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Enhanced climatic warming in the Tibetan Plateau due to doubling CO2: a model study Received: 5 April 2002 / Accepted: 7 August 2002 / Published online: 19 December 2002 Ó Springer-Verlag 2002 Abstract The National Center for Atmospheric Research (NCAR) regional climate model (RegCM2), together with initial conditions and time-dependent lat- eral boundary conditions provided by a 130-year tran- sient increasing CO 2 simulation of the NCAR Climate System Model (CSM), has been used to investigate the mechanism of ground warming over the Tibetan Plateau (TP). The model results show that when CO 2 in the at- mosphere is doubled, a strong ground warming occurs in the TP. Two regions within it with the largest warming are in the eastern TP (region I) and along the south- western and western slopes (region II). Moreover, in region I the ground warming in the winter half year is stronger than that in the summer half year, but in region II the warming difference between the seasons becomes opposite to that in region I, i.e., the warming is strong in the summer half year and weak in the winter half year. There are indications that the summer monsoon en- hances but the winter monsoon weakens when CO 2 is doubled. A strong elevation dependency of ground warming is found in region I for the winter half year, and in region II for both winter and summer half years at elevations below 5 km. The simulated characteristics of ground warming in the TP are consistent with the observations. In region I, when CO 2 is doubled, the cloud amount increases at lower elevations and decreases at higher elevation for the winter half year. As a consequence, at lower elevations the short wave solar radiation absorbed at the surface declines, and the downward long wave flux reaching the surface enhances; on the other hand, at higher elevations the surface solar radiation flux increases and the surface infrared radia- tion flux shows a more uniform increase. The net effect of the changes in both radiation fluxes is an enhanced surface warming at higher elevations, which is the pri- mary cause of the elevation dependency in the surface warming. In the summer half year the cloud amount reduces as a result of doubling CO 2 in region I for all elevations, and there is no elevation dependency de- tected in the ground warming. Furthermore, there is little snow existing in region I for both summer and winter half years, and the impact of snow-albedo feed- back is not significant. In region II, although the chan- ges in the cloud amount bear a resemblance to those in region I, the most significant factor affecting the surface energy budget is the depletion of the snow cover at higher elevations, which leads to a reduction of the surface albedo. This reduction in turn leads to an en- hancement in the solar radiation absorbed in the surface. The snow-albedo feedback mechanism is the most es- sential cause of the elevation dependency in the surface warming for region II. 1 Introduction There are growing concerns over the climate change in high elevation areas. Specifically, the climatic warming induced by the greenhouse gases could severely impact human activities and ecosystems in these regions. A number of studies have presented evidence that surface climate change associated with the global warming at high elevation sites shows more pronounced warming than that at low elevation sites, i.e., an elevation de- pendency of climatic warming. Beniston et al. (1997) Climate Dynamics (2003) 20: 401–413 DOI 10.1007/s00382-002-0282-4 B. Chen W.C. Chao X. Liu B. Chen GEST Center, University of Maryland, Baltimore County, Baltimore, MD, USA W.C. Chao NASA/Goddard Space Fight Center, Greenbelt, MD, USA X. Liu Institute of Earth Environment, Chinese Academy of Sciences, Xian, China B. Chen (&) GSFC/NASA, Mail Code 913, Greenbelt, MD 20711, USA E-mail: [email protected]

B. Chen Æ W.C. Chao Æ X. Liu Enhanced climatic warming in ...tibet.ieecas.cn/papers/CD03ChenBD.pdf · tion flux shows a more uniform increase. The net effect of the changes in

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Page 1: B. Chen Æ W.C. Chao Æ X. Liu Enhanced climatic warming in ...tibet.ieecas.cn/papers/CD03ChenBD.pdf · tion flux shows a more uniform increase. The net effect of the changes in

Enhanced climatic warming in the Tibetan Plateau dueto doubling CO2: a model study

Received: 5 April 2002 / Accepted: 7 August 2002 / Published online: 19 December 2002� Springer-Verlag 2002

Abstract The National Center for AtmosphericResearch (NCAR) regional climate model (RegCM2),together with initial conditions and time-dependent lat-eral boundary conditions provided by a 130-year tran-sient increasing CO2 simulation of the NCAR ClimateSystem Model (CSM), has been used to investigate themechanism of ground warming over the Tibetan Plateau(TP). The model results show that when CO2 in the at-mosphere is doubled, a strong ground warming occurs inthe TP. Two regions within it with the largest warmingare in the eastern TP (region I) and along the south-western and western slopes (region II). Moreover, inregion I the ground warming in the winter half year isstronger than that in the summer half year, but in regionII the warming difference between the seasons becomesopposite to that in region I, i.e., the warming is strong inthe summer half year and weak in the winter half year.There are indications that the summer monsoon en-hances but the winter monsoon weakens when CO2 isdoubled. A strong elevation dependency of groundwarming is found in region I for the winter half year,and in region II for both winter and summer half yearsat elevations below 5 km. The simulated characteristicsof ground warming in the TP are consistent with theobservations. In region I, when CO2 is doubled, the

cloud amount increases at lower elevations anddecreases at higher elevation for the winter half year. Asa consequence, at lower elevations the short wave solarradiation absorbed at the surface declines, and thedownward long wave flux reaching the surface enhances;on the other hand, at higher elevations the surface solarradiation flux increases and the surface infrared radia-tion flux shows a more uniform increase. The net effectof the changes in both radiation fluxes is an enhancedsurface warming at higher elevations, which is the pri-mary cause of the elevation dependency in the surfacewarming. In the summer half year the cloud amountreduces as a result of doubling CO2 in region I for allelevations, and there is no elevation dependency de-tected in the ground warming. Furthermore, there islittle snow existing in region I for both summer andwinter half years, and the impact of snow-albedo feed-back is not significant. In region II, although the chan-ges in the cloud amount bear a resemblance to those inregion I, the most significant factor affecting the surfaceenergy budget is the depletion of the snow cover athigher elevations, which leads to a reduction of thesurface albedo. This reduction in turn leads to an en-hancement in the solar radiation absorbed in the surface.The snow-albedo feedback mechanism is the most es-sential cause of the elevation dependency in the surfacewarming for region II.

1 Introduction

There are growing concerns over the climate change inhigh elevation areas. Specifically, the climatic warminginduced by the greenhouse gases could severely impacthuman activities and ecosystems in these regions. Anumber of studies have presented evidence that surfaceclimate change associated with the global warming athigh elevation sites shows more pronounced warmingthan that at low elevation sites, i.e., an elevation de-pendency of climatic warming. Beniston et al. (1997)

Climate Dynamics (2003) 20: 401–413DOI 10.1007/s00382-002-0282-4

B. Chen Æ W.C. Chao Æ X. Liu

B. ChenGEST Center, University of Maryland,Baltimore County,Baltimore, MD, USA

W.C. ChaoNASA/Goddard Space Fight Center,Greenbelt, MD, USA

X. LiuInstitute of Earth Environment,Chinese Academy of Sciences, Xian, China

B. Chen (&)GSFC/NASA, Mail Code 913,Greenbelt, MD 20711, USAE-mail: [email protected]

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indicated that, as far as the same latitudes of northernland are concerned, the observed surface air temperaturechange seems to be related to elevation. In addition,Beniston and Rebetez (1996) found that the surface cli-mate change in the Swiss Alps in association with theglobal warming displayed an altitudinal dependency. Inthe Tien Shan of central Asia, during the second half ofthe twentieth century, the warming trend in the regionsover 2 km above sea level (a.s.l.) appeared to be greaterthan that below 2 km a.s.l. (e.g., Aizen et al. 1997).Using an early version of the National Center of At-mosphere Research (NCAR) regional climate model,Giorgi et al. (1997) showed that the snow-albedo feed-back may be responsible for the excessive warming in theSwiss Alps. From an ensemble of climate change ex-periments with increasing greenhouse gases and aerosolsusing an air–sea coupled climate model, Fyfe and Flato(1999) found a marked elevation dependency of thesimulated surface screen temperature increase over theRocky Mountains.

The Tibetan Plateau (TP) is located in central Asiawith a mean elevation of more than 4 km a.s.l. and anarea of about 2.3 · 106 km2. It is surrounded by thehighest mountains in the world, such as the Himalayas,Pamir, Kunlun Shan and others, and exerts profoundthermal and dynamical influences on the local weatherand climate as well as on the atmospheric circulation inthe Northern Hemisphere (e.g., Manabe and Terpstra1974; Yeh and Gao 1979; Manabe and Broccoli 1990;Yanai et al. 1992; Kutzbach et al. 1993). Analysis of icecore from the TP indicates that there was a significantincrease in the ground temperature over the last fewdecades (e.g., Thompson et al. 1993; Yao et al. 1995),which appeared to be associated with the retreat of mostmountain glaciers on the TP (see Tang et al. 1998 fordetails). Using almost all the available instrumentalrecords, Liu and Chen (2000) showed that the mainportion of the TP had experienced significant surfacewarming since the mid-1950s, especially in winter. Thelinear rates of increase in the surface air temperature inthe TP during the period of 1955–1996 were about0.16 �C/decade for the annual mean and 0.32 �C/decadefor the winter mean, which exceeded those for the samelatitudinal zone in the Northern Hemisphere during thesame period. The surface warming in different parts ofthe TP was not completely the same in form, and thestronger warming trend occurred in the central, easternand northwestern TP. In addition, they found that therewas a tendency for the warming trend to increase withelevation in the TP as well as its surrounding areas.

The cause of the recent surface warming in the TP hasnot been fully understood. However, numerical experi-ments have shown that, with enhanced greenhouse ga-ses, there is an increase in the TP surface air temperaturefor most current climate models (Manabe et al. 1991;Cubasch et al. 1992; Murphy and Mitchell 1995;Houghton et al. 1996). This fact implies that the ob-served TP warming could be attributed to increasedgreenhouse gases in the atmosphere, which are believed

to result from human activities. Moreover, Liu andChen (2000) have made a detailed analysis of the TPsurface air temperature from the doubling CO2 experi-ments produced by three well-known global climatemodels. The results indicate that, although the surfacewarming in the TP is evident, the elevation dependencyof the warming as shown in the observations could notbe found. They argued that this disagreement may beowing partly to the coarse resolution of the models andpartly to the inadequate treatment of physical processes,in particular, land surface processes in complex topo-graphic areas like the TP.

With its vast area the TP has unique topography,landscape and climate compared with other high eleva-tion regions. It is natural to consider that the climatewarming induced by enhanced greenhouse gases and itselevation dependency in the TP are closely associatedwith the TP’s inherent complexity of topography andclimatic variability among various terrestrial regimes.Therefore, in order to investigate the climatic warmingover the TP, the use of high-resolution models is es-sential. In this study, by using a high-resolution regionalclimate model, the climatic response in the TP to adoubling of CO2 in the global atmosphere will be ex-amined and the focus will be on the ground warmingand its mechanism.

In the next section the model used and experimentaldesign will be outlined. A brief description of the lateralboundary conditions will also be given in this section.Section 3 will show the results simulated from two three-year integrations. Section 4 will discuss the surface en-ergy budget and the relevant atmospheric and surfaceprocesses that make impacts on the surface energyexchange. Conclusion and discussion will be presentedin Section 5.

2 Description of model used and experimental design

The latest version of the NCAR regional climate model version 2(RegCM2) is used. The dynamical component of the RegCM2 isessentially the same as that of the MM4 (The NCAR-PennsylvaniaState University Meso-scale Model version 4), which is a com-pressible, grid point model with hydrostatic balance and verticalr-coordinates. Exceptions are the use of a split-explicit timeintegration scheme and of an algorithm for reducing horizontaldiffusion in the presence of steep topographical gradients (Giorgiet al. 1993a, b). A number of physics parametrization schemes havebeen adopted in the model for applications to climate studies. Theradiative transfer package is that of the NCAR CommunityClimate Model version 3 (CCM3), and the boundary layer schemefrom Holtslag et al. (1990). The latest version of BATS 1E (Bio-sphere–Atmosphere Transfer Scheme) (Dickinson et al. 1992) wasincorporated into the model to perform the surface physics cal-culations. The mass flux scheme of Grell et al. (1994) wasimplemented for cumulus convection parametrization.

Figure 1 illustrates the domain and topography in our study.The domain is covered by dotted lines, which represent the long-itudes and latitudes included in the model’s domain, and containsmost of Asia and a portion of Eastern Europe. It should be pointedout that the model grid points are projected on a Lambert con-formal projection map, and that to display all model points on aconventional longitude/latitude grid map, certain extraneous

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longitude/latitude points which do not belong to the model’sdomain have to be included in the plot. Also shown in Fig. 1 is asub-region that encompasses the entire TP and is selected todemonstrate our results. Because the selected sub-region is far fromthe lateral boundary of the model, the simulation to be shown inthe subsequent sections is believed to be mostly the results of themodel internal physical processes and relevant local forcing. A60 km grid size and 14 levels with the model top at 80 hPa are used.The climate in the model’s domain, where the land surface typevaries from tropical rain forest to desert, is characterized byremarkable monsoon circulations, and the spatial pattern of theprecipitation is frequently enhanced by topographical forcing. Toevaluate the model’s performance in the domain, the RegCM2 wasfirst integrated for a 4-month period (June–September, 1994) usingthe TOGA analyses of European Centre for Medium-RangeWeather Forecasts (ECMWF) as the lateral boundary conditions.The results (not shown) indicate that the RegCM2 did fairly well inthe simulations of precipitation, ground temperature and monsooncirculations. Moreover, Kato et al. (2001) evaluated the perfor-mance of RegCM2 for the simulation of climate change in EastAsia caused by global warming, and indicated that the typicalprecipitation phenomena during the winter and summer monsoonswere well reproduced in the RegCM2.

The lateral boundary conditions used for our experiments arefrom a 130-year transient increasing CO2 run produced by theNCAR Climate System Model (CSM), in which atmospheric CO2

was increased at a rate of 1% y–1. The models included in theNCAR CSM are the NCAR Community Climate Model (CCM)(atmosphere model version CCM3.2), the NCAR Land SurfaceModel (version 1), the NCAR Sea Ice Model (version CSIM-3.5.3),and the NCAR global Ocean Model (version NCOM-1.1). Thevarious component models are connected by a flux coupler inwhich interfacial fluxes between the models are calculated and aredistributed to all component models while ensuring the conserva-tion of fluxed quantities. Meehl et al. (2000) indicated that thesimulated globally averaged surface air temperature increase nearthe time of CO2 doubling is about 1.43 �C, with an increase ofglobally averaged precipitation of 2%. In addition, the greatestsurface warming is found in the winter hemisphere at high lati-tudes, particularly in the Northern Hemisphere during December–February (DJF). As compared with other global coupled models,global warming due to increased CO2 is relatively low in the NCARCSM (Kattenberg et al. 1996).

Figure 2 shows the 12-month running means of monthly aver-aged surface air temperatures for the globe (thin solid line) and for

the area selected in our analysis (thick solid line). In Fig. 2, theyears when CO2 level was held at the present day value (355 ppm)and the years when doubling CO2 was achieved are highlighted.Over the analysis area the surface air temperature near the time ofCO2 doubling increases about 1.9 �C. Mean amplitude of inter-annual fluctuation (�0.4 �C) is larger than that in the global mean,however, and is far smaller than the warming induced by doublingCO2. In our study the CSM model results starting from years 10and 80 are selected as the initial conditions and boundary condi-tions for the control and 2·CO2 runs respectively. The lateral andsurface boundary conditions are supplied at 6-h intervals from therun of the NCAR-CSM with a horizontal resolution of T42. Bothruns have been integrated for three years and four months, and thefirst four months are neglected in the analysis to ensure that theclimatology obtained is in dynamical equilibrium between the lat-eral boundary forcing and the internal model physics and dy-namics. Moreover, to be consistent with the boundary conditions,the CO2 concentration used in the radiation transfer package wasset to 355 ppm in the control run and 710 ppm in the 2·CO2 run.Details of the parametrization for the CO2 absorber are given inKiehl and Briegleb (1991). For both simplicity and an attempt toinclude as much information as possible, the outputs are onlyaveraged into the winter half year (October to March) and thesummer half year (April to September). Compared with conven-tional means (e.g., JJA as summer and DJF as winter etc.), such achoice of analysis period is rather representative.

3 The enhanced climatic warming signal detectedfrom the experiments

Figure 3a–c shows the ground temperature simulatedfrom the control run (Fig. 3a) and the 2·CO2 run(Fig. 3b), and the difference between them (Fig. 3c) forthe winter half year. The ground temperature patterns(Fig. 3a, b) closely follow the topographic character-istics of the TP with cooler temperature at higher alti-tudes and strong temperature gradient corresponding tolarge elevation gradient. In comparison with the simu-lation from the CSM (not shown), the ground tem-perature produced by the RegCM2 shows a more

Fig. 1 Model domain andtopography (units are 100 m).Also shown is the area selectedfor analysis

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detailed structure. In Fig. 3c, it can be seen that in thewinter the ground temperature warming covers almostthe entire TP, and two regions with maximum groundtemperature increases can be observed in the eastern TPand along the southwestern and western slopes. There-fore these two regions with the strongest warming areselected, and labeled as region I and II, for detailedanalysis. In particular, region II covers the highestmountains, such as the Himalayas etc. Figure 4a–c is thesame as Fig. 3a–c but for the summer half year. In thesummer half year, the surface warming is reduced andmore evenly distributed in region I and, however, sub-stantially enhanced in region II. It is found that in regionI the ground warming in the winter half year is strongerthan that in the summer half year, and that in region IIthe warming difference between the seasons becomesopposite to that in region I, i.e., the warming is strong inthe summer half year and weak in the winter half year.This strong seasonality in the ground warming is con-sidered to be associated with the remarkable monsooncirculation around the TP and the surface characteristicsas well, and will be demonstrated shortly. In addition,another small region with large increase in the groundtemperature is found in the middle of northern slope inFig. 4c, but it will not be studied because of its muchsmaller area in comparison with region I and II. Fur-thermore the statistical significance of the ground tem-perature difference between two runs is tested (seeAppendix A), and the result indicates that the area–averaged ground temperature difference between tworuns is statistically significant and conclusive at the 95%significance level even though our RegCM runs arerelatively short.

In order to provide a planetary scale background forthe ground temperature changes shown in Figs. 3a–cand 4a–c, as well as to obtain clues on the changes in themonsoon circulations resulting from the doubling of

Fig. 3a–c Simulated ground temperature for a the control run,b the 2·CO2 run and c the difference between them for the winterhalf year (units: �K). Shaded is topography

Fig. 2 NCAR CSM simulated12-month running means ofmonthly averaged surface airtemperatures for the globe (thinsolid line) and for the areaselected in the analysis (thicksolid line) as a function of modelyears. Shaded are the yearswhen CO2 level was held at thepresent day value (355 ppm)and the years when doublingCO2 was achieved

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CO2, June–August (JJA) and December–February(DJF) mean 200 hPa stream lines from the control run,2·CO2 run and the difference between them are illu-strated for the whole model domain in Figs. 5a–c and6a–c. The most striking features associated with summermonsoon in Fig. 5a (control run) are the huge anti-cyclonic circulation (the Tibetan High) over southernAsia centered at the TP and the associated easterly jet tothe south of the TP. Compared with observation (notshown), the simulated center of the Tibetan High shiftswestward about 4� longitudes. In addition, strong wes-terlies are dominant in the middle and high latitudes anda deep trough is seen close to the eastern coast of Asia.In the 2·CO2 run the Tibetan High is intensified withenhanced wind speed and its center moves north-eastward to central Asia (Fig. 5b). In Fig. 5c a strongintensification of anti-cyclonic circulation is found alonga wide latitude band centered at 30�N with two maximaover central Asia and China. In addition, enhancedcyclonic circulations are seen over the high latitudes andthe sub-tropical regions, however the enhancement inthe high latitudes is much stronger. This change in thecirculation is closely related to warmer air mass over theregions from central Asia to the TP (not shown), which

results in the intensified temperature gradients in boththe north–south and east–west directions. In DJF mean,westerly is dominating over the whole model’s region forboth the control and 2·CO2 runs (Fig. 6a, b). As shownin Fig. 6c, the westerly is enhanced in South Asia for the2·CO2 run, and the intensified southerly is overMongolia and flanked by an enhanced cyclone to thewest and an anti-cyclone to the east. Based on Websterand Yang’s broad monsoon index (Webster and Yang1992), which is the magnitude of the vertical shear zonalwind averaged in the region (0�–20�N; 40�E–110�E) andhas a clear relationship with the strength of the heatingover South Asia, in JJA the enhanced easterlies at upperlevel over South Asia, together with the enhanced wes-terlies at lower level (not shown) give an indication of astronger summer monsoon in the 2·CO2 run, although asmall portion of the region defined by Webster andYang (1992) is included in the model’s domain. On theother hand, in DJF the winter monsoon seems tobecome weaker in terms of the sea level pressure (notshown), for example, the strength of the Mongolia hightends to decline in the 2·CO2 run. However it should bepointed out that our model’s domain is too small tocover the whole monsoon regions, thus further

Fig. 5a–c JJA mean 200 hPa stream lines for a the control run,b the 2·CO2 run and c the differenceFig. 4a–c The same as Fig. 3, but for the summer half year

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clarification needs to be made by analyzing simulationswith a larger domain.

The ground temperature differences between the2·CO2 and control runs in region I are plotted inFig. 7a, b as functions of elevation over the model gridpoints for the summer and winter half years respec-tively. In Fig. 7a, b, topographical elevation is dividedinto 10 categories with a 500-m interval, i.e., 0.5–1.0 km, 1.0–1.5 km,…,5.0–5.5 km, and the value oftemperature difference is obtained by averaging resultsover all grid points in each elevation category. It isnoticed that there is no grid point fitting in the cate-gory of 0.5–1.0 km. In the winter half year (Fig. 7a) theground warming is about 1.0 to 1.1�K at the elevationsbelow 3.0 km and shows a rather uniform distributionwith elevation. The most remarkable feature is a ten-dency of ground temperature warming increasing withelevation above 3.0 km, and the maximum temperatureincrease is 2.2�K at the elevations of 4.5 to 5.5 km.This elevation dependency of surface warming in thewinter half year is consistent with Liu and Chen’sobservational study (2000). For the summer half year(Fig. 7b), the surface warming is approximately equalamong the elevation categories, and the ground

temperature has increased by 2�K with a deviationabout ±0.1�K. There is no elevation dependency ofsurface warming, also in agreement with Liu and Chen(2000). Considering that the most meteorological sta-tions used in Liu and Chen (2000) are located in theeastern TP, our simulated surface warming is quitesuccessful in terms of being consistent with theobservations.

Figure 8a, b is the same as Fig. 7a, b but for regionII. In the winter half year the strongest warming is about2.5�K at the elevations of 4.5–5.0 km and the weakestwarming 0.5�K below 2.5 km (Fig. 8a). An elevationdependency of surface warming is evident although thewarming at the highest elevations (5.0–5.5 km) is slightlyweaker than that at the elevations of 4.5–5.0 km. In thesummer half year (Fig. 8b), the most outstandingfeature is that the surface warming is substantiallyenhanced with a maximum of 5.2�K at the elevationsof 4.0–4.5 km, and a minimum of 1.4�K around 2.0–2.5 km. At the elevations between 2.0 km and 4.5 km,the surface warming intensifies from 1.5�K to 5.2�K withelevation increasing and further declines to 3.8�K at theelevations of 5.0–5.5 km. It should be pointed out thatbecause there are few meteorological stations andno continuous records were collected in region II, it isdifficult to verify our simulations with observations inthat region.

Fig. 7a, b The ground temperature from the 2·CO2 run, thecontrol run and the difference between them as functions ofelevation in region I for a the winter and b the summer half years

Fig. 6a–c The same as Fig. 5, but for DJF mean

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4 The physical processes responsible for the surfacewarming in the TP

4.1 Region I

4.1.1 Surface energy budget

The ground temperature is determined by surface energyexchanges and governed by the surface energy budgetequation, which can be written as

C@Tg

@t¼ Sg þ F #IR � F "IR � SHF � LHF � Sm

where C is the total heat capacity of ground, Tg isground temperature, Sg is surface absorbed solar flux,FIR

fl is downward long-wave flux reaching surface, FIR›

is infrared radiation flux emitted from ground, SHF andLHF represent atmospheric sensible and latent heatfluxes from ground to atmosphere respectively, and Sm isthe energy flux associated with snow melt in the presenceof snow. In order to demonstrate the roles ofvarious surface energy exchanges in the local groundtemperature response, an analysis of the surface energybalance in region I and region II (see Sect. 4.2) has beenmade.

Figure 9a and c shows the differences between the2·CO2 and control run for Sg, FIR

fl, FIR›, SHF and

LHF, which are displayed as functions of elevation inregion I for the winter and summer half years. In addi-tion, the differences in combinations of (Sg + FIR

fl),(SHF + LHF) and (Sg + FIR

fl) – (SHF + LHF) arealso plotted in Fig. 9b and d for the purpose of inter-preting the results more easily. Hereafter the difference

Fig. 9a–d The surface fluxdifferences between 2·CO2 andcontrol run as functions ofelevation in region I. Shown aredifferences in a the surfaceabsorbed solar flux (DSg), thedownward long-wave flux at thesurface (DFIR

fl), the infraredradiation flux emitted from thesurface (DFIR

›), the surfacesensible heating flux (DSHF)and latent heating flux (DLHF),and b the combinations ofD(Sg + FIR

fl), D(SHF + LHF)and D[(Sg + FIR

fl) – (SHF +LHF)] for the winter as well asc, d for the summer half years

Fig. 8a, b The same as Fig. 7, but for region II

Chen et al.: Enhanced climatic warming in the Tibetan Plateau 407

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between two runs is denoted by D, for instance, DSg

represents difference in Sg (that of the 2·CO2 run minusthat of the control run) and so forth.

During the winter half year (Fig. 9a), below theelevations of 3.0–3.5 km DSg is negative and its mag-nitude declines as elevation increasing, however DFIR

fl

is positive but its magnitude decreases as well showinga characteristic compensating mechanism. At the ele-vations above 3.0–3.5 km both DSg and DFIR

fl arepositive, and their magnitudes show a slight increase inDSg and a decrease in DFIR

fl as elevation increases. Thecharacteristics of DSg and DFIR

fl are closely associatedwith the changes in cloud effects related to the doublingof CO2, and the details will be presented shortly. FromFig. 9b it can be seen that D(Sg + FIR

fl) > 0 is shownat all elevations, i.e., (Sg + FIR

fl) in the 2·CO2 run isenhanced, and the magnitude becomes enlarged withincreasing elevation indicating a strong elevation de-pendency. (Sg + FIR

fl) acts to warm the surface,therefore the enhanced (Sg + FIR

fl) in the 2·CO2 run ismost responsible for the surface warming in the TP andits elevation dependency as well. Below the elevationsof 3.0–3.5 km, DSHF is negative and its magnitudedeclines with elevation. Above 3.5–4.0 km DSHF turnspositive and the magnitude shows a steady increasewith elevation. At all elevations DLHF is positive andrelatively uniform. Except at the elevations below3.5 km where negative DSHF exits, both DSHF andDLHF act to cool the surface. Also shown in Fig. 9b,D(SHF + LHF) offsets some of D(Sg + FIR

fl). Finally,as a result of the greater ground temperature, thesurface emission of infrared radiation (FIR

›) enhancesat all elevations to make the surface energy budgetbalance.

For the summer half year (Fig. 9c), at all elevationsboth DSg and DFIR

fl are positive indicating enhancedSg and FIR

fl in the 2·CO2 run. Moreover the magni-tudes of DSg and DFIR

fl show a feature of ‘‘out-phase’’with respect to elevation in the sense that an en-hancement in one flux is corresponding to a reductionin the other flux and vice versa. As shown in Fig. 9d,since the larger magnitude is at lower elevations andthe smaller one at higher elevations, there is a reverseelevation dependency shown in D(Sg + FIR

fl). Al-though D(Sg + FIR

fl) > 0 is a primary cause of groundwarming in the 2·CO2 run, unlike the winter half year,it does not show a controlling influence on the eleva-tion dependency of ground warming. In Fig. 9cDSHF > 0 exists at all elevations and the largestmagnitude is below 3.0–3.5 km elevations. In addition,DLHF < 0 is shown at the elevations below 3.0 kmand it turns into positive values above. As seen inFig. 9d, the net effect of D(SHF + LHF) acts to coolthe surface because of its positive value, and offsets aportion of the enhanced (Sg + FIR

fl). It is that thecombination of D(Sg + FIR

fl) – D(SHF + LHF)determines the distribution of surface warming withelevation, which is balanced by the enhanced FIR

resulting from warmer ground temperature.

4.1.2 Factors responsible for the change in the surfaceenergy exchange

From an energetic point of view, to make the surfaceenergy budget balance, changes in the surface radiativeheat fluxes, which are due to enhanced greenhouse ef-fects resulting from a doubling of CO2, must be com-pensated by changes in other surface energy fluxes. Thisenergy balance is achieved, from a dynamical point ofview, by adjusting the atmosphere to a new structure tobe compatible with the new energetic constraintsthrough the dynamics and thermodynamics operatingwithin the atmosphere. Among various surface energyfluxes, the enhanced (Sg + FIR

fl) is the primary cause ofsurface warming in the TP, and is determined by manyfactors including the surface states, such as surfacealbedo which most depends on the particular feature ofthe surface, e.g., the presence of snow and vegetationetc., the temperature distribution and trace gasesthroughout the atmosphere, and especially the dis-tribution and nature of cloudiness. Moreover, FIR

›,SHF and LHF act to counter the enhanced (Sg + FIR

fl).Amongst them FIR

› depends only on the state of thesurface, and SHF and LHF depend both on the surfaceand on the atmospheric structure near the surface.

In region I there is little snow for both winter andsummer half years, and the impact of snow-albedofeedback on DSg is not significant. The cloud effectsrelated to the doubling of CO2 are essential to thecharacteristics of D(Sg + FIR

fl). Figure 10a, b illustratesthe cloud amount (cloud fraction) difference between the2·CO2 and control run in region I for the cool (Fig. 10a)and warm (Fig. 10b) seasons, in which the differencesare plotted as functions of both elevation and height(pressure). In the winter half year (Fig. 10a) a significantincrease in the cloud amount for the 2·CO2 run can befound in the elevations below 3.0 km under 400 hPa,and a decrease above 3.5 km. The enhanced cloudamount, in particular, in middle and low levels, exertstwo compensating effects on the radiation field. On onehand, increased cloudiness in lower elevations reflects asignificant portion of the incoming solar flux, whichleads to a decrease in Sg; on the other hand, it trapsmore outgoing thermal infrared fluxes emitted from theatmosphere below the clouds and from the surface,which results in an increase in FIR

fl. At elevations above3.5 km, the cloud amount is reduced and the reductionleads to an increase in Sg. Because of smaller cloudamount, FIR

fl shows a relatively uniform increase atelevations above 3.5 km, which is mainly due to dou-bling CO2. Figure 11a, b shows the precipitation of re-gion I for the control and 2·CO2 runs together withtheir difference in the winter and summer half years re-spectively, in which the precipitation and differences areplotted as functions of elevation. In the winter half year(Fig. 11a), in association with the enhanced cloudamount at lower elevations, the precipitation increasesat the same locations with a maximum around 2.0–2.5 km, and with elevation becoming higher, the

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precipitation increases tend to be weaker. Along with theenhanced precipitation LHF increases but SHF de-creases, and the net effect of D(SHF + LHF) is to act tocool the surface as shown in Fig. 9a, b. In addition,there is only small snow cover found at higher elevationsin region I, and therefore the effects of the snow coverdifferences between two runs can be neglected comparedwith those in region II (see Fig. 12a, b). In the summerhalf year (Fig. 10b), the cloud amount reduces at allelevations with more reduction at lower elevations. Be-cause of reduced cloud amount, Sg enhances at all ele-vations with a stronger enhancement at lower locations,and the increase in FIR

fl shows a rather uniform dis-tribution with elevation. Associated with the decreasesin cloud amount, precipitation (Fig. 11b) declines at allelevations and the largest declines occur at lower loca-tions. As a result of the reduced precipitation, LHFdecreases but SHF increases, D(SHF + LHF) is positiveand acts to cool the surface.

4.2 Region II

4.2.1 Surface energy budget

Figure 12a, d is the same as Fig. 9a, d but for region II.In the winter half year (Fig. 12a), DSg is negative in the

elevation range of 1.0 km to 3.0 km and the magnitudebecomes smaller as elevation increases. As the topo-graphy reaches up to more than 3.0 km DSg turns po-sitive and its maximum magnitude can be found aroundthe elevations of 4.0–5.0 km indicating an enhancementin solar radiation absorbed at the surface for the 2·CO2

run. On the other hand, positive DFIRfl exists at all ele-

vations, and a maximum shows at lower elevations and aminimum at higher elevations. Although DSg and DFIR

fl

exhibit a compensating characteristic similar to that inregion I (see Fig. 9a), unlike in region I, the net solarradiation absorbed at the surface D(Sg + FIR

fl) does notdisplay any tendency of an elevation dependency (seeFig. 12b). Moreover DLHF is positive at all elevationsindicating enhanced LHF in the 2·CO2 run, and a sig-nificant increase in LHF can be found below 3.0–3.5 km(up to 10 w/m2) compared with that in the higher ele-vations. However, below 3.0–3.5 km DSHF is negativeand SHF exhibits a maximum decrease in the 2·CO2 runat the elevations where the largest increase in LHFshows, although a slight increase at the lowest location.The combined effect of DLHF and DSHF (Fig. 12b)counteracts the enhanced (Sg + FIR

fl) by acting to coolthe surface at all elevations. In consequence, the com-bination of D(Sg + FIR

fl) – D(LHF + SHF) exhibitsa relatively weak elevation dependency, and is balancedby the enhanced surface emission of infrared radiation(FIR

›).

Fig. 10a, b The difference of cloud amount (cloud fraction) between2·CO2 and control run as a function of elevation and pressure inregion I for a the winter and b the summer years (units: %)

Fig. 11a, b The precipitation from the 2·CO2 run, the control runand the difference between them as functions of elevation in regionI for a the winter and b the summer half years

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In the summer half year (Fig. 12c), the most out-standing feature in region II is that Sg significantly en-hances above 3.0 km with a maximum at 4.0–4.5 kmaltitudes in the 2·CO2 run, and this enhancement isclosely associated with the snow-albedo feedback me-chanism (see next section). In addition, there is a smalldecrease in Sg found below 3.0 km. For the 2·CO2 run,FIR

fl increases at all elevations and the increase alsoamplifies at the elevations above 3.0 km. It can be seenthat the enhanced (Sg + FIR

fl) (Fig. 12d) is mostresponsible for the strong enhancement of ground tem-perature increase at higher elevations (see Fig. 8b).Moreover, LHF intensifies at all elevations with amaximum at the elevation of 4.0–4.5 km, and SHFshows a decline at elevations below 3.0 km and an in-crease above with the largest intensification at the ele-vation of 4.0–4.5 km. D(SHF + LHF) (Fig. 12d) acts tocool the surface and partially offsets the enhanced (Sg +FIR

fl). Finally, the net increase in (Sg + FIRfl) – (SHF +

LHF) is compensated by the increase in the FIR›.

In summary, the surface energy exchange displaysdifferent characteristics for different locations and sea-sons, although the ground temperatures in regions I andII all show warming for both the winter and summerhalf years. In addition, the types of surface energy ex-change responsible for the elevation dependency ofground temperature, if there is one, varies dependingboth on the region and on the season.

4.2.2 Factors responsible for the change in the surfaceenergy exchange

Figure 13a, b is the same as Fig. 10a, b but for region II.In the winter half year (Fig. 13a) the cloud amount at

middle and low levels increases at the elevation range of1.0–3.0 km and decreases at elevations above 3.0 km.The largest decrease is found at 4.5–5.0 km or at500 hPa level which is a relatively low level consideringthe topographic height. Related to the increased cloudamount, stronger intensification in the precipitation (notshown) is seen at lower elevations, and weaker and nointensification at higher attitudes. The role played by theincreased cloud amount in the surface energy budget isvery similar to that in region I. In addition, there is apeak in DSg at the elevation range of 4.0–5.0 km(Fig. 12a), which is also associated with reduced snowcover there besides the largest decrease in the cloudmount. Figure 14a, b depicts the snow cover in region IIfor the control and 2·CO2 runs as well as their differencein the winter and summer half years respectively. Thesnow cover in Fig. 14a, b is measured in terms ofequivalent liquid water contents, which is updated in theRegCM2 through a prognostic equation involving thesnow precipitation rate, the rates of sublimation andsnow melt. In the winter half year (Fig. 14a) a largedepletion of snow cover is found at the elevations above3.5 km with a maximum of about 820 mm in equivalentliquid water at an elevation of 3.5–4.5 km. Due to thisdepletion of snow cover the surface albedo reduces, andas a result, together with decreased cloud amounts, Sg

enhances as shown in Fig. 12a. In the summer half year(Fig. 13b) a mild decrease in the low-level cloud amountcan be seen at the elevations of 2.0–3.5 km. Above3.0 km the cloudiness increases with a maximum at thehighest elevation. Most significantly, the snow coverdramatically reduces in an elevation range between 3.0and 5.0 km with a largest value about 1200 mm inequivalent liquid water (Fig. 14b). The decreased surface

Fig. 12a–d The same as Fig. 9,but for region II

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albedo resulting from this reduction in the snow coverleads to the strongest enhancement in Sg at the sameelevations, which is a main feature in Fig. 12c. Moreoverthe large increase in the cloud amount shown in Fig. 13bat the highest attitudes weakens the increase in DSg.

Summary and discussion

The NCAR RegCM2 with time-dependent lateral me-teorological fields provided by a 130-year transient in-creasing CO2 simulation of the NCAR CSM has beenused to investigate the mechanism of surface warmingover the TP. From our model results, when CO2 isdoubled, a strong ground warming occurs in the TP, andthe two regions with the largest warming are in theeastern TP (region I) and along the southwestern andwestern slopes (region II). Moreover, in region I theground warming in the winter half year is stronger thanthat in the summer half year, but in region II thewarming difference between the seasons becomes oppo-site to that in region I, i.e., the warming is strong in thesummer half year and weak in the winter half year.There are indications that the summer monsoonenhances but the winter monsoon weakens when CO2

is doubled. A strong elevation dependency of groundwarming is found in region I for the winter half year,

and in region II for both winter and summer half yearsat the elevations below 5 km. The simulated character-istics of ground warming in the TP are consistent withthe observations. In region I, when CO2 is doubled, thecloud amount increases at lower elevations and de-creases at higher elevation for the winter half year. Inconsequence, at lower elevations the short wave solarradiation absorbed at the surface declines, and thedownward long wave flux reaching the surface enhances;on the other hand, at higher elevations the solar radia-tion flux increases and the infrared radiation flux showsa more uniform increase. The net effect of both radiationfluxes results in an enhanced surface warming at higherelevations, which is the primary cause of the elevationdependency in the surface warming. In the summer halfyear the clouds reduce in region I for all elevations, andthere is no elevation dependency detected in the groundwarming. Moreover, there is little snow existing in re-gion I for both summer and winter half years, and theinfluence of snow-albedo feedback is negligible. In re-gion II, although the changes in the cloud amount bear aresemblance to those in region I, the most significantfactor affecting the surface energy budget is the deple-tion of the snow cover at higher elevations, which leadsto a reduction of the surface albedo and, as a result, toan enhancement in the solar radiation absorbed in thesurface. The snow-albedo feedback mechanism is the

Fig. 13a, b The same as Fig. 10, but for region II

Fig. 14a, b The snow cover measured in terms of equivalent liquidwater from the 2·CO2 run, the control run and the differencebetween them as functions of elevation in region II for a the winterand b the summer half years

Chen et al.: Enhanced climatic warming in the Tibetan Plateau 411

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most essential cause of the elevation dependency in thesurface warming for region II.

Both Giorgi et al. (1997) and Fyfe et al. (1999) haveshown that the snow-albedo feedback mechanism playsa major role in elevation dependency of the surface cli-mate change signal in the Alps and Rocky mountainsbased on the results from two models with quite differentresolutions. In particular, the model used by Fyfe et al.(1999) has a relatively coarse T32 resolution, but as theyclaimed, the topography of the Rockies in the modelreaches high enough over a large enough area to be ableto support appreciable winter and spring snow cover. Inboth studies, reduced snow cover in high elevation isessential to the elevation effect. Compared with the Alpsand Rocky mountain complexes, the TP has much largerarea and higher elevations as well as far more terrestrialregimes. In the NCAR CSM transient increasing CO2

run (having a T42 resolution), used as the lateral forcingfor the RegCM2 in our study, there is no clear elevationdependency detected over the TP (not shown), althoughsnow depletion occurs when the CO2 concentrationreaches doubling level, suggesting other factors may playa role in the topography dependency in the TP. Ourmodel results from the RegCM2 indicate that, besidesthe snow-albedo feedback, the enhanced cloud amountsand precipitation are also responsible for the elevationdependency of surface warming in the TP, particularly inthe eastern TP. The topography forced cloudiness andprecipitation are certainly underestimated in the NCARCSM because of a much smoother topographical re-presentation for the TP.

Moreover, during the summer half year, in additionto precipitation induced by low level convergence asso-ciated with the monsoon flows and upward motionsdynamically forced by topography, at high elevations,surface heating also destabilizes the overlying atmo-sphere and enhances convective precipitation. Thus thelocal response to global warming over the TP is muchmore complicated than that in winter half year. In orderto get more reliable results, an accurate simulation ofsummer monsoon is essential for either the GCM or theregional model.

Finally, it should be pointed out that our results hereshould not be viewed as a quantitative estimation ofclimate change or climate predication because they areonly based on sensitivity of climate to atmospheric CO2

concentration. Our purpose is only to suggest a physicalinterpretation for the elevation effect on climaticwarming in the model, which has an observationalcounterpart. Many more numerical experiments need tobe done in order to get results more applicable to thereal atmosphere.

Acknowledgements The authors would like to thank Drs. J. Qianand X. Bi for providing the model code and data. They also wish toexpress appreciations to Dr. C. Liu at NCAR and Mr. C. Hung atUCLA for their help in processing the NCAR CSM outputs. Theauthors are grateful to two anonymous reviewers for their con-structive comments. The first author thanks Prof. Zhisheng An forhis hospitality and valuable discussions. The first two authors

acknowledge the support from NASA/Office of Earth Science; andthe first and last authors acknowledge the support from theNKBRSF (G1999043401), NSFC (40121303, 40023003) and CASPresident Fund.

Appendix A

Testing the difference between means

To test statistical significance of the simulated ground temperaturedifference between the control and 2·CO2 runs, a simple approachis used (e.g. Freund and Walpole 1987). Let {x1, x2,…, xn} and {y1,y2,…, ym} be two independent random samples with size n and mrespectively. Compute their means and variances as

�xx ¼ 1n

Pni¼1 xi �yy ¼ 1

m

Pmi¼1 yi and rx ¼ 1

n

Pni¼1 ðxi � �xxÞ2ry ¼ 1

m

Pmi¼1

ðyi � �yyÞ. Suppose we want to test the null hypothesis: H0 : �xx� �yy ¼ 0

against the alternative H1 : �xx� �yy 6¼ 0. The V defined byV ¼ �xx��yyffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi

rx=nþry=mp has a than 1.96, the null hypothesis can be rejected

at the 95% confidence level, in other words, the difference between�xx and �yy is significant at the 95% significance level. The means andvariances of averaged ground temperature for the area in Fig. 3 arecalculated with a sample size of 1095 (last three years). They are278.9 �K (mean) and 59.9 (�K)2 (variance) for the control run, and280.9 �K and 66.9 (�K)2 for the 2·CO2 run. Then the V=5.88 >1.96 is obtained. Therefore the ground temperature differencebetween two runs is statistically significant and conclusive at the95% significance level.

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