Zobrazeno 1 - 10
of 6 629
pro vyhledávání: '"Wang, S. H."'
Autor:
Ali, S., Allison, P., Archambault, S., Beatty, J. J., Besson, D. Z., Bishop, A., Chen, P., Chen, Y. C., Clark, B. A., Clay, W., Connolly, A., Couberly, K., Cremonesi, L., Cummings, A., Dasgupta, P., Debolt, R., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Flaherty, J., Friedman, E., Gaior, R., Giri, P., Hanson, J., Harty, N., Hoffman, K. D., Huang, J. J., Huang, M. -H., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Kim, K. -C., Kim, M. -C., Kravchenko, I., Krebs, R., Kuo, C. Y., Kurusu, K., Latif, U. A., Liu, C. H, Liu, T. C., Luszczak, W., Mase, K., Muzio, M. S., Nam, J., Nichol, R. J., Novikov, A., Nozdrina, A., Oberla, E., Pan, Y., Pfendner, C., Punsuebsay, N., Roth, J., Salcedo-Gomez, A., Seckel, D., Seikh, M. F. H., Shaio, Y. -S., Smith, D., Toscano, S., Torres, J., Touart, J., van Eijndhoven, N., Vieregg, A., Wang, M. -Z., Wang, S. -H., Wissel, S. A., Xie, C., Yoshida, S., Young, R.
We develop an in-situ index of refraction profile using the transit time of radio signals broadcast from an englacial transmitter to 2-5 km distant radio-frequency receivers, deployed at depths up to 200 m. Maxwell's equations generally admit two ray
Externí odkaz:
http://arxiv.org/abs/2406.00857
Autor:
Seikh, M. F. H, Besson, D. Z., Ali, S., Allison, P., Archambault, S., Beatty, J. J., Bishop, A., Chen, P., Chen, Y. C., Clark, B. A., Clay, W., Connolly, A., Couberly, K., Cremonesi, L., Cummings, A., Dasgupta, P., Debolt, R., De Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Flaherty, J., Friedman, E., Gaior, R., Giri, P., Hanson, J., Harty, N., Hendricks, B., Hoffman, K. D., Huang, J. J., Huang, M. H. A., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Kim, K. C., Kim, M. C., Kravchenko, I., Krebs, R., Kuo, C. Y., Kurusu, K., Latif, U. A., Liu, C. H., Liu, T. C., Luszczak, W., Mase, K., Muzio, M. S., Nam, J., Nichol, R. J., Novikov, A., Nozdrina, A., Oberla, E., Pan, Y., Pfendner, C., Punsuebsay, N., Roth, J., Salcedo-Gomez, A., Seckel, D., Seikh, M. F. H., Shiao, Y. S., Smith, D. J. B., Toscano, S., Torres, J., Touart, J., van Eijndhoven, N., Varner, G. S., Vieregg, A., Wang, M. Z., Wang, S. H., Wissel, S. A., Xie, C., Yoshida, S., Young, R.
Publikováno v:
PoS ICRC2023 (2023) 1163
The Askaryan Radio Array Station 1 (A1), the first among five autonomous stations deployed for the ARA experiment at the South Pole, is a unique ultra-high energy neutrino (UHEN) detector based on the Askaryan effect that uses Antarctic ice as the de
Externí odkaz:
http://arxiv.org/abs/2308.07292
Autor:
ARIANNA Collaboration, Anker, A., Baldi, P., Barwick, S. W., Beise, J., Besson, D. Z., Chen, P., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Liu, J., Nam, J., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Rice-Smith, R., Tatar, J., Terveer, K., Wang, S. -H, Zhao, L.
The ARIANNA experiment is an Askaryan radio detector designed to measure high-energy neutrino induced cascades within the Antarctic ice. Ultra-high-energy neutrinos above $10^{16}$ eV have an extremely low flux, so experimental data captured at trigg
Externí odkaz:
http://arxiv.org/abs/2307.07188
Autor:
Wang, S. H.1,2, Tu, P. A.1, Liao, H. H.1, Chen, Y. K.2, Huang, T. Y.3, Yang, Y. K.3, Tsai, M. W.3, Yu, H. K.3, Liu, Y. T.3, Hsu, J. T.2 jthsu@ntu.edu.tw
Publikováno v:
Indian Journal of Animal Research. Jul2024, Vol. 58 Issue 7, p1157-1164. 8p.
Autor:
Allison, P., Archambault, S., Beatty, J. J., Besson, D. Z., Bishop, A., Chen, C. C., Chen, C. H., Chen, P., Chen, Y. C., Clark, B. A., Clay, W., Connolly, A., Cremonesi, L., Dasgupta, P., Davies, J., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Flaherty, J., Friedman, E., Gaior, R., Hanson, J., Harty, N., Hendricks, B., Hoffman, K. D., Hong, E., Hsu, S. Y., Hu, L., Huang, J. J., Huang, M. -H., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Kim, K. -C., Kim, M. -C., Kravchenko, I., Krebs, R., Ku, Y., Kuo, C. Y., Kurusu, K., Landsman, H., Latif, U. A., Li, C. -J., Liu, T. -C., Lu, M. -Y., Madison, B., Madison, K., Mase, K., Meures, T., Nam, J., Nichol, R. J., Nir, G., Novikov, A., Nozdrina, A., Oberla, E., Osborn, J., Pan, Y., Pfendner, C., Punsuebsay, N., Roth, J., Seckel, D., Seikh, M. F. H., Shiao, Y. -S., Shultz, A., Smith, D., Toscano, S., Torres, J., Touart, J., van Eijndhoven, N., Varner, G. S., Vieregg, A., Wang, M. -Z., Wang, S. -H., Wang, Y. H., Wissel, S. A., Xie, C., Yoshida, S., Young, R.
In the pursuit of the measurement of the still-elusive ultrahigh-energy (UHE) neutrino flux at energies of order EeV, detectors using the in-ice Askaryan radio technique have increasingly targeted lower trigger thresholds. This has led to improved tr
Externí odkaz:
http://arxiv.org/abs/2202.07080
Autor:
Prechelt, R., Wissel, S. A., Romero-Wolf, A., Burch, C., Gorham, P. W., Allison, P., Alvarez-Muñiz, J., Banerjee, O., Batten, L., Beatty, J. J., Belov, K., Besson, D. Z., Binns, W. R., Bugaev, V., Cao, P., Carvalho Jr., W., Chen, C. H., Chen, P., Chen, Y., Clem, J. M., Connolly, A., Cremonesi, L., Dailey, B., Deaconu, C., Dowkontt, P. F., Fox, B. D., Gordon, J. W. H., Hast, C., Hill, B., Hsu, S. Y., Huang, J. J., Hughes, K., Hupe, R., Israel, M. H., Liewer, K. M., Liu, T. C., Ludwig, A. B., Macchiarulo, L., Matsuno, S., McBride, K., Miki, C., Mulrey, K., Nam, J., Naudet, C., Nichol, R. J., Novikov, A., Oberla, E., Prohira, S., Rauch, B. F., Ripa, J., Roberts, J. M., Rotter, B., Russell, J. W., Saltzberg, D., Seckel, D., Schoorlemmer, H., Shiao, J., Stafford, S., Stockham, J., Stockham, M., Strutt, B., Sutherland, M. S., Varner, G. S., Vieregg, A. G., Wang, N., Wang, S. H., Zas, E., Zeolla, A.
We study in detail the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to possible $\nu_\tau$ point source fluxes detected via $\tau$-lepton-induced air showers. This investigation is framed around the observation of four upward-goin
Externí odkaz:
http://arxiv.org/abs/2112.07069
Autor:
ARIANNA Collaboration, Anker, A., Baldi, P., Barwick, S. W., Beise, J., Besson, D. Z., Bouma, S., Cataldo, M., Chen, P., Gaswint, G., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Liu, J., Magnuson, M., McAleer, S., Meyers, Z. M., Nam, J., Nelles, A., Novikov, A., Paul, M. P., Persichilli, C., Plaisier, I., Pyras, L., Rice-Smith, R., Tatar, J., Wang, S. -H, Welling, C., Zhao, L.
Publikováno v:
JINST 17 P03007 (2022)
The ARIANNA experiment is an Askaryan detector designed to record radio signals induced by neutrino interactions in the Antarctic ice. Because of the low neutrino flux at high energies ($E > 10^{16} $), the physics output is limited by statistics. He
Externí odkaz:
http://arxiv.org/abs/2112.01031
Autor:
ARIANNA Collaboration, Anker, A., Baldi, P., Barwick, S. W., Beise, J., Besson, D. Z., Bouma, S., Cataldo, M., Chen, P., Gaswint, G., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Liu, J., Magnuson, M., McAleer, S., Meyers, Z. S., Nam, J., Nelles, A., Novikov, A., Paul, M. P., Persichilli, C., Plaisier, I., Pyras, L., Rice-Smith, R., Tatar, J., Wang, S. -H, Welling, C., Zhao, L.
Publikováno v:
JCAP04(2022)022
The ARIANNA detector is designed to detect neutrinos with energies above $10^{17}$eV. Due to the similarities in generated radio signals, cosmic rays are often used as test beams for neutrino detectors. Some ARIANNA detector stations are equipped wit
Externí odkaz:
http://arxiv.org/abs/2112.01501
Publikováno v:
Metalurgija. 2024, Vol. 63 Issue 2, p187-190. 4p.
Autor:
Chen, T., Li, L., Zhang, X. -X., Wang, C., Jin, X. -B., Ma, Q. -M., Xu, J. -Y., He, Z. -H., Li, H., Xiao, S. -G., Wang, X. -Z., Shen, X. -H., Zhang, X. -M., Li, H. -B., Zeren, Z. -M., Huang, J. -P., Huang, F. -Q., Che, S., Zou, Z. -M., Xiong, P., Liu, J., Zhang, L. -Q., Guo, Q., Roth, I., Makhmutov, V. S., Liu, Yong, Huang, Z. -H., Luo, J., Jiang, X. -J., Dai, L., Duan, S. -P., Peng, X. -D., Hu, X., Wu, H., Ti, S., Zeng, C., Song, J. -J., Xiao, F., Guo, J. -G., Yao, L., Du, A. -M., Wei, Y., Yuan, H., Wang, S., Cui, H. -Y., Li, C., Liu, Y., Yang, J., Sun, Q., Su, J. -F., Li, W., Zhang, Y. -C., Li, D. -L., Wang, S. -H., Cai, C. -L., Yan, G. -Q.
A promising perspective is presented that humans can provide hourly warning for strong land earthquakes (EQs, Ms6). Two important atmospheric electrostatic signal features are described. A table that lists 9 strong land EQs with shock time, epicenter
Externí odkaz:
http://arxiv.org/abs/2106.12721