MOUNTAIN ORDERING: A METHOD FOR CLASSIFYING MOUNTAINS BASED ON THEIR MORPHOMETRY

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Earth Surface Processes and Landforms Earth Surf. Process. Landforms 24, 653±660 (1999) MOUNTAIN ORDERING: A METHOD FOR CLASSIFYING MOUNTAINS BASED ON THEIR MORPHOMETRY SHUJI YAMADA Department of Geography, Tokyo Metropolitan University, Hachioji, Tokyo 192-0397, Japan Received 15 May 1998; Revised 27 October 1998; Accepted 30 November 1998 ABSTRACT A new method for classifying mountain morphology, `mountain ordering,' is proposed, and quantitative expressions for various morphological parameters of two ordered mountains in northern Japan were obtained using this method. Mountain order was defined in terms of the closed contour lines on a topographic map. A set of closed, concentric contour lines defines a first-order mountain. Higher-order mountains can be defined as a set of closed contour lines that contain lower-order mountains and that have only one closed contour line for each elevation; they are identified as m 1th-order mountains, where m represents the order of the enclosed, lower-order mountains. The geomorphometry for a mountain ordered according to this definition permits the identification of systematic relationships between various morphological parameters. The relationships between mountain order and these morphological parameters follow a form similar to that of Horton's laws, and permit the calculation of the ratios of number, area and height; these parameters are sufficient to express the magnitude of a mountain's dissection. The size±frequency distribution for area and height shows self-similarity for ordered mountains, and determines their fractal dimensions. Furthermore, the relationship between area and height, which has the form of a power function, describes the relief structure of ordered mountains. Copyright # 1999 John Wiley & Sons, Ltd. KEY WORDS: mountain ordering; morphology; morphometry; fractal analysis; relief structure INTRODUCTION The Earth's surface is shaped into various relief patterns, and any land with an elevation substantially higher than that of its surroundings is recognized as a mountain. Mountain morphology depends on geology or climate; and thus, the geomorphometry of mountains has been conducted in different areas using different methods (e.g. Strahler, 1952; Ahnert, 1970, 1984; Ohmori, 1978; Parsons and Abrahams, 1984; Schmidt and Montgomery, 1995). In particular, the application of fractal geometry and digital elevation models has led to a significant evolution in the techniques of mountain geomorphometry (e.g. Huang and Turcotte, 1989; Chase, 1992; Lifton and Chase, 1992; Ouchi and Matsushita, 1992). These geomorphometrical studies have revealed the morphological characteristics of mountains and have discussed the development of mountains. The extent of a mountain, however, has not yet been determined by a certain definition, because of the lack of a geomorphological definition for mountains. Most morphological parameters (e.g. relief, slope and fractal dimension) vary in value as the selected extent of the mountain varies. Therefore, it is necessary to define the extent of a mountain before it is possible to determine the mountain's morphological parameters unequivocally. This paper presents a method, `mountain ordering,' for defining the extent of a mountain, and uses this method to examine the morphological characteristics of a set of ordered mountains in northern Japan. As an example of geomorphometry based on the method of mountain ordering, mountain order and the number, area and height for mountains of each order were determined for these mountains. * Correspondence to: Department of Geography, Tokyo Metropolitan University, Hachioji, Tokyo 192-0397, Japan. Email: syamada@andes.geog.metro±u.ac.jp CCC 0197-9337/99/070653±08 $17.50 Copyright # 1999 John Wiley & Sons, Ltd.

654 S. YAMADA Figure 1. The definition of mountain order, and the areas and heights of ordered mountains. Although the second- and third-order mountains in this figure are only indicated by using different pixel patterns on the lower parts of the illustrations, these mountains nonetheless include the entire shaded upper parts. The area of an mth-order mountain, A m, is defined as the inner area of the lowestelevation contour line for that mountain, and was measured with a planimeter. The height of an mth-order mountain, H m, is defined as H m = N c I c 05 I c, where I c is the height of a contour interval and N c is the number of contour lines that make up the mth-order mountain Figure 2. A comparison between the proposed mountain order system and the stream order system of Strahler (1952) THE MOUNTAIN ORDERING METHOD Mountain order is defined by the contour lines on a topographic map (Figure 1), in which each mountain is represented as a series of closed contour lines. These sets of contour lines include only a single closed contour line for each elevation unless a col that divides the mountain has a height that exceeds the contour interval. Thus, the closed contour lines form a series of concentric shapes. Each set of these contour lines defines a first-order mountain. Higher-order mountains can be defined as a set of closed contour lines that contain the contour lines for one or more lower-order mountains and that have only one closed contour line for each elevation. If the highest of the enclosed lower-order mountains are of level m, then the surrounding higher-order mountain is identified as an m 1th-order mountain.

HoUniJo I,JOJIJ 140" E 1",* E 46 N o 5th order 4th order 3rd order Contour line Shore line 20 km o 4th order 3rd order 2nd order Contour line "W-ir 0 3rd order ~~. 2nd order r km 1st order Contour line Figure 3. The study area (A) and the areal patterns of the ordered mountains (B, C and D). The contour intervals of maps B, C and D, are 200, 100 and 50 m, respectively. The arrow in B shows the col that divides the fifth-order mountains of the Northern and Southern parts. Although the first-order and second-order mountains are only illustrated in C or D, all the lowerorder mountains contained within the fifth-order mountains illustrated in B were identified and measured during the study CLASSIFYING MOUNTAIN MORPHOLOGY 655

656 S. YAMADA Table 1. Morphological parameters of ordered mountains. A g and H g indicate geometrical mean of area and height, respectively Order Number, N Area, A (km 2 ) Height, H (km) A g A max A min H g H max H min Northern part 1st 541 0008 066 0001 0011 0185 0005 2nd 68 018 23 001 0059 0255 0015 3rd 10 67 24 12 0272 0525 0155 4th 2 117 130 104 0626 0825 0475 5th 1 369 0895 Southern part 1st 2690 0006 16 0001 0009 0185 0005 2nd 262 022 95 0006 0057 0615 0015 3rd 33 46 49 029 0205 0685 0035 4th 6 73 154 22 0454 0705 0205 5th 1 2251 1085 The proposed definition for mountain order is similar to that defined for stream order by Strahler (1952) (Figure 2). In accordance with Strahler's model, two first-order mountains can form a second-order mountain, but another first-order mountain at a lower elevation cannot make the second-order mountain into a thirdorder mountain; only the second-order mountain and another second-order mountain can form a third-order mountain. The mountain order system implies that a well-dissected mountain range would be identified as a higherorder mountain, whereas a poorly dissected mountain such as a young stratovolcano would be identified as a lower-order mountain, if the selected areas of the two mountains were similar. A col that divides two higherorder mountains will be deeper than a col that divides the lower-order mountains that make up each higherorder mountain. Thus, a higher-order mountain would have a number of cols that vary widely in depth. Since a poorly dissected mountain would have a little col, it would be identified as a lower-order mountain unless the selected area expanded to encompass some additional mountains or mountain ranges. MOUNTAIN ORDER IN A MOUNTAIN RANGE IN WESTERN HOKKAIDO A mountain range in western Hokkaido (northern Japan) was selected to test the usefulness of the mountain ordering method in the geomorphometry of these mountains (Figure 3A). The length of the mountain range, which extended from 43 20'N, 140 30'E to42 20'N, 140 90'E, was 120 km. The elevation of the highest point of the mountain range was 1480 m a.s.l. The rocks that form the mountains range from Tertiary and Quaternary andesite to Tertiary sedimentary rocks. A 1:25 000 topographic map (published by the Geographical Survey Institute of Japan) that used a contour interval of 10 m was used for the geomorphometry exercise. Two fifth-order mountains were identified in the mountain range, which included approximately 3000 mountains ranging from first order to fourth order (Figure 3B, C and D). The fifth-order mountains were divided by a col at 400 m a.s.l. in the northwestern part of the mountain range. In this paper, the fifth-order mountain located on the northwestern side of that col is henceforth called the `northern part'; the other fifthorder mountain is henceforth referred to as the `southern part'. The highest point in the southern part (1480 m a.s.l.) was slightly higher than that in the northern part (1290 m a.s.l.). The two parts differed significantly in area: the southern part (2251 km 2 ) was more than six times the size of the northern part (369 km 2 ).

CLASSIFYING MOUNTAIN MORPHOLOGY 657 Figure 4. The number of mountains (N), their areas (A) and their heights (H) plotted against the corresponding mountain orders. A and H are the geometric mean values for the mountains in each mountain order. The equations for the best-fitting lines for the northern part are as follows: N m =421 j m (r 2 =096),where j is thehighest mountain order and m isthe mountain order; A m =0008 1897 m 1 (r 2 =097); and H m =0011 353 m -1 (r 2 =091). For the southern part, the best-fitting equations are as follows: N m =670 j m (r 2 =099), A m =0006 2490 m 1 (r 2 =099) and H m =0009 367 m 1 (r 2 =095) MORPHOLOGICAL CHARACTERISTICS OF ORDERED MOUNTAINS The morphological parameters of ordered mountains in the study area (number, N, area, A, and height, H), which are defined in Figure 1, were determined (Table I) and the data were analysed for each fifth-order mountain. The geometric means for each fifth-order mountain were used for the analysis of the areas and heights. The number, area and height of the ordered mountains change systematically with changes in mountain order (Figure 4). The number of mountains of a given order approximates an inverse geometric series with respect to mountain order (Figure 4a). It follows that a mountain is divided into lower-order mountains at a constant rate, as is the case for streams (Horton, 1945), and the ratio, R n, is given by: N m ˆ R n j m 1 where N m is the number of mth-order mountains, and j is the highest order. The R n values for the northern and southern parts of the study area were 421 and 670, respectively. A minimum of two mth-order mountains can form an m 1th order mountain; that is, the minimum R n value is 2. The R n values for the northern and southern parts were much larger than this minimum value. Since different heights of a col are needed to form a mountain with an order higher than 1, the number of mth-order mountains increases if the cols that divide the mth-order mountains are similar in height. This means that the R n value becomes large for mountains that are dissected by cols with similar heights, but converges on 2 for mountains that are dissected by cols with different heights. Area approximates a geometric series with respect to mountain order (Figure 4b). The area of a given mountain order, A m, can be written as: A m ˆ A 1 R a m 1 2 where A 1 is the geometric mean area for all first-order mountains, and R a is the ratio of area. The R a values for the northern and southern parts were 1897 and 2490, respectively; as was the case for R n, the R a value is larger for the southern part. Since the A 1 values for the two parts were similar, the area occupied by a given mth-order mountain for the northern part is smaller than the comparable value for the southern part. This result means that the mountains of the northern part, which have a lower R a value, are more finely dissected than those of the southern part, which have a higher R a value.

658 S. YAMADA Figure 5. The area (A) and height (H) for the specific mountain orders plotted against the corresponding number of mountains of that order (N). A and H are the geometric mean values for the mountains in each order (m). The equations for the best-fitting lines for the northern part are as follows: N m =2988 A m 058 (r 2 =099) and N m =11 H m 141 (r 2 =099). For the southern part, N m = 10044A m 062 (r 2 =099) and N m =166H m 164 (r 2 =099) The heights of mountains of various orders also approximate a geometric series (Figure 4c). The height of a mountain of a given order, H m, can be written as: H m ˆ H 1 R h m 1 3 where H 1 is the geometric mean height for all first-order mountains, and R h is the ratio of height. The R h values for the northern and southern parts were 353 and 367, respectively; these values are similar. Larger R h values show higher mth-order mountains if the H 1 values are similar. Because the H 1 values were similar for the northern and southern parts, the depths of the cols that dissect the two mountains are also similar. The systematic relationships between mountain order and the selected morphological parameters suggest that the mountain system exhibits self-similarity, as is the case for streams (Horton, 1945). For ordered streams, the relationship between the number of tributaries and their lengths can be represented by a power function, and this shows that stream networks have fractal properties (Turcotte, 1997). The relationships between the number of mountains and their area can also be represented in the form of a power function (Figure 5a) as can those between the number of mountains and their height (Figure 5b), and this suggests that mountain orders also have fractal properties. This can be seen in the following two equations: N m ˆ c 1 A m D a =2 4 N m ˆ c 2 H m D h 5 where m is a given mountain order, D a and D h are the fractal dimensions for area and height, respectively, and c 1 and c 2 are constants. These relationships demonstrate that the areal pattern and height distribution for ordered mountains are self-similar, and that the self-similarity is characterized by their respective fractal dimensions, D a and D h. The D a values for the northern and southern parts were 116 and 124, respectively, and the corresponding D h values were 141 and 164. Since the D h values were larger than the D a values, the area of ordered mountains increases faster than the height. This relationship is clearly shown in Figure 6, and can be defined by the expression: H m ˆ r c A m =2 6 where is the relief parameter and r c is the characteristic relief. The values for the northern and southern parts were 080 and 074, respectively. Since both values are less than 1, the relief of ordered mountains (H/

CLASSIFYING MOUNTAIN MORPHOLOGY 659 Figure 6. The relationship between the corresponding areas (A) and heights (H) for the specific mountain orders. A and H are the geometric mean valuesfor themountains ofeach order. The best-fitting equation forthe northern part is H m =0097A m 040 (r 2 =099); for thesouthern part, the best fit was obtained with the equation H m =0083A m 037 (r 2 =098) A 1/2 ) decreases with increasing mountain order. Therefore, for a mountain with <1, the relief around the summit, which consists of lower-order mountains, is higher than that of the mountain from summit to piedmont, which consists of higher-order mountains. In addition to, r c also shows the relief structure of an ordered mountain. Since r c is the height per unit area, it represents a characteristic relief of the mountain. Thus, the relationship between A and H characterizes both the magnitude of the relief and its change from summit to piedmont. CONCLUSIONS The method of mountain ordering can define a mountain's extent, and yields quantitative expressions for describing the morphology of ordered mountains. The relationships between mountain order and various morphological parameters are similar in form to Horton's law and permit the calculation of the ratios for number, area and height; these parameters are sufficient to express the magnitude of the mountain's dissection. The size±frequency distributions for area and height suggest self-similarity for ordered mountains, and determine the fractal dimensions of the mountains. Furthermore, the relationship between area and height, which was found in this paper to take the form of a power function, describes the relief structure of the ordered mountains. Although further examination of the technique is necessary, the relationships obtained from the mountain ordering technique appear to describe adequately certain basic geomorphometric characteristics of a mountain. Since the definition of a mountain's order is very simple, the morphological parameters presented in this paper and additional morphological parameters can be obtained from geomorphometry based on mountain ordering exercises conducted in various mountains over a broader range of areas. These morphological data will be a useful tool for discussing the development of mountains. ACKNOWLEDGEMENTS I would like to thank Professor Kazuomi Hirakawa and Dr Yoshimasa Kurashige of Hokkaido University for critical comments on an earlier draft of this manuscript. Discussions with Mr Yuichiro Fusejima of the Geological Survey of Japan helped to clarify the conceptual framework. REFERENCES Ahnert, F. 1970 `Functional relationships between denudation, relief, and uplift in large mid-latitude drainage basins', Am. J. Sci., 268, 243±263. Ahnert, F. 1984 `Local relief and the height limits of mountain ranges', Am. J. Sci., 284, 1035±1055.

660 S. YAMADA Chase, C. G. 1992 `Fluvial landsculpting and the fractal dimension of topography', Geomorphology, 5, 39±57. Horton, R. E. 1945 `Erosional development of streams and their drainage basins: hydrophysical approach to quantitative morphology', Geol. Soc. Am. Bull., 56, 275±370. Ohmori, H. 1978. `Relief structure of the Japanese mountains and their stages in geomorphic development', Bull. Dept. Geogr. Univ. Tokyo, 10, 31±85. Ouchi, S. and Matsushita, M. 1992. `Measurement of self-affinity on surfaces as a trial application of fractal geometry to landform analysis', Geomorphology, 5, 115±130. Parsons, A. J. and Abrahams, A. D. 1984. `Mountain mass denudation and piedmont formation in the Mojave and Sonoran Deserts', Am. J. Sci., 284, 255±271. Schmidt, K. M. and Montgomery, D. R. 1995. `Limits to relief', Science, 270, 617±620. Strahler, A. N. 1952. `Hypsometric (area±altitude) analysis of erosional topography', Geol. Soc. Am. Bull., 63, 1117±1142. Turcotte, D. L. 1997. Fractals and Chaos in Geology and Geophysics, 2nd edn, Cambridge University Press, New York, 398pp.