Howarth Mood-Adjective Checklist--Version 4

Howarth, Edgar; Young, Paul David

doi:10.1037/t09283-000

Cited by 2 publications

(2 citation statements)

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“…The primary focus of this paper is on [2 à3] above Much work has also been done in the interpretation of remote sensing sensing images of urbanization, a focus that may be represented as [1 ‡2] in the context of figure 2. Remote sensing image data have been used to detect land use change in China by Yeh (2001) and by Li and Yeh (1998) applying and extending methods introduced by Howarth (1986) and by Mesev, Longley, Batty, and Xie (1995). The [1 ‡2] designation also includes fuzzy classification techniques as applied to the production of remote sensing images.…”

Section: Dynamic Modelmentioning

confidence: 99%

Fuzzy Urban Sets: Theory and Application to Desakota Regions in China

Heikkila

Yang

2003

Environ Plann B Plann Des

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This paper outlines a method for using the mathematics of fuzzy sets that is well suited to measure and characterize peri-urbanizing ("desakota") systems typical of China, Southeast Asia, and other areas experiencing rapid urbanization. Drawing on Kosko's "fuzzy hypercube", three distinct but interdependent measures are derived: (i) extent of urbanization, (ii) level of fuzziness, and (iii) degree of entropy. The feasibility of the proposed method is demonstrated using remote sensing data for Ningbo, China. * The research presented here was undertaken in part while Eric Heikkila was a Visiting Fullbright Scholar at Peking University, and support from the Council for International Exchange of Scholars is gratefully acknowledged. We are also grateful for supplementary funding from USC's Center for International Studies and the USC Lusk Center for Real Estate to support additional collaboration on this research vital to finalizing this draft.

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Section: Dynamic Modelmentioning

confidence: 99%

Fuzzy Urban Sets: Theory and Application to Desakota Regions in China

Heikkila

Yang

2003

Environ Plann B Plann Des

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“…Such a procedure however does not guarantee a correct estimate of the chromospheric flux, since Linsky and Ayres (1978) have shown that in a model atmosphere with no chromosphere, the radiative equilibrium profile is substantially different from the one obtained doing a simple gaussian interpolation of the absorption line wings. The Howarth and Phillips 1986). Determining the continuum can be a rather difficult task, especially in later spectral types with weak Ha, due to the presence of absorption and emission features in the Ha region which deform the shape of the surrounding continuum.…”

Section: Line Fluxes -Equivalent Widthsmentioning

confidence: 99%

Magnetic activity phenomena in dwarf m and k stars

Μαθιουδάκης¹

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During the preparation of this thesis I received a great deal of support from many sources. It is impossible to mention everyone by name, but I wish to mention some of the people who helped to make this thesis possible. Primarily I would like to thank the Department of Education for Northern Ireland for generous financial support through the scholarship awarded to me by the Management Committee of Armagh Observatory. I express my gratitude to my thesis supervisor Dr. Gerry Doyle for suggesting the subject, his constant direction and friendship. Thanks to my University supervisor Prof. Arthur Kingston for his continual support on this work. I extend my thanks to the astronomers of Armagh Observatory Drs. Mart de Groot, P.B. Byrne, A.D. Andrews, C.J. Butler, postdocs P.M. Panagi, E. Houdebine and my fellow Ph.D. student A.C. Lanzafame for many interesting discussions. My thanks to H.M. Murphy and P.J.F. Brown for their assistance with the computer software and hardware. I acknowledge the support provided by STARLINK which is funded by the UK SERC. I also acknowledge the advice received from Drs. H.J. Walker and D.C. Parsons of RAL on handling the IRAS data. I wish to thank Poly for her encouragement and moral support throughout the preparation of this thesis. Finally and most importantly I want to thank my parents for their love, continual support and encouragement without whom this work would have no meaning. 4 2.2.4 M-dwarfs with Balmer lines in emission 48 2.2.5 M dwarfs with weak or no Ha 51 2.2.6 Do M dwarfs with no chromospheres exist ? 52 2.3 H7 versus X-ray emission in 'quiescent' and eruptive phenomena in M dwarfs 54 3 Optical Flare Activity 64 3.1 Discovery of flare activity on Gl 375 and Gl 431 64 3.1.

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Howarth Mood-Adjective Checklist--Version 4

Cited by 2 publications

References 0 publications

Fuzzy Urban Sets: Theory and Application to Desakota Regions in China

Fuzzy Urban Sets: Theory and Application to Desakota Regions in China

Magnetic activity phenomena in dwarf m and k stars

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