Fast Nearest Neighbor Classification Methods for Multispectral Imagery     

Perry J. Hardin  Curtis N. Thomson 《The Professional geographer》1992,44(2):191-202

Nearest neighbor classifiers have not been widely used by remote sensing practitioners. The lack of acceptance of these classifiers may be partially due to their notoriously slow speed of execution which makes them impractical for the classification of mega-pixel images. However, training data reduction, distance measure optimization, and neighbor searching algorithms based on the modified k-d tree can speed nearest neighbor classification substantially.  相似文献   

Röntgenographische Gefügeanalyse mit dem Texturgoniometer am Beispiel von Quarziten aus kaledonischen Überschiebungszonen     

Dr. Kurt v. Gehlen  Dr. Gerhard Voll 《International Journal of Earth Sciences》1962,51(2):440-450

Zusammenfassung Quantitative Gefügediagramme können röntgenographisch mit einem Zählrohr-Textur-Goniometer gemessen werden. Diese Methode kommt besonders in Frage bei sehr feinkörnigen Gesteinen oder aber dann, wenn etwa bei einachsigen Mineralen auch die Regelung anderer Gitterrichtungen außer der c-Achsen-Richtung interessiert. Das beim Quarz anzuwendende Verfahren wird behandelt und gezeigt, wie man hier im Einzelfall Prismenregelungen nachweisen kann. Als praktische Beispiele werden Quarzitgefüge mit Prismenregelung aus kaledonischen Überschiebungszonen Schottlands und Norwegens abgebildet und ihre Entstehung diskutiert. Die Messungen scheinen darauf hinzuweisen, daß beim Quarz bevorzugt Translation mit (11¯20) als Gleitfläche und c als Gleitgerade maßgebend war.  相似文献   

Die Kernfragen der Sonnenstrahlung in gedrängter Darstellung     

Kurt Wegener 《Pure and Applied Geophysics》1959,43(1):278-284

Summary The development of the law of radiation, and his consequences, shortly exposed.

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Résumé La loi de la radiation, developpement et consequences.

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Die röntgenographische und optische Gefügeanalyse von Erzen,insbesondere mit dem Zählrohr-Texturgoniometer     

Dr. Kurt v. Gehlen 《Contributions to Mineralogy and Petrology》1960,7(5):340-388

Quantitative determinations of preferred orientation of opaque minerals have been made only in a few cases by measuring cleavage faces (galena,D. Schachner-Korn). In this paper several methods are investigated critically which are likely to allow the determination of pole figures of ore minerals in a reasonable time. In the first part the special difficulties are discussed which occur in measurements of preferred orientation with X-ray pole figure goniometers (reflection method byL. G. Schulz) when the specimen consists of more than one mineral, when the mineral investigated is coarse-grained, and when the specimen is small. A critical discussion of instrumental errors is included. This method can now also be applied to the determination of preferred orientation in rocks, ceramic materials, etc. In the second part optical methods are given which include the construction of pole figures from measurements of bireflection and polarization figures of uniaxial minerals in reflected light. Examples of pole figures of pyrrhotite, hematite, pyrite, sphalerite, and chromite are given.

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Der Naturwissenschaftlichen Fakultät der Friedrich-Alexander-Universität Erlangen als Habilitationsschrift vorgelegt.  相似文献   

Computation of 5-day temperature normals in western Europe and the Mediterranean area     

Kurt Bender  Ulrich Chorus  Raymond Nybro  Robert Sanderson  Ingrid Weiss 《Pure and Applied Geophysics》1957,38(1):265-285

Summary UsingCraddock's method of representing the annual temperature variation by a two-term harmonic form fitted to monthly means, the harmonic coefficients of 63 stations in western Europe and around the Mediterranean Sea, as well as the 5-day normals for 24 Mediterranean stations, were computed and tabulated. In addition, some of the harmonic coefficients were charted and isoplethed, showing very distinctly the influence of continentality and topography. These charts, together withCraddock's charts for northern and northwestern Europe, provide fairly complete coverage of Europe and the Mediterranean area.This paper was prepared in the offices of the Technical Support Division of the 2d Weather Wing, United States Air Force, as a matter of routine business. The information contained herein was presented at the 5th Meeting of the Italian Society of Geophysics and Meteorology by Dr.Ingrid Weiss (Genoa: 23–25 April 1957). Since the paper is of general interest to all meteorologists of the Mediterranean area, it is published here with the permission of the originating agency as «Mémoire No. 3 du Centre International de Recherches sur la Météorologie de la Méditerranée (CIRMM)».  相似文献   

Vergleichende Messungen der SO2-Immissions-Konzentration mit den Meßgeräten Picoflux und SO2-Monitor     

Ing. Kurt Chalupa 《Theoretical and Applied Climatology》1971,19(2):225-230

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Solar radiation extinction,sky radiation,sky light polarization and aerosol particle total number and size distribution on the Island Maui (Hawaii)     

Kurt Bullrich  Reiner Eiden  Ruprecht Jaenicke  Wolfram Nowak 《Pure and Applied Geophysics》1968,69(1):280-319

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Improved three-dimensional mapping of the electron density distribution of the solar corona     

R. Michael Perry  Martin D. Altschuler 《Solar physics》1973,28(2):435-456

Three-dimensional maps of the distribution of coronal electron density can now be computed with two radial functions in the series expansion for the density (rather than with only one radial function as shown in our previous paper). With the improved maps we can determine the topological variation of the electron density with radial distance, and thus can (1) distinguish coronal condensations from coronal streamers, (2) trace the structure of a streamer as a function of height, and (3) determine the non-radial orientation of a streamer. We summarize the previous work in concise mathematical notation, show examples of the improved maps derived from two radial functions, and discuss in detail the expectations and limitations of the method. Of great utility are computer-simulated pictures showing the solar corona as it would appear if veiwed from above the north (or south) pole.The National Center for Atmospheric Research is sponsored by the National Science Foundation.  相似文献   

MAPPING FROM AN AUTOMATED DISPLAY SYSTEM*     

Kurt E. Brassel  Jack J. Utano 《The Professional geographer》1979,31(2):191-200

This paper outlines recent developments in computer mapping and points out its importance for visualizing contents of geographic information systems. The authors present an integrated system of mapping packages and spatial-data files. Map examoles generated with this system are used to illustrate characteristics of various computer-mapping methods. The diversity of displays created from a single set of data demonstrates that mapping from automated display systems requires the user to take some decisions which have to be based on an understanding of the phenomena displayed, of cartographic communication, and of technical aspects of automated map processing.  相似文献   

Altitude profile of H in the atmosphere of Venus from Lyman α observations of Venera 11 and Venera 12 and origin of the hot exospheric component     

J.L. Bertaux  V.M. Lepine  V.G. Kurt  A.S. Smirnov 《Icarus》1982,52(2):221-244

Two extreme ultraviolet (EUV) spectrophotometers flown in December 1978 on Venera 11 and Venera 12 measured the hydrogen Lyman α emission resonantly scattered in the atmosphere of Venus. Measurements were obtained across the dayside of the disk, and in the exosphere up to 50,000 km. They were analyzed with spherically symmetric models for which the radiative transfer equation was solved. The H content of the Venus atmosphere varies from optically thin to moderately thick regions. A shape fit at the bright limb allows one to determine the exospheric temperature T_c and the number density n_c independently of the calibration of the instrument or the exact value of the solar flux. The dayside exospheric temperature was measured for the first time in the polar regions, with T_c = 300 ± 25°K for Venera 11 (79°S) and T_c = 275 ± 25°K (59°S) for Venera 12. At the same place, the density is n_c = 4_?2⁺³ × 10⁴ atom.cm^?3, and the integrated number density N_t from 250 to 110 km (the level of CO₂ absorption) is 2.1 × 10¹² atom.cm^?2, a factor of 3 to 6 lower than that predicted in aeronomical models. This probably indicates that the models should be revised in the content of H-bearing molecules and should include the effect of dynamics. Across the disk the value of N_t decreases smoothly with a total variation of two from the morning side to the afternoon side. Alternately it could be a latitude effect, with less hydrogen in the polar regions. The nonthermal component if clearly seen up to 40,000 km of altitude. It is twice as abundant as at the time of Mariner 10 (solar minimum). Its radial distribution above 4000 km can be simulated by an exospheric distribution with T = 10³⁰K and n = 10³ atom.cm^?3 at the exobase level. However, there are less hot atoms between 2000 and 4000 km than predicted by an ionospheric source. A by-product of the analysis is a determination of a very high solar Lyman α flux of 7.6 × 10¹¹ photons (cm² sec Å)^?1 at line center (1 AU) in December 1978.  相似文献