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人类活动对热河(Rur)流域降雨-径流关系的影响

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人民黄河 2005年第11期27卷 75-75页

作者： DeLaat P.j.M calderon Hijuma M.P 图敏联合国教科文组织水教育学院

热河是默兹河的一条支流，占默兹河流域总面积的10％。热河流域几乎全部位于德国境内。20世纪下半叶热河（Rur）流域受到了人类活动的严重影响：流域内建成9座大坝，总库容约为3亿m^3；自18世纪就已开始的矿业活动，20世纪50年代达到了... 详细信息

热河是默兹河的一条支流，占默兹河流域总面积的10％。热河流域几乎全部位于德国境内。20世纪下半叶热河（Rur）流域受到了人类活动的严重影响：流域内建成9座大坝，总库容约为3亿m^3；自18世纪就已开始的矿业活动，20世纪50年代达到了高峰，年开采量从1000万t猛增至1亿t。矿业公司把印登煤矿和部分海姆巴赫煤矿的水排入热河，而海姆巴赫大部分水则排入鄂伏特河，鄂伏特河是流入热河东部的一条支流。热河峡谷断层系统的地下水受到断层水力学特征的强烈影响。

关键词：人类活动降雨-径流关系河流域热河 20世纪50年代 20世纪下半叶矿业活动 18世纪矿业公司力学特征

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玻利维亚过去30年土地覆被变化

AMBIO－人类环境杂志 2007年第B11期36卷 565-571页

作者： Timothy j.Killeen Veronica calderon Liliana Soria Belem Quezada Marc K.Steininger Grady Harper Luis A.Solórzano Compton j.Tucker 田玉军马国霞生物多样性应用科学中心(CABS) 生物多样性应用科学中心摩尔基金会

利用5个时段的Landsat图像对玻利维亚东部低地所有山区树木生长线(大约3000m)以下的陆地景观的土地覆被变化进行研究,包括湿润森林、泛滥森林、季节性旱地林、云雾林及灌丛地和草地。2004年玻利维亚东部森林砍伐面积为45 411km^2,大约... 详细信息

利用5个时段的Landsat图像对玻利维亚东部低地所有山区树木生长线(大约3000m)以下的陆地景观的土地覆被变化进行研究,包括湿润森林、泛滥森林、季节性旱地林、云雾林及灌丛地和草地。2004年玻利维亚东部森林砍伐面积为45 411km^2,大约占原始森林覆盖面积的9%,另外有9042km^2的灌丛、热带稀树草原生境转为它用,占土地覆被总历史变化的17%。玻利维亚土地覆被变化速度从20世纪60年代的400km^2/a上升到2001～2004年间的大约2900km^2/a。本研究为玻利维亚提供监测未来土地覆被变化的可靠空间数据,这是建议的补偿机制,即补偿通过减少森林砍伐来降低碳排放的国家的前提。对比最近和以前各时期的土地覆被变化,发现20世纪90年代颁布的有关森林保护政策并没有对降低森林砍伐起明显的作用,在有些保护区内森林砍伐事实上增加了。全国范围内土地覆被变化的速度继续呈线性上升趋势,但是在圣克鲁斯区上升速度更快,这与该地区动农业机械化和养牛业的扩展有关。

关键词：土地覆被变化玻利维亚森林覆盖面积森林砍伐热带稀树草原上升速度补偿机制上升趋势

Calderón–Zygmund Operators in the Bessel Setting for All Possible Type Indices

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Acta Mathematica Sinica,English Series 2014年第4期30卷 637-648页

作者： Alejandro j.CASTRO Tomasz Z.SZAREK Departamento de Análisis Matemático Universidad de La LagunaCampus de AnchietaAvda.Astrofísico Francisco Sánchezs/n38271 La Laguna (Sta.Cruz de Tenerife)Spain Instytut Matematyczny Polska Akademia NaukSniadeckich 800–956 WarszawaPoland

We show that many harmonic analysis operators in the Bessel setting, including maximal operators, Littlewood-PMey-Stein type square functions, multipliers of Laplace or Laplace-Stieltjes transform type and Riesz transforms are, or can be viewed as, CalderSn-Zygmund operators for all possible values of type parameter λ, in this context. This extends results existing in the literature, but being justified only for a restricted range of λ.

关键词： Bessel operator Bessel semigroup maximal operator square function multiplier Riesztransform Calder6n-Zygmund operator

Measurements of dihadron correlations relative to the event plane in Au+Au collisions at√^(S)NN=200 GeV

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Chinese Physics C 2021年第4期45卷 198-241页

作者： H.Agakishiev M.M.Aggarwal Z.Ahammed A.V.Alakhverdyants I.Alekseev j.Alford B.D.Anderson C.D.Anson D.Arkhipkin G.S.Averichev j.Balewski D.R.Beavis N.K.Behera R.Bellwied M.j.Betancourt R.R.Betts A.Bhasin A.K.Bhat H.Bichsel j.Bieleik j.Bielcikova B.Biritz L.C.Bland W.Borowski j.Bouchet E.Braidot A.V.Brandin A.Bridgeman S.G.Brovko E.Bruna S.Bueltmann I.Bunzarov T.P.Burton X.Z.Cai H.Caines M.calderon de la Barca Sanchez D.Cebra R.Cendejas M.C.Cervantes Z.Chajecki P.Chaloupka S.Chattopadhyay H.F.Chen j.H.Chen j.Y.Chen L.Chen j.Cheng M.Cherney A.Chikanian K.E.Choi W.Christie P.Chung M.j.M.Codrington R.Corliss j.G.Cramer H.j.Crawford S.Dash A.Davila Leyva L.C.De Silvat R.R.Debbe T.G.Dedovich A.A.Derevschikov R.Derradi de Souza L.Didenko P.Djawotho S.M.Dogra X.Dong j.L.Drachenberg j.E.Draper j.C.Dunlop L.G Efimov M.Elnim j.Engelage G Eppley M.Estienne L.Eun O.Evdokimov R.Fatemi j.Fedorisin A.Feng R.G.Fersch P.Filip E.Finch V.Fine Y.Fisyak C.A.Gagliardi D.R.Gangadharan A.Geromitsos F.Geurts P.Ghosh Y.N.Gorbunov A.Gordon O.Grebenyuk D.Grosnick S.M.Guertin A.Gupta W.Guryn B.Haag O.Hajkova A.Hamed L-X.Han j.W.Harris j.P.Hays-Wehle M.Heinz S.Heppelmann A.Hirsch E.Hjort G.W.Hoffmann D.j.Hofiman B.Huang H.Z.Huang T.j.Humanic L.Huo G.Igo P.jacobs W.W.jacobs C.jena F.jin j.joseph E.G.judd S.Kabana K.Kang j.Kapitan K.Kauder H.Ke D.Keane A.Kechechyan D.Kettler D.P.Kikola j.Kiryluk A.Kisiel V.Kizka A.G.Knospe D.D.Koetke T.Kollegger j.Konzer I.Koralt L.Koroleva W.Korsch L.Kotchenda V.Kouchpil P.Kravtsov K.Krueger M.Krus L.Kumar P.Kurnadi M.A.C.Lamont j.M.Landgraf S.LaPointe j.Lauret A.Lebedev R.Lednicky j.H.Lee W.Leight M.j.LeVine C.Lil L.Li N.Li W.Li X.Li X.Li Y.Li Z.M.Li M.A.Lisa F.Liu H.Liu j.Liu T.Ljubicic W.j.Llope R.S.Longacre W.A.Love Y.Lu E.V.Lukashov X.Luo G.L.Ma Y.G.Mai D.P.Mahapatra R.Majka O.I.Mall L.K.Mangotra R.Manweiler S.Margetis C.Markert H.Masui H.S.Matis Yu.A.Matulenko D.MeDonald T.S.McShane A.Meschanin R.Milner N.G.Minaev S.Mioduszewski A.Mischke M.K.Mitrovski B.Mohanty M.M.Mondal B.Morozov D.A.Morozov M.G.Munhoz M Argonne National Laboratory Argonnellinois 60439USA Brookhaven National Laboratory UptonNew York 11973USA University of Califomia BerkeleyCaliformnia 94720USA University of California DavisCalifornia 95616USA University of Califormnia Los AngelesCalifomia 90095USA Universidade Estadual de Campinas Sao PauloBrazil University of Illinois at Chicago ChicagoIlinois 60607USA Creighton University OmahaNebraska 68178USA Czech Technical University in Prague FNSPEPrague11519Czech Republic Nuclear Physics Institute AS CR 25068 Rez/PragueCzech Republic University of Frankfurt FrankfurtGermany Institute of Physics Bhubaneswar 751005India Indian Institute of Technology MumbaiIndia Indiana University BloomingtonIndiana 47408USA Alikhanov Instiute for Theoretical and Experimental Physics MoscowRussia University of jammu Jammu 180001India joint Institute for Nuclear Research Dubna141980Russia Kent State University KentOhio 44242USA University of Kentucky LexingtonKentucky40506-0055USA Institute of Modern Physics LanzhouChina Lawrence Berkeley National Laboratory BerkeleyCalifornia 94720USA Massachusetts Institute of Technology CambridgeMA 02139-4307USA Mx-Planck-Institut fir Physik MunichGermany Michigan State University East LansingMichigan 48824USA Moscow Engineering Physics Institute Moscow Russia NIKHEF and Utrecht University AmsterdamThe Netherlands Ohio State University ColumbusOhio 43210USA Old Dominion University NorfolkVA23529USA Panjab University Chandigarh 160014India PennsyIvania State University University ParkPennsylvania 16802USA Institute of High Energy Physics ProtvinoRussia Purdue University West LafayetteIndiana 47907USA Pusan National University PusanRepublic of Korea University of Rajasthan Jaipur 302004India Rice University HoustonTexas 77251USA Universidade de Sao Paulo Sao PauloBrazil University of Science&Technology of China Hefei 230026.China Shandong University JinanShandong 250100China Shanghai Institute of Applied Physics Shanghai 201800Chi

Dihadron azimuthal correlations containing a high transverse momentum(pr)trigger particle are sensit-ive to the properties of the nuclear medium created at RHIC through the strong interactions occurring between the traversing parton and the medium,*** measurements revealed a strong modification to di-hadron azimuthal correlations in Au+Au collisions with respect to ptp and d+Au *** modification in-creases with the collision centrality,suggesting a path-length or energy density dependence to the je-quenching *** paper reports STAR measurements of dihadron azimuthal correlations in mid-central(20%-60%)Au+Au collisions at√^(S)NN=200 GeV as a function of the trigger particle's azimuthal angle relative to the event plane,Ф_(s)=|Ф_(t)-ψ_(Ep)|.The azimuthal correlation is studied as a function of both the trigger and associated particle *** subtractions of the combinatorial background and anisotropic flow,assuming Zero Yield At Minimum(ZYAM),are *** correlation results are first discussed with subtraction of the even harmonic(elliptic and quadrangu-lar)flow *** away-side correlation is strongly modifed,and the modification varies withФ_(s),with a double-peak structure for out-of-plane trigger *** near-side ridge(long range pseudo-rapidity△_(η)correla-tion)appears to drop with increasingФ_(s)while the jet-like component remains approximately *** correla-tion functions are further studied with the subtraction of odd harmonic triangular flow background arising from *** is found that the triangular flow,while responsible for the majority of the amplitudes,is not sufficient to explain theφs-dependence of the ridge or the away-side double-peak *** dropping ridge withФ_(s)could be attributed to aФ_(s)-dependent lliptie anisotropy;however,the physics mechanism of the ridge remains an open *** with aФ_(s)-dependent elliptic flow,the away-side correlation structure

关键词： relativistic heavy ion collisions dihadron correlations jet-medium interactions anisotropic flow background event plane

滋生真菌的蒸汽压片玉米对肉牛瘤胃和总消化道消化的影响

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饲料博览 2012年第3期22卷 53-53页

作者： Alvareza E Barajasb R calderon F Montano M Salinas-Chavira j Zinn R A 不详

选用4头荷斯坦奶牛(407±4 kg)采用4×4拉丁方试验设计,进行瘤胃和十二指肠近端瘘管试验。处理组应用滋生真菌的蒸汽压缩玉米755 ***-1分别取代空白组150、300和450 ***-1的片状玉米。对照组酵母菌和霉菌的平均数量分别为2.9×102和1.2... 详细信息

选用4头荷斯坦奶牛(407±4 kg)采用4×4拉丁方试验设计,进行瘤胃和十二指肠近端瘘管试验。处理组应用滋生真菌的蒸汽压缩玉米755 ***-1分别取代空白组150、300和450 ***-1的片状玉米。对照组酵母菌和霉菌的平均数量分别为2.9×102和1.2×104 cfu.g-1;处理组平均数量分别为7.0×105和6.2×106。瘤胃pH、挥发性脂肪酸的摩尔比例各组间无显著差异(P>0.10)。瘤胃消化的有机物(OM;线性构造成分,P0.10)。氨基酸的摄入量随滋生真菌的增加呈线性增加(P0.10)。试验中滋生霉菌的蒸汽压片玉米的饲用价值降低。结果表明,并不是由于生长真菌而影响消化,而是在其腐败过程中损失了一定程度的营养物质,降低了氮的消化率。另一方面,滋生病菌的蒸汽压片玉米蛋白质的代谢值高于滋生真菌的玉米。

关键词：牛真菌玉米代谢

Methods for a blind analysis of isobar data collected by the STAR collaboration

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Nuclear Science and Techniques 2021年第5期32卷 43-50页

作者： j.Adam L.Adamczyk j.R.Adams j.K.Adkins G.Agakishiev M.M.Aggarwal Z.Ahammed I.Alekseev D.M.Anderson A.Aparin E.C.Aschenauer M.U.Ashraf F.G.Atetalla A.Attri G.S.Averichev V.Bairathi K.Barish A.Behera R.Bellwied A.Bhasin j.Bielcik j.Bielcikova L.C.Bland I.G.Bordyuzhin j.D.Brandenburg A.V.Brandin j.Butterworth H.Caines M.calderon de la Barca Sanchez D.Cebra I.Chakaberia P.Chaloupka B.K.Chan F-H.Chang Z.Chang N.Chankova-Bunzarova A.Chatterjee D.Chen j.Chen j.H.Chen X.Chen Z.Chen j.Cheng M.Cherney M.Chevalier S.Choudhury W.Christie X.Chu H.j.Crawford M.Csanad M.Daugherity T.G.Dedovich I.M.Deppner A.A.Derevschikov L.Didenko X.Dong j.L.Drachenberg j.C.Dunlop T.Edmonds N.Elsey j.Engelage G.Eppley S.Esumi O.Evdokimov A.Ewigleben O.Eyser R.Fatemi S.Fazio P.Federic j.Fedorisin C.j.Feng Y.Feng P.Filip E.Finch Y.Fisyak A.Francisco L.Fulek C.A.Gagliardi T.Galatyuk F.Geurts A.Gibson K.Gopal X.Gou D.Grosnick W.Guryn A.I.Hamad A.Hamed S.Harabasz j.W.Harris S.He W.He X.H.He Y.He S.Heppelmann S.Heppelmann N.Herrmann E.Hoffman L.Holub Y.Hong S.Horvat Y.Hu H.Z.Huang S.L.Huang T.Huang X.Huang T.j.Humanic P.Huo G.Igo D.Isenhower W.W.jacobs C.jena A.jentsch Y.ji j.jia K.j.ang S.jowzaee X.ju E.G.judd S.Kabana M.L.Kabir S.Kagamaster D.Kalinkin K.Kang D.Kapukchyan K.Kauder H.W.Ke D.Keane A.Kechechyan M.Kelsey Y.V.Khyzhniak D.P.Kikoła C.Kim B.Kimelman D.Kincses T.A.Kinghorn I.Kisel A.Kiselev M.Kocan L.Kochenda L.K.Kosarzewski L.Kramarik P.Kravtsov K.Krueger N.Kulathunga Mudiyanselage L.Kumar S.Kumar R.Kunnawalkam Elayavalli j.H.Kwasizur R.Lacey S.Lan j.M.Landgraf j.Lauret A.Lebedev R.Lednicky j.H.Lee Y.H.Leung C.Li C.Li W.Li W.Li X.Li Y.Li Y.Liang R.Licenik T.Lin Y.Lin M.A.Lisa F.Liu H.Liu P.Liu P.Liu T.Liu X.Liu Y.Liu Z.Liu T.Ljubicic W.j.Llope R.S.Longacre N.S.Lukow S.Luo X.Luo G.L.Ma L.Ma R.Ma Y.G.Ma N.Magdy R.Majka D.Mallick S.Margetis C.Markert H.S.Matis j.A.Mazer N.G.Minaev S.Mioduszewski B.Mohanty I.Mooney Z.Moravcova D.A.Morozov M.Nagy j.D.Nam Md.Nasim K.Nayak D.Neff j.M.Nelson D.B.Nemes M.Nie G.Nigmatkulov T.Niida L.V.Nogach T.Nonak Christian University AbileneTX 796992 AGH University of Science and Technology FPACSCracow 30-059Poland Alikhanov Institute for Theoretical and Experimental Physics NRC"Kurchatov Institute" MoscowRussia 117218 Argonne National Laboratory ArgonneIL 60439 American University of Cairo New CairoNew Cairo 11835Egypt Brookhaven National Laboratory UptonNY 11973 University of California BerkeleyCA 94720 University of California DavisCA 95616 University of California Los AngelesCA 90095 University of California RiversideCA 92521 Central China Normal University Wuhan 430079 University of Illinois at Chicago ChicagoIL 60607 Creighton University OmahaNE 68178 Czech Technical University in Prague FNSPEPrague 11519Czech Republic Technische Universitat Darmstadt Darmstadt 64289Germany ELTE Eotvos Lorand University Budapest 1117Hungary Frankfurt Institute for Advanced Studies FIAS Frankfurt 60438Germany Fudan University Shanghai 200433 University of Heidelberg 69120 HeidelbergGermany University of Houston HoustonTX 77204 Huzhou University Huzhou 313000 Indian Institute of Science Education and Research(IISER) Berhampur 760010India Indian Institute of Science Education and Research(IISER)Tirupati Tirupati 517507India Indian Institute Technology PatnaBihar 801106India Indiana University BloomingtonIN 47408 Institute of Modern Physics Chinese Academy of SciencesLanzhou 730000 University of jammu Jammu 180001India joint Institute for Nuclear Research DubnaRussia 141980 Kent State University KentOH 44242 University of Kentucky LexingtonKY 40506-0055 Lawrence Berkeley National Laboratory BerkeleyCA 94720 Lehigh University BethlehemPA 18015 Max-Planck-Institut fur Physik 80805 MunichGermany Michigan State University East LansingMI 48824 National Research Nuclear University MEPhI MoscowRussia 115409 National Institute of Science Education and Research HBNIJatni 752050India National Cheng Kung University Tainan 70101 Nuclear Physics Institute of the CAS Rez 25068Czech Republic Ohio State University

In 2018,the STAR collaboration collected data from^(96)_(44)Ru+^(96)_(44)Ru and^(96)_(40)Zr+^(96)_(40)Zr at√^(S)NN=200 Ge V to search for the presence of the chiral magnetic effect in collisions of *** isobar collision species alternated frequently between 9644 Ru+^(96)_(44)Ru and^(96)_(40)Zr+^(96)_(40)*** order to conduct blind analyses of studies related to the chiral magnetic effect in these isobar data,STAR developed a three-step blind analysis *** are initially provided a"reference sample"of data,comprised of a mix of events from the two species,the order of which respects time-dependent changes in run *** tuning analysis codes and performing time-dependent quality assurance on the reference sample,analysts are provided a species-blind sample suitable for calculating efficiencies and corrections for individual≈30-min data-taking *** this sample,species-specific information is disguised,but individual output files contain data from a single isobar *** run-by-run corrections and code alteration subsequent to these corrections are allowed at this *** these modifications,the"frozen"code is passed over the fully un-blind data,completing the blind *** a check of the feasibility of the blind analysis procedure,analysts completed a"mock data challenge,"analyzing data from Au+Au collisions at√^(S)NN=27 Ge V,collected in *** Au+Au data were prepared in the same manner intended for the isobar blind *** details of the blind analysis procedure and results from the mock data challenge are presented.

关键词： Blind analysis Chiral magnetic effect Heavy-ion collisions

2-6 First Direct Measurement of 12C(12C, n)23Mg at Stellar Energies

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IMP & HIRFL Annual Report 2015年第1期 56-58页

作者： Tang Xiaodong B. Bucher X. Fang A. Heger S. Almaraz-calderon A. Alongi A.D. Ayangeakaa M. Beard A. Best j. Browne C. Cahillane M. Couder R.j. deBoer A. Kontos L. Lamm Y.j. Li A. Long W. Lu S. Lyons M. Notani D. Patel N. Paul M. Pignatari A. Roberts D. Robertson K. Smith E. Stech R. Talwar W.P. Tan M. Wiescher S.E. Woosley Institute of Modern Physics Chinese Academy of Science Lanzhou 730000 China Institute for Structure and Nuclear Astrophysics Joint Institute for Nuclear AstrophysicsUniversity of Notre Dame Notre Dame Indiana 46556 USA Lawrence Livermore National Laboratory Livermore California 94550 USA Monash Center for Astrophysics School of Physics and Astronomy Monash University Victoria 3800 Australia Department of Physics and Astronomy Shanghai Jiao-Tong University CNA Shanghai 200240 China School of Physics and Astronomy University of Minnesota Minneapolis Minnesota 55455 USA China Institute of Atomic Energy Beijing 102413 China Konkoly Observatory Research Centre for Astronomy and Earth Sciences Hungarian Academy of SciencesKonkoly Thege Mikl′os′ut 15-17 H-1121 Budapest Hungary Department of Physics University of Basel Basel CH-4056 Switzerland Department of Astronomy and Astrophysics University of California Santa Cruz California 95064 USA

The first stars in the early Universe were formed about 400 million years after the big bang. Verification of the existence of these stars is important for our understanding of the evolution of the Universe[1]. It has been predicted that for Population-III stellar production yields, the abundances of odd-Z elements are remarkably deficient compared to their adjacent even-Z elements[2]. Astronomers are searching for long-lived, low mass stars with the unique nucleosynthetic pattern matching the predicted yields[3].

关键词： First Direct Measurement

多器官床旁即时超声在新型冠状病毒肺炎中的应用:国际专家共识

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中国呼吸与危重监护杂志 2021年第2期20卷 77-84页

作者：王臻(译) Arif Hussain Gabriele Via Lawrence Melniker Alberto Goffi Guido Tavazzi Luca Neri Tomas Villen Richard Hoppmann Francesco Mojoli Vicki Noble Laurent Zieleskiewicz Pablo Blanco Irene W.Y.Ma Mahathar Abd.Wahab Abdulmohsen Alsaawi Majid AI Salamah Martin Balik Diego Barca Karim Bendjelid Belaid Bouhemad Pablo Bravo-Figueroa Raoul Breitkreutz j.an calderon jim Connolly Roberto Copetti Francesco Corradi Anthony j.Dean AndréDenault Deepak Govil Carmela Graci Young-Rock Ha Laura Hurtado Toru Kameda Michael Lanspa Christian B Laursen Francis Lee Rachel Liu Massimiliano Meineri Miguel Montorfano Peiman Nazerian Bret P.Nelson Aleksandar N.Neskovic Ramon Nogue Adi Osman joséPazeli Elmo Pereira-junior Tomislav Petrovic Emanuele Pivetta jan Poelaert Susanna Price Gregor Prosen Shalim Rodriguez Philippe Rola Colin Royse Yale Tung Chen Mike Wells Adrian Wong Wang Xiaoting Wang Zhen Yaseen Arabi 中国人民解放军空军军医大学航空航天医学系陕西西安710032 Department of Cardiac Sciences King Abdulaziz Medical City and King Abdullah International Medical Research Center 不详

新型冠状病毒肺炎(简称新冠肺炎,COVID-19)自首次报道以来,已造成全球超一亿人感染,给各国的公共卫生体系造成了巨大威胁。新冠肺炎的临床表现以呼吸系统体征和症状为主,80%的患者症状轻微,约5%为危重症患者,常表现为急性呼吸窘迫综合征... 详细信息

新型冠状病毒肺炎(简称新冠肺炎,COVID-19)自首次报道以来,已造成全球超一亿人感染,给各国的公共卫生体系造成了巨大威胁。新冠肺炎的临床表现以呼吸系统体征和症状为主,80%的患者症状轻微,约5%为危重症患者,常表现为急性呼吸窘迫综合征(ARDS)。前期,由于缺乏相关研究,面对日益紧迫的临床困境,医务人员不得不借鉴采取一些经验性措施以应对疫情。

关键词：体征和症状肺炎公共卫生体系呼吸系统首次报道专家共识疫情