7,214 research outputs found
Mining in Alaska - environmental impact and pollution control
Environmental factors affecting mining are difficult to establish in Alaska due to the absence of large scale hard rock mining activities at the present time. Currently, experience is gathered from (and to a large degree based on) construction of above ground facilities such as roads, pipelines, and buildings. Past mining activities appear to have had little lasting effect on the natural environment, the exceptions being mine tailings and surface structures. This report, sponsored by the U. S. Bureau of Mines, present general engineering activities, considers the interaction of permafrost and underground mining, summarizes available literature and indicates possible environmental problems that might be encountered in Alaska based on Scandinavian experiences in large-scale northern mining operations. How the Scandinavians are solving their problems is also discussed.This paper was sponsored by the U. S. Bureau of Mines, Contract No. 0133059.Abstract -- Acknowledgements -- Table of contents -- List of illustrations -- List of tables -- Introduction -- Climatic parameters -- Alaska climatic regions -- Construction and mining activities in the Arctic -- General -- Cold weather construction practices -- Permafrost and underground mining operations -- Environmental considerations -- Mining and exploration parameters -- Conclusions -- Recommendations -- Bibliography -- Appendices -- Appendix A: Bibliography - Lost River area -- Appendix B: Mining and environmental considerations as practiced in Norway and Sweden -- Appendix C: Mining vs. the environment -- Figure 1. Alaska climatic regions -- Figure 2. Index map showing mining districts examined -- List of tables -- Table 1. Dates of break-up and freeze-up
Inverse Statistics in the Foreign Exchange Market
We investigate intra-day foreign exchange (FX) time series using the inverse
statistic analysis developed in [1,2]. Specifically, we study the time-averaged
distributions of waiting times needed to obtain a certain increase (decrease)
in the price of an investment. The analysis is performed for the Deutsch
mark (DM) against the US. With high statistical
significance, the presence of "resonance peaks" in the waiting time
distributions is established. Such peaks are a consequence of the trading
habits of the markets participants as they are not present in the corresponding
tick (business) waiting time distributions. Furthermore, a new {\em stylized
fact}, is observed for the waiting time distribution in the form of a power law
Pdf. This result is achieved by rescaling of the physical waiting time by the
corresponding tick time thereby partially removing scale dependent features of
the market activity.Comment: 8 pages. Accepted Physica
Optimal Investment Horizons for Stocks and Markets
The inverse statistics is the distribution of waiting times needed to achieve
a predefined level of return obtained from (detrended) historic asset prices
\cite{optihori,gainloss}. Such a distribution typically goes through a maximum
at a time coined the {\em optimal investment horizon}, , which
defines the most likely waiting time for obtaining a given return . By
considering equal positive and negative levels of return, we reported in
\cite{gainloss} on a quantitative gain/loss asymmetry most pronounced for short
horizons. In the present paper, the inverse statistics for 2/3 of the
individual stocks presently in the DJIA is investigated. We show that this
gain/loss asymmetry established for the DJIA surprisingly is {\em not} present
in the time series of the individual stocks nor their average. This observation
points towards some kind of collective movement of the stocks of the index
(synchronization).Comment: Subm. to Physica A as Conference Proceedings of Econophysics
Colloquium, ANU Canberra, 13-17 Nov. 2005. 6 pages including figure
Diversity of flux avalanche patterns in superconducting films
The variety of morphologies in flux patterns created by thermomagnetic
dendritic avalanches in type-II superconducting films is investigated using
numerical simulations. The avalanches are triggered by introducing a hot spot
at the edge of a strip-shaped sample, which is initially prepared in a
partially penetrated Bean critical state by slowly ramping the transversely
applied magnetic field. The simulation scheme is based on a model accounting
for the nonlinear and nonlocal electrodynamics of superconductors in the
transverse geometry. By systematically varying the parameters representing the
Joule heating, heat conduction in the film, and heat transfer to the substrate,
a wide variety of avalanche patterns is formed, and quantitative
characterization of areal extension, branch width etc. is made. The results
show that branching is suppressed by the lateral heat diffusion, while large
Joule heating gives many branches, and heat removal into the substrate limits
the areal size. The morphology shows significant dependence also on the initial
flux penetration depth.Comment: 6 pages, 6 figure
Avalanche-driven fractal flux distributions in NbN superconducting films
Flux distributions in thin superconducting NbN films placed in a
perpendicular magnetic field have been studied using magneto-optical imaging.
Below 5.5 K the flux penetrates in the form of abrupt avalanches resulting in
dendritic structures. Magnetization curves in this regime exhibit extremely
noisy behavior. Stability is restored both above a threshold temperature T* and
applied field H*, where H* is smaller for increasing field than during descent.
The dendrite size and morphology are strongly T dependent, and fractal analysis
of the first dendrites entering into a virgin film shows that dendrites formed
at higher T have larger fractal dimension.Comment: 3 pages, 5 figure
Ray optics in flux avalanche propagation in superconducting films
Experimental evidence of wave properties of dendritic flux avalanches in
superconducting films is reported. Using magneto-optical imaging the
propagation of dendrites across boundaries between a bare NbN film and areas
coated by a Cu-layer was visualized, and it was found that the propagation is
refracted in full quantitative agreement with Snell's law. For the studied film
of 170 nm thickness and a 0.9 mkm thick metal layer, the refractive index was
close to n=1.4. The origin of the refraction is believed to be caused by the
dendrites propagating as an electromagnetic shock wave, similar to damped modes
considered previously for normal metals. The analogy is justified by the large
dissipation during the avalanches raising the local temperature significantly.
Additional time-resolved measurements of voltage pulses generated by segments
of the dendrites traversing an electrode confirm the consistency of the adapted
physical picture.Comment: 4 pages, 4 figure
Inverse Statistics for Stocks and Markets
In recent publications, the authors have considered inverse statistics of the
Dow Jones Industrial Averaged (DJIA) [1-3]. Specifically, we argued that the
natural candidate for such statistics is the investment horizons distribution.
This is the distribution of waiting times needed to achieve a predefined level
of return obtained from detrended historic asset prices. Such a distribution
typically goes through a maximum at a time coined the {\em optimal investment
horizon}, , which defines the most likely waiting time for
obtaining a given return . By considering equal positive and negative
levels of return, we reported in [2,3] on a quantitative gain/loss asymmetry
most pronounced for short horizons. In the present paper, this gain/loss
asymmetry is re-visited for 2/3 of the individual stocks presently in the DJIA.
We show that this gain/loss asymmetry established for the DJIA surprisingly is
{\em not} present in the time series of the individual stocks. The most
reasonable explanation for this fact is that the gain/loss asymmetry observed
in the DJIA as well as in the SP500 and Nasdaq are due to movements in the
market as a whole, {\it i.e.}, cooperative cascade processes (or
``synchronization'') which disappear in the inverse statistics of the
individual stocks.Comment: Revtex 13 pages, including 15 figure
Dendritic flux avalanches in rectangular superconducting films -- numerical simulations
Dendritic flux avalanches is a frequently encountered instability in the
vortex matter of type II superconducting films at low temperatures. Previously,
linear stability analysis has shown that such avalanches should be nucleated
where the flux penetration is deepest. To check this prediction we do numerical
simulations on a superconducting rectangle. We find that at low substrate
temperature the first avalanches appear exactly in the middle of the long
edges, in agreement with the predictions. At higher substrate temperature,
where there are no clear predictions from the theory, we find that the location
of the first avalanche is decided by fluctuations due to the randomly
distributed disorder.Comment: 3 pages, 2 figure
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