메뉴 건너뛰기




Volumn 271, Issue 5251, 1996, Pages 962-963

Dust: A diagnostic of the hydrologic cycle during the last glacial maximum

Author keywords

[No Author keywords available]

Indexed keywords

DUST; HYDROLOGICAL CYCLE; ICE CORE; LAST GLACIAL MAXIMUM;

EID: 0029657734     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.271.5251.962     Document Type: Article
Times cited : (119)

References (38)
  • 1
    • 84967885639 scopus 로고
    • Cambridge Univ. Press, Cambridge
    • Intergovernmental Panel on Climate Change, Climate Change: The IPCC Scientific Assessment (Cambridge Univ. Press, Cambridge, 1990); Climate Change 1992 Supplement to the IPCC Scientific Assessment (Cambridge Univ Press, Cambridge, 1992), C. A Senior and J. F. B. Mitchell, J Climate 6, 393 (1993); B C. Weare, ibid. 7, 248 (1994); R. D. Cess et al., J Geophys. Res. 95, 16601 (1990).
    • (1990) Climate Change: The IPCC Scientific Assessment
  • 2
    • 0003619462 scopus 로고
    • Cambridge Univ Press, Cambridge
    • Intergovernmental Panel on Climate Change, Climate Change: The IPCC Scientific Assessment (Cambridge Univ. Press, Cambridge, 1990); Climate Change 1992 Supplement to the IPCC Scientific Assessment (Cambridge Univ Press, Cambridge, 1992), C. A Senior and J. F. B. Mitchell, J Climate 6, 393 (1993); B C. Weare, ibid. 7, 248 (1994); R. D. Cess et al., J Geophys. Res. 95, 16601 (1990).
    • (1992) Climate Change 1992 Supplement to the IPCC Scientific Assessment
  • 3
    • 0027532797 scopus 로고
    • Intergovernmental Panel on Climate Change, Climate Change: The IPCC Scientific Assessment (Cambridge Univ. Press, Cambridge, 1990); Climate Change 1992 Supplement to the IPCC Scientific Assessment (Cambridge Univ Press, Cambridge, 1992), C. A Senior and J. F. B. Mitchell, J Climate 6, 393 (1993); B C. Weare, ibid. 7, 248 (1994); R. D. Cess et al., J Geophys. Res. 95, 16601 (1990).
    • (1993) J Climate , vol.6 , pp. 393
    • Senior, C.A.1    Mitchell, J.F.B.2
  • 4
    • 0028313809 scopus 로고
    • Intergovernmental Panel on Climate Change, Climate Change: The IPCC Scientific Assessment (Cambridge Univ. Press, Cambridge, 1990); Climate Change 1992 Supplement to the IPCC Scientific Assessment (Cambridge Univ Press, Cambridge, 1992), C. A Senior and J. F. B. Mitchell, J Climate 6, 393 (1993); B C. Weare, ibid. 7, 248 (1994); R. D. Cess et al., J Geophys. Res. 95, 16601 (1990).
    • (1994) J Climate , vol.7 , pp. 248
    • Weare, B.C.1
  • 5
    • 0025680011 scopus 로고
    • Intergovernmental Panel on Climate Change, Climate Change: The IPCC Scientific Assessment (Cambridge Univ. Press, Cambridge, 1990); Climate Change 1992 Supplement to the IPCC Scientific Assessment (Cambridge Univ Press, Cambridge, 1992), C. A Senior and J. F. B. Mitchell, J Climate 6, 393 (1993); B C. Weare, ibid. 7, 248 (1994); R. D. Cess et al., J Geophys. Res. 95, 16601 (1990).
    • (1990) J Geophys. Res. , vol.95 , pp. 16601
    • Cess, R.D.1
  • 7
    • 0025523995 scopus 로고    scopus 로고
    • R S Lindzen, Bull Am Meteor. Soc. 71, 288 (1990); ibid., p. 1465.
    • Bull Am Meteor. Soc. , pp. 1465
  • 8
    • 0022179249 scopus 로고
    • D Rind and D Peteet, Quat. Res. 24, 1 (1985); T. J. Crowley and G. R. North, Paleoclimatology (Oxford Univ. Press, Oxford, 1991); J. E Hansen et al, in Climate Processes and Climate Sensitivity, J. E. Hansen and T. Takahashi, Eds. (Geophysical Monograph 29, American Geophysical Union, Washington, DC, 1984), pp. 130-163.
    • (1985) Quat. Res. , vol.24 , pp. 1
    • Rind, D.1    Peteet, D.2
  • 9
    • 85040896350 scopus 로고
    • Oxford Univ. Press, Oxford
    • D Rind and D Peteet, Quat. Res. 24, 1 (1985); T. J. Crowley and G. R. North, Paleoclimatology (Oxford Univ. Press, Oxford, 1991); J. E Hansen et al, in Climate Processes and Climate Sensitivity, J. E. Hansen and T. Takahashi, Eds. (Geophysical Monograph 29, American Geophysical Union, Washington, DC, 1984), pp. 130-163.
    • (1991) Paleoclimatology
    • Crowley, T.J.1    North, G.R.2
  • 10
    • 0021571496 scopus 로고
    • J. E. Hansen and T. Takahashi, Eds. Geophysical Monograph 29, American Geophysical Union, Washington, DC
    • D Rind and D Peteet, Quat. Res. 24, 1 (1985); T. J. Crowley and G. R. North, Paleoclimatology (Oxford Univ. Press, Oxford, 1991); J. E Hansen et al, in Climate Processes and Climate Sensitivity, J. E. Hansen and T. Takahashi, Eds. (Geophysical Monograph 29, American Geophysical Union, Washington, DC, 1984), pp. 130-163.
    • (1984) Climate Processes and Climate Sensitivity , pp. 130-163
    • Hansen, J.E.1
  • 11
    • 0019679029 scopus 로고
    • J -R Petit et al., Nature 293, 391 (1981).
    • (1981) Nature , vol.293 , pp. 391
    • Petit, J.R.1
  • 12
    • 0002386320 scopus 로고
    • C. C. Langway, H Oeschger, W. Dansgaard, Eds Geophysical Monograph 33, American Geophysical Union, Washington, DC
    • C U. Hammer et al., in Greenland Ice Core: Geophysics, Geochemistry, and the Environment, C. C. Langway, H Oeschger, W. Dansgaard, Eds (Geophysical Monograph 33, American Geophysical Union, Washington, DC, 1985), pp. 90-94.
    • (1985) Greenland Ice Core: Geophysics, Geochemistry, and the Environment , pp. 90-94
    • Hammer, C.U.1
  • 14
    • 4243052336 scopus 로고    scopus 로고
    • note
    • From (4, 5) we obtained the following: The enhancement factor for dust particles (radius > 0 4 μm) at dome C in Antarctica is 9 to 14; the enhancement factors for the elements Al, Na, and Cl are 34, 4 9, and 3.8, respectively; and the enhancement factor for dust particles in Greenland is 100.
  • 15
    • 0027038336 scopus 로고
    • C Genthon, Tellus 44B, 371 (1992).
    • (1992) Tellus , vol.44 B , pp. 371
    • Genthon, C.1
  • 17
    • 0024850924 scopus 로고
    • There is no ice core data for low latitudes at sea level. However, ice cores taken from mountain glaciers show that dust contents are enhanced in the LGM layer [L. G Thompson et al., Science 246, 474 (1989); L G. Thompson et al , ibid. 269, 46 (1995)]. It is difficult to interpret the dust deposition rates in the high mountains because of possible changes in local meteorology during the LGM. The beauty of the polar data is that the poles are remote regions of the globe and any enhancement must be related to changes on a global scale (global change)
    • (1989) Science , vol.246 , pp. 474
    • Thompson, L.G.1
  • 18
    • 0029541741 scopus 로고
    • There is no ice core data for low latitudes at sea level. However, ice cores taken from mountain glaciers show that dust contents are enhanced in the LGM layer [L. G Thompson et al., Science 246, 474 (1989); L G. Thompson et al , ibid. 269, 46 (1995)]. It is difficult to interpret the dust deposition rates in the high mountains because of possible changes in local meteorology during the LGM. The beauty of the polar data is that the poles are remote regions of the globe and any enhancement must be related to changes on a global scale (global change)
    • (1995) Science , vol.269 , pp. 46
    • Thompson, L.G.1
  • 21
    • 0022237844 scopus 로고
    • V. M Bryant and R. G Holloway, Eds, American Association of Stratigraphic Palynologists, Calgary, Ontario
    • V M. Bryant Jr. and R. G Holloway, in Pollen Records of Late Quaternary North American Sediments, V. M Bryant and R. G Holloway, Eds, (American Association of Stratigraphic Palynologists, Calgary, Ontario, 1985), pp. 39-70.
    • (1985) Pollen Records of Late Quaternary North American Sediments , pp. 39-70
    • Bryant Jr., V.M.1    Holloway, R.G.2
  • 23
    • 0029487656 scopus 로고
    • M. Stute, P. Schlosser, J. F. Clark, W. S. Broecker, Science 256, 1000 (1992); M Stute et al., ibid. 269, 379 (1995)
    • (1995) Science , vol.269 , pp. 379
    • Stute, M.1
  • 25
    • 0026272343 scopus 로고
    • The 2D model has four components: the photochemical module, the solar-radiative module, the infrared-radiative module, and the transport module. The model has 18 latitudes, from pole to pole There are 40 layers, from 0 to 80 km in log pressure coodinates. Time-stepping is 1 to 4 steps per day. We usually used model times of 10 to 20 years to obtain convergence. The monthly averaged transport coefficients were computed by the method of H Yang et al. [J Atmos. Sci 48, 442 (1991)]. The details are described in R. L. Shia et al [J. Geophys. Res. 94, 18467 (1989)]. We adopted in the 2D model washout lifetimes computed with a 3D model by Y J. Balkanski et al [ibid. 98, 20573 (1993)].
    • (1991) J Atmos. Sci , vol.48 , pp. 442
    • Yang, H.1
  • 26
    • 0024975415 scopus 로고
    • The 2D model has four components: the photochemical module, the solar-radiative module, the infrared-radiative module, and the transport module. The model has 18 latitudes, from pole to pole There are 40 layers, from 0 to 80 km in log pressure coodinates. Time-stepping is 1 to 4 steps per day. We usually used model times of 10 to 20 years to obtain convergence. The monthly averaged transport coefficients were computed by the method of H Yang et al. [J Atmos. Sci 48, 442 (1991)]. The details are described in R. L. Shia et al [J. Geophys. Res. 94, 18467 (1989)]. We adopted in the 2D model washout lifetimes computed with a 3D model by Y J. Balkanski et al [ibid. 98, 20573 (1993)].
    • (1989) J. Geophys. Res. , vol.94 , pp. 18467
    • Shia, R.L.1
  • 27
    • 0001397678 scopus 로고
    • The 2D model has four components: the photochemical module, the solar-radiative module, the infrared-radiative module, and the transport module. The model has 18 latitudes, from pole to pole There are 40 layers, from 0 to 80 km in log pressure coodinates. Time-stepping is 1 to 4 steps per day. We usually used model times of 10 to 20 years to obtain convergence. The monthly averaged transport coefficients were computed by the method of H Yang et al. [J Atmos. Sci 48, 442 (1991)]. The details are described in R. L. Shia et al [J. Geophys. Res. 94, 18467 (1989)]. We adopted in the 2D model washout lifetimes computed with a 3D model by Y J. Balkanski et al [ibid. 98, 20573 (1993)].
    • (1993) J. Geophys. Res. , vol.98 , pp. 20573
    • Balkanski, Y.J.1
  • 28
    • 4243109194 scopus 로고    scopus 로고
    • Our result should be compared with figure 23 in (9)
    • Our result should be compared with figure 23 in (9).
  • 31
    • 0027808040 scopus 로고
    • Recent work has shown that the total area of deserts during the LGM was about twice that in the Holocene [J. A Chappellaz et al., Tellus 45B, 228 (1993); P. Friedlingstein et al., J. Geophys. Res. 100, 7203 (1995)]
    • (1993) Tellus , vol.45 B , pp. 228
    • Chappellaz, J.A.1
  • 32
    • 0028806918 scopus 로고
    • Recent work has shown that the total area of deserts during the LGM was about twice that in the Holocene [J. A Chappellaz et al., Tellus 45B, 228 (1993); P. Friedlingstein et al., J. Geophys. Res. 100, 7203 (1995)]
    • (1995) J. Geophys. Res. , vol.100 , pp. 7203
    • Friedlingstein, P.1
  • 33
    • 84879881554 scopus 로고
    • G Kukla et al., Geology 16, 811 (1988)
    • (1988) Geology , vol.16 , pp. 811
    • Kukla, G.1
  • 34
    • 4243157072 scopus 로고    scopus 로고
    • note
    • The saturated vapor pressure of water decreases by 34% from 30° to 25°C; thus, a change of 5°C in SST alone is not sufficient to cause a difference of a factor of 2 in the water vapor content of the atmosphere.
  • 35
    • 0024223497 scopus 로고
    • L D D Harvey, Nature 334, 333 (1988). We wish to speculate on the effect of atmospheric dust on the tropical "warm pool." Today a major source of moisture is the warm pool (with SSTs often >29°C) in the tropical western Pacific Ocean around Indonesia and New Guinea. If the combination of a lower ocean level (by 150 m), stronger winds, and atmospheric dust opacity were to reduce the SST of the warm pool by 10°C, this would decrease the source of moisture by half The reduced moisture would greatly reduce the greenhouse effect caused by water vapor, thereby contributing to the cooling of the tropics.
    • (1988) Nature , vol.334 , pp. 333
    • Harvey, L.D.D.1
  • 36
    • 0027388671 scopus 로고    scopus 로고
    • The martian atmosphere is characterized by extreme aridity and dustiness, and dust plays a fundamental role in regulating the climate of Mars [J R. Murphy et al , J. Geophys. Res. 98, 3197 (1993); M. Santee and D. Crisp, ibid , p. 3261.
    • (1993) J. Geophys. Res. , vol.98 , pp. 3197
    • Murphy, J.R.1
  • 37
    • 0027388671 scopus 로고    scopus 로고
    • The martian atmosphere is characterized by extreme aridity and dustiness, and dust plays a fundamental role in regulating the climate of Mars [J R. Murphy et al , J. Geophys. Res. 98, 3197 (1993); M. Santee and D. Crisp, ibid , p. 3261.
    • J. Geophys. Res. , pp. 3261
    • Santee, M.1    Crisp, D.2
  • 38
    • 4243152546 scopus 로고    scopus 로고
    • note
    • Supported in part by NASA grant NAGW 2204 to the California Institute of Technology and by NSC 84-2111-M-001-027GP from the National Science Council of the Republic of China Y.L.Y thanks the Institute of Earth Sciences and Academia Sinica for their hospitality during his sabbatical year and A Ingersoll, L. Jaegle, C. Leovy, D. Rind, and I. Tegen for helpful discussions.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.