Showing 1 - 7 results of 7 for search 'Burns Mantle', query time: 0.07s Refine Results
  1. 1

    GRAVITY ANOMALIES OF THE CRUST AND UPPER MANTLE FOR CENTRAL AND SOUTH ASIA by V. N. Senachin, A. A. Baranov

    Published 2016-12-01
    “…The map of calculated crustal gravity anomalies also shows submarine ridges (+280 mGal) that trend from south to north and seem to trace ‘hot spots’ that burn through the lithospheric plate (Fig. 7).Gravitational anomalies in the mantle were calculated by subtracting the gravity effect of the crust from the observed gravity field. …”
    Get full text
    Article
  2. 2
  3. 3

    Combustion behavior of single iron particles-part I: An experimental study in a drop-tube furnace under high heating rates and high temperatures by Aidin Panahi, Di Chang, Martin Schiemann, Aki Fujinawa, Xiaocheng Mi, Jeffrey M. Bergthorson, Yiannis A. Levendis

    Published 2023-03-01
    “…There was evidence of formation of envelope micro-flames around iron particles (nanometric particle mantles) during the bright stage of combustion. As the burning iron particles fell by gravity in the DTF, contrails of these fine particles formed in their wakes. …”
    Get full text
    Article
  4. 4
  5. 5

    Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei by Lorenzo Roberti, Marco Limongi, Alessandro Chieffi

    Published 2024-01-01
    “…Our main findings may be summarized as follows: (a) rotating models above Z = 0 are able to produce nuclei up to the neutron closure shell N = 50, and in a few cases up to N = 82; (b) rotation drastically inhibits the penetration of the He convective shell in the H-rich mantle, a phenomenon often found in zero metallicity nonrotating massive stars; (c) vice versa, rotation favors the penetration of the O convective shell in the C-rich layers with the consequence of significantly altering the yields of the products of the C, Ne, and O burning; (d) none of the models that reach the critical velocity while in H burning lose more the 1 M _⊙ in this phase; (e) conversely, almost all models able to reach their Hayashi track exceed the Eddington luminosity and dynamically lose almost all their H-rich mantle. …”
    Get full text
    Article
  6. 6

    Evaluation of Various Forms of Geothermal Energy Release in the Beijing Region, China by Zebin Luo, Mingbo Yang, Xiaocheng Zhou, Guiping Liu, Jinlong Liang, Zhe Liu, Peixue Hua, Jingchen Ma, Leyin Hu, Xiaoru Sun, Bowen Cui, Zhiguo Wang, Yuxuan Chen

    Published 2024-02-01
    “…The heat sources are upper mantle heat, radioactive heat in granite, and residual heat from magma cooling. …”
    Get full text
    Article
  7. 7

    Seismic Signatures of the 12C(α, γ)16O Reaction Rate in White Dwarf Models with Overshooting by Morgan T. Chidester, F. X. Timmes, Ebraheem Farag

    Published 2023-01-01
    “…These signatures hold because the resonating mantle region, encompassing ≃0.2 M _⊙ in a typical ≃0.6 M _⊙ WD model, still undergoes radiative helium burning during the evolution to a WD. …”
    Get full text
    Article