model and a strategy is efficient if it does better than a strategy without a model based on equal volumes. Even with a simple and relatively poor model, it can be concluded that the different strategies are efficient and show similar efficiency in spite of their different levels of conceptual and algorithmic complexity.  相似文献   

Effect of magnetic activity on ionospheric time delay at low latitude     

Soumi Bhattacharya  Smita Dubey  Rajesh Tiwari  P. K. Purohit  A. K. Gwal 《Journal of Astrophysics and Astronomy》2008,29(1-2):269-274

The purpose of this work is to investigate the effect of magnetic activity on ionospheric time delay at low latitude Station Bhopal (geom. lat. 23.2°N, geom. long. 77.6°E) using dual frequency (1575.42 and 1227.60 MHz) GPS measurements. Data from GSV4004A GPS Ionospheric Scintillation and TEC monitor (GISTM) have been chosen to study these effects. This paper presents the results of ionospheric time delay during quiet and disturbed days for the year 2005. Results show that maximum delay is observed during quiet days in equinoxial month while the delays of disturbed period are observed during the months of winter. We also study the ionospheric time delay during magnetic storm conditions for the same period. Results do not show any clear relationship either with the magnitude of the geomagnetic storm or with the main phase onset (MPO) of the storm. But most of the maximum ionospheric time delay variations are observed before the main phase onset (MPO) or sudden storm commencement (SSC) as compared to storm days.  相似文献