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  1. 139 大気海洋研究所
  2. 10 気候システム研究系
  3. 1391010 学術雑誌
  1. 0 資料タイプ別
  2. 10 学術雑誌論文
  3. 014 自然科学

Aerosol Optical Properties in the Iranian Region Obtained by Ground-Based Solar Radiation Measurements in the Summer of 1991

http://hdl.handle.net/2261/51863
http://hdl.handle.net/2261/51863
c9d48d31-256c-48f7-b1ac-c7cb10d12af5
名前 / ファイル ライセンス アクション
Nakajima1996JAM_H24P38.pdf Nakajima1996JAM_H24P38.pdf (1.3 MB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2012-07-03
タイトル
タイトル Aerosol Optical Properties in the Iranian Region Obtained by Ground-Based Solar Radiation Measurements in the Summer of 1991
言語
言語 eng
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ journal article
著者 Nakajima, Teruyuki

× Nakajima, Teruyuki

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Nakajima, Teruyuki

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Hayasaka, Tadahiro

× Hayasaka, Tadahiro

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Hayasaka, Tadahiro

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Higurashi, Akiko

× Higurashi, Akiko

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Higurashi, Akiko

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Hashida, Gen

× Hashida, Gen

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Hashida, Gen

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Moharram-Nejad, Naser

× Moharram-Nejad, Naser

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Moharram-Nejad, Naser

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Najafi, Yahya

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Valavi, Hamzeh

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Valavi, Hamzeh

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著者所属
著者所属 Center for Climate System Research, University of Tokyo
著者所属
著者所属 Faculty of Science, Tohoku University
著者所属
著者所属 Department of the Environment of Iran
抄録
内容記述タイプ Abstract
内容記述 Solar radiation measurements were made using sun photometers and pyranometers during 31 May-7 June 1991 at several places in Iran and during 12 June-17 September 1991 at a fixed place, Bushehr, Iran. In the first period the aerosol optical thickness had values about 0.4 at the wavelength of 0.5 μm in the coastal area and about 0.2 in the plateau area. The Ångström's exponent, which is the slope of optical thickness spectrum, had values around 1 for large city areas and less than 0.5 for inland arid areas. Chemical analyses of sampled air indicate an effect of fossil fuel burning from local sources. Such optical and chemical characteristics of atmospheres suggest that soil-derived coarse particles contributed considerably to the atmospheric turbidity in arid areas, whereas an active generation of aerosols was dominant near large cities. Significant rises in atmospheric turbidity were observed in the earlier part of the second period at Bushehr about once a week with a duration of about one day, which may have been caused by smoke from oil-well fires in Kuwait. The aerosol optical thickness in these events had values of about 1.5, which is equivalent to a columnar aerosol volume of 4.4 × 10-4 cm3 cm-2. The absorption index ranged from 0.005 to 0.02 with several peaks reaching 0.1 in the second period. These peaks can be attributed to prevailing smoke particles. In spite of the large variety of optical thicknesses and absorption indices, there existed stable power-law size distributions with an exponent about 3.7.
書誌情報 Journal of applied meteorology

巻 35, 号 8, p. 1265-1278, 発行日 1996-08
ISSN
収録物識別子タイプ ISSN
収録物識別子 08948763
書誌レコードID
収録物識別子タイプ NCID
収録物識別子 AA10678641
DOI
識別子タイプ DOI
関連識別子 info:doi/10.1175/1520-0450(1996)035<1265:AOPITI>2.0.CO;2
権利
権利情報 © Copyright 1996 American Meteorological Society (AMS). Permission to use figures, tables, and brief excerpts from this work in scientific and educational works is hereby granted provided that the source is acknowledged. Any use of material in this work that is determined to be “fair use” under Section 107 of the U.S. Copyright Act or that satisfies the conditions specified in Section 108 of the U.S. Copyright Act (17 USC §108, as revised by P.L. 94-553) does not require the AMS’s permission. Republication, systematic reproduction, posting in electronic form, such as on a web site or in a searchable database, or other uses of this material, except as exempted by the above statement, requires written permission or a license from the AMS. Additional details are provided in the AMS Copyright Policy, available on the AMS Web site located at (http://www.ametsoc.org/) or from the AMS at 617-227-2425 or copyright@ametsoc.org.
日本十進分類法
主題Scheme NDC
主題 451
出版者
出版者 American Meteorological Society
関係URI
識別子タイプ URI
関連識別子 http://journals.ametsoc.org/doi/abs/10.1175/1520-0450%281996%29035%3C1265%3AAOPITI%3E2.0.CO%3B2
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