Correction: Tabassum Abbasi et al., Modelling Methane and Nitrous Oxide Emissions from Rice Paddy Wetlands in India Using Artificial Neural Networks (ANNs). Water 2019, 11, 2169

Abbasi, Tabassum; Abbasi, Tasneem; Luithui, Chirchom; Abbasi, S. A.

doi:10.3390/w12030751

Cited by 5 publications

(4 citation statements)

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“…Several additional indications of cosmic-ray energyspectrum anisotropy have also recently been observed by the TA experiment [8,9]. A difference in the spectral cut-offs above and below the declination δ = 24.8 • has been reported in [8]: the high and low declination band cutoffs were found to be 10 19.85 +0.03 −0.03 eV and 10 19.59 +0.05 −0.07 eV, respectively. The difference was updated in [10].…”

Section: Introductionmentioning

confidence: 64%

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Current status of the TAx4 surface detectors

Kido¹

2023

EPJ Web Conf.

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Telescope Array (TA) is the largest ultrahigh-energy cosmic-ray (UHECR) observatory in the northern hemisphere. It explores the origin of UHECRs using a surface detector (SD) array, covering approximately 700 km2, and a fluorescence detector (FD) stations viewing the skies above the array. TA has found evidence for a cluster of cosmic rays with energies greater than 57 EeV known as a HotSpot. Recently, TA has obtained additional evidence for an excess of cosmic rays with energies above 1019.4 eV and also found implications of spectrum anisotropy. An expanded SD array and FD stations called TAx4 experiment was designed to increase the data collection rate at the highest energies to confirm the anisotropies with more data. We have constructed and deployed more than half of the SDs for the TAx4 experiment and began stable data taking operations. We present TAx4 SD’s current status.

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Section: Introductionmentioning

confidence: 64%

“…More recently, an additional excess of events with energies greater than 10 19. 4 eV with a significance of more than 3σ in the direction of the Perseus-Pisces supercluster was also found [7].…”

Section: Introductionmentioning

confidence: 67%

Current status of the TAx4 surface detectors

Kido¹

2023

EPJ Web Conf.

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“…The amplitudes at select laboratories are shown in Figure 6 with experimental data added where available. Because the IceCube detector is located at the South Pole it observes the most extreme muon and neutrino seasonal variations on the planet [23,31].…”

Section: William Woodleymentioning

confidence: 99%

Challenges and Opportunities for Predicting Muons in Underground and Underwater Labs Using MUTE

Woodley¹,

Fedynitch²,

Piro³

2023

Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)

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“…Figure 7: P-ONE simulation results for both 10-string and 70-string geometries. (a) Effective area at trigger level (minimum three PMTs hit in 10 ns) as a function of neutrino energy in comparison to an IceCube reference [19] (b) P-ONE angular resolution as a function of muon energy shown together with an IceCube reference[22]. The study is based on simulated data for both 10-and 70-string geometries, and the labels indicate the used inter-module/line/cluster spacing.…”

mentioning

confidence: 99%

Pacific Ocean Neutrino Experiment: Expected performance of the first cluster of strings

Henningsen¹

2023

Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)

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The Pacific Ocean Neutrino Experiment (P-ONE) is a proposed large-volume neutrino telescope in the Northeast Pacific Ocean, off the coast of Vancouver Island, Canada. With more than one cubic-kilometer of instrumented deep sea volume, P-ONE will target measuring high-energy neutrinos to shed light on the nature of astrophysical accelerators and the cosmos. With low expected scattering in the deep ocean, water-based detectors theoretically allow for sub-degree event resolution but carry various challenges. With changing ocean currents, and an abundance of organic matter, the detector geometry, water optical properties, and bioluminescent light background vary with time. This dynamic environment of the deep ocean requires rugged detector technologies and multiple, precise calibration and monitoring systems in order to enable and maintain the detector's full scientific potential. In cooperation with Ocean Networks Canada (ONC), the P-ONE collaboration aims to develop long-lived, deep-sea detector systems which target continuous and precise monitoring to overcome these challenges. The first mooring of P-ONE will be deployed between 2024 and 2025, and will provide first insights into the performance of the developed detector systems. Following this first step, this work summarizes the ongoing efforts of the P-ONE collaboration targeting the development, simulation and operation of the first cluster of strings, and will present the expected performance of the calibration systems and physics potential.

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Correction: Tabassum Abbasi et al., Modelling Methane and Nitrous Oxide Emissions from Rice Paddy Wetlands in India Using Artificial Neural Networks (ANNs). Water 2019, 11, 2169

Abstract: The authors wish to make the following corrections to this paper [...]

Cited by 5 publications

References 1 publication

Current status of the TAx4 surface detectors

Current status of the TAx4 surface detectors

Challenges and Opportunities for Predicting Muons in Underground and Underwater Labs Using MUTE

Pacific Ocean Neutrino Experiment: Expected performance of the first cluster of strings

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