The current status of orbital experiments for UHECR studies
The current status of orbital experiments for UHECR studies
复制标题
UHECR研究的轨道实验现状
DOI：
--
复制
发表时间：
2015
期刊：
影响因子：
--
通讯作者：
M. Zotov
中科院分区：
文献类型：
--
作者：
M. Panasyuk;M. Casolino;G. Garipov;T. Ebisuzaki;P. Gorodetzky;B. Khrenov;P. Klimov;V. Morozenko;N. Sakaki;O. Saprykin;S. Sharakin;Y. Takizawa;L. Tkachev;I. Yashin;M. Zotov
目前正在开发的两种极端能量宇宙射线轨道探测器：(1)带有反射光学系统（反射镜）的TUS和KLYPVE；(2)带有高透射率菲涅耳透镜的JEM-EUSO。它们将比现有的地面阵列覆盖更大的区域，几乎均匀地监测天球。TUS探测器是SINP MSU与几个俄罗斯和外国机构合作开发的开创性任务。它的视野相对较小（±4.5°），相当于6.4•103 km2的地面面积。望远镜由一个菲涅耳式镜面聚光器（约2平方米）和一个光接收器（一个16 × 16光电倍增管矩阵）组成。它将被部署在罗蒙诺索夫卫星上，目前正处于飞行前测试的最后阶段。最近，SINP MSU开始了KLYPVE项目，该项目将安装在国际空间站的俄罗斯部分。该探测器的光学系统包含一个更大的主镜（10平方米），这允许降低能量阈值。总有效视场将至少达到±14°，以超过现有地面实验的年曝光量。目前正在考虑探测器的几种配置。最后，JEM-EUSO是一个宽视场（±30°）探测器。光学系统由两个外径2.65 m的双面菲涅耳曲面透镜、一个精密衍射中间透镜和一个瞳孔组成。紫外光子被聚焦到由近5000个多阳极光电倍增管组成的焦面上。它是由大型国际合作开发的。由于连续监测各种大气现象，这三种轨道探测器都具有多用途特性。报告了TUS和KLYPVE任务的发展现状，并与JEM-EUSO项目进行了简要比较。
Two types of orbital detectors of extreme energy cosmic rays are being developed nowadays: (i) TUS and KLYPVE with reflecting optical systems (mirrors) and (ii) JEM-EUSO with high- transmittance Fresnel lenses. They will cover much larger areas than existing ground-based arrays and almost uniformly monitor the celestial sphere. The TUS detector is the pioneering mission developed in SINP MSU in cooperation with several Russian and foreign institutions. It has relatively small field of view (±4.5°), which corresponds to a ground area of 6.4 • 103 km2. The telescope consists of a Fresnel-type mirror-concentrator (∼ 2 m2) and a photo receiver (a matrix of 16 x 16 photomultiplier tubes). It is to be deployed on the Lomonosov satellite, and is currently at the final stage of preflight tests. Recently, SINP MSU began the KLYPVE project to be installed on board of the Russian segment of the ISS. The optical system of this detector contains a larger primary mirror (10 m2), which allows decreasing the energy threshold. The total effective field of view will be at least ±14° to exceed the annual exposure of the existing ground-based experiments. Several configurations of the detector are being currently considered. Finally, JEM-EUSO is a wide field of view (±30°) detector. The optics is composed of two curved double-sided Fresnel lenses with 2.65 m external diameter, a precision diffractive middle lens and a pupil. The ultraviolet photons are focused onto the focal surface, which consists of nearly 5000 multi-anode photomultipliers. It is developed by a large international collaboration. All three orbital detectors have multi-purpose character due to continuous monitoring of various atmospheric phenomena. The present status of development of the TUS and KLYPVE missions is reported, and a brief comparison of the projects with JEM-EUSO is given.
影响因子：
8.6
作者：
J. Abraham;P. Abreu;M. Aglietta;C. Aguirre;D. Allard;I. Allekotte;J. Allen;P. Allison;J. Alvarez-Muñiz;M. Ambrosio;L. Anchordoqui;S. Andringa;A. Anzalone;C. Aramo;S. Argirò;K. Arisaka;E. Armengaud;F. Arneodo;F. Arqueros;T. Asch;Hernán Asorey;P. Assis;B. S. Atulugama;J. Aublin;M. Ave;G. Avila;T. Bäcker;D. Badagnani;A. F. Barbosa;D. Barnhill;S. Barroso;B. Baughman;P. Bauleo;J. Beatty;T. Beau;B. Becker;K. Becker;J. Bellido;S. BenZvi;C. Bérat;T. Bergmann;P. Bernardini;X. Bertou;P. Biermann;P. Billoir;O. Blanch-Bigas;F. Blanco;P. Blasi;C. Bleve;H. Blümer;M. Boháčová;C. Bonifazi;R. Bonino;J. Brack;P. Brogueira;W. C. Brown;P. Buchholz;A. Bueno;R. Burton;N. Busca;K. Caballero-Mora;B. Cai;D. Camin;L. Caramete;R. Caruso;W. Carvalho;A. Castellina;O. Catalano;G. Cataldi;L. Cazon;R. Cester;J. Chauvin;A. Chiavassa;J. Chinellato;A. Chou;J. Chudoba;J. Chye;P. Clark;R. Clay;E. Colombo;R. Conceição;B. Connolly;F. Contreras;J. Coppens;A. Cordier;U. Cotti;S. Coutu;C. Covault;A. Creusot;A. Criss;J. Cronin;A. Curuţiu;S. Dagoret-Campagne;K. Daumiller;B. Dawson;R. D. de Almeida;C. De Donato;S. de Jong;G. de la Vega;W. D. M. Junior;J. D. M. Neto;I. De Mitri;V. de Souza;L. Del Peral;O. Deligny;A. Della Selva;C. Fratte;H. Dembinski;C. Di Giulio;J. Diaz;P. Diep;C. Dobrigkeit;J. D'Olivo;P. N. Dong;D. Dornic;A. Dorofeev;J. D. dos Anjos;M. Dova;D. D’Urso;I. Duţan;M. DuVernois;R. Engel;L. Epele;M. Erdmann;C. Escobar;A. Etchegoyen;P. F. S. Luis;H. Falcke;G. Farrar;A. Fauth;N. Fazzini;F. Ferrer;A. Ferrero;B. Fick;A. Filevich;A. Filipčič;I. Fleck;C. Fracchiolla;W. Fulgione;B. Garcia;D. Gámez;D. García-Pinto;X. Garrido;H. Geenen;G. Gelmini;H. Gemmeke;P. Ghia;M. Giller;H. Glass;M. Gold;G. Golup;F. G. Albarracín;M. G. Berisso;P. Gonçalves;M. do Amaral;D. Gonzalez;J. G. Gonzalez;M. González;D. Góra;A. Gorgi;P. Gouffon;V. Grassi;A. Grillo;C. Grunfeld;Y. Guardincerri;F. Guarino;G. Guedes;J. Gutiérrez;J. Hague;V. Halenka;J. Hamilton;P. Hansen;D. Harari;S. Harmsma;J. Harton;A. Haungs;T. Hauschildt;M. Healy;T. Hebbeker;G. Hebrero;D. Heck;C. Hojvat;V. C. Holmes;P. Homola;J. Hörandel;A. Horneffer;M. Hrabovsky;T. Huege;M. Hussain;M. Iarlori;A. Insolia;F. Ionita;A. Italiano;M. Kaducak;K. Kampert;T. Karova;P. Kasper;B. Kégl;B. Keilhauer;E. Kemp;R. Kieckhafer;H. Klages;M. Kleifges;J. Kleinfeller;R. Knapik;J. Knapp;D. Koang;A. Krieger;O. Krömer;D. Kuempel;N. Kunka;A. Kusenko;G. La Rosa;C. Lachaud;B. Lago;D. Lebrun;P. Lebrun;J. Lee;M. D. de Oliveira;A. Letessier-Selvon;M. Leuthold;I. Lhenry-Yvon;R. Lopez;Á. Agüera;J. L. Bahilo;A. Lucero;R. García;M. Maccarone;C. Macolino;S. Maldera;G. Mancarella;M. Manceñido;D. Mandát;P. Mantsch;A. Mariazzi;I. Mariş;H. M. Falcon;D. Martello;J. Martinez;O. M. Bravo;H. Mathes;J. Matthews;J. Matthews;G. Matthiae;D. Maurizio;P. Mazur;T. McCauley;M. Mcewen;R. Mcneil;M. Medina;G. Medina-Tanco;D. Melo;E. Menichetti;A. Menschikov;C. Meurer;R. Meyhandan;M. Micheletti;G. Miele;W. Miller;S. Mollerach;M. Monasor;D. Ragaigne;F. Montanet;B. Morales;C. Morello;J. Moreno;C. Morris;M. Mostafá;M. Muller;R. Mussa;G. Navarra;J. Navarro;S. Navas;P. Nečesal;L. Nellen;C. Newman-Holmes;D. Newton;P. T. Nhung;N. Nierstenhoefer;D. Nitz;D. Nosek;L. Nožka;J. Oehlschläger;T. Ohnuki;A. Olinto;V. Olmos-Gilbaja;M. Ortiz;F. Ortolani;S. Ostapchenko;L. Otero;N. Pacheco;D. P. Selmi-Dei;M. Palatka;J. Pallotta;G. Parente;É. Parizot;S. Parlati;S. Pastor;M. Patel;T. Paul;V. Pavlidou;K. Payet;M. Pech;J. Pȩkala;R. Pelayo;I. Pepe;L. Perrone;R. Pesce;S. Petrera;P. Petrinca;Y. Petrov;A. Pichel;R. Piegaia;T. Pierog;M. Pimenta;T. Pinto;V. Pirronello;O. Pisanti;M. Platino;J. Pochon;P. Privitera;M. Prouza;E. Quel;J. Rautenberg;A. Redondo;S. Reucroft;B. Revenu;F. Rezende;J. Řídký;S. Riggi;M. Risse;C. Rivière;V. Rizi;M. Roberts;C. Robledo;G. Rodriguez;J. Martino;J. Rojo;I. Rodríguez-Cabo;M. Rodríguez-Frías;G. Ros;J. Rosado;M. Roth;B. Rouillé-d’Orfeuil;E. Roulet;A. Rovero;F. Salamida;H. Salazar;G. Salina;F. Sánchez;M. Santander;C. E. Santo;E. Santos;F. Sarazin;S. Sarkar;R. Sato;V. Scherini;H. Schieler;A. Schmidt;F. Schmidt;T. Schmidt;O. Scholten;P. Schovánek;F. Schroeder;S. Schulte;F. Schüssler;S. Sciutto;M. Scuderi;A. Segreto;D. Semikoz;M. Settimo;R. Shellard;I. Sidelnik;B. B. Siffert-B.;G. Sigl;N. Grande;A. Śmiałkowski;R. Šmída;A. Smith;B. Smith;G. Snow;P. Sokolsky;P. Sommers;J. Sorokin;H. Spinka;R. Squartini;E. Strazzeri;A. Stutz;F. Suarez;T. Suomijärvi;A. Supanitsky;M. Sutherland;J. Swain;Z. Szadkowski;J. Takahashi;A. Tamashiro;A. Tamburro;T. Tarutina;O. Tascau;R. Tcaciuc;N. T. Thao;D. Thomas;R. Ticona;J. Tiffenberg;C. Timmermans;W. Tkaczyk;C. T. Peixoto;B. Tomé;A. Tonachini;I. Torres;P. Trávníček;A. Tripathi;G. Tristram;D. Tscherniakhovski;V. Tuci;M. Tueros;V. Tunnicliffe;R. Ulrich;M. Unger;M. Urban;J. F. V. Galicia;I. Valiño;L. Valore;A. M. van den Berg;V. Van Elewyck;R. Vazquez;D. Veberič;A. Veiga;A. Velarde;T. Venters;V. Verzi;M. Videla;L. Villaseñor;S. Vorobiov;L. Voyvodic;H. Wahlberg;P. Wahrlich;O. Wainberg;P. Walker;D. Warner;A. Watson;S. Westerhoff;G. Wieczorek;L. Wiencke;B. Wilczynska;H. Wilczynski;C. Wileman;M. G. Winnick;H. Wu;B. Wundheiler;T. Yamamoto;P. Younk;E. Zas;D. Zavrtanik;M. Zavrtanik;I. Zaw;A. Zepeda;M. Ziolkowski
通讯作者：
J. Abraham;P. Abreu;M. Aglietta;C. Aguirre;D. Allard;I. Allekotte;J. Allen;P. Allison;J. Alvarez-Muñiz;M. Ambrosio;L. Anchordoqui;S. Andringa;A. Anzalone;C. Aramo;S. Argirò;K. Arisaka;E. Armengaud;F. Arneodo;F. Arqueros;T. Asch;Hernán Asorey;P. Assis;B. S. Atulugama;J. Aublin;M. Ave;G. Avila;T. Bäcker;D. Badagnani;A. F. Barbosa;D. Barnhill;S. Barroso;B. Baughman;P. Bauleo;J. Beatty;T. Beau;B. Becker;K. Becker;J. Bellido;S. BenZvi;C. Bérat;T. Bergmann;P. Bernardini;X. Bertou;P. Biermann;P. Billoir;O. Blanch-Bigas;F. Blanco;P. Blasi;C. Bleve;H. Blümer;M. Boháčová;C. Bonifazi;R. Bonino;J. Brack;P. Brogueira;W. C. Brown;P. Buchholz;A. Bueno;R. Burton;N. Busca;K. Caballero-Mora;B. Cai;D. Camin;L. Caramete;R. Caruso;W. Carvalho;A. Castellina;O. Catalano;G. Cataldi;L. Cazon;R. Cester;J. Chauvin;A. Chiavassa;J. Chinellato;A. Chou;J. Chudoba;J. Chye;P. Clark;R. Clay;E. Colombo;R. Conceição;B. Connolly;F. Contreras;J. Coppens;A. Cordier;U. Cotti;S. Coutu;C. Covault;A. Creusot;A. Criss;J. Cronin;A. Curuţiu;S. Dagoret-Campagne;K. Daumiller;B. Dawson;R. D. de Almeida;C. De Donato;S. de Jong;G. de la Vega;W. D. M. Junior;J. D. M. Neto;I. De Mitri;V. de Souza;L. Del Peral;O. Deligny;A. Della Selva;C. Fratte;H. Dembinski;C. Di Giulio;J. Diaz;P. Diep;C. Dobrigkeit;J. D'Olivo;P. N. Dong;D. Dornic;A. Dorofeev;J. D. dos Anjos;M. Dova;D. D’Urso;I. Duţan;M. DuVernois;R. Engel;L. Epele;M. Erdmann;C. Escobar;A. Etchegoyen;P. F. S. Luis;H. Falcke;G. Farrar;A. Fauth;N. Fazzini;F. Ferrer;A. Ferrero;B. Fick;A. Filevich;A. Filipčič;I. Fleck;C. Fracchiolla;W. Fulgione;B. Garcia;D. Gámez;D. García-Pinto;X. Garrido;H. Geenen;G. Gelmini;H. Gemmeke;P. Ghia;M. Giller;H. Glass;M. Gold;G. Golup;F. G. Albarracín;M. G. Berisso;P. Gonçalves;M. do Amaral;D. Gonzalez;J. G. Gonzalez;M. González;D. Góra;A. Gorgi;P. Gouffon;V. Grassi;A. Grillo;C. Grunfeld;Y. Guardincerri;F. Guarino;G. Guedes;J. Gutiérrez;J. Hague;V. Halenka;J. Hamilton;P. Hansen;D. Harari;S. Harmsma;J. Harton;A. Haungs;T. Hauschildt;M. Healy;T. Hebbeker;G. Hebrero;D. Heck;C. Hojvat;V. C. Holmes;P. Homola;J. Hörandel;A. Horneffer;M. Hrabovsky;T. Huege;M. Hussain;M. Iarlori;A. Insolia;F. Ionita;A. Italiano;M. Kaducak;K. Kampert;T. Karova;P. Kasper;B. Kégl;B. Keilhauer;E. Kemp;R. Kieckhafer;H. Klages;M. Kleifges;J. Kleinfeller;R. Knapik;J. Knapp;D. Koang;A. Krieger;O. Krömer;D. Kuempel;N. Kunka;A. Kusenko;G. La Rosa;C. Lachaud;B. Lago;D. Lebrun;P. Lebrun;J. Lee;M. D. de Oliveira;A. Letessier-Selvon;M. Leuthold;I. Lhenry-Yvon;R. Lopez;Á. Agüera;J. L. Bahilo;A. Lucero;R. García;M. Maccarone;C. Macolino;S. Maldera;G. Mancarella;M. Manceñido;D. Mandát;P. Mantsch;A. Mariazzi;I. Mariş;H. M. Falcon;D. Martello;J. Martinez;O. M. Bravo;H. Mathes;J. Matthews;J. Matthews;G. Matthiae;D. Maurizio;P. Mazur;T. McCauley;M. Mcewen;R. Mcneil;M. Medina;G. Medina-Tanco;D. Melo;E. Menichetti;A. Menschikov;C. Meurer;R. Meyhandan;M. Micheletti;G. Miele;W. Miller;S. Mollerach;M. Monasor;D. Ragaigne;F. Montanet;B. Morales;C. Morello;J. Moreno;C. Morris;M. Mostafá;M. Muller;R. Mussa;G. Navarra;J. Navarro;S. Navas;P. Nečesal;L. Nellen;C. Newman-Holmes;D. Newton;P. T. Nhung;N. Nierstenhoefer;D. Nitz;D. Nosek;L. Nožka;J. Oehlschläger;T. Ohnuki;A. Olinto;V. Olmos-Gilbaja;M. Ortiz;F. Ortolani;S. Ostapchenko;L. Otero;N. Pacheco;D. P. Selmi-Dei;M. Palatka;J. Pallotta;G. Parente;É. Parizot;S. Parlati;S. Pastor;M. Patel;T. Paul;V. Pavlidou;K. Payet;M. Pech;J. Pȩkala;R. Pelayo;I. Pepe;L. Perrone;R. Pesce;S. Petrera;P. Petrinca;Y. Petrov;A. Pichel;R. Piegaia;T. Pierog;M. Pimenta;T. Pinto;V. Pirronello;O. Pisanti;M. Platino;J. Pochon;P. Privitera;M. Prouza;E. Quel;J. Rautenberg;A. Redondo;S. Reucroft;B. Revenu;F. Rezende;J. Řídký;S. Riggi;M. Risse;C. Rivière;V. Rizi;M. Roberts;C. Robledo;G. Rodriguez;J. Martino;J. Rojo;I. Rodríguez-Cabo;M. Rodríguez-Frías;G. Ros;J. Rosado;M. Roth;B. Rouillé-d’Orfeuil;E. Roulet;A. Rovero;F. Salamida;H. Salazar;G. Salina;F. Sánchez;M. Santander;C. E. Santo;E. Santos;F. Sarazin;S. Sarkar;R. Sato;V. Scherini;H. Schieler;A. Schmidt;F. Schmidt;T. Schmidt;O. Scholten;P. Schovánek;F. Schroeder;S. Schulte;F. Schüssler;S. Sciutto;M. Scuderi;A. Segreto;D. Semikoz;M. Settimo;R. Shellard;I. Sidelnik;B. B. Siffert-B.;G. Sigl;N. Grande;A. Śmiałkowski;R. Šmída;A. Smith;B. Smith;G. Snow;P. Sokolsky;P. Sommers;J. Sorokin;H. Spinka;R. Squartini;E. Strazzeri;A. Stutz;F. Suarez;T. Suomijärvi;A. Supanitsky;M. Sutherland;J. Swain;Z. Szadkowski;J. Takahashi;A. Tamashiro;A. Tamburro;T. Tarutina;O. Tascau;R. Tcaciuc;N. T. Thao;D. Thomas;R. Ticona;J. Tiffenberg;C. Timmermans;W. Tkaczyk;C. T. Peixoto;B. Tomé;A. Tonachini;I. Torres;P. Trávníček;A. Tripathi;G. Tristram;D. Tscherniakhovski;V. Tuci;M. Tueros;V. Tunnicliffe;R. Ulrich;M. Unger;M. Urban;J. F. V. Galicia;I. Valiño;L. Valore;A. M. van den Berg;V. Van Elewyck;R. Vazquez;D. Veberič;A. Veiga;A. Velarde;T. Venters;V. Verzi;M. Videla;L. Villaseñor;S. Vorobiov;L. Voyvodic;H. Wahlberg;P. Wahrlich;O. Wainberg;P. Walker;D. Warner;A. Watson;S. Westerhoff;G. Wieczorek;L. Wiencke;B. Wilczynska;H. Wilczynski;C. Wileman;M. G. Winnick;H. Wu;B. Wundheiler;T. Yamamoto;P. Younk;E. Zas;D. Zavrtanik;M. Zavrtanik;I. Zaw;A. Zepeda;M. Ziolkowski
最高能量宇宙射线与附近活动星系核位置的相关性
影响因子：
3.5
作者：
Abraham J
通讯作者：
Abraham J