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  • English  (3)
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  • 1
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-07-25
    Description: One of the characteristics that distinguishes the storm-time plasma sheet from the non-storm-time plasma sheet is the enhanced contribution of ionospheric heavy ions, particularly O+. Enhanced outflow is observed throughout the auroral oval during a storm, from the dayside cusp region to the nightside auroral region. The dayside cusp outflow can be enhanced prior to the storm main phase, particularly in association with coronal mass ejections, and it then convects through the lobe to reach the plasma sheet. The nightside aurora shows high fluxes of bursty outflow during the main phase. Recent results have shown that the source of the near-earth plasma sheet can change dramatically during storms in response to changes in the interplanetary magnetic field. This talk will use a combination of statistical measurements from FAST/TEAMS in the auroral regions with recent measurements from the Arase, MMS and Van Allen Probes satellites to address the conditions that drive the outflow and bring it into the plasma sheet. The goal is to understand how the system-level drivers enhance the ionospheric contribution, and how that affects the geomagnetic storms.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 2
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-08-09
    Description: Magnetospheric processes and instabilities are significantly impacted by the ion composition within the magnetosphere. During geomagnetic storm times, the O+/H+ density ratio increases in the plasma sheet. The increased population is then convected adiabatically inward to feed the storm time ring current. It is still not understood which of the competing sources is the main plasma sheet O+ source. Dayside cusp and nightside aurora are two major sources for O+ in the plasma sheet. The cusp-origin O+ ions travel along the lobe open field lines to the plasma sheet. They become more abundant during storms, but can be present during all geomagnetic conditions. On the nightside, auroral outflow travels on a direct path to the plasma sheet along closed field lines. While O+ observed within the lobes can be identified as a cusp origin source population, the O+ in the plasma sheet boundary layer and the plasma sheet could be from either source. The auroral origin O+ will have a dispersion signature due to the time-of-flight of the ions along the field line. By scanning the MMS / HPCA and Van Allen Probes / HOPE data for the dispersion signatures, and testing the dispersion for consistency with a nightside auroral source, we study the characteristic properties and access the importance of the nightside aurora as a source for the plasma sheet O+.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 3
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    In:  Journal of Geophysical Research: Solid Earth
    Publication Date: 2024-03-27
    Description: Rift propagation is a 3D thermo-mechanical process that often precedes continental breakup. Pre-existing microcontinental blocks and the associated lithospheric strength heterogeneities influence the style of rift propagation. Interestingly, some rifts propagate into pre-existing blocks and eventually cut through them (e.g., the Zhongsha Block and the Reed Bank), while others bypass these microcontinental blocks forming distinct overlapping rift branches (e.g., the East African Rift System). In this study, we use 3D numerical models to investigate the interaction between microcontinental blocks and rift propagation under different far-field extension rates. In doing so, we assess the impact of mantle lithospheric thicknesses and lower crustal rheology on the style of rift propagation. Our models reproduce the two types of rift propagation, characterized by propagating rifts that either split or bypass the pre-existing microcontinental blocks. We find that lithospheric thickness exerts dominant control, while lower crustal rheology of microcontinental blocks and the extension rate have less effect on rift propagation. Our model results can explain rift propagation patterns, block rotation and strong lithospheric thinning in the South China Sea, the East African Rift System, and the Woodlark Basin.
    Language: English
    Type: info:eu-repo/semantics/article
    Format: application/pdf
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