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Ninth International Conference on Permafrost ... - IARC Research

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Ni n t h In t e r n at i o n a l Co n f e r e n c e o n Pe r m a f r o s tDur − the time interval for analysisSkyGap,− the gap fracti<strong>on</strong> for the sky sectorElev − elevati<strong>on</strong> above sea levelGzG,s− surface zenith,azimuth angleWeight,(cos2−=cos1)/Divazizenith angles of the sky sector1,2− the boundingDivazi− the number of azimuthal divisi<strong>on</strong>s in the skymapSunGap,− gap fracti<strong>on</strong> for the sunmapUsing equati<strong>on</strong> (1), we calculated the m<strong>on</strong>thly mean ofISWSR at all sites. Figure 2 shows the m<strong>on</strong>thly mean ofISWSR by calculati<strong>on</strong> and by measurement at Terelj GL.Using the data given in Table 1, we obtained the followingregressi<strong>on</strong> equati<strong>on</strong>:t −= 2 . 1755 + 0 . 0116 R(2)ξyearlyFrom regressi<strong>on</strong> equati<strong>on</strong> (2) the threshold value belowwhich the permafrost occurs is 187.5WM -2 .Mapping <strong>Permafrost</strong> Distributi<strong>on</strong>We generated the map of YM of ISWSR. The YM ofISWSR fluctuates from 50.7WM -2 to 409.1WM -2 , depending<strong>on</strong> topography and forests. Mountain permafrost distributi<strong>on</strong>was mapped based <strong>on</strong> the threshold value of 187.5WM -2 .The permafrost island exists al<strong>on</strong>g the small river valleys(valley permafrost) and <strong>on</strong> the bottom of depressi<strong>on</strong>(depressi<strong>on</strong> permafrost), where a YM of ISWSR is morethan 187.5WM -2 . From DEM data, we generated the slopemap. From this slope map we have separated the areaswith a slope angle between 0–1°. The area with slope anglebetween 0–1° corresp<strong>on</strong>ds to the bottom of depressi<strong>on</strong> inNalaikh. This area of Nalaikh was mapped as a depressi<strong>on</strong>permafrost area (relict permafrost). From the slope map wehave separated the areas with a slope angle between 0–5°.The areas with 0–5° indicate the small river valleys. In theseareas, we have calculated the NDVI and NDWI as follows:NDVINDWINIR − VIS= (4)NIR + VIS(3)NIR − SWIR= (4) (5)NIR + SWIRThe areas with high NDVI and NDWI were mapped aswetland areas. NDVI lies between the limits of -0.4667 and+0.7042. A high value of NDVI is between the limits of +0.30and +0.7042. NDWI lies between the limits of -0.6 and +0.6129.A high value of NDWI is between the limits of 0.0 and +0.6129.The wetland areas overlie the more vegetated areas, and weseparated more wetland areas. These areas corresp<strong>on</strong>d with thepermafrost island areas al<strong>on</strong>g the small river valleys.The study area divides into two areas: permafrost areasand no permafrost areas. The permafrost areas divide intothree kinds of permafrost: 1 – mountain permafrost, 2 –depressi<strong>on</strong> permafrost (relict permafrost), and 3 – valleypermafrost (Fig. 3).Figure 2. M<strong>on</strong>thly mean of ISWSR at Terelj GL AWS site.Figure 3. <strong>Permafrost</strong> map of areas surrounding Ulaanbaatar.C<strong>on</strong>clusi<strong>on</strong>In summer 2007, we carried out the 1D geophysicalmeasurements by instrument AE-72 <strong>on</strong> 30 more points andexcavated 10 pits in our study area for validati<strong>on</strong> of thepermafrost distributi<strong>on</strong>. The probability is about 90%.ReferencesEtzelmuller, B. & Hoelzle, M. 2001. Mapping and Modellingthe Occurrence and Distributi<strong>on</strong> of Mountain<strong>Permafrost</strong>. Status Report at First European<str<strong>on</strong>g>C<strong>on</strong>ference</str<strong>on</strong>g> <strong>on</strong> <strong>Permafrost</strong>, Roma, Italy, March 2001.Fu, P. & Rich, P.M. 1999–2000. The solar analyst 1.0. UserManual, Helios Envir<strong>on</strong>mental Modeling InstituteLLC, USA.Kudryavtsev, V.A. 1978. General Geocryology. Moscow:Moscow University Press, 462 pp.114

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