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Is th. globa. sea.surfa.e tempera.ure rise a.celera.ing?

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Geodesy a.d Geodyna.ics 2018年第6期9卷 432-438页

作者： h.Ba.i iz Division of Geodetic science School of Earth Sciences The Ohio State University Columbus OH 43210 USA

Th.s is a. explora.ory investiga.ion to sea.ch.for th. presence of a. a.celera.ion in globa. sea.surfa.e tempera.ure rise, wh.ch.is essentia. to identify a.th.opogenic contributions to th. clima.e ch.nge during th. 20 th.century. a.weigh.ed sta.istica. model with.a. a.celera.ion pa.a.eter wa. built progressively to reconstruct th. va.ia.ions in th. globa. sea.surfa.e tempera.ure da.a.considering sta.istica.ly significa.t confounders a.d a.toregressive disturba.ces in th. process. From th. prelimina.y residua. a.a.ysis of a.weigh.ed regression model, emerged a.pa.simonious model with.first order a.toregressive disturba.ces with.a.deterministic trend, a.celera.ion a.d periodicity of 69 yr a.d its 138 yr subh.rmonic. Th. fina. model solution, selected from 29 a.terna.ive combina.ions of th. model pa.a.eters using Ma.lows' s Cp metric, revea.ed a.sta.istica.ly significa.t deterministic trend, 0.40 ± 0.03C/c(p a.d a.celera.ion, 0.67 ± 0.11C/c^2(p a.ning 33% of th. globa. sea.surfa.e tempera.ure va.ia.ions. Th. combined yea.ly trend a.d a.celera.ion in globa. sea.surfa.e tempera.ure a. predicted by th. model,exh.bit a.strong correla.ion with.th. yea.ly increa.e in th. globa. CO^2 concentra.ions observed during th. 20th.century.

关键词： Clima.e ch.nge First order a.toregressive model Globa. sea.surfa.e tempera.ure Globa. sea.surfa.e tempera.ure a.celera.ion Globa. CO^2 concentra.ion

Th. a.th.cya.in's role on th. food meta.olic pa.h.a.s,color a.d drying processes:a. experimenta. a.d th.oretica. a.proa.h

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Food Bioscience 2022年第3期47卷 91-110页

作者： sa.dra.Peña.oza.Cornelio Delesma.Jesús Muñiz López-Ortiz a. Instituto de Energía. Renova.les Universidad Nacional Autónoma de MéxicoPriv.Xochicalco s/nCol.CentroTemixco62580MorelosMexico

Th.s review is intended to cover th. works rela.ed to th. a.th.cya.in beh.vior in food th.t is subjected to *** experimenta. a.d th.oretica. results a.a.la.le in scientific litera.ure a.e *** increa.e in a.th.cya.in concentra.ion h.s been observed upon th.rma. ***,a.conclusive expla.a.ion is still *** a.cessible studies suggest a. increa.e in concentra.ion during ma.ura.ions,wh.ch.could be rela.ed to th. enzyma.ic *** possible enzymes involved in such.a.procedure h.ve a.so been covered,including th.ir role pla.ed in th. *** possible a.tiva.ion mech.nisms a.d th. rela.ed fa.tors such.a. tempera.ure,ph.oxygen contents a.d th. presence of UV-ligh. irra.ia.ion were a.so ***,th. meta.olic pa.h.a.s were a.so explored including experimenta. eva.ua.ion a.d th.oretica. models ba.ed on a.omistic meth.dologies such.a. density functiona. th.ory(DFT).Th.s review is a.med to provide a.compreh.nsive overview of th. proba.le mech.nisms beh.nd th. increa.e of a.th.cya.in concentra.ion during drying.

关键词： a.th.cya.in Meta.olic pa.h.a. Pa. Ch. UFGT h.LC Th.oretica. model

ON sELECTIONs OF sET-Va.UED EULER-La.Ra.GE INCLUsIONs WITh.a.PLICa.IONs

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a.ta.Ma.h.ma.ica.scientia 2020年第4期40卷 1105-1115页

作者： h.mid Kh.Da.I iz-iddine EL-Fa.sI Ba.0}a. h.Ya. Fa.ulty of Ma.h.ma.ica. sciences a.d sta.istics Malayer UniversityP.O.Bor 65719-95863MalayerIran Depa.tment of Ma.h.ma.ics Faculty of Sciences and TechniquesSidi Mohamed ben Abdellah UniversityB.P.2202FezMoroccc.

We discuss th. set-va.ued dyna.ics rela.ed to th. th.ory of functiona. *** look for selections of convex set-va.ued functions sa.isfying set-va.ued Euler-La.ra.ge *** improve a.d extend upon some of th. results in[13,... 详细信息

关键词： set-va.ued dyna.ics Euler-La.ra.ge inclusion composite opera.or selection

Th. rigorous a.justment of th. globa. mea. sea.level budget during 2005-2015

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Geodesy a.d Geodyna.ics 2021年第3期12卷 175-180页

作者： h.Bâki iz T.Y.Ya.g C.K.sh.m Division of Geodetic science School of Earth SciencesThe Ohio State UniversityColumbusOHUSA

Globa. mea. sea.level budget is rigorously a.justed during th. period *** emph.sis is to provide th. best estima.es for th. linea. ra.es of ch.nges(trends)of th. globa. mea. sea.level budget components during th.s period subject to th. constra.nt:Ea.th.s h.drosph.re conserves *** newly simulta.eously a.justed trends of th. budget components suggest a.la.ger correction for th. globa. mea. sea.level trend implica.ed by th. oth.r budget components’trends under th. budget *** simulta.eous estima.ion of th. linea. trends of th. budget components subject to th. constra.nt for closure improves th.ir uncerta.nties a.d ena.les a.h.listic a.sessment of th. globa. mea. sea.budget,wh.ch.h.s implica.ions for future sea.level science studies,including th. future Intergovernmenta. Pa.el on Clima.e Ch.nge(IPCC)a.sessment Reports,a.d th. Us Clima.e a.sessment Reports.

关键词： Clima.e ch.nge Misclosure Globa. mea. sea.level Rigorous a.justment

Th. sTOCh.sTIC EsTIMa.ION OF sa.ELLITE CLOCK CORRECTION INFORMa.ION IN Wa.GPs

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Geo-spa.ia. Informa.ion science 2000年第1期3卷 66-69页

作者： h.seyin Bki iz GE Ma.rong Esmond Mok

Using a.tocorrela.ion informa.ion of th. pseudora.ge errors genera.ed by se- lective a.a.la.ility (sa. frequency dith.ring, we h.ve constructed a.simple first order stoch.s- tic model for sa.effects. Th.s model h.s been used in a.Ka.ma. filter to a.count for th. stoch.stic beh.vior of sa.dith.ring in estima.ing sa.ellite clock informa.ion in wide a.ea.dif- ferentia. GPs. We h.ve obta.ned fifteen percent improvement in th. user positioning using th. correla.ion informa.ion on th. sa.ellite clock informa.ion in a.Ka.ma. filter, wh.n compa.ing th. results obta.ned using a.regula. lea.t squa.e estima.ion.

关键词： stoch.stic model wide a.ea.differentia. GPs(Wa.GPs) selective a.a.la.ility

Evidence for pa.ticle a.celera.ion a.proa.h.ng PeV energies in th. W51 complex

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science Bulletin 2024年第18期69卷 2833-2841页

作者： Lh.a.O Colla.ora.ion Zh.n Ca. F.a.0}ronia. a.ikegu Y.X.Ba. Y.W.Ba. D.Ba.tieri X.J.Bi Y.J.Bi W.Bia. a.V.Bukevich.Q.Ca. W.Y.Ca. Zh. Ca. J.Ch.ng J.F.Ch.ng a.M.Ch.n E.s.Ch.n h.X.Ch.n Lia.g Ch.n Lin Ch.n Long Ch.n M.J.Ch.n M.L.Ch.n Q.h.Ch.n s.Ch.n s.h.Ch.n s.Z.Ch.n T.L.Ch.n Y.Ch.n N.Ch.ng Y.D.Ch.ng M.Y.Cui s.W.Cui X.h.Cui Y.D.Cui B.Z.Da. h.L.Da. Z.G.Da. Da.zengluobu X.Q.Dong K.K.Dua. J.h.Fa. Y.Z.Fa. J.Fa.g J.h.Fa.g K.Fa.g C.F.Feng h.Feng L.Feng s.h.Feng X.T.Feng Y.Feng Y.L.Feng s.Ga.ici B.Ga. C.D.Ga. Q.Ga. W.Ga. W.K.Ga. M.M.Ge L.s.Geng G.Gia.inti G.h.Gong Q.B.Gou M.h.Gu F.L.Guo X.L.Guo Y.Q.Guo Y.Y.Guo Y.a.h.n M.h.sa. h.h.h. h.N.h. J.Y.h. Y.h. Y.K.h.r B.W.h.u C.h.u X.h.u h.B.h. Q.h. s.C.h. D.h.h.a.g T.Q.h.a.g W.J.h.a.g X.T.h.a.g X.Y.h.a.g Y.h.a.g X.L.Ji h.Y.Jia.K.Jia.K.Jia.g X.W.Jia.g Z.J.Jia.g M.Jin M.M.Ka.g I.Ka.pikov D.Kulesh.v K.Kurinov B.B.Li C.M.Li Ch.ng Li Cong Li D.Li F.Li h.B.Li h.C.Li Jia. Li Jie Li K.Li s.D.Li W.L.Li W.L.Li X.R.Li Xin Li Y.Z.Li Zh. Li Zh.o Li E.W.Lia.g Y.F.Lia.g s.J.Lin B.Liu C.Liu D.Liu D.B.Liu h.Liu h.D.Liu J.Liu J.L.Liu M.Y.Liu R.Y.Liu s.M.Liu W.Liu Y.Liu Y.N.Liu Q.Luo Y.Luo h.K.Lv B.Q.Ma.L.L.Ma.X.h.Ma.J.R.Ma. Z.Min W.Mitth.msiri h.J.Mu Y.C.Na. a.Neronov L.J.Ou P.Pa.ta.a.ijwa.ich.Z.Y.Pei J.C.Qi M.Y.Qi B.Q.Qia. J.J.Qin a.Ra.a.D.Ruffolo a.sáiz M.sa.ed D.semikoz L.shao O.sh.h.golev X.D.sh.ng F.W.sh. h.C.song Yu.V.stenkin V.stepa.ov Y.su D.X.sun Q.N.sun X.N.sun Z.B.sun J.Ta.a.a.P.h.T.Ta. Q.W.Ta.g R.Ta.g Z.B.Ta.g W.W.Tia. C.Wa.g C.B.Wa.g G.W.Wa.g h.G.Wa.g h.h.Wa.g J.C.Wa.g Ka. Wa.g Ka. Wa.g L.P.Wa.g L.Y.Wa.g P.h.Wa.g R.Wa.g W.Wa.g X.G.Wa.g X.Y.Wa.g Y.Wa.g Y.D.Wa.g Y.J.Wa.g Z.h.Wa.g Z.X.Wa.g Zh.n Wa.g Zh.ng Wa.g D.M.Wei J.J.Wei Y.J.Wei T.Wen C.Y.Wu h.R.Wu Q.W.Wu s.Wu X.F.Wu Y.s.Wu s.Q.Xi J.Xia.G.M.Xia.g D.X.Xia. G.Xia. Y.L.Xin Y.Xing D.R.Xiong Z.Xiong D.L.Xu R.F.Xu R.X.Xu W.L.Xu L.Xue D.h.Ya. J.Z.Ya. T.Ya. C.W.Ya.g C.Y.Ya.g F.Ya.g F.F.Ya.g L.L.Ya.g M.J.Ya.g R.Z.Ya.g W.X.Ya.g Y.h.Ya. Z.G.Ya. L.Q.Yin N.Yin X.h.You Z.Y.You Y.h.Yu Q.Yua. h.Yue h.D.Zeng T.X.Zeng W.Zeng M.Zh. B.B.Zh.ng F.Zh.ng h.Zh.ng 不详 Key La.ora.ory of Pa.ticle a.troph.sics&Experimenta. Ph.sics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Ch.nese a.a.emy of sciences Beijing 100049China TIa.FU Cosmic Ra. Resea.ch.Center ChengduChina Dublin Institute for a.va.ced studies 31 Fitzwilliam Place2 DublinIreland Ma.-Pla.ck-Institut for Nuclea. Ph.sics P.O.Box 103980Heidelberg 69029Germany sch.ol of Ph.sica. science a.d Tech.ology&sch.ol of Informa.ion science a.d Tech.ology Southwest Jiaotong UniversityChengdu 610031China sch.ol of a.tronomy a.d spa.e science Nanjing UniversityNanjing 210023China Center for a.troph.sics Guangzhou UniversityGuangzhou 510006China Tsung-Da. Lee Institute&sch.ol of Ph.sics a.d a.tronomy Shanghai Jiao Tong UniversityShanghai 200240China Institute for Nuclea. Resea.ch.of Russia. a.a.emy of sciences Moscow 117312Russia h.bei Norma. University Shijiazhuang 050024China University of science a.d Tech.ology of Ch.na Hefei 230026China sta.e Key La.ora.ory of Pa.ticle Detection a.d Electronics China Key La.ora.ory of Da.k Ma.ter a.d spa.e a.tronomy&Key La.ora.ory of Ra.io a.tronomy Purple Mountain ObservatoryChinese Academy of SciencesNanjing 210023China Resea.ch.Center for a.tronomica. Computing Zhejiang LaboratoryHangzhou 311121China Key La.ora.ory for Resea.ch.in Ga.a.ies a.d Cosmology Shanghai Astronomical ObservatoryChinese Academy of SciencesShanghai 200030China sch.ol of Ph.sics a.d a.tronomy Yunnan UniversityKunming 650091China Key La.ora.ory of Cosmic Ra.s(Tibet University) Ministry of EducationLhasa 850000China Na.iona. a.tronomica. Observa.ories Chinese Academy of SciencesBeijing 100101China sch.ol of Ph.sics a.d a.tronomy(Zh.h.i)&sch.ol of Ph.sics(Gua.gzh.u)&sino-French.Institute of Nuclea. Engineering a.d Tech.ology(Zh.h.i) Sun Yat-sen UniversityZhuhai 519000&Guangzhou 510275GuangdongChina Institute of Frontier a.d Interdisciplina.y science Shandong UniversityQingdao 266237China a.C UniversitéParis Cité

Th.γ-ra. emission from th. W51 complex is widely a.knowledged to be a.tributed to th. intera.tion between th. cosmic ra.s(CRs)a.celera.ed by th. sh.ck of supernova.remna.t(sNR)W51C a.d th. dense molecula. clouds in th. a.ja.ent sta.-forming region,***,th. ma.imum a.celera.ion ca.a.ility of W51C for CRs rema.ns *** on observa.ions conducted with.th. La.ge h.gh.a.titude a.r sh.wer Observa.ory(Lh.a.O),we report a.significa.t detection ofγra.s ema.a.ing from th. W51 complex,with.energies from 2 to 200 *** Lh.a.O mea.urements,for th. first time,extend th.γ-ra. emission from th. W51 complex beyond 100 TeV a.d revea. a.significa.t spectrum bending a. tens of *** combining th."π^(0)-deca. bump"fea.ured da.a.from Fermi-La.,th. broa.ba.dγ-ra. spectrum of th. W51 region ca. be well-ch.ra.terized by a.simple pp-collision *** observed spectra. bending fea.ure suggests a. exponentia. cutoff a.~400 TeV or a.power-la. brea. a.~200 TeV in th. CR proton spectrum,most likely providing th. first evidence of sNRs serving a. CR a.celera.ors a.proa.h.ng th. PeV ***,two young sta. clusters with.n W51B could a.so be th.oretica.ly via.le to produce th. most energeticγra.s observed by *** findings strongly support th. presence of extreme CR a.celera.ors with.n th. W51 complex a.d provide new insigh.s into th. origin of Ga.a.tic CRs.

关键词： Uh. c-ra. Cosmic ra.s sNR W51C sta. clusters

ON h.PERsTa.ILITY OF Th. BIa.DITIVE FUNCTIONa. EQUa.ION

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a.ta.Ma.h.ma.ica.scientia 2017年第6期37卷 1727-1739页

作者： iz-iddine EL-Fa.sI Ja.usz BRZDEK a.della.if Ch.h.I sa.ir Ka.Ba. Depa.tment of Ma.h.ma.ics Faculty of SciencesIbn Tofail UniversityBP 133KenitraMorocco Depa.tment of Ma.h.ma.ics Pedagogical UniversityPodchorazych 230-084 KrakowPoland

We present results on a.proxima.e solutions to th. bia.ditive equa.ionf（x＋y,z-w）＋f（x-y,z＋w）=2f（x,z）-2f（y,w）on a.restricted doma.n. Th. proof is ba.ed on a.quite recent fixed point th.orem in some function spa.es. Our ma.n results sta.e th.t, under some wea. na.ura. a.sumptions, functions sa.isfying th. equa.ion a.proxima.ely （in some sense） must be a.tua.ly solutions to it. In th.s wa. we obta.n inequa.ities ch.ra.terizing bia.ditive ma.pings a.d inner product spa.es. Our outcomes a.e connected with.th. well known issues of Ula. sta.ility a.d h.persta.ility.

关键词： h.persta.ility Ula. sta.ility bia.ditive functiona. equa.ion fixed point th.-orem ch.ra.teriza.ion of inner product spa.e

a.PROXIMa.E sOLUTION OF a.p-th.ROOT FUNCTIONa. EQUa.ION IN NON-a.Ch.MEDEa. (2,β)-Ba.a.h.sPa.Es

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a.ta.Ma.h.ma.ica.scientia 2019年第2期39卷 369-381页

作者： iz-iddine EL-Fa.sI h.mid Kh.Da.I Th.mistocles M.Ra.sIa. Depa.tment of Ma.h.ma.ics Faculty of SciencesIbn Tofail University Depa.tment of Ma.h.ma.ics Malayer University Depa.tment of Ma.h.ma.ics National Technical University of Athens Zografou Campus

In th.s pa.er, using th. Brzdek's fixed point th.orem [9,Th.orem 1] in non-a.ch.medea.(2,β)-Ba.a.h.spa.es, we prove some sta.ility a.d h.persta.ility results for a. p-th.root functiona. equa.ion ■wh.re p∈{1, …, 5}... 详细信息

关键词： fixed point th.orem p-th root functiona. equa.ion sta.ility non-a.ch.medea. (2,β)-normed spa.es

由超拍电子伏特加速器产生的超高能伽马射线气泡

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science Bulletin 2024年第4期69卷 449-457页

作者： Lh.a.O Colla.ora.ion Zh.n Ca. Ch.a.dong Ga. Cong Li Ruo-Yu Liu Ruizh. Ya.g 不详 Key La.ora.ory of Pa.ticle a.troph.ics&Experimenta. Ph.sics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Ch.nese a.a.emy of sciences Beijing 100049China TIa.FU Cosmic Ra. Resea.ch.Center ChengduChina Institute of Frontier a.d Interdisciplina.y science Shandong UniversityQingdao 266237China sch.ol of a.tronomy a.d spa.e science Nanjing UniversityNanjing 210023China University of science a.d Tech.ology of Ch.na Hefei 230026China

We report th. detection of a.-ra. bubble spa.ning a. lea.t 100deg2 in ultra.h.gh.energy(Uh.)up to a.few PeV in th. direction of th. sta.-forming region Cygnus X,implying th. presence super PeVa.ron(s)a.celera.ing protons to a. lea.t 10 PeV.a.log-pa.a.ola.form with.th. ph.ton indexΓ(E)=(2.71±0.02)+(0.11±0.02)×log10(E/10 TeV)is found fitting th. ga.ma.ra. energy spectrum of th. bubble *** sources,“h.t spots”correla.ed with.very ma.sive molecula. clouds,a.d a.qua.i-sph.rica. a.orph.usγ-ra. emitter with.a.sharp centra. brigh.ening a.e observed in th. *** th. core of~0.5°,spa.ia.ly a.socia.ing with.a.region conta.ning ma.sive OB a.socia.ion(Cygnus OB2)a.d a.microqua.a.(Cygnus X-3),a. well a. previously reported multi-TeV sources,a. enh.nced concentra.ion of Uh.γ-ra.s is observed with.2 ph.tons a. energies a.ove 1 *** genera. fea.ure of th. bubble,th. morph.logy,a.d th. energy spectrum,a.e rea.ona.ly reproduced by th. a.sumption of a.pa.ticle a.celera.or in th. core,continuously injecting protons into th. a.bient medium.

关键词： Cosmic ra.s γ-ra.s Interstella. medium sta. cluster