Exploring Mobility Indoors: an Application of Sensor‐based and GIS Systems     

Anastasia Petrenko  Anton Sizo  Winchel Qian  A. Dylan Knowles  Amin Tavassolian  Kevin Stanley  Scott Bell 《Transactions in GIS》2014,18(3):351-369

The popularization of tracking devices, such as GPS, accelerometers and smartphones, have made it possible to detect, record, and analyze new patterns of human movement and behavior. However, employing GPS alone for indoor localization is not always possible due to the system's inability to determine location inside buildings or in places of signal occlusion. In this context, the application of local wireless networks for determining position is a promising alternative solution, although they still suffer from a number of limitations due to energy and IT‐resources. Our research outlines the potential for employing indoor wireless network positioning and sensor‐based systems to improve the collection of tracking data indoors. By applying various methods of GIScience we developed a methodology that can be applicable for diverse human indoor mobility analysis. To show the advantage of the proposed method, we present the result of an experiment that included mobility analysis of 37 participants. We tracked their movements on a university campus over the course of 41 days and demonstrated that their movement behavior can be successfully studied with our proposed method.  相似文献   

Economic and subsistence values of the standing stocks of seagrass fisheries: Potential benefits of no-fishing marine protected area management     

Richard K.F. Unsworth  Leanne C. Cullen  Jules N. Pretty  David J. Smith  James J. Bell 《Ocean & Coastal Management》2010,53(5-6):218-224

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Design and application of a constant head well permeameter for shallow high saturated hydraulic conductivity soils     

R. W. Bell  N. J. Schofield 《水文研究》1990,4(4):327-342

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Hubble Space Telescope imaging polarimetry of Mars during the 2003 opposition     

Yu. Shkuratov  M. Kreslavsky  V. Kaydash  J. Bell III  M. Hubbard  A. Lubenow 《Icarus》2005,176(1):1-11

We report results of polarimetric imaging observations of Mars with the Hubble Space Telescope during the 2003 opposition. Through careful calibration, the observations with the ACS camera allow measurements of the polarization degree with an absolute accuracy better than 0.5% and detection of features with polarization degree contrast as small as 0.2%. The general distribution of linear polarization parameters over the Mars disk and their dependence on phase angle and wavelength are well explained qualitatively by a combination of scattering separately by the martian surface and atmosphere. We have discovered transient polarization phenomena interpreted as clouds that are best observed in ultraviolet light. These clouds are optically thin but strongly polarizing, and their origin may be related to atmospheric ice condensation processes.  相似文献   

A study of two post-common envelope binary systems     

K. M. Exter †  D. L. Pollacco  P. F. L. Maxted  R. Napiwotzki  S. A. Bell 《Monthly notices of the Royal Astronomical Society》2005,359(1):315-327

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Pseudospectral time-domain modeling of non-Rayleigh reverberation: synthesis and statistical analysis of a sidescan sonar image of sand ripples     

Elston  G.R. Bell  J.M. 《Oceanic Engineering, IEEE Journal of》2004,29(2):317-329

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Effective collision strengths for fine-structure forbidden transitions among the 3s²3p⁴ levels of Cl ii     

N. J.Wilson  K. L.Bell 《Monthly notices of the Royal Astronomical Society》2002,331(2):389-393

The ab initio R -matrix method is used to calculate effective collision strengths for electron-impact excitation of the sulphur-like ion Cl  ii in the close-coupling approximation. All 10 astrophysically important fine-structure forbidden transitions within the 3s²3p⁴     ,     ,     ground configuration levels are considered. The 12 lowest LS target states are included in the calculation. Effective collision strengths are obtained by averaging the electron collision strengths over a Maxwellian distribution of electron velocities. Results are presented for electron temperatures in the range  log  T (K)=3.3  to  log  T (K)=5.5  , appropriate for astrophysical applications. These are the only effective collision strength data that are currently available.  相似文献   

ASOCAM Observations of CYG X-3: Search for a Hot Stellar Wind     

R.N. Ogley  S.J. Bell Burnell  R.P. Fender 《Astrophysics and Space Science》1997,255(1-2):205-210

Six CAM observations have been made in the 4 - 14 μm wavelength region to search for further evidence of emission from a hot stellar wind. Initial results suggest that the spectrum detected by Fender et al. using UKIRT extends into the wavelength region covered by ISOCAM. There is also evidence that the source is variable on timescales of ≈ 70 seconds. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

Nature and completeness of galaxies detected in the Two Micron All Sky Survey     

Daniel H. McIntosh  Eric F. Bell  Martin D. Weinberg  Neal Katz 《Monthly notices of the Royal Astronomical Society》2006,373(4):1321-1338

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Evolution and Morphodynamics of a Prograded Beach‐Ridge Foreland,Northern Baffin Island,Canadian Arctic Archipelago          下载免费PDF全文

Dominique St‐Hilaire‐Gravel  Donald L. Forbes  Trevor Bell 《Geografiska Annaler: Series A, Physical Geography》2015,97(3):615-631

Landward retreat (marine transgression) is a common response of coastal systems to rising relative sea level. However, given sufficient sediment supply, the coast may advance seaward. The latter response of gravel barriers has been recorded in parts of southeastern and northwestern Canada, where seaward‐rising sets of beach ridges are observed in areas of Holocene RSL rise. Cape Charles Yorke, northern Baffin Island, is a 5 km long gravel foreland characterized by seaward‐rising beach‐ridge crest elevations. The prograded morphology of the Cape Charles Yorke foreland is a prime example of coastal response to a combination of rising RSL and abundant sediment supply, an unusual and little‐documented pattern in the Canadian Arctic. The main gravel supply to Cape Charles Yorke is likely from eroding bedrock and raised marine deposits southwest of the foreland. Although not the dominant sediment source, the Cape Charles Yorke delta contributed to the formation of the foreland by sheltering it from easterly storm waves and providing an anchor point for the prograding ridges. The truncation of relict ridges by the modern shoreline suggests a recent regime shift from continuous deposition to predominant erosion. The cause and timing of this shift are unknown but could result from a recent dwindling in sediment supply, increased accommodation space, increased wave energy, and/or an accelerated rise of relative sea level.  相似文献