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蒙药治疗流行性腮腺炎

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中国民族医药杂志 2004年第4期10卷 32-32页

作者：白玉华关宝柱付金莲萨如拉内蒙古民族大学蒙医院药学院 028000 内蒙古通辽市蒙医研究所内蒙古民族大学蒙医药学院 028000 内蒙古民族大学98级高护班

流行性腮腺炎是儿科常见的病毒性传染病,多流行于冬春二季.临床上以腮腺肿大、疼痛为特征,若治疗不当或不及时可并发脑炎、睾丸炎、胰腺炎等疾病.我们对60例门诊患儿采用蒙药外敷及内服治疗,取得了较好的疗效.现报告如下.

关键词：流行性腮腺炎蒙药治疗

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运用多媒体搞好《人体寄生虫学》的教学改革

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华北煤炭医学院学报 2003年第2期5卷 235-235页

作者：贺宝玲田喜凤赵丽娜张更路董路蒋龙芳华北煤炭医学院寄生虫教研室河北唐山063000 华北煤炭医学院计算机教研室河北唐山063000 华北煤炭医学院预防医学系 98级11班河北唐山063000

计算机的普及应用,推动了教学方法现代化的进程.多媒体教学也在教学改革的浪潮中应运而生,成为热门的辅助教学手段.随着招生规模的不断扩大,寄生虫学课时的不断缩减,课程的教学现代化势在必行.

关键词：寄生虫学多媒体教学

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STUDY ON HEMODYNAMICS OF ERECTION IN DIABETIC ERECTILE DYSFUNCTION

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Journal of Shanghai Second Medical University(Foreign Language Edition) 2004年第2期16卷 121-124页

作者：傅强姚德鸿蒋跃庆 Department of Urology the Ninth People' s Hospital SSMU Shanghai 200011 China Department of Urology the Ninth People' s Hospital SSMU Shanghai 200011 Chinabjective To study the cavernosa hemodynamics in diabetic erectile dysfunction ( ED).Methods 22 diabetic and 35 psychic ED patients were studied by intracavernosum injection of a mixture papaver-ine and phentolamine (30/1mg) to assess the hemodynamics changes of the corpus cavernosum by means of colour duplex ultrasonography. Results The average hemodynamics data of the diabetic ED patients vs that of the psy-chogenic ED patients in terms of peak flow velocity (PFV):20. 06±7.15cm/s vs 35. 82±9. 41cm/s end diastolic velocity (EDV) : 8. 82±0. 35cm/s vs 5. 51±0. 42cm/sartery diameter (Ad) : 0. 78±0. 25cm vs 1. 01±0. 42cm vein diameter ( Vd) : 1.05±0. 32mm vs 1.21±0. 45mm resistance index(RI) : 0. 72±0. 28 vs 0. 98±0. 31mean velocity of artery (MV):6. 71±0. 27cm/s vs 10. 31±3. 32cm/s dorsal deep vein flow(DDVF) : 28. 81±6. 32cm/ s vs 25. 74±0. 58cm/s. Stasticstical differences existed in PFV AdRI and MV(P <0. 01). The arterial wall is thick and rigid in diabetic ED patients. Conclusion Atheroscleorsis and veno-occlusive dysfunction of the corpus cavernosum are essential to the development of diabetic ED.

Objective To study the cavernosa hemodynamics in diabetic erectile dysfunction ( ED).Methods 22 diabetic and 35 psychic ED patients were studied by intracavernosum injection of a mixture papaver-ine and phentolamine (30/1mg) to assess the hemodynamics changes of the corpus cavernosum by means of colour duplex ultrasonography. Results The average hemodynamics data of the diabetic ED patients vs that of the psy-chogenic ED patients in terms of peak flow velocity (PFV):20. 06±7.15cm/s vs 35. 82±9. 41cm/s, end diastolic velocity (EDV) : 8. 82±0. 35cm/s vs 5. 51±0. 42cm/s,artery diameter (Ad) : 0. 78±0. 25cm vs 1. 01±0. 42cm, vein diameter ( Vd) : 1.05±0. 32mm vs 1.21±0. 45mm, resistance index(RI) : 0. 72±0. 28 vs 0. 98±0. 31,mean velocity of artery (MV):6. 71±0. 27cm/s vs 10. 31±3. 32cm/s, dorsal deep vein flow(DDVF) : 28. 81±6. 32cm/ s vs 25. 74±0. 58cm/s. Stasticstical differences existed in PFV, Ad,RI and MV(P <0. 01). The arterial wall is thick and rigid in diabetic ED patients. Conclusion Atheroscleorsis and veno-occlusive dysfunction of the corpus cavernosum are essential to the development of diabetic ED.

关键词： diabetes mellitus erectile dysfunction colour duplex ultrasonography

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The Giant Radio Array for Neutrino Detection(GRAND):Science and design

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Science China(Physics,Mechanics & Astronomy) 2020年第1期63卷 1-43页

作者： Jaime Alvarez-Muniz Rafael Alves Batista Aswathi Balagopal V. Julien Bolmont Mauricio Bustamante Washington Carvalho Jr. Didier Charrier Ismael Cognard Valentin Decoene Peter B.Denton Sijbrand De Jong Krijn D.De Vries Ralph Engel Ke Fang Chad Finley Stefano Gabici Quan Bu Gou Jun Hua Gu Claire Guépin Hong Bo Hu Yan Huang Kumiko Kotera Sandra Le Coz Jean-Philippe Lenain Guo Liang Léü Olivier Martineau-Huynh Miguel Mostafá Fabrice Mottez Kohta Murase Valentin Niess Foteini Oikonomou Tanguy Pierog Xiang Li Qian Bo Qin Duan Ran Nicolas Renault-Tinacci Markus Roth Frank G.Schroder Fabian Schüssler Cyril Tasse Charles Timmerman Matías Tueros Xiang Ping Wu Philippe Zarka Andreas Zech B.Theodore Zhang Jian Li Zhang Yi Zhang Qian Zheng Anne Zilles Departamento de Fisica de Particulas&lnstituto Galego de Fisica de Altas Enerxias Universidad de Santiago de CompostelaSantiago de Compostela 15782Spain Instituto de Astronomia Geofisica e Ciencias AtmosfericasUniversidade de Sao PauloSao Paulo-SP 05508-090Brazil Department of Physics-Astrophysics University of OxfordDWBOxford 0X13RHUK Institute of Experimental Particle Physics(ETP) Karlsruhe Institute of Technology(KIT)Karlsru he D-76021Germany Laboratoire de Physique Nucleeaire et de Hautes Energies(LPNHE) Sorbonne UniversiteUniversite Paris DiderotSorbonne Paris CiteCNRS place Jussieu F-75252Paris Cedex 5France Niels Bohr International Academy and DARK Niels Bohr InstituteCopenhagen 2100Denmark Discovery Center Niels Bohr InstituteCopenhagen 2100Denmark Center for Cosmology and AstroParticle Physics(CCA.PP)&Department of Physics Ohio State UniversityColumbus OH 43210USA Universidade de Santiago de Compostela Santiago de Compostela 15782Spain 0SUBATECH Institut Mines-Telecom Atlantique-CNRS/IN2P3-Universite de NantesNantes 44300France Laboratoire de Physique et Chimie de KEnvironnement et de VEspace LPC2E CNRS-Universite d'Orleans Orleans F-45071France Station de Radioastronomie de Nancay Observatoire de ParisCNRS/INSU F-18330 NangayFrance Sorbonne Universite UMR 7095Institut d'Astrophysique de Paris98 bis bd AragoParis 75014France Institute for Mathematics Astrophysics and Particle Physics(IMAPP)Radboud UniversiteitNijmegen 6500Netherlands Nationaal Instituut voor Kemfysica en Hoge Energie Fysica(NIKHEF) Amsterdam NL-1009Netherlands IIHE/ELEM Vrije Universiteit BrusselPleinlaan 2Brussels 1050Belgium Institute for Nuclear Physics(IKP) Karlsruhe Institute of Technology(KIT)Karlsruhe D-76021Germany Einstein Fellow Stanford UniversityStanford CA 94305USA Department of Astronomy University of MarylandCollege Park MD 20742-2421USA Joint Space-Science Institute College Park MD 20742-2421USA Oskar Klein Centre Stockholm UniversityStockholm SE-10691Sweden Department of Phy

The Giant Radio Array for Neutrino Detection(GRAND)is a planned large-scale observatory of ultra-high-energy(UHE)cosmic particles,with energies exceeding 10~8 Ge *** goal is to solve the long-standing mystery of the origin of UHE cosmic *** do this,GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched *** will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the *** design is modular:20 separate,independent sub-arrays,each of 10000 radio antennas deployed over 10000 km^2.A staged construction plan will validate key detection techniques while achieving important science goals *** we present the science goals,detection strategy,preliminary design,performance goals,and construction plans for GRAND.

关键词： radio telescopes neutrinos in astronomical observations cosmic rays in astronomical observations radiowave radiation:sources galactic and extragalactic cosmic rays:galactic and extragalactic

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