Tourism and landscape in South Tyrol     

Werner Kreisel  Tobias Reeh 《Central European Journal of Geosciences》2011,3(4):410-423

An increasing number of the people responsible for promoting tourism understand the necessity of landscape conservation and sustainable development. Sustainability and the maintenance of regional identity depend on the kind of tourism that takes account of the landscape and stops short of a blind modification of it, for instance through the installation of inappropriate large-scale tourist infrastructure. Since the 1970s South Tyrol, Italy’s most northern province (Autonome Provinz Bozen/Südtirol; Provincia Autonoma di Bolzano/Alto Adige), has engaged in tourism of outstanding quality, centreed on the existing landscape potential. Until today this has been the basis for successful tourism development. In the meantime however, there have been calls in South Tyrol for a quantitative expansion, founded on the implementation of an artificial touristic infrastructure and products. As is the case in many other alpine regions, this could be detrimental to the quality of the landscape. Supported by tourism research and based on the authors’ own long-standing experience, this article analyzes the development and trends of tourism in South Tyrol from a geographical perspective and takes a critical look at the various planning prospects and the problems which might evolve for the landscape and for tourism marketing.  相似文献   

Glacier fluctuations between 1975 and 2008 in the Greater Himalaya Range of Zanskar, southern Ladakh     

Ulrich KAMP  Martin BYRNE  Tobias BOLCH 《山地科学学报》2011,8(3):374-389

Glaciers in the Himalaya are often heavily covered with supraglacial debris,making them difficult to study with remotely-sensed imagery alone.Various methods such as band ratios can be used effectively to map clean-ice glaciers;however,a thicker layer of debris often makes it impossible to distinguish between supraglacial debris and the surrounding terrain.Previously,a morphometric mapping approach employing an ASTER-derived digital elevation model has been used to map glaciers in the Khumbu Himal and the Tien Shan.This study on glaciers in the Greater Himalaya Range in Zanskar,southern Ladakh,aims (i) to use the morphometric approach to map large debris-covered glaciers;and (ii) to use Landsat and ASTER data and GPS and field measurements to document glacier change over the past four decades.Field work was carried out in the summers of 2008.For clean ice,band ratios from the ASTER dataset were used to distinguish glacial features.For debris-covered glaciers,topographic features such as slope were combined with thermal imagery and supervised classifiers to map glacial margins.The method is promising for large glaciers,although problems occurred in the distal and lateral parts and in the fore field of the glaciers.A multi-temporal analysis of glaciers in Zanskar showed that in general they have receded since at least the mid-to late-1970s.However,some few glaciers that advanced or oscillated - probably because of specific local environmental conditions - do exist.  相似文献   

A spectroscopic study of the surfaces of Saturn's large satellites: H₂O ice, tholins, and minor constituents     

Dale P. Cruikshank  Tobias C. Owen  Thomas R. Geballe  Catherine de Bergh  Francois Poulet  Joshua P. Emery 《Icarus》2005,175(1):268-283

We present spectra of Saturn's icy satellites Mimas, Enceladus, Tethys, Dione, Rhea, and Hyperion, 1.0-2.5 μm, with data extending to shorter (Mimas and Enceladus) and longer (Rhea and Dione) wavelengths for certain objects. The spectral resolution (R=λ/Δλ) of the data shown here is in the range 800-1000, depending on the specific instrument and configuration used; this is higher than the resolution (R=225 at 3 μm) afforded by the Visual-Infrared Mapping Spectrometer on the Cassini spacecraft. All of the spectra are dominated by water ice absorption bands and no other features are clearly identified. Spectra of all of these satellites show the characteristic signature of hexagonal H₂O ice at 1.65 μm. We model the leading hemisphere of Rhea in the wavelength range 0.3-3.6 μm with the Hapke and the Shkuratov radiative transfer codes and discuss the relative merits of the two approaches to fitting the spectrum. In calculations with both codes, the only components used are H₂O ice, which is the dominant constituent, and a small amount of tholin (Ice Tholin II). Tholin in small quantities (few percent, depending on the mixing mechanism) appears to be an essential component to give the basic red color of the satellite in the region 0.3-1.0 μm. The quantity and mode of mixing of tholin that can produce the intense coloration of Rhea and other icy satellites has bearing on its likely presence in many other icy bodies of the outer Solar System, both of high and low geometric albedos. Using the modeling codes, we also establish detection limits for the ices of CO₂ (a few weight percent, depending on particle size and mixing), CH₄ (same), and NH₄OH (0.5 weight percent) in our globally averaged spectra of Rhea's leading hemisphere. New laboratory spectral data for NH₄OH are presented for the purpose of detection on icy bodies. These limits for CO₂, CH₄, and NH₄OH on Rhea are also applicable to the other icy satellites for which spectra are presented here. The reflectance spectrum of Hyperion shows evidence for a broad, unidentified absorption band centered at 1.75 μm.  相似文献   

Compositional constraints on giant planet formation     

Tobias Owen  Therese Encrenaz 《Planetary and Space Science》2006,54(12):1188-1196

Using Ockham's razor as a guide, we have tried to find the simplest model for the formation of giant planets that can explain current observations of atmospheric composition. While this “top-down” approach is far from sufficient to define such models, it establishes a set of boundary conditions whose satisfaction is necessary. Using Jupiter as the prototype, we find that a simple model for giant planet formation that begins with a solar nebula of uniform composition and relies on accretion of low temperature icy planetesimals plus collapse of surrounding solar nebula gas supplies that satisfaction. We compare the resulting predictions of elemental abundances and isotope ratios in the atmospheres of the other giants with those from contrasting models and suggest some key measurements to make further progress.  相似文献   

Cooling flows within galactic haloes: the kinematics and properties of infalling multiphase gas   总被引：1，自引：0，他引：1  

Tobias Kaufmann  Lucio Mayer  James Wadsley  Joachim Stadel  Ben Moore 《Monthly notices of the Royal Astronomical Society》2006,370(4):1612-1622

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Iapetus dark and bright material:: giving compositional interpretation some latitude     

Faith Vilas  Kandy S. Jarvis  Susan M. Lederer  Michael S. Kelley  Tobias C. Owen 《Icarus》2004,170(1):125-130

Narrowband reflectance spectra (0.53-1.0 μm) of Iapetus' leading and trailing sides were obtained in 2000 to test the presence of an absorption feature located near 0.67 μm seen in reflectance spectra of Iapetus' dark material and Hyperion's surface material. No feature was observed. The difference in reflectance across the UV/VIS/NIR spectral region, and the dependence of the presence or absence of this absorption feature on angular separation from the apex of Iapetus in its orbit, phase angle, and heliocentric distance (affecting temperature), were examined. A trend of increased reddening, and the presence of the absorption feature, correlate with an angular separation from the apex of ? approximately 10°. Spectral information is lost when the contribution of the bright water ice signal to the reflectance spectrum increases sufficiently. In order to optimize compositional studies of Iapetus, we encourage future ground-based and space-based spectral observations to maximize the concentration of dark material in the instrumental field of view.  相似文献   

Site-descriptive modelling for a final repository for spent nuclear fuel in Sweden   总被引：2，自引：0，他引：2  

Johan Andersson  Kristina Skagius  Anders Winberg  Tobias Lindborg  Anders Ström 《Environmental Earth Sciences》2013,69(3):1045-1060

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Analysis of current trends in climate parameters,river discharge and glaciers in the Aksu River basin (Central Asia)     

Valentina Krysanova  Michel Wortmann  Tobias Bolch  Bruno Merz  Doris Duethmann  Judith Walter 《水文科学杂志》2013,58(4):566-590

Abstract

Climate variability and change play a crucial role in the vulnerable system of the Aksu River basin located in Kyrgyzstan and northwest China, providing precious water resources for the intense oasis agriculture of the Xinjiang Province (China). Ubiquitous warming and increase in precipitation (in the lower part of the basin) have been detected. Glaciers in the region are retreating. Seasonal trends in river discharge show an increase. A clear link could be demonstrated between daily temperature and lagged river discharge at two headwater stations in summer. However, the correlation breaks over short periods in the end of summer or beginning of autumn at the Xiehela station, when the high (over 95th percentile) flow peaks caused by the glacier lake outburst floods of the Merzbacher Lake occur. This feature is a challenge for the climate impact assessment in the region, as these regular outbursts have to be represented in the projections for the future as well.