Estimation of anisoplanatism in adaptive optics by generalized SCIDAR profiling     

R. W. Wilson  N. J. Wooder  F. Rigal  J. C. Dainty 《Monthly notices of the Royal Astronomical Society》2003,339(2):491-494

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Detection of carbon monoxide within the Magellanic Bridge     

E. Muller  L. Staveley-Smith  W. J. Zealey 《Monthly notices of the Royal Astronomical Society》2003,338(3):609-615

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Late/Middle/Early/Ichnocambrian： a communication-friendly nomenclature for the epochs of a quadripartite Cambrian Period     

Stephen M. Rowland Melissa Hicks 《《幕》》2006,29(2):128-129

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A high-resolution rotation curve of NGC 6822: a test-case for cold dark matter     

D. T. F. Weldrake  W. J. G. de Blok †  F. Walter 《Monthly notices of the Royal Astronomical Society》2003,340(1):12-28

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Explicit solution of the overdetermined three-dimensional resection problem   总被引：1，自引：1，他引：0  

J. L. Awange  E. W. Grafarend 《Journal of Geodesy》2003,76(11-12):605-616

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STORING AND CATALOGUING ARCHITECTURAL PHOTOGRAMMETRY MATERIAL     

R. W. A. Dallas 《The Photogrammetric Record》1989,13(73):133-136

The paper describes the material generated in carrying out architectural photogrammetric surveys. The importance of the archival nature of this material is highlighted and reference is made to the indexing and storing of the records.  相似文献   

Preface: Shunso Ishihara     

Bruce W. Chappell 《Resource Geology》2004,54(3):213-214

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Modeling the distribution of aluminum speciation in acid soil solution equilibria with the mineral phase alunite     

S. Bi  S. An  W. Tang  M. Yang  H. Qian  J. Wang 《Environmental Geology》2001,41(1-2):25-36

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HIGH POSSIL AND STRATHMORE—A STUDY OF TWO L6 CHONDRITES     

A.W.R. Bevan  R. Hutchison  A.J. Easton  G.P. Durant  C.M. Farrow 《Meteoritics & planetary science》1985,20(3):491-501

High Possil and Strathmore are the first (1804) and last (1917) meteorite falls, respectively, of the three recorded in Scotland. Olivine compositions and total Fe contents in High Possil (Fa_25.2; 21.35 wt %) and Strathmore (Fa_25.3; 20.6 wt %) confirm their classification as L-group chondrites (Mason, 1963), and the presence of abundant plagioclase feldspar shows that both chondrites belong to petrologic type 6. Both chondrites display thermal and mechanical alteration attributable to moderate shock-loading appropriate to facies c (High Possil) and c-d (Strathmore) (Dodd and Jarosewich, 1979). Incipient shock-melting of metal and troilite in both chondrites is the first described from Lc chondrites, and differences in the responses of metallic and silicate minerals to shock-loading are discussed.  相似文献   

The surface properties of small asteroids: Peculiar Betulia—A case study     

Alan W. Harris  Michael Mueller  Schelte J. Bus 《Icarus》2005,179(1):95-108

We present the results of extensive thermal-infrared observations of the C-type near-Earth Asteroid (1580) Betulia obtained in June 2002 with the 3-m NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawaii. Betulia is a highly unusual object for which earlier radiometric observations, interpreted on the basis of simple thermal models, indicated a surface of high thermal inertia. A high thermal inertia implies a lack of thermally insulating regolith. Radiometric observations of other asteroids of comparable size indicate that regolith is present in nearly all cases. Knowledge of the surface thermal properties of small near-Earth asteroids is crucial for meaningful calculations of the Yarkovsky effect, which is invoked to explain the delivery of collisional fragments from the main belt into near-Earth orbits, and apparently has a significant influence on the orbital evolution of potentially hazardous near-Earth asteroids. Furthermore, apart from being an indicator of the presence of thermally insulating regolith on the surface of an asteroid, the thermal inertia determines the magnitude of the diurnal temperature variation and is therefore of great importance in the design of instrumentation for lander missions to small asteroids. In the case of Betulia our database is sufficiently broad to allow the use of more sophisticated thermal models than were available for earlier radiometric observations. The measured fluxes have been fitted with thermal-model emission continua to determine the asteroid's size and geometric albedo, pv. Fits obtained with a new thermophysical model imply an effective diameter of 4.57±0.46 km and an albedo of 0.077±0.015 and indicate a moderate surface thermal inertia of around 180 J m⁻² s^−0.5 K⁻¹. It is difficult to reconcile our results with earlier work, which indicate a larger diameter for Betulia and a high-thermal-inertia surface of bare rock.  相似文献