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Terrestrial

The construction and mining industries offer additional applications for temporary structures, such as concrete forms and geo-textiles, as well as a wide variety of products for restoration of land including sand bags, turf covers and temporary protection for trees and plants. [Pg.595]

As in aquatic applications, weathering and hydrolysis are the dominant degradation mechanisms for terrestrial applications. Polymer articles covered with dirt can be problematic since photodegradation is not available however, the higher humidity levels and microbial activity in the soil when compared to the atmosphere are advantageous for degradation. [Pg.595]

Interesting innovations of a tagging procedure were to study the tracing of several foods of granivores in the field (Smigel et aL, 1974) and also to study the survival rate of a beetle in the field (Bate et al., 1974). In both studies, items were marked with a stable element, and during the course of the study, samples of interest were collected in the field, neutron-activated, and identified as to whether or not the sample had been previously maiiced with the stable tracer element. [Pg.13]

The granivores studied by Smigel et al. (1974) were the Merriam kangaroo rat (Dipodomys merriami) and the desert pocket mouse (Perognathus penicillatus). Seeds were solution-tagged with stable isotopes of rare elements, and the [Pg.13]

Bate et al, (1974) inunersed live elm bark beetles (Scolytus multistriatus) in a solution of 0.01% gold, placed them on elm (Ulmus) twigs, and collected live beetles at a later date. All beetles were subjected to a neutron flux, the tagged beetles were identified, and the survival rate was estimated. [Pg.15]

Bern 3. Concentration of tracer ° e components of East as a ftoi on [Pg.15]


To define the thennodynamic state of a system one must specify fhe values of a minimum number of variables, enough to reproduce the system with all its macroscopic properties. If special forces (surface effecls, external fields—electric, magnetic, gravitational, etc) are absent, or if the bulk properties are insensitive to these forces, e.g. the weak terrestrial magnetic field, it ordinarily suffices—for a one-component system—to specify fliree variables, e.g. fhe femperature T, the pressure p and the number of moles n, or an equivalent set. For example, if the volume of a surface layer is negligible in comparison with the total volume, surface effects usually contribute negligibly to bulk thennodynamic properties. [Pg.322]

Smith D and Spanel P 1995 Ions in the terrestrial atmosphere and in interstellar olouds Mass Spectrom. Rev. 14 255-78... [Pg.829]

Dalgarno A 1994 Terrestrial and extraterrestrial Advances In Atomic, Molecular and Optical Physics ed B Bederson and A Dalgarno (New York Aoademio)... [Pg.829]

Plenary 21 A. Alian Wang et al, e-mail address alianw levee.wustl.edu (RS). (Unable to attend IGORS, but abstract is available in proceedings.) With teclmological advances, Raman spectroscopy now has become a field tool for geologists. Mineral characterization for terrestrial field work is feasible and a Raman instrument is being designed for the next rover to Mars, scheduled for 2003. [Pg.1219]

Wisemberg J and Kockarts G 1980 Negative ion chemistry in the terrestrial D region and signal flow graph theory J. Geophys. Res 85 4642-52... [Pg.2813]

Zirconium is found in abundance in S-type stars, and has been identified in the sun and meteorites. Analysis of lunar rock samples obtained during the various Apollo missions to the moon show a surprisingly high zirconium oxide content, compared with terrestrial rocks. [Pg.55]

Gr. technetos, artificial) Element 43 was predicted on the basis of the periodic table, and was erroneously reported as having been discovered in 1925, at which time it was named masurium. The element was actually discovered by Perrier and Segre in Italy in 1937. It was found in a sample of molybdenum, which was bombarded by deuterons in the Berkeley cyclotron, and which E. Eawrence sent to these investigators. Technetium was the first element to be produced artificially. Since its discovery, searches for the element in terrestrial material have been made. Finally in 1962, technetium-99 was isolated and identified in African pitchblende (a uranium rich ore) in extremely minute quantities as a spontaneous fission product of uranium-238 by B.T. Kenna and P.K. Kuroda. If it does exist, the concentration must be very small. Technetium has been found in the spectrum of S-, M-, and N-type stars, and its presence in stellar matter is leading to new theories of the production of heavy elements in the stars. [Pg.106]

When considering how the evolution of life could have come about, the seeding of terrestrial life by extraterrestrial bacterial spores traveling through space (panspermia) deserves mention. Much is said about the possibility of some form of life on other planets, including Mars or more distant celestial bodies. Is it possible for some remnants of bacterial life, enclosed in a protective coat of rock dust, to have traveled enormous distances, staying dormant at the extremely low temperature of space and even surviving deadly radiation The spore may be neither alive nor completely dead, and even after billions of years it could have an infinitesimal chance to reach a planet where liquid water could restart its life. Is this science fiction or a real possibility We don t know. Around the turn of the twentieth century Svante Arrhenius (Nobel Prize in chemistry 1903) developed this theory in more detail. There was much recent excitement about claimed fossil bacterial remains in a Martian meteorite recovered from Antarctica (not since... [Pg.16]

It is interesting to note that recent evidence shows that even extra-terrestrially formed hydrocarbons can reach the Earth. The Earth continues to receive some 40,000 tons of interplanetary dust every year. Mass-spectrometric analysis has revealed the presence of hydrocarbons attached to these dust particles, including polycyclic aromatics such as phenanthrene, chrysene, pyrene, benzopyrene, and pentacene of extraterrestrial origin indicated by anomalous isotopic ratios. [Pg.128]

Basically, Newtonian mechanics worked well for problems involving terrestrial and even celestial bodies, providing rational and quantifiable relationships between mass, velocity, acceleration, and force. However, in the realm of optics and electricity, numerous observations seemed to defy Newtonian laws. Phenomena such as diffraction and interference could only be explained if light had both particle and wave properties. Indeed, particles such as electrons and x-rays appeared to have both discrete energy states and momentum, properties similar to those of light. None of the classical, or Newtonian, laws could account for such behavior, and such inadequacies led scientists to search for new concepts in the consideration of the nature of reahty. [Pg.161]

Percentage of meteorites seen to fall. Chondrites. Over 90% of meteorites that are observed to fall out of the sky are classified as chondrites, samples that are distinguished from terrestrial rocks in many ways (3). One of the most fundamental is age. Like most meteorites, chondrites have formation ages close to 4.55 Gyr. Elemental composition is also a property that distinguishes chondrites from all other terrestrial and extraterrestrial samples. Chondrites basically have undifferentiated elemental compositions for most nonvolatile elements and match solar abundances except for moderately volatile elements. The most compositionaHy primitive chondrites are members of the type 1 carbonaceous (Cl) class. The analyses of the small number of existing samples of this rare class most closely match estimates of solar compositions (5) and in fact are primary source solar or cosmic abundances data for the elements that cannot be accurately determined by analysis of lines in the solar spectmm (Table 2). Table 2. Solar System Abundances of the Elements ... [Pg.96]

Extraterrestrial dust particles can be proven to be nonterrestrial by a variety of methods, depending on the particle si2e. Unmelted particles have high helium. He, contents resulting from solar wind implantation. In 10-)J.m particles the concentration approaches l/(cm g) at STP and the He He ratio is close to the solar value. Unmelted particles also often contain preserved tracks of solar cosmic rays that are seen in the electron microscope as randomly oriented linear dislocations in crystals. Eor larger particles other cosmic ray irradiation products such as Mn, Al, and Be can be detected. Most IDPs can be confidently distinguished from terrestrial materials by composition. Typical particles have elemental compositions that match solar abundances for most elements. TypicaUy these have chondritic compositions, and in descending order of abundance are composed of O, Mg, Si, Ee, C, S, Al, Ca, Ni, Na, Cr, Mn, and Ti. [Pg.100]

The earth s cmst consists of 0.09% fluoiine. Among the elements fluorine ranks about thirteenth ia terrestrial abundance. [Pg.137]

As of this writing, the primary focus of research and development in PEFC technology is a fuel-ceU system for terrestrial transportation appHcations... [Pg.578]

The intensity of bioluminescence emission is > 2 x 10 photon /s-cm in the dinoflageUate Gonyaulax and the spectmm of light emission ranges from 450—490 nm (blue) in deep sea species, 490—520 nm (green) in coastal water species, and 510—580 nm (yeUow-green) in terrestrial and freshwater species. [Pg.271]

Exposure. The exposure of humans and animals to mercury from the general environment occurs mainly by inhalation and ingestion of terrestrial and aquatic food chain items. Pish generally rank the highest (10—300 ng/g) in food chain concentrations of mercury. Swordfish and pike may frequently exceed 1 p.g/g (27). Most of the mercury in fish is methyl mercury [593-74-8]. Worldwide, the estimated average intake of total dietary mercury is 5—10 p-g/d in Europe, Russia, and Canada, 20 pg/d in the United States, and 40—80 pg/d in Japan (27). [Pg.108]

There is a general relationship between metal price and terrestrial concentration. Metals present at relatively high concentrations, in the earth s cmst, such as iron and aluminum, are the least expensive rare metals such as gold and platinum are the most valuable. This situation has existed for gold and silver valuation for centuries. The amount of silver in the earth s cmst is approximately 20 times that of gold, and the historical price ratio for gold and silver varied between 10 and 16 for over 3000 years. Since 1970 that price ratio has been strongly affected by market forces and investor speculation. [Pg.159]


See other pages where Terrestrial is mentioned: [Pg.2794]    [Pg.277]    [Pg.278]    [Pg.17]    [Pg.34]    [Pg.379]    [Pg.969]    [Pg.25]    [Pg.26]    [Pg.37]    [Pg.38]    [Pg.213]    [Pg.96]    [Pg.98]    [Pg.98]    [Pg.100]    [Pg.259]    [Pg.577]    [Pg.581]    [Pg.582]    [Pg.9]    [Pg.10]    [Pg.35]    [Pg.273]    [Pg.4]    [Pg.56]    [Pg.271]    [Pg.272]    [Pg.273]    [Pg.104]    [Pg.82]    [Pg.82]    [Pg.93]   
See also in sourсe #XX -- [ Pg.26 , Pg.28 , Pg.40 , Pg.48 , Pg.49 , Pg.53 , Pg.54 , Pg.67 , Pg.68 , Pg.74 , Pg.95 , Pg.108 , Pg.109 , Pg.244 ]

See also in sourсe #XX -- [ Pg.490 ]

See also in sourсe #XX -- [ Pg.4 , Pg.5 , Pg.12 , Pg.13 , Pg.55 , Pg.59 , Pg.65 , Pg.71 , Pg.74 , Pg.77 , Pg.82 , Pg.85 , Pg.114 , Pg.116 , Pg.118 , Pg.119 , Pg.121 , Pg.126 , Pg.128 , Pg.130 , Pg.136 , Pg.143 , Pg.169 , Pg.174 ]




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Abundances terrestrial

Acrolein terrestrial plants

Air-Terrestrial Surface Exchange

Alkaloids, terrestrial

Aquatic-terrestrial linkages, water

Arvicola terrestris

Atmosphere composition of the terrestrial

Atmosphere primitive terrestrial

Atrazine terrestrial

Atrazine terrestrial plants

Bacteria, terrestrial

Baseline Terrestrial Experiments

Bioaccumulation in Terrestrial Systems

Biogeochemical Cycling of Macroelements in Terrestrial Aquatic Ecosystems

Biomass growth terrestrial

Biomass terrestrial production

Biota terrestrial

Biotransformation terrestrial mammals

Bombus terrestris

Boron terrestrial invertebrates

Boron terrestrial plants

Bufo terrestris

Cadmium terrestrial system

Calcium terrestrial distribution

Calcium terrestrial samples

Carbon Fluxes in Terrestrial Ecosystems

Carbon cycle terrestrial

Carbon dioxide terrestrial

Carbon reservoirs terrestrial biosphere

Carbon terrestrial biota

Carbon terrestrial, distribution

Carbonates, terrestrial distribution

Chemical evolution terrestrial planets

Coelotes terrestris

Comparative terrestrial transport

Comparison of Carbon Biogeochemical Processes in Terrestrial and Aquatic Ecosystems

Core formation terrestrial

Cosmogenic isotopes terrestrial

Cyanide terrestrial plants

Cycling studies terrestrial

Data bases terrestrial

Decomposition terrestrial

Densities terrestrial bodies

Differentiation terrestrial planets

Diflubenzuron terrestrial invertebrates

Distribution in Terrestrial Biota

Ecosystem terrestrial-aquatic model

Effects on Terrestrial Plants

Elements abundance, terrestrial

Elements from terrestrial

Evolution of the terrestrial planets

Example of the lake history approach to terrestrial P cycling

Excretion by terrestrial animals

Expansion of the Shikimate Pathway in Terrestrial Plants

Extra-Terrestrial Phosphorus and Reduced Forms

Extra-terrestrial Processing

Extra-terrestrial radiation

Extra-terrestrial samples

Fate of Drugs in Terrestrial Species

Feldspar terrestrial weathering

Fenvalerate terrestrial invertebrates

Fenvalerate terrestrial plants

Flood plains terrestrial

Food chains terrestrial

Formation of the terrestrial planets

Freshwater Terrestrial Ecosystems

From terrestrial

Fungi terrestrial

Hafnium-tungsten chronometry terrestrial core formation

Halogen-containing antibiotics in terrestrial organisms

Hederae terrestris herba

Higher plants terrestrial

Hostile terrestrial environments

Humic Substances terrestrial

Humic acids soil/terrestrial

Humic acids terrestrial

Humic material/substances soil/terrestrial

In terrestrial food chain

Indicators terrestrial

Interactions of Biogeochemical Cycles in Terrestrial Ecosystems

Introduction comparison of aquatic and terrestrial canopies

Invertebrates in terrestrial decomposition

Invertebrates terrestrial

Invertebrates, terrestrial arsenic

Invertebrates, terrestrial cadmium

Invertebrates, terrestrial chromium

Invertebrates, terrestrial copper

Invertebrates, terrestrial nickel

Invertebrates, terrestrial paraquat

Invertebrates, terrestrial radiation

Isotopes, stable terrestrial abundances

Known Polyacetylenic Compounds from Terrestrial Plants

Lichens, terrestrial

Lumbricus terrestris

Magma ocean terrestrial

Marine vs. Terrestrial Organic Matter

Mercury terrestrial component

Microcosms terrestrial

Microorganisms terrestrial

Mineral samples, terrestrial

Minerals terrestrial, from Allende

Minerals terrestrial, isotope

Molybdenum terrestrial plants

Monitoring terrestrial

Neutron activation terrestrial

New Polyacetylenic Compounds from Terrestrial Plants

Nitrogen compounds terrestrial systems

Ocean-atmosphere-terrestrial biosphere

Ocean-atmosphere-terrestrial biosphere systems

Organic matter terrestrial

Organic matter terrestrial weathering

Organic matter terrestrial/terrigenous

Origin of Terrestrial Noble Gas

Paraquat terrestrial plants

Phoma terrestris

Phosphorus cycle terrestrial

Phosphorus dynamics, terrestrial ecosystems

Phosphorus terrestrial

Planets terrestrial

Plants, terrestrial arsenic

Plants, terrestrial chromium

Plants, terrestrial copper

Plants, terrestrial mercury

Plants, terrestrial nickel

Plants, terrestrial pentachlorophenol

Plants, terrestrial polycyclic aromatic hydrocarbons

Plants, terrestrial radiation

Plants, terrestrial selenium

Plants, terrestrial silver

Polychlorinated biphenyls terrestrial

Polyphenolics terrestrial

Primordial terrestrial

Production mechanisms of cosmogenic nuclides in terrestrial rocks

Production/productivity terrestrial

Pyrenochaeta terrestris

Recent Development of ESR Dating in Terrestrial Materials

SNA and Metal Transport in Terrestrial Plants

Salamander terrestrial species

Shales terrestrial weathering

Shell terrestrial

Silicon bond terrestrial

Soil organisms, terrestrial decomposition

Soil-Biogeochemical Conditions in the Worlds Terrestrial Ecosystems

Soils - a unique environment for iron oxide formation in terrestrial ecosystems

Solar System terrestrial planet region

Solar and Terrestrial Radiation

Solar radiation and terrestrial environment

Solid CH4 on Triton and Terrestrial Methane Hydrate

Starting Point for the Development of a Terrestrial or Groundwater Standard

Stoichiometric Aspects of Nutrient Recycling in Terrestrial Ecosystems

Stoichiometry of Terrestrial Plants and Its Implications According to SNA

Terrestrial Ecosystem Model

Terrestrial Flora and Invertebrates

Terrestrial Laser Scanner

Terrestrial Mammals

Terrestrial Mammals and Humans

Terrestrial Mars analogues

Terrestrial Noble Gases

Terrestrial Plants and Invertebrates

Terrestrial Polyacetylenes and Derived Thiophenes

Terrestrial Toxicity

Terrestrial Vertebrate Toxicity Tests

Terrestrial abiotic elements

Terrestrial abundance and distribution

Terrestrial ages

Terrestrial alkaloids, halogenated

Terrestrial and Aquatic Plants

Terrestrial animals

Terrestrial animals bioaccumulation

Terrestrial animals environmental fate

Terrestrial areas

Terrestrial areas land surface

Terrestrial areas sediments soils

Terrestrial biogenic sulfur emissions

Terrestrial biomarkers

Terrestrial biomass

Terrestrial biosphere

Terrestrial biosphere, carbon dioxide

Terrestrial biosphere, carbon dioxide cycle

Terrestrial biosynthesis processes

Terrestrial carbon dioxide levels

Terrestrial carbon values

Terrestrial chemistry

Terrestrial compartment

Terrestrial component

Terrestrial conditions

Terrestrial crops

Terrestrial cyanobacteria

Terrestrial detritus

Terrestrial distribution

Terrestrial ecosystem nitrogen deposition

Terrestrial ecosystem sulfur cycling

Terrestrial ecosystems

Terrestrial ecosystems, diversity

Terrestrial ecotoxicity potential

Terrestrial ecotoxicology, guidance document

Terrestrial environments

Terrestrial environments export

Terrestrial enzymes

Terrestrial food chains biomagnification

Terrestrial foodwebs

Terrestrial fractionation line

Terrestrial fulvic acids

Terrestrial geophysics

Terrestrial global carbon sink

Terrestrial habitats

Terrestrial haloperoxidase

Terrestrial humics

Terrestrial invertebrate tests

Terrestrial invertebrates, metal

Terrestrial iron

Terrestrial leads compared with

Terrestrial material from

Terrestrial materials

Terrestrial microorganisms conditions

Terrestrial minerals

Terrestrial model

Terrestrial monomers

Terrestrial nitrogen loading

Terrestrial ocean atmosphere ecosystem model

Terrestrial organic carbon

Terrestrial organic realm

Terrestrial organics/marine shell

Terrestrial organisms

Terrestrial plagioclase

Terrestrial planet region, Solar

Terrestrial planets accretion

Terrestrial planets accretion models

Terrestrial planets compositions

Terrestrial planets evolution

Terrestrial planets physical properties

Terrestrial planets planetary embryos

Terrestrial planets volatile element depletion

Terrestrial plant tests

Terrestrial plants

Terrestrial plants, hydrocarbons

Terrestrial radiation

Terrestrial radiation cooling

Terrestrial realm

Terrestrial reservoirs

Terrestrial responses

Terrestrial samples

Terrestrial samples elements

Terrestrial samples first searches

Terrestrial sediments, carbon isotope

Terrestrial situations

Terrestrial solar

Terrestrial solar modules

Terrestrial species

Terrestrial substrates

Terrestrial surface

Terrestrial system results

Terrestrial transport from

Terrestrial turtles

Terrestrial vegetation

Terrestrial vegetation climatic change, effect

Terrestrial vegetation contaminants

Terrestrial vertebrates

Terrestrial waters

Terrestrial wildlife, toxicological

Terrestrial-based telescopes

The Early Sun and Evolution of Terrestrial Planets

The Terrestrial Biosphere

The Utilization of Terrestrial Biomass

The geological and extra-terrestrial distribution of amino acids

The terrestrial environment, crust and material cycling

The terrestrial planets

Thielavia terrestris

Three Isotope Plots of Terrestrial and Extraterrestrial Samples

Triad in terrestrial ecosystems and selection of biological tests

Tribulus terrestris

Tribulus terrestris tribulusamide A from

Tribulus terrestris tribulusamide B from

Utilization terrestrial biomass

Voles Arvicola terrestris

Water, acid terrestrial

Weathering terrestrial

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