Model for the curvature response of the CDF II drift chamber by Ashutosh Vijay Kotwal

“…Constraints on the model parameters are obtained from cosmic-ray data and from information published by CDF in the context of the W boson mass measurement. …”
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JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7–14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe by Yuichi Harikane, Akio K. Inoue, Richard S. Ellis, Masami Ouchi, Yurina Nakazato, Naoki Yoshida, Yoshiaki Ono, Fengwu Sun, Riku A. Sato, Giovanni Ferrami, Seiji Fujimoto, Nobunari Kashikawa, Derek J. McLeod, Pablo G. Pérez-González, Marcin Sawicki, Yuma Sugahara, Yi Xu, Satoshi Yamanaka, Adam C. Carnall, Fergus Cullen, James S. Dunlop, Eiichi Egami, Norman Grogin, Yuki Isobe, Anton M. Koekemoer, Nicolas Laporte, Chien-Hsiu Lee, Dan Magee, Hiroshi Matsuo, Yoshiki Matsuoka, Ken Mawatari, Kimihiko Nakajima, Minami Nakane, Yoichi Tamura, Hiroya Umeda, Hiroto Yanagisawa

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Virtual Joint Field Campaign: a framework of synthetic landscapes to assess multiscale measurement methods of water storage by T. Francke, C. Brogi, A. Duarte Rocha, M. Förster, M. Heistermann, M. Köhli, D. Rasche, M. Reich, P. Schattan, P. Schattan, L. Scheiffele, M. Schrön

“…<p>Various methods are available to measure water storage across different landscape compartments, e.g. cosmic-ray neutron sensing, remote sensing, or hydrogravimetry. …”
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A Model for Cosmic Magnetic Field Amplification: Effects of Pressure Anisotropy Perturbations by Ji-Hoon Ha

“…By considering the balance between isotropization through magnetic field amplification and anisotropy generation by external sources such as turbulence and anisotropic cosmic-ray scattering, it is reasonable to assume that the system evolves around an equilibrium anisotropy value. …”
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Modeling of the Near-Earth Low-Energy Antiproton Fluxes by U. B. Jayanthi, A. A. Gusev

“…Simulated flux of the trapped antiprotons in the inner magnetosphere due to galactic cosmic ray (GCR) interactions with the atmospheric constituents exceeds the galactic antiproton flux up to several orders. …”
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Recent results from NA61/SHINE by Rybicki Andrzej

“…Its research program includes studies of strong interactions as well as reference measurements for neutrino and cosmic-ray physics. A significant advantage of NA61/SHINE over collider experiments is its extended coverage of phase space available for hadron production. …”
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Kinematic Approach to the 24th Solar Cycle Prediction by Vladimir Kaftan

“…Time series of solar and cosmic ray monthly mean indices were received from web resources of international data centers. …”
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Extended Linear and Nonlinear Lorentz Transformations and Superluminality by Dara Faroughy

“…Particle energies are evaluated in this scenario at c for several particles, including the neutrinos, and are auspiciously found to be below the GKZ energy cutoff and in compliance with a host of worldwide ultrahigh energy cosmic ray data. Section 3 presents two broad scenarios involving a number of novel nonlinear LTs (NLTs) featuring small Lorentz invariance violations (LIVs), as well as resurrecting the notion of simultaneity for limited spacetime events as perceived by two observers in URM. …”
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The interplay of geology, climate and tectonics on river incision: the example of the High Verdon Gorges, Southwestern French Alps by Cardinal, Thibaut, Petit, Carole, Rolland, Yann, Schwartz, Stéphane, Valla, Pierre Gaston, Scalabrino, Bruno, Audin, Laurence, Bertauts, Maxime, Zerathe, Swann, Thiéblemont, Denis, Braucher, Régis, Team, ASTER

“…We collected 24 samples along three polished surfaces for Cosmic Ray Exposure (CRE) $^{36}$Cl dating, which allowed us to constrain short-term incision rates ranging from 0.06 to 0.2 mm/yr between 60 and 15 ka. …”
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Intelligent methods for natural data analysis: application to space weather by O.V. Mandrikova

“…The efficiency of network sharing an Autoencoder with adaptive wavelet threshold filtering is shown in the problem of anomaly detection in cosmic ray flux intensity data.…”
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Observing Supernova Neutrino Light Curves with Super-Kamiokande. V. Distance Estimation with Neutrinos by Yudai Suwa, Akira Harada, Masamitsu Mori, Ken’ichiro Nakazato, Ryuichiro Akaho, Masayuki Harada, Yusuke Koshio, Fumi Nakanishi, Kohsuke Sumiyoshi, Roger A. Wendell

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Monster Radio Jet (>66 kpc) Observed in Quasar at z ∼​​​​​ 5 by Anniek J. Gloudemans, Frits Sweijen, Leah K. Morabito, Emanuele Paolo Farina, Kenneth J. Duncan, Yuichi Harikane, Huub J. A. Röttgering, Aayush Saxena, Jan-Torge Schindler

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