Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM)

Seo, E. S.; Amare, Y.; Angelaszek, D.; Anthony, N.; Choi, Gwangho; Chung, М.; Copley, M.; Derome, L.; Eraud, L.; Falana, C.; Gerrety, A.; Hagenau, L.; Han, Ji Hye; Huh, H.G.; Hwang, Yong Seok; Hyun, H.J.; Jeon, H.B.; Jeon, J. A.; Jeong, Sang Jin; Kang, Sinchul; Kim, H J.; Kim, K C.; Kim, M H.; Lee, H Y.; Lee, J.; Lee, M H.; Lamb, C. R.; Liang, J. F.; Lu, Lina; Lundquist, Jon Paul; Lutz, L.; Mark, B.; Mechaca-Rocha, A.; Mernik, T.; Nester, M.; Ofoha, O.; Park, H.; Park, I H.; Park, J M.; Picot-Clémente, N.; Rostsky, S.; Smith, J.R.; Takeishi, Ryuji; Tatoli, Teresa; Walpole, P.; Weinmann, R.; Wu, Jian; Yin, Zhye; Yoon, Y. S.; Zhang, H G.

doi:10.22323/1.358.0137

Cited by 5 publications

(9 citation statements)

References 20 publications

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“…In addition, the near-inertial energy flux (Figure 4) showed strong energy input to the Kuroshio east of Taiwan, but there was no significant enhancement of NIKE under 50 m west of 122.5°E. According to Jeon (Jeon et al, 2019), after the typhoon's passage, strong NIKE existed upstream of the Kuroshio east of Taiwan at 4 m, but at 100 m, NIKE began to appear only north of 25°N. Therefore, this phenomenon may be due to advection of the upstream Kuroshio, with NIWs being carried poleward before propagating downwards.…”

Section: Temporal and Spatial Variationsmentioning

confidence: 98%

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Near-inertial waves generated by typhoon MITAG under the influence of anticyclonic eddy east of Taiwan

Zheng

Ren

et al. 2023

Front. Mar. Sci.

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Based on subsurface mooring observations and HYCOM data, a complete investigation was conducted of the near-inertial waves (NIWs) caused by Typhoon MITAG to the east of Taiwan. HYCOM data were mainly used to reveal the role played by anticyclonic eddies in the propagation of NIWs. The results show that most typhoon-generated NIWs propagate towards negative vorticity, and NIWs near the edge gradually accumulated towards the eddy center and down to 800 m. NIWs propagating through the thermocline to the deep ocean were mainly concentrated in the eddy, and the near-inertial energy flux showed a significant enhancement from 400 to 600 m. Moreover, the downwards propagation of NIWs in the eddy enhanced the kinetic energy of background flow. NIWs outside the anticyclonic eddy dissipated quickly, while inside the eddy, there were high value areas of e-folding time. Dynamic mode decomposition illustrates that the anticyclonic eddy mainly captures higher modes of NIWs, and the state of continuous energy growth of higher modes can be maintained for more than a week. In addition, NIWs can also be carried westwards by the advection of the mean background flow at the eddy’s edge.

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Section: Temporal and Spatial Variationsmentioning

confidence: 98%

“…There was a significant elevation of NIKE in the Kuroshio. The negative vorticity region of the Kuroshio acts as a waveguide, advecting NIWs to the northeast over 300 km (Rainville and Pinkel, 2004;Jeon et al, 2019).…”

mentioning

confidence: 99%

Near-inertial waves generated by typhoon MITAG under the influence of anticyclonic eddy east of Taiwan

Zheng

Ren

et al. 2023

Front. Mar. Sci.

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“…All data, including science and housekeeping data, were transferred near real-time through TDRSS. The Science Operations Center at the University of Maryland controlled the ISS-CREAM instrument by sending commands and transferring data from the Science Flight Computer on board ISS-CREAM (Kim et al 2019a;Seo et al 2019).…”

Section: Iss-cream Flightmentioning

confidence: 99%

Measurement of High-energy Cosmic-Ray Proton Spectrum from the ISS-CREAM Experiment

Choi

Seo

Aggarwal

et al. 2022

ApJ

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The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) experiment successfully recorded data for 539 days from 2017 August to 2019 February. We report the energy spectrum of cosmic-ray protons from the ISS-CREAM experiment at energies from 1.60 × 103 to 6.55 × 105 GeV. The measured spectrum deviates from a single power law. A smoothly broken power-law fit to the data, including statistical and systematic uncertainties, shows the spectral index change at 9.0 × 103 GeV from 2.57 ± 0.03 to 2.82 ± 0.02 with a significance of greater than 3σ. This bump-like structure is consistent with a spectral softening recently reported by the balloon-borne CREAM, DAMPE, and NUCLEON, but ISS-CREAM extends measurements to higher energies.

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“…The AMS-02 spectrometer consists of a permanent magnet and several instruments (subdetectors) and in particular, a it was successfully installed and activated on the Japanese Experiment Module Exposed Facility as an attached payload in 2017. The instrument is configured with complementary particle detectors capable of measuring elemental spectra for Z=1 up to Z=26 nuclei in the energy range from 1 up to 1000 TeV; as well as electrons at multi-TeV energies add the CREAM instrument [10]. -the Advanced Composition Explorer (ACE) is a satellite-based space mission that started its operation on 1998 with the aim to observe particles of solar, interplanetary, interstellar, and galactic origins, spanning the energy range from solar wind ions to galactic cosmic ray nuclei.…”

Section: Principal Operating Cosmic Ray Space Detectorsmentioning

confidence: 99%

High Energy Physics Astroparticle Experiments to Improve the Radiation Health Risk Assessment in Space Missions

Bartoloni¹,

Paolani²,

Santoro³

et al. 2022

Proceedings of the European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)

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Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM)

Cited by 5 publications

References 20 publications

Near-inertial waves generated by typhoon MITAG under the influence of anticyclonic eddy east of Taiwan

Near-inertial waves generated by typhoon MITAG under the influence of anticyclonic eddy east of Taiwan

Measurement of High-energy Cosmic-Ray Proton Spectrum from the ISS-CREAM Experiment

High Energy Physics Astroparticle Experiments to Improve the Radiation Health Risk Assessment in Space Missions

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