Donald Grant Mitchell

Donald Grant Mitchell in 1883 Donald Grant Mitchell (April 12, 1822December 15, 1908) was an American essayist and novelist who usually wrote under the pen name Ik Marvel. Provided by Wikipedia
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  1. 1
    Storm time dynamics of ring current protons: Implications for the long‐term energy budget in the inner magnetosphere

    Storm time dynamics of ring current protons: Implications for the long‐term energy budget in the inner magnetosphere by Matina Gkioulidou, A. Y. Ukhorskiy, D. G. Mitchell, L. J. Lanzerotti

    Published 2016-05-01
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  2. 2
    Shock and SEP Modeling Study for the 2022 September 5 SEP Event

    Shock and SEP Modeling Study for the 2022 September 5 SEP Event by A. Kouloumvakos, N. Wijsen, I. C. Jebaraj, A. Afanasiev, D. Lario, C. M. S. Cohen, P. Riley, D. G. Mitchell, Z. Ding, A. Vourlidas, J. Giacalone, X. Chen, M. E. Hill

    Published 2025-01-01
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  3. 3
    Viewing Global Changes in the Heliosheath with IMAP’s Energetic Neutral Atom Imagers

    Viewing Global Changes in the Heliosheath with IMAP’s Energetic Neutral Atom Imagers by E. J. Zirnstein, J. Heerikhuisen, D. J. McComas, J. Bower, G. Clark, M. A. Dayeh, H. O. Funsten, M. Gkioulidou, D. G. Mitchell, D. B. Reisenfeld, N. A. Schwadron

    Published 2025-01-01
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  4. 4
    Diverse Dust Populations in the Near-Sun Environment Characterized by PSP/ISʘIS

    Diverse Dust Populations in the Near-Sun Environment Characterized by PSP/ISʘIS by M. M. Shen, J. R. Szalay, P. Pokorný, J. G. Mitchell, M. E. Hill, D. G. Mitchell, D. J. McComas, E. R. Christian, C. M. S. Cohen, N. A. Schwadron, S. D. Bale, D. M. Malaspina

    Published 2025-01-01
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  5. 5
    Delay of Near-relativistic Electrons with Respect to Type III Radio Bursts throughout the Inner Heliosphere

    Delay of Near-relativistic Electrons with Respect to Type III Radio Bursts throughout the Inner Heliosphere by J. G. Mitchell, E. R. Christian, G. A. de Nolfo, C. M. S. Cohen, M. E. Hill, A. Kouloumvakos, A. W. Labrador, R. A. Leske, D. J. McComas, R. L. McNutt Jr., D. G. Mitchell, M. Shen, N. A. Schwadron, M. E. Wiedenbeck, S. D. Bale, M. Pulupa

    Published 2025-01-01
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  6. 6
    Magnetic Reconnection–driven Energization of Protons up to ∼400 keV at the Near-Sun Heliospheric Current Sheet

    Magnetic Reconnection–driven Energization of Protons up to ∼400 keV at the Near-Sun Heliospheric Current Sheet by M. I. Desai, J. F. Drake, T. Phan, Z. Yin, M. Swisdak, D. J. McComas, S. D. Bale, A. Rahmati, D. Larson, W. H. Matthaeus, M. A. Dayeh, M. J. Starkey, N. E. Raouafi, D. G. Mitchell, C. M. S. Cohen, J. R. Szalay, J. Giacalone, M. E. Hill, E. R. Christian, N. A. Schwadron, R. L. McNutt Jr., O. Malandraki, P. Whittlesey, R. Livi, J. C. Kasper

    Published 2025-01-01
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  7. 7
    Longitudinal Dependence of Heavy Ion Composition in the 2021 October 28 Ground Level Enhancement Event

    Longitudinal Dependence of Heavy Ion Composition in the 2021 October 28 Ground Level Enhancement Event by C. M. S. Cohen, G. M. Mason, E. R. Christian, A. C. Cummings, G. A. de Nolfo, M. I. Desai, J. Giacalone, M. E. Hill, A. W. Labrador, R. A. Leske, D. J. McComas, R. L. McNutt Jr, D. G. Mitchell, J. G. Mitchell, G. D. Muro, J. S. Rankin, N. A. Schwadron, M. M. Shen, M. E. Wiedenbeck, Z. G. Xu, G. C. Ho, R. F. Wimmer-Schweingrüber

    Published 2025-01-01
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