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Träfflista för sökning "WFRF:(Jones Michael P.) srt2:(2020-2024)"

Search: WFRF:(Jones Michael P.) > (2020-2024)

  • Result 1-10 of 101
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1.
  • 2021
  • swepub:Mat__t
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2.
  • Niemi, MEK, et al. (author)
  • 2021
  • swepub:Mat__t
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3.
  • Kanai, M, et al. (author)
  • 2023
  • swepub:Mat__t
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4.
  • Murari, A., et al. (author)
  • A control oriented strategy of disruption prediction to avoid the configuration collapse of tokamak reactors
  • 2024
  • In: Nature Communications. - 2041-1723 .- 2041-1723. ; 15:1
  • Journal article (peer-reviewed)abstract
    • The objective of thermonuclear fusion consists of producing electricity from the coalescence of light nuclei in high temperature plasmas. The most promising route to fusion envisages the confinement of such plasmas with magnetic fields, whose most studied configuration is the tokamak. Disruptions are catastrophic collapses affecting all tokamak devices and one of the main potential showstoppers on the route to a commercial reactor. In this work we report how, deploying innovative analysis methods on thousands of JET experiments covering the isotopic compositions from hydrogen to full tritium and including the major D-T campaign, the nature of the various forms of collapse is investigated in all phases of the discharges. An original approach to proximity detection has been developed, which allows determining both the probability of and the time interval remaining before an incoming disruption, with adaptive, from scratch, real time compatible techniques. The results indicate that physics based prediction and control tools can be developed, to deploy realistic strategies of disruption avoidance and prevention, meeting the requirements of the next generation of devices.
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9.
  • Fenstermacher, M.E., et al. (author)
  • DIII-D research advancing the physics basis for optimizing the tokamak approach to fusion energy
  • 2022
  • In: Nuclear Fusion. - : IOP Publishing. - 0029-5515 .- 1741-4326. ; 62:4
  • Journal article (peer-reviewed)abstract
    • DIII-D physics research addresses critical challenges for the operation of ITER and the next generation of fusion energy devices. This is done through a focus on innovations to provide solutions for high performance long pulse operation, coupled with fundamental plasma physics understanding and model validation, to drive scenario development by integrating high performance core and boundary plasmas. Substantial increases in off-axis current drive efficiency from an innovative top launch system for EC power, and in pressure broadening for Alfven eigenmode control from a co-/counter-I p steerable off-axis neutral beam, all improve the prospects for optimization of future long pulse/steady state high performance tokamak operation. Fundamental studies into the modes that drive the evolution of the pedestal pressure profile and electron vs ion heat flux validate predictive models of pedestal recovery after ELMs. Understanding the physics mechanisms of ELM control and density pumpout by 3D magnetic perturbation fields leads to confident predictions for ITER and future devices. Validated modeling of high-Z shattered pellet injection for disruption mitigation, runaway electron dissipation, and techniques for disruption prediction and avoidance including machine learning, give confidence in handling disruptivity for future devices. For the non-nuclear phase of ITER, two actuators are identified to lower the L-H threshold power in hydrogen plasmas. With this physics understanding and suite of capabilities, a high poloidal beta optimized-core scenario with an internal transport barrier that projects nearly to Q = 10 in ITER at ∼8 MA was coupled to a detached divertor, and a near super H-mode optimized-pedestal scenario with co-I p beam injection was coupled to a radiative divertor. The hybrid core scenario was achieved directly, without the need for anomalous current diffusion, using off-axis current drive actuators. Also, a controller to assess proximity to stability limits and regulate β N in the ITER baseline scenario, based on plasma response to probing 3D fields, was demonstrated. Finally, innovative tokamak operation using a negative triangularity shape showed many attractive features for future pilot plant operation.
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10.
  • Akiyama, Kazunori, et al. (author)
  • The persistent shadow of the supermassive black hole of M 87: I. Observations, calibration, imaging, and analysis*
  • 2024
  • In: Astronomy and Astrophysics. - 0004-6361 .- 1432-0746. ; 681
  • Journal article (peer-reviewed)abstract
    • In April 2019, the Event Horizon Telescope (EHT) Collaboration reported the first-ever event-horizon-scale images of a black hole, resolving the central compact radio source in the giant elliptical galaxy M 87. These images reveal a ring with a southerly brightness distribution and a diameter of ∼42 μas, consistent with the predicted size and shape of a shadow produced by the gravitationally lensed emission around a supermassive black hole. These results were obtained as part of the April 2017 EHT observation campaign, using a global very long baseline interferometric radio array operating at a wavelength of 1.3 mm. Here, we present results based on the second EHT observing campaign, taking place in April 2018 with an improved array, wider frequency coverage, and increased bandwidth. In particular, the additional baselines provided by the Greenland telescope improved the coverage of the array. Multiyear EHT observations provide independent snapshots of the horizon-scale emission, allowing us to confirm the persistence, size, and shape of the black hole shadow, and constrain the intrinsic structural variability of the accretion flow. We have confirmed the presence of an asymmetric ring structure, brighter in the southwest, with a median diameter of 43.3-3.1+1.5 μas. The diameter of the 2018 ring is remarkably consistent with the diameter obtained from the previous 2017 observations. On the other hand, the position angle of the brightness asymmetry in 2018 is shifted by about 30 relative to 2017. The perennial persistence of the ring and its diameter robustly support the interpretation that the ring is formed by lensed emission surrounding a Kerr black hole with a mass ∼6.5× 109M. The significant change in the ring brightness asymmetry implies a spin axis that is more consistent with the position angle of the large-scale jet.
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  • Result 1-10 of 101
Type of publication
journal article (92)
research review (5)
doctoral thesis (1)
Type of content
peer-reviewed (96)
other academic/artistic (2)
Author/Editor
Kaaks, Rudolf (9)
Wolk, Alicja (9)
Patel, A (8)
Lee, S (7)
Walker, R. (6)
Marshall, R. (6)
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Clark, M. (6)
Lewis, J (6)
Ali, M (6)
Davies, A (6)
Thomas, J. (6)
Johnson, R (6)
King, D. (6)
Linet, Martha (6)
Li, Y. (5)
Price, D. (5)
Silva, J. (5)
Garcia, J. (5)
Chang-Claude, Jenny (5)
Young, R. (5)
Khan, K (5)
Baylor, L (5)
Bolzonella, T (5)
Bonnin, X (5)
Giacomelli, L (5)
Giroud, C (5)
Gohil, P (5)
Groth, M (5)
Joffrin, E (5)
Lehnen, M (5)
Luce, T (5)
Moreira, L (5)
Nocente, M (5)
Ongena, J (5)
Pereira, R (5)
Pironti, A (5)
Pitts, R (5)
Ruiz, M (5)
Saarelma, S (5)
Salewski, M (5)
Salmi, A (5)
Sauter, O (5)
Tala, T (5)
Vega, J (5)
Walker, M (5)
Wiesen, S (5)
Zakharov, L (5)
Zerbini, M (5)
Wang, Qin (5)
Edwards, J (5)
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University
Karolinska Institutet (28)
Uppsala University (22)
Stockholm University (22)
Lund University (20)
Chalmers University of Technology (15)
University of Gothenburg (14)
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Linköping University (14)
Umeå University (13)
Royal Institute of Technology (6)
Luleå University of Technology (2)
Örebro University (2)
University of Gävle (1)
University West (1)
Malmö University (1)
Stockholm School of Economics (1)
Mid Sweden University (1)
Karlstad University (1)
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Language
English (101)
Research subject (UKÄ/SCB)
Medical and Health Sciences (52)
Natural sciences (40)
Engineering and Technology (9)
Social Sciences (9)

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