Showing 61 - 80 results of 5,209 for search '"The Parkers"', query time: 0.12s Refine Results
  1. 61

    Alpha-to-proton Temperature Ratio Distributions Using Parker Solar Probe Measurements by Mário B. Amaro, Andris Vaivads

    Published 2024-01-01
    “…The distributions of the temperature excess of alphas to protons ( ε ) were studied using Parker Solar Probe measurements for Encounters 2 through 14. …”
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    Article
  2. 62

    The Parker Project: Cross-Brand Service Testing Using V2G by Peter Bach Andersen, Seyedmostafa Hashemi, Tiago Sousa, Thomas Meier Soerensen, Lance Noel, Bjoern Christensen

    Published 2019-10-01
    “…The Parker project sought to experimentally validate that contemporary series-produced electric vehicles (EVs), capable of V2G, are ready to participate in a number of advanced grid services. …”
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    Radial Evolution of the Near-Sun Solar Wind: Parker Solar Probe Observations by Wen Liu, Huan-Yu Jia, Si-Ming Liu

    Published 2024-01-01
    “…A statistical study of the radial evolution of the solar wind within 0.3 au is shown in this Letter based on Parker Solar Probe observations. We show the radial distribution of the main solar wind parameters, including the solar wind speed V _sw , magnetic field ∣ B ∣, the number density of electrons N _e , protons N _p , and α particles N _α , and the temperature of protons T _p and α particles T _α . …”
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    Can the Parker Solar Probe Detect a CME-flare Current Sheet? by Yuhao Chen, Zhong Liu, Pengfei Chen, David F. Webb, Qi Hao, Jialiang Hu, Guanchong Cheng, Zhixing Mei, Jing Ye, Qian Wang, Jun Lin

    Published 2023-01-01
    “…However, the detailed physical properties and fine structures of the CS are still unknown, since there is no relevant information obtained via in situ detections. The Parker Solar Probe (PSP) may provide us with such information should it traverse a CS in an eruption. …”
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    Article
  10. 70

    Heliospheric Diffusion of Stochastic Parker Spirals in Radially Evolving Solar Wind Turbulence by N. H. Bian, R. D. Strauss, G. Li, N. E. Engelbrecht

    Published 2024-01-01
    “…Our model predicts a spiral angle that is smaller by ∼5° than the Parker spiral angle at Earth’s orbit for the same solar wind speed of V _sw = 400 km s ^−1 . …”
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    Scale and Time Dependence of Alfvénicity in the Solar Wind as Observed by the Parker Solar Probe by Panisara Thepthong, Peera Pongkitiwanichakul, David Ruffolo, Rungployphan Kieokaew, Riddhi Bandyopadhyay, William H. Matthaeus, Tulasi N. Parashar

    Published 2024-01-01
    “…Alfvénicity is a well-known property, common in the solar wind, characterized by a high correlation between magnetic and velocity fluctuations. Data from the Parker Solar Probe (PSP) enable the study of this property closer to the Sun than ever before, as well as in the sub-Alfvénic solar wind. …”
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    Article
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    The Eruption of a Magnetic Flux Rope Observed by Solar Orbiter and Parker Solar Probe by David M. Long, Lucie M. Green, Francesco Pecora, David H. Brooks, Hanna Strecker, David Orozco-Suárez, Laura A. Hayes, Emma E. Davies, Ute V. Amerstorfer, Marilena Mierla, David Lario, David Berghmans, Andrei N. Zhukov, Hannah T. Rüdisser

    Published 2023-01-01
    “…The erupting flux rope then passed over the Parker Solar Probe spacecraft during its encounter (13), enabling in situ diagnostics of the structure. …”
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  17. 77

    Parker Solar Probe Observations of Magnetic Reconnection Exhausts in Quiescent Plasmas near the Sun by Stefan Eriksson, Marc Swisdak, Alfred Mallet, Oksana Kruparova, Roberto Livi, Orlando Romeo, Stuart D. Bale, Justin C. Kasper, Davin E. Larson, Marc Pulupa

    Published 2024-01-01
    “…Parker Solar Probe observations are analyzed for the presence of reconnection exhausts across current sheets (CSs) within R < 0.26 au during encounters 4–11. …”
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    Nature, Generation, and Dissipation of Alfvénic Kinks/Switchbacks Observed by Parker Solar Probe and WIND by Chuanpeng Hou, Xingyu Zhu, Rui Zhuo, Jiansen He, Daniel Verscharen, Die Duan

    Published 2023-01-01
    “…The discovery of very prominent magnetic kinks/switchbacks in the solar wind within 0.3 au has become a scientific highlight of the Parker Solar Probe (PSP) mission. This discovery points at the promising impact of small-scale solar activity on the inner heliosphere. …”
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