Zobrazeno 1 - 10
of 626
pro vyhledávání: '"Hare B"'
Autor:
Scholten, O., Trinh, T. N. G., Buitink, S., Corstanje, A., Hare, B. M., Huege, T., Jhansi, B. V., Mulrey, K., Nelles, A., Schoorlemmer, H., Thoudam, S., Turekova, P., de Vries, K.
For high-energy cosmic-ray physics, it is imperative to determine the mass and energy of the cosmic ray that initiated the air shower in the atmosphere. This information can be extracted from the longitudinal profile of the air shower. In radio-metri
Externí odkaz:
http://arxiv.org/abs/2411.12324
Autor:
Terveer, K., Bouma, S., Buitink, S., Corstanje, A., Desmet, M., Falcke, H., Hare, B. M., Hörandel, J. R., Huege, T., Karastathis, N., Laub, P., Mulrey, K., Nelles, A., Scholten, O., Turekova, P., Thoudam, S., Trinh, G., ter Veen, S.
The LOw Frequency ARray (LOFAR) has successfully measured cosmic rays for over a decade now. With its dense core of antenna fields in the Netherlands, it is an ideal tool for studying the radio emission from extensive air showers in the $10^{16}$ eV
Externí odkaz:
http://arxiv.org/abs/2410.07681
Autor:
Mitra, P., Scholten, O., Trinh, T. N. G., Buitink, S., Bhavani, J., Corstanje, A., Desmet, M., Falcke, H., Hare, B. M., Hörandel, J. R., Huege, T., Karastathis, N., Krampah, G. K., Mulrey, K., Nelles, A., Pandya, H., Thoudam, S., de Vries, K. D., ter Veen, S.
Measuring the radio emission from cosmic ray particle cascades has proven to be a very efficient method to determine their properties such as the mass composition. Efficient modeling of the radio emission from air showers is crucial in order to extra
Externí odkaz:
http://arxiv.org/abs/2307.04242
Autor:
Buitink, S., Corstanje, A., Bhavani, J., Desmet, M., Falcke, H., Hare, B. M., Hörandel, J. R., Huege, T., Karasthatis, N., Krampah, G. K., Mitra, P., Mulrey, K., Nelles, A., Nivedita, K., Pandya, H., Rachen, J. P., Scholten, O., Thoudam, S., Trinh, G., ter Veen, S.
The current generation of air shower radio arrays has demonstrated that the atmospheric depth of the shower maximum Xmax can be reconstructed with high accuracy. These experiments are now contributing to mass composition studies in the energy range w
Externí odkaz:
http://arxiv.org/abs/2307.02907
Autor:
Corstanje, A., Buitink, S., Desmet, M., Falcke, H., Hare, B. M., Hörandel, J. R., Huege, T., Jhansi, V. B., Karastathis, N., Krampah, G. K., Mitra, P., Mulrey, K., Nelles, A., Nivedita, K., Pandya, H., Scholten, O., Terveer, K., Thoudam, S., Trinh, G., ter Veen, S.
Publikováno v:
JINST 18 P09005, 2023
Analysis of radio signals from cosmic-ray induced air showers has been shown to be a reliable method to extract shower parameters such as primary energy and depth of shower maximum. The required detailed air shower simulations take 1 to 3 days of CPU
Externí odkaz:
http://arxiv.org/abs/2306.13514
Autor:
Corstanje, A., Buitink, S., Bhavani, J., Desmet, M., Falcke, H., Hare, B. M., Hörandel, J. R., Huege, T., Karasthatis, N., Krampah, G. K., Mitra, P., Mulrey, K., Nelles, A., Nivedita, K., Pandya, H., Rachen, J. P., Scholten, O., Thoudam, S., Trinh, G., ter Veen, S.
We explore the possibilities of measuring the longitudinal profile of individual air showers beyond $X_{\rm max}$ when using very dense radio arrays such as SKA. The low-frequency part of the Square Kilometre Array, to be built in Australia, features
Externí odkaz:
http://arxiv.org/abs/2303.09249
Autor:
Winchen T., Bonardi A., Buitink S., Corstanje A., Falcke H., Hare B. M., Hörandel A., Mitra P., Mulrey K., Nelles A., Rachen J.P., Rossetto L., Schellart P., Scholten O., ter Veen S., Thoudam S., Trinh T.N.G.
Publikováno v:
EPJ Web of Conferences, Vol 216, p 04010 (2019)
The steep decrease of the flux of ultra-high energy cosmic rays (UHECR) provides a challenge to answer the long standing question about their origin and nature. A significant increase in detector volume may be achieved byemploying Earth’s moon as a
Externí odkaz:
https://doaj.org/article/ce653ddc0e044cb8be0b9bb971ad1944
Autor:
Corstanje, A., Buitink, S., Falcke, H., Hare, B. M., Hörandel, J. R., Huege, T., Krampah, G. K., Mitra, P., Mulrey, K., Nelles, A., Pandya, H., Rachen, J. P., Scholten, O., ter Veen, S., Thoudam, S., Trinh, G., Winchen, T.
Publikováno v:
Phys. Rev. D 103, 102006 (2021)
We present an updated cosmic-ray mass composition analysis in the energy range $10^{16.8}$ to $10^{18.3}$ eV from 334 air showers measured with the LOFAR radio telescope, and selected for minimal bias. In this energy range, the origin of cosmic rays
Externí odkaz:
http://arxiv.org/abs/2103.12549
Autor:
Scholten, O., Hare, B. M., Dwyer, J., Sterpka, C., Kolmašová, I., Santolík, O., Lán, R., Uhlíř, L., Buitink, S., Corstanje, A., Falcke, H., Huege, T., Hörandel, J. R., Krampah, G. K., Mitra, P., Mulrey, K., Nelles, A., Pandya, H., Pel, A., Rachen, J. P., Trinh, T. N. G., ter Veen, S., Thoudam, S., Winchen, T.
With LOFAR we have been able to image the development of lightning flashes with meter-scale accuracy and unprecedented detail. We discuss the primary steps behind our most recent lightning mapping method. To demonstrate the capabilities of our techni
Externí odkaz:
http://arxiv.org/abs/2007.03934
Autor:
Hare, B. M., Scholten, O., Dwyer, J., Ebert, U., Nijdam, S., Bonardi, A., Buitink, S., Corstanje, A., Falcke, H., Huege, T., Hörandel, J. R., Krampah, G. K., Mitra, P., Mulrey, K., Neijzen, B., Nelles, A., Pandya, H., Rachen, J. P., Rossetto, L., Trinh, T. N. G., ter Veen, S., Winchen, T.
Publikováno v:
Phys. Rev. Lett. 124, 105101 (2020)
We use the Low Frequency ARray (LOFAR) to probe the dynamics of the stepping process of negatively-charged plasma channels (negative leaders) in a lightning discharge. We observe that at each step of a leader, multiple pulses of VHF (30~--~80 MHz) ra
Externí odkaz:
http://arxiv.org/abs/2007.03231