Results 41 to 50 of about 46,883 (245)

Quantification of Perturbation to the Daytime Lower Ionosphere From a Gamma Ray Burst Using ELF Remote Sensing

Geophysical Research Letters, Volume 52, Issue 22, 28 November 2025.
Abstract On 9 October 2022, a powerful gamma ray burst (GRB), GRB221009A, caused significant changes in the electron density of the lower ionosphere, as evidenced by VLF (3–30 kHz) radio wave observations. However, GRB221009A did not yield any observable signatures at the Schumann resonances (∼8, ∼14 Hz), which are also sensitive to the lower ...
M. Gołkowski, Z. Nieckarz, J. Mlynarczyk, M. Ostrowski, J. Kubisz, A. Michalec, J. Lichtenberger, A. Klekociuk, P. Nicholson   +8 more
wiley   +1 more source

Cosmic Ray Counting Variability From Water‐Cherenkov Detectors as a Proxy of Stratospheric Conditions in Antarctica

Earth and Space Science, Volume 12, Issue 11, November 2025.
Abstract This work examines atmospheric effects on cosmic ray counts observed by a Water‐Cherenkov detector at the Argentine Antarctic Marambio Station. We analyze the influence of ground‐level barometric pressure and geopotential height at various pressure levels on daily particle rates, finding the strongest association at 100 hPa, linked to ...
N. A. Santos, N. Gómez, S. Dasso, A. M. Gulisano, L. Rubinstein, M. Pereira, O. Areso, for the LAGO Collaboration   +7 more
wiley   +1 more source

The Dawn of Multi-Messenger Astronomy

, 2016
The recent discoveries of high-energy astrophysical neutrinos and gravitational waves have opened new windows of exploration to the Universe. Combining neutrino observations with measurements of electromagnetic radiation and cosmic rays promises to ...
Santander, Marcos
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IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica [PDF]

, 2014
The recent observation by the IceCube neutrino observatory of an astrophysical flux of neutrinos represents the "first light" in the nascent field of neutrino astronomy.
:, Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., andaz-Vélez, J. C. Dí, Anderson, T., andić, andl, A. Stöß, Anton, G., Arguelles, C., Arlen, T. C., Auffenberg, J., Axani, S., Bai, X., Bartos, I., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Becker, K. -H., BenZvi, S., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bos, F., Bose, D., Botner, O., Brayeur, L., Bretz, H. -P., Brown, A. M., Buzinsky, N., Böser, S., Casey, J., Casier, M., Cheung, E., Chirkin, D., Christov, A., Christy, B., Clark, K., Classen, L., Clevermann, F., Coenders, S., Collaboration, IceCube-Gen2, Collin, G. H., Conrad, J. M., Cowen, D. F., Daughhetee, J., Davis, J. C., Day, M., de André, J. P. A. M., De Clercq, C., De Ridder, S., de Vries, K. D., de With, M., Desiati, P., DeYoung, T., Dunkman, M., Eagan, R., Eberhardt, B., Ehrhardt, T., Eichmann, B., Eisch, J., Euler, S., Evans, J. J., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Felde, J., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Frantzen, K., Fuchs, T., Gaior, R., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gier, D., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Gonzalez, J. G., Goodman, J. A., Grant, D., Gretskov, P., Groh, J. C., Groß, A., Góra, D., Ha, C., Haack, C., Hallen, P., Hallgren, A., Halzen, F., Hanson, K., Haugen, J., Hebecker, D., Heereman, D., Heinen, D., Helbing, K., Hellauer, R., Hellwig, D., Heros, C. Pérez de los, Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huang, F., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Ishihara, A., Ismail, A. Haj, Jacobi, E., Jacobsen, J., Japaridze, G. S., Jero, K., Jlelati, O., Jones, B. J. P., Jurkovic, M., Kalekin, O., Kappes, A., Karg, T., Karle, A., Katori, T., Katz, U. F., Kauer, M., Keivani, A., Kelley, J. L., Kheirandish, A., Kiryluk, J., Klein, S. R., Kläs, J., Kohnen, G., Kolanoski, H., Koob, A., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krauss, C. B., Kriesten, A., Krings, K., Kroll, G., Kroll, M., Kunnen, J., Kurahashi, N., Kuwabara, T., Köhne, J. -H., Köpke, L., Labare, M., Lanfranchi, J. L., Larsen, D. T., Larson, M. J., Lesiak-Bzdak, M., Leuermann, M., LoSecco, J., Lünemann, J., Madsen, J., Maggi, G., Mahn, K. B. M., Marka, S., Marka, Z., Maruyama, R., Mase, K., Matis, H. S., Maunu, R., McNally, F., Meagher, K., Medici, M., Meli, A., Meures, T., Miarecki, S., Middell, E., Middlemas, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Moore, R. W., Morse, R., Nahnhauer, R., Naumann, U., Niederhausen, H., Nowicki, S. C., Nygren, D. R., O'Murchadha, A., Obertacke, A., Odrowski, S., Olivas, A., Omairat, A., Palczewski, T., Paul, L., Penek, Ö., Pepper, J. A., Pfendner, C., Pieloth, D., Pinat, E., Pinfold, J. L., Posselt, J., Price, P. B., Przybylski, G. T., Pütz, J., Quinnan, M., Rameez, M., Rawlins, K., Redl, P., Rees, I., Reimann, R., Relich, M., Resconi, E., Rhode, W., Richman, M., Riedel, B., Robertson, S., Rodrigues, J. P., Rongen, M., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Rädel, L., Saba, S. M., Sander, H. -G., Sandroos, J., Sandstrom, P., Santander, M., Sarkar, S., Schatto, K., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schukraft, A., Schulte, L., Schulz, O., Schöneberg, S., Schönwald, A., Seckel, D., Sestayo, Y., Seunarine, S., Shaevitz, M. H., Shanidze, R., Silva, A. H. Cruz, Smith, M. W. E., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stanisha, N. A., Stasik, A., Stezelberger, T., Stokstad, R. G., Strahler, E. A., Strotjohann, N. L., Ström, R., Sullivan, G. W., Söldner-Rembold, S., Taavola, H., Taboada, I., Taketa, A., Tamburro, A., Tanaka, H. K. M., Tepe, A., Ter-Antonyan, S., Terliuk, A., Teš, G., Tilav, S., Tjus, J. Becker, Toale, P. A., Tobin, M. N., Tosi, D., Tselengidou, M., Unger, E., Usner, M., Vallecorsa, S., van Eijndhoven, N., van Santen, J., Vandenbroucke, J., Vanheule, S., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Wallraff, M., Weaver, Ch., Wellons, M., Wendt, C., Westerhoff, S., Whelan, B. J., Whitehorn, N., Wichary, C., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Wren, S., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zoll, M.   +328 more
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High energy neutrino astronomy [PDF]

Nuclear Physics B - Proceedings Supplements, 1991
Invited talk at Int. Conf.
openaire   +2 more sources

NEUTRINO ASTRONOMY WITH ICECUBE [PDF]

Modern Physics Letters A, 2009
IceCube is a kilometer-scale high energy neutrino telescope under construction at the South Pole, a second-generation instrument expanding the capabilities of the AMANDA telescope. The scientific portfolio of IceCube includes the detection of neutrinos from astrophysical objects such as the sources of the cosmic rays, the search for dark matter, and ...
openaire   +2 more sources

Compressibility Function and Speed of Sound in the Non‐Commutative Quantum Hadrodynamics Type‐I Model for Neutron Stars

Astronomische Nachrichten, Volume 346, Issue 7-8, September 2025.
ABSTRACT We investigate the effects of a minimal measurable length on neutron stars, within the quantum hadrodynamics (QHD‐I) model modified by the Generalized Uncertainty Principle (GUP). Working in a deformed Poisson algebra framework, we incorporate GUP effects via a time‐invariant transformation of the phase space volume, effectively reducing the ...
João Gabriel Galli Gimenez, Dimiter Hadjimichef, César A. Zen Vasconcellos   +2 more
wiley   +1 more source

Checking T and CPT violation with sterile neutrino

Nuclear Physics B, 2016
Post LSND results, sterile neutrinos have drawn attention and motivated the high energy physics, astronomy and cosmology to probe physics beyond the standard model considering minimal 3+1 (3 active and 1 sterile) to 3+N neutrino schemes.
Yogita Pant, Sujata Diwakar, Jyotsna Singh, R.B Singh   +3 more
doaj   +1 more source

The Giant Radio Array for Neutrino Detection (GRAND) Project

SciPost Physics Proceedings, 2022
GRAND is designed to detect ultra-high-energy cosmic particles -- specially neutrinos, cosmic rays and gamma rays using radio antennas. With $\sim$20 mountainous sites around the world it will cover a total area of 200,000 km$^{2}$.
Bruno Lazarotto Lago
doaj   +1 more source

Monitoring Fracture Hydromechanical Evolution in the Lab and Field Using Unsupervised Metric Learning

Journal of Geophysical Research: Machine Learning and Computation, Volume 2, Issue 3, September 2025.
Abstract Fractures evolve in time through thermal‐hydraulic‐mechanical‐chemical (THMC) processes that alter their long‐range hydraulic transport properties and modify subsurface behavior and activities. The location of subsurface fractures makes it necessary to use remote sensing techniques such as passive or active seismic monitoring for fracture ...
David D. Nolte, Laura J. Pyrak‐Nolte, Chet Hopp   +2 more
wiley   +1 more source