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1. An examination of land use impacts of flooding induced by sea level rise

Author

J. Song, X. Fu, Y. Gu, Y. Deng, and Z.-R. Peng

Subjects
Environmental technology. Sanitary engineering, TD1-1066, Geography. Anthropology. Recreation, Environmental sciences, GE1-350, Geology, QE1-996.5
Abstract

Coastal regions become unprecedentedly vulnerable to coastal hazards that are associated with sea level rise. The purpose of this paper is therefore to simulate prospective urban exposure to changing sea levels. This article first applied the cellular-automaton-based SLEUTH model (Project Gigalopolis, 2016) to calibrate historical urban dynamics in Bay County, Florida (USA) – a region that is greatly threatened by rising sea levels. This paper estimated five urban growth parameters by multiple-calibration procedures that used different Monte Carlo iterations to account for modeling uncertainties. It then employed the calibrated model to predict three scenarios of urban growth up to 2080 – historical trend, urban sprawl, and compact development. We also assessed land use impacts of four policies: no regulations; flood mitigation plans based on the whole study region and on those areas that are prone to experience growth; and the protection of conservational lands. This study lastly overlaid projected urban areas in 2030 and 2080 with 500-year flooding maps that were developed under 0, 0.2, and 0.9 m sea level rise. The calibration results that a substantial number of built-up regions extend from established coastal settlements. The predictions suggest that total flooded area of new urbanized regions in 2080 would be more than 25 times that under the flood mitigation policy, if the urbanization progresses with few policy interventions. The joint model generates new knowledge in the domain between land use modeling and sea level rise. It contributes to coastal spatial planning by helping develop hazard mitigation schemes and can be employed in other international communities that face combined pressure of urban growth and climate change.

Published
2017
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2. Sensitivity of ARGO-YBJ to different composition models in the energy range 10 ÷ 500 TeV

Author

C. BACCI, K. Z. BAO, F. BARONE, B. BARTOLI, S. BUSSINO, E. CALLONI, B. Y. CAO, R. CARDARELLI, S. CATALANOTTI, S. CAVALIERE, F. CESARONI, P. CRETI, DANZENGLUOBU, B. D'ETTORRE PIAZZOLI, M. DE VINCENZI, T. DI GIROLAMO, G. DI SCIASCIO, Z. Y. FENG, Y. FU, X. Y. GAO, Q. X. GENG, H. W. GUO, H. H. HE, M. HE, Q. HUANG, M. IACOVACCI, N. IUCCI, H. Y. JAI, C. L. JING, F. M. KONG, H. H. KUANG, LABACIREN, B. LI, J. Y. LI, Z. Q. LIU, H. LU, X. H. MA, S. M. MARI, X. R. MENG, L. MILANO, J. MU, Z. R. PENG, P. PISTILLI, L. SAGGESE, R. SANTONICO, P. R. SHEN, C. STANESCU, L. R. SUN, S. C. SUN, A. SURDO, Y. H. TAN, S. VERNETTO, C. R. WANG, H. WANG, H. Y. WANG, Y. N. WEI, H. T. YANG, Q. K. YAO, G. C. YU, X. D. YUE, A. F. YUAN, M. ZHA, H. M. ZHANG, J. L. ZHANG, N. J. ZHANG, X. Y. ZHANG, ZHAXISANGZHU, ZHAXICIREN, Q. Q. ZHU, BERNARDINI, Paolo, DE MITRI, Ivan, MANCARELLA, Giovanni, MARSELLA, GIOVANNI, MARTELLO, Daniele, PANAREO, Marco, C., Bacci, K. Z., Bao, F., Barone, B., Bartoli, Bernardini, Paolo, S., Bussino, E., Calloni, B. Y., Cao, R., Cardarelli, S., Catalanotti, S., Cavaliere, F., Cesaroni, P., Creti, Danzengluobu, B., D'ETTORRE PIAZZOLI, DE MITRI, Ivan, M., DE VINCENZI, T., DI GIROLAMO, G., DI SCIASCIO, Z. Y., Feng, Y., Fu, X. Y., Gao, Q. X., Geng, H. W., Guo, H. H., He, M., He, Q., Huang, M., Iacovacci, N., Iucci, H. Y., Jai, C. L., Jing, F. M., Kong, H. H., Kuang, Labaciren, B., Li, J. Y., Li, Z. Q., Liu, H., Lu, X. H., Ma, Mancarella, Giovanni, S. M., Mari, Marsella, Giovanni, Martello, Daniele, X. R., Meng, L., Milano, J., Mu, Panareo, Marco, Z. R., Peng, P., Pistilli, L., Saggese, R., Santonico, P. R., Shen, C., Stanescu, L. R., Sun, S. C., Sun, A., Surdo, Y. H., Tan, S., Vernetto, C. R., Wang, H., Wang, H. Y., Wang, Y. N., Wei, H. T., Yang, Q. K., Yao, G. C., Yu, X. D., Yue, A. F., Yuan, M., Zha, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Zhaxisangzhu, Zhaxiciren, Q. Q., Zhu, Baccia, The ARGO YBJ C. o. l. l. a. b. o. r. a. t. i. o. n. C., K. Z., Baob, F., Baronec, B., Bartolic, P., Bernardinid, S., Bussinoa, E., Callonic, B. Y., Caoe, R., Cardarellif, S., Catalanottic, S., Cavalierec, F., Cesaronid, P., Cretid, Danzengluobug, B., D’Ettorrepiazzolic, M., De Vincenzia, T., Di Girolamoc, G., Di Sciascioc, Z. Y., Fengh, Y., Fue, X. Y., Gaoi, Q. X., Gengi, H. W., Guog, H. H., Hej, M., Hee, Q., Huangh, M., Iacovaccic, N., Iuccia, H. Y., Jaih, C. L., Jingj, F. M., Konge, H. H., Kuangj, Labacireng, B., Lib, J. Y., Lie, Z. Q., Liui, H., Luj, X. H., Maj, G., Mancarellad, Mari, Stefano Maria, A, G., Marsellad, D., Martellod, X. R., Mengg, L., Milanoc, J., Mui, M., Panareod, Z. R., Pengj, P., Pistillia, L., Saggesec, R., Santonicof, P. R., Shenj, C., Stanescua, L. R., Sunb, S. C., Sunb, A., Surdod, Y. H., Tanj, S., Vernettok, C. R., Wange, H., Wangj, H. Y., Wangj, Y. N., Weib, H. T., Yangj, Q. K., Yaob, G. C., Yuh, X. D., Yueb, A. F., Yuang, M., Zhaj, H. M., Zhangj, J. L., Zhangj, N. J., Zhange, X. Y., Zhange, Zhaxisangzhug, Zhaxicireng, and Q. Q., Zhuj

Subjects
Physics, Nuclear and High Energy Physics, Resistive touchscreen, Range (particle radiation), ARGO-YBJ, Detector, Cosmic ray, STRIPS, Cosmic Ray, Atomic and Molecular Physics, and Optics, Charged particle, law.invention, Nuclear physics, law, Shower detectors, Cosmic Ray, Resistive Plate Counters, Composition Model, Extensive Air Showers, Energy (signal processing), Argo
Abstract

The ARGO-YBJ experiment is currently under construction at the Yangbajing Cosmic Ray Laboratory (4300 m a.s.l.).The detector consists of a central carpet, 74 × 78 m2, made of a single layer of Resistive Plate Counters (RPCs), and surrounded by a partially instrumented guard ring for a total instrumented area of about 6700 m2. The digital read-out, performed by means of pick-up electrodes 6.7 × 62 cm2 (strip), allows to measure the charged particle number of small size air showers. The technique of counting the number of fired strips on the ARGO carpet corresponds to operate in the 10÷500 TeV energy region where both direct and indirect measurements on the primary cosmic radiation have been performed. Many composition models have been proposed by different experiments. In this work we discuss the ability of the ARGO detector to discriminate among some models.

Published
2004

3. The ARGO-YBJ experiment in Tibet

Author

A. ALOISIO, C. BACCI, K. Z. BAO, F. BARONE, B. BARTOLI, P. BERNARDINI, C. BLEVE, P. BRANCHINI, S. BUSSINO, E. CALLONI, P. CAMARRI, B. Y. CAO, R. CARDARELLI, M. CASOLINO, S. CATALANOTTI, A. CAVALIERE, S. CAVALIERE, F. CESARONI, M. CHA, P. CRETI, G. CUSIMANO, G. D'ALI STAITI, DANZENGLUOBU, V. D'ELIA, B. D'ETTORRE PIAZZOLI, M. DE VINCENZI, T. DI GIROLAMO, G. DI SCIASCIO, Z. Y. FENG, Y. FU, X. Y. GAO, Q. X. GENG, H. W. GUO, H. H. HE, Q. HUANG, M. IACOVACCI, N. IUCCI, H. Y. JAI, F. M. KONG, H. H. KUANG, LABACIREN, B. LI, J. Y. LI, B. LIBERTI, G. LIGUORI, Z. Q. LIU, H. LU, X. H. MA, G. MANCARELLA, S. M. MARI, MARSELLA, GIOVANNI, MARTELLO, Daniele, X. R. MENG, L. MILANO, T. MINEO, J. MU, L. NICASTRO, D. ORLANDO, A. PAOLONI, Z. R. PENG, P. PISTILLI, G. RASO, B. SACCO, L. SAGGESE, R. SANTONICO, L. SCARSI, P. R. SHEN, C. STANESCU, M. STORINI, L. R. SUN, S. C. SUN, A. SURDO, Y. H. TAN, P. VALLANIA, S. VERNETTO, C. R. WANG, H. WANG, H. Y. WANG, Y. N. WEI, Q. K. YAO, G. C. YU, X. D. YUE, A. F. YUAN, H. M. ZHANG, J. L. ZHANG, N. J. ZHANG, T. J. ZHANG, X. Y. ZHANG, ZHAXISANGZHU, ZHAXICIREN, Q. Q. ZHU, DE MITRI, Ivan, PANAREO, Marco, Aloisio, A., Bacci, C., Bao, K. Z., Barone, F., Bartoli, B., Bernardini, P., Bleve, C., Branchini, P., Bussino, S., Calloni, E., Camarri, P., Cao, B. Y., Cardarelli, R., Casolino, M., Catalanotti, S., Cavaliere, A., Cavaliere, S., Cesaroni, F., Cha, M., Creti, P., Cusimano, G., D'ALI STAITI, G., Danzengluobu, D'Elia, V., DE MITRI, Ivan, D'ETTORRE PIAZZOLI, B., DE VINCENZI, M., DI GIROLAMO, T., DI SCIASCIO, G., Feng, Z. Y., Fu, Y., Gao, X. Y., Geng, Q. X., Guo, H. W., H. H., He, Huang, Q., Iacovacci, M., Iucci, N., Jai, H. Y., Kong, F. M., Kuang, H. H., Labaciren, Li, B., J. Y., Li, Liberti, B., Liguori, G., Liu, Z. Q., Lu, H., X. H., Ma, Mancarella, G., Mari, S. M., Marsella, Giovanni, Martello, Daniele, Meng, X. R., Milano, L., Mineo, T., Mu, J., Nicastro, L., Orlando, D., Panareo, Marco, Paoloni, A., Peng, Z. R., Pistilli, P., Raso, G., Sacco, B., Saggese, L., Santonico, R., Scarsi, L., Shen, P. R., Stanescu, C., Storini, M., Sun, L. R., Sun, S. C., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Wang, C. R., Wang, H., Wang, H. Y., Wei, Y. N., Yao, Q. K., G. C., Yu, Yue, X. D., Yuan, A. F., Zhang, H. M., Zhang, J. L., Zhang, N. J., Zhang, T. J., Zhang, X. Y., Zhaxisangzhu, Zhaxiciren, and Zhu, Q. Q.

Subjects
Ground based detectors, Gamma-ray sources, Gamma-ray bursts, Cosmic rays
Published
2001

4. A study of the shadowing of galactic cosmic rays by the sun in a quiet phase of solar activity with the Tibet air shower array

Author

M. Amenomori, S. Ayabe, null Caidong, null Danzengluobu, L. K. Ding, Z. Y. Feng, Y. Fu, H. W. Guo, M. He, K. Hibino, N. Hotta, Q. Huang, A. X. Huo, K. Izu, H. Y. Jia, F. Kajino, K. Kasahara, Y. Katayose, null Labaciren, J. Y. Li, H. Lu, S. L. Lu, G. X. Luo, X. R. Meng, K. Mizutani, J. Mu, H. Nanjo, M. Nishizawa, M. Ohnishi, I. Ohta, T. Ouchi, Z. R. Peng, J. R. Ren, T. Saito, M. Sakata, T. Sasaki, Z. Z. Shi, M. Shibata, A. Shiomi, T. Shirai, Y. Suga, H. Sugimoto, K. Taira, Y. H. Tan, N. Tateyama, S. Torii, T. Utsugi, C. R. Wang, H. Wang, X. W. Xu, Y. Yamamoto, G. C. Yu, A. F. Yuan, T. Yuda, C. S. Zhang, H. M. Zhang, J. L. Zhang, N. J. Zhang, X. Y. Zhang, null Zhaxiciren, and null Zhaxisangzhu

Subjects
Physics, Solar minimum, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Solar cycle, Air shower, Earth's magnetic field, Space and Planetary Science, Shadow, Physics::Space Physics, Astrophysics::Solar and Stellar Astrophysics, Ultra-high-energy cosmic ray, Astrophysics::Earth and Planetary Astrophysics, Interplanetary spaceflight
Abstract

We have shown that the Sun's shadow by high energy cosmic rays moves year by year and its behavior is correlated with a time variation of the large-scale structure of the solar and interplanetary magnetic fields. The solar activity was near minimum in the period from 1996 through 1997. Using the data obtained with the Tibet air shower array, we examined the shadowing of cosmic rays by the Sun in this quiet phase of solar cycle, and found that the Sun's shadow was just in the apparent direction of the Sun, though it was observed at the position considerably away from the Sun to the south-west in the period between 1990 and 1993. It is known that the magnetic pole of equivalent solar dipole was reversed during the previous active phase, and near solar minimum the dipole was aligned with the rotating axis, preserving its N-pole on the north pole side of the Sun. This causes the solar magnetic field to shift the Sun's shadow to the east. Thus, the observed results suggest that the shift of the Sun's shadow due to the solar magnetic field was pushed back by the effect of the geomagnetic field, since the geomagnetic field always make the shadow shift to the west. We discuss the Sun's shadow observed during the period near solar minimum in 1996-1997 and compare it with the simulation results., 13 pages, 6 figures, to appear in ApJ

Published
2000

5. Measurement of air shower cores to study the cosmic ray composition in the knee energy region

Author

A. X. Huo, K. Izu, N. J. Zhang, S. L. Lu, N. Tateyama, H. W. Guo, Jia Zhang, S. Torii, X. R. Meng, Y. Fu, M. He, Z. Z. Shi, M. Amenomori, C. S. Zhang, Jieru Ren, T. Sasaki, Huaguang Wang, Masaki Nishizawa, Zhaxisangzhu, Z. Y. Feng, M. Shibata, M. Sakata, K. Hibino, T. Yuda, A. Shiomi, T. Ouchi, Y. H. Tan, Zhaxiciren, H. M. Zhang, J. Y. Li, J. Mu, I. Ohta, H. Sugimoto, H. Nanjo, C. R. Wang, Danzengluobu, Y. Yamamoto, G. C. Yu, X. W. Xu, Q. Huang, S. Ayabe, L. K. Ding, A. F. Yuan, F. Kajino, Caidong, Z. R. Peng, G. X. Luo, Labaciren, M. Ohnishi, T. Shirai, H. Y. Jia, T. Utsugi, N. Hotta, X. Y. Zhang, Hsiao-Chi Lu, K. Taira, To. Saito, K.Mizutani K.Mizutani, Katsuaki Kasahara, and Y. Katayose

Subjects
Physics, Nuclear and High Energy Physics, Astrophysics (astro-ph), Monte Carlo method, FOS: Physical sciences, Cosmic ray, Astrophysics, Nuclear physics, Air shower, Event data, Scintillation counter, Nuclear emulsion, Detector array, Energy (signal processing)
Abstract

Since 1996, a hybrid experiment consisting of an emulsion chamber and a burst detector array and the Tibet-II air shower array has been operated at Yangbajing (4300 m above sea level) in Tibet. This experiment can detect air-shower cores, called burst events, accompanied by air showers in excess of about 100 TeV. Using the burst event data observed by this experiment, we discuss the primary cosmic ray composition around the knee in comparison with the Monte Carlo simulations. In this paper, we show that all the features of burst events are wholly compatible with the heavy enriched composition in the knee energy region., 20 pages, 21 figures, to appear in Physical Review D

Published
2000

6. Results from the ARGO-YBJ test experiment ARGO-YBJ collaboration

Author

Bacci C, Bao KZ, Barone F, Bartoli B, Bernardini P, BUSSINO, Severino Angelo Maria, Calloni E, Cao BY, Cardarelli R, Catalanotti S, Cavaliere S, Cesaroni F, Creti P, Danzengluobu, Piazzoli BD, De Vincenzi M, Di Girolamo T, Di Sciascio G, Feng ZY, Fu Y, Gao XY, Geng QX, Guo HW, He HH, He M, Huang Q, Iacovacci M, Iucci N, Jai HY, Jing CL, Kong FM, Kuang HH, Labaciren, Li B, Li JY, Liu ZQ, Lu H, Ma XH, Mancarella G, MARI, Stefano Maria, Marsella G, Martello D, Meng XR, Milano L, Mu J, Panareo M, Peng ZR, Pistilli P, Santonico R, Shen PR, Stanescu C, Sun LR, Sun SC, Surdo A, Tan YH, Vernetto S, Wang CR, Wang H, Wang HY, Wei YN, Yang HT, Yao QK, Yu GC, Yue XD, Yuan AF, Zha M, Zhang HM, Zhang JL, Zhang NJ, Zhang XY, Zhaxisangzhu, Zhaxiciren, Zhu QQ, C., Bacci, K. Z., Bao, F., Barone, Bartoli, Bruno, P., Bernardini, S., Bussino, Calloni, Enrico, B. Y., Cao, R., Cardarelli, Catalanotti, Sergio, S., Cavaliere, F., Cesaroni, P., Creti, Danzengluobu, D'ETTORRE PIAZZOLI, Benedetto, M. D., Vincenzi, DI GIROLAMO, Tristano, G. D., Sciascio, Z. Y., Feng, Y., Fu, X. Y., Gao, Q. X., Geng, H. W., Guo, H. H., He, M., He, Q., Huang, Iacovacci, Michele, N., Iucci, H. Y., Jai, C. L., Jing, F. M., Kong, H. H., Kuang, Labaciren, B., Li, J. Y., Li, Z. Q., Liu, H., Lu, X. H., Ma, G., Mancarella, S. M., Mari, G., Marsella, D., Martello, X. R., Meng, L., Milano, J., Mu, M., Panareo, Z. R., Peng, P., Pistilli, R., Santonico, P. R., Shen, C., Stanescu, L. R., Sun, S. C., Sun, A., Surdo, Y. H., Tan, S., Vernetto, C. R., Wang, H., Wang, H. Y., Wang, Y. N., Wei, H. T., Yang, Q. K., Yao, G. C., Yu, X. D., Yue, A. F., Yuan, M., Zha, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Zhaxisangzhu, Zhaxiciren, Q. Q., Zhu, Bacci, C, Bao, Kz, Barone, F, Bartoli, B, Bernardini, P, Bussino, Severino Angelo Maria, Calloni, E, Cao, By, Cardarelli, R, Catalanotti, S, Cavaliere, S, Cesaroni, F, Creti, P, Piazzoli, Bd, De Vincenzi, M, Di Girolamo, T, Di Sciascio, G, Feng, Zy, Fu, Y, Gao, Xy, Geng, Qx, Guo, Hw, He, Hh, He, M, Huang, Q, Iacovacci, M, Iucci, N, Jai, Hy, Jing, Cl, Kong, Fm, Kuang, Hh, Li, B, Li, Jy, Liu, Zq, Lu, H, Ma, Xh, Mancarella, G, Mari, Stefano Maria, Marsella, G, Martello, D, Meng, Xr, Milano, L, Mu, J, Panareo, M, Peng, Zr, Pistilli, P, Santonico, R, Shen, Pr, Stanescu, C, Sun, Lr, Sun, Sc, Surdo, A, Tan, Yh, Vernetto, S, Wang, Cr, Wang, H, Wang, Hy, Wei, Yn, Yang, Ht, Yao, Qk, Yu, Gc, Yue, Xd, Yuan, Af, Zha, M, Zhang, Hm, Zhang, Jl, Zhang, Nj, Zhang, Xy, and Zhu, Qq

Subjects
AIR SHOWERS, RPCS
Abstract

A resistive plate counters (RPCs) carpet of similar to50 m(2) has been put in operation in the Yangbajing Laboratory (Tibet, P.R. China) at 4300 in a.s.l., in order to study the RPCs performance at high altitude and the detector capability of imaging the EAS disc. This test has been performed in view of an enlarged use of RPCs for the ARGO-YBJ experiment. This experiment will be devoted to a wide range of fundamental issues in cosmic rays and astroparticle physics, including in particular gamma-ray astronomy and gamma-ray bursts physics at energies greater than or equal to 100 GeV. In this paper we present and discuss the procedures adopted to calibrate the detector and reconstruct the shower direction. Results concerning many shower features as the angular distribution, the density spectrum, the time profile of the shower front, are found well consistent with the expectation. (C) 2002 Elsevier Science B.V. All rights reserved.

Published
2002

7. Study on the performance of YBJ 50m(2) RPC carpet

Author

He HH, Bacci C, Bao KZ, Barone F, Bartoli B, Bernardini P, BUSSINO, Severino Angelo Maria, Calloni E, Cardarelli R, Catalanotti S, Cavaliere S, Cesaroni F, Cha M, Creti P, Danzengluobu, Piazzoli BD, de Vincenzi M, di Girolamo T, di Sciascio G, Feng ZY, Fu Y, Gao XY, Geng QX, Guo HW, He M, Huang Q, Iacovacci M, Iucci N, Jia HY, Jing CL, Kong FM, Kuang HH, Labaciren, Li JY, Liu CQ, Lu H, Ma XH, Mancarella G, Marsella G, Martello D, Meng XR, Milano L, Mu J, Peng ZR, Pistilli P, Qu RF, Santonico R, Sbarra C, Shen PR, Stanescu C, Sun LR, Sun SC, Surdo A, Tan YH, Vernetto S, Wang CR, Wang H, Wang HY, Wei YN, Yang HT, Yao QK, Yu GC, Yue XD, Yuan AF, Zhang HM, Zhang JL, Zhang NJ, Zhang XY, Zhaxisangzhu, Zhaxiciren, Zhu QQ, MARI, Stefano Maria, H. H., He, C., Bacci, K. Z., Bao, F., Barone, B., Bartoli, P., Bernardini, S., Bussino, E., Calloni, R., Cardarelli, S., Catalanotti, S., Cavaliere, F., Cesaroni, M., Cha, P., Creti, Danzengluobu, B. D., Piazzoli, M. d., Vincenzi, T. d., Girolamo, G. d., Sciascio, Z. Y., Feng, Y., Fu, X. Y., Gao, Q. X., Geng, H. W., Guo, M., He, Q., Huang, M., Iacovacci, N., Iucci, H. Y., Jia, C. L., Jing, F. M., Kong, H. H., Kuang, Labaciren, J. Y., Li, C. Q., Liu, H., Lu, X. H., Ma, Mancarella, Giovanni, S. M., Mari, Marsella, Giovanni, Martello, Daniele, X. R., Meng, L., Milano, J., Mu, Z. R., Peng, P., Pistilli, R. F., Qu, R., Santonico, C., Sbarra, P. R., Shen, C., Stanescu, L. R., Sun, S. C., Sun, A., Surdo, Y. H., Tan, S., Vernetto, C. R., Wang, H., Wang, H. Y., Wang, Y. N., Wei, H. T., Yang, Q. K., Yao, G. C., Yu, X. D., Yue, A. F., Yuan, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Zhaxisangzhu, Zhaxiciren, Q. Q., Zhu, Bartoli, Bruno, Calloni, Enrico, Catalanotti, Sergio, D'ETTORRE PIAZZOLI, Benedetto, DI GIROLAMO, Tristano, Iacovacci, Michele, G., Mancarella, G., Marsella, D., Martello, He, Hh, Bacci, C, Bao, Kz, Barone, F, Bartoli, B, Bernardini, P, Bussino, Severino Angelo Maria, Calloni, E, Cardarelli, R, Catalanotti, S, Cavaliere, S, Cesaroni, F, Cha, M, Creti, P, Piazzoli, Bd, de Vincenzi, M, di Girolamo, T, di Sciascio, G, Feng, Zy, Fu, Y, Gao, Xy, Geng, Qx, Guo, Hw, He, M, Huang, Q, Iacovacci, M, Iucci, N, Jia, Hy, Jing, Cl, Kong, Fm, Kuang, Hh, Li, Jy, Liu, Cq, Lu, H, Ma, Xh, Mancarella, G, Mari, Stefano Maria, Marsella, G, Martello, D, Meng, Xr, Milano, L, Mu, J, Peng, Zr, Pistilli, P, Qu, Rf, Santonico, R, Sbarra, C, Shen, Pr, Stanescu, C, Sun, Lr, Sun, Sc, Surdo, A, Tan, Yh, Vernetto, S, Wang, Cr, Wang, H, Wang, Hy, Wei, Yn, Yang, Ht, Yao, Qk, Yu, Gc, Yue, Xd, Yuan, Af, Zhang, Hm, Zhang, Jl, Zhang, Nj, Zhang, Xy, Zhu, Qq, Bussino, S, DE VINCENZI, M, DI GIROLAMO, T, DI SCIASCIO, G, and Mari, Sm

Abstract

The characteristics of a 50m(2) RPC carpet(prototype of YBJ-ARGO experiment)was analyzed using its test run data. A correction method of the systematic time error is suggested, and nonuniform azimuthal angle distribution possibly due to direction reconstruction error on an asymmetric carpet is reported.

Published
2001

8. The ARGO-YBJ detector and high energy GRBs

Author

J. Mu, H.H. He, A. Cavaliere, R. Santonico, J. Su, Q. X. Geng, M. Vietri, A. Surdo, H.H. Kuang, S. M. Mari, N. Iucci, Jy Li, K.Z. Bao, M. Parisi, F Cesaroni, T. Di Girolamo, Paolo Padovani, G. Marsella, Cristian Stanescu, H.T. Yang, D. Martello, B. Bartoli, Z.Q. Liu, L.R. Sun, S.C. Sun, G.C. Yu, H.Y. Jai, Y.N. Wei, Paolo Bernardini, B.Y. Cao, S. Vernetto, L. Milano, P. Pistilli, H. M. Zhang, M. Oliviero, X.D. Yue, Denis Bastieri, M. Iacovacci, Roberta Sparvoli, Labaciren, N.J. Zhang, Hong-peng Lu, G. Mancarella, Enrico Calloni, M. Panareo, Zhaxiciren, Severino Angelo Maria Bussino, M. He, Q. Huang, P. Creti, A Morselli, C Sbarra, T.J. Zhang, P. R. Shen, C.R. Wang, X. Y. Gao, Q. Q. Zhu, X. R. Meng, G. Pellizzoni, Q.K. Yao, F.M. Kong, Dongming Mei, Danzengluobu, G. Sartori, Z.Y. Feng, BD Piazzoli, Roberto Cardarelli, Huaguang Wang, Fabrizio Barone, Y. H. Tan, J.L. Zhang, X. Y. Zhang, G. Severino, A. F. Yuan, Zhaxisangzhu, Z.R. Peng, H.Y. Wang, B. Li, Xh Ma, C. Bacci, Y Fu, G. Di Sciascio, M. De Vincenzi, S. Catalanotti, Hw Guo, R. Buonomo, C., Bacci, K. Z., Bao, F., Barone, Bartoli, Bruno, D., Bastieri, P., Bernardini, R., Buonomo, S., Bussino, Calloni, Enrico, B. Y., Cao, R., Cardarelli, Catalanotti, Sergio, A., Cavaliere, F., Cesaroni, P., Creti, Danzengluobu, D'ETTORRE PIAZZOLI, Benedetto, M., De Vincenzi, DI GIROLAMO, Tristano, G., Di Sciascio, Z. Y., Feng, Y., Fu, X. Y., Gao, Q. X., Geng, H. W., Guo, H. H., He, M., He, Q., Huang, Iacovacci, Michele, N., Iucci, H. Y., Jai, F. M., Kong, H. H., Kuang, Labaciren, B., Li, J. Y., Li, Z. Q., Liu, H., Lu, X. H., Ma, G., Mancarella, S. M., Mari, G., Marsella, D., Martello, D. M., Mei, X. R., Meng, Milano, Leopoldo, A., Morselli, J., Mu, M., Oliviero, P., Padovani, M., Panareo, M., Parisi, G., Pellizzoni, Z. R., Peng, P., Pistilli, R., Santonico, G., Sartori, C., Sbarra, G., Severino, P. R., Shen, R., Sparvoli, C., Stanescu, J., Su, L. R., Sun, S. C., Sun, A., Surdo, Y. H., Tan, S., Vernetto, M., Vietri, C. R., Wang, H., Wang, H. Y., Wang, Y. N., Wei, H. T., Yang, Q. K., Yao, G. C., Yu, X. D., Yue, A. F., Yuan, H. M., Zhang, J. L., Zhang, N. J., Zhang, T. J., Zhang, X. Y., Zhang, Zhaxisangzhu, Zhaxiciren, Q. Q., Zhu, B., Bartoli, E., Calloni, S., Catalanotti, B. D., Piazzoli, M. D., Vincenzi, T. D., Girolamo, G. D., Sciascio, M., Iacovacci, Mancarella, Giovanni, Marsella, Giovanni, Martello, Daniele, L., Milano, Panareo, Marco, Bacci, C., Bao, K. Z., Barone, F., Bartoli, B., Bastieri, D., Bernardini, P., Buonomo, R., Bussino, S., Calloni, E., Cao, B. Y., Cardarelli, R., Catalanotti, S., Cavaliere, A., Cesaroni, F., Creti, P., D'ETTORRE PIAZZOLI, B., DE VINCENZI, M., DI GIROLAMO, T., DI SCIASCIO, G., Feng, Z. Y., Fu, Y., Gao, X. Y., Geng, Q. X., Guo, H. W., He, M., Huang, Q., Iacovacci, M., Iucci, N., Jai, H. Y., Kong, F. M., Kuang, H. H., Li, B., Liu, Z. Q., Lu, H., Mancarella, G., Mari, S. M., Mei, D. M., Meng, X. R., Milano, L., Morselli, A., Mu, J., Oliviero, M., Padovani, P., Parisi, M., Pellizzoni, G., Peng, Z. R., Pistilli, P., Santonico, R., Sartori, G., Sbarra, C., Severino, G., Shen, P. R., Sparvoli, R., Stanescu, C., Su, J., Sun, L. R., Sun, S. C., Surdo, A., Tan, Y. H., Vernetto, S., Vietri, M., Wang, C. R., Wang, H., Wang, H. Y., Wei, Y. N., Yang, H. T., Yao, Q. K., Yue, X. D., Yuan, A. F., Zhang, H. M., Zhang, J. L., Zhang, N. J., Zhang, T. J., Zhang, X. Y., and Zhu, Q. Q.

Subjects
Astroparticle physics, Physics, Range (particle radiation), Physics::Instrumentation and Detectors, Large detector systems for particle and astroparticle physics, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, General Physics and Astronomy, Astronomy, Cosmic ray, Astrophysics, Radiation, gamma-ray: bursts, gamma-ray detector, Gamma Ray Burst, Observatory, Gamma-ray burst, Argo
Abstract

ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimized to study small size air showers. It consists of a layer of Resistive Plate Counters (RPCs) covering an area of similar to 6500 m(2) and will be located in the Yangbajing Laboratory (Tibet, China) at 4300 m a.s.l. ARGO-YBJ will be devoted to a wide range of fundamental issues in cosmic rays and astroparticle physics, including in particular gamma-ray astronomy and gamma-ray bursts physics in the range 10 GeV divided by 500 TeV. The sensitivity of ARGO-YBJ to detect high energy GRBs is presented.

Published
1999

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