Search Results - "Lario, D"

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    The Solar Probe Plus Mission: Humanity’s First Visit to Our Star by Fox, N. J., Velli, M. C., Bale, S. D., Decker, R., Driesman, A., Howard, R. A., Kasper, J. C., Kinnison, J., Kusterer, M., Lario, D., Lockwood, M. K., McComas, D. J., Raouafi, N. E., Szabo, A.

    Published in Space science reviews (01-12-2016)
    “…Solar Probe Plus (SPP) will be the first spacecraft to fly into the low solar corona. SPP’s main science goal is to determine the structure and dynamics of the…”
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    Journal Article
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    High-energy (>40 MeV) Proton Intensity Enhancements Associated with the Passage of Interplanetary Shocks at 1 au by Lario, D., Richardson, I. G., Aran, A., Wijsen, N.

    Published in The Astrophysical journal (01-06-2023)
    “…We analyze periods with elevated >40 MeV proton intensities observed near Earth over a time span of 43 years (1973-2016) that coincide with the passage of…”
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    Influence of interplanetary coronal mass ejections on the peak intensity of solar energetic particle events by Lario, D., Karelitz, A.

    “…We study whether the presence of coronal mass ejections (CMEs) in interplanetary space (ICMEs) affects the maximum intensity of solar energetic particle (SEP)…”
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    THE SOLAR ENERGETIC PARTICLE EVENT ON 2013 APRIL 11: AN INVESTIGATION OF ITS SOLAR ORIGIN AND LONGITUDINAL SPREAD by Lario, D, RAOUAFI, N E, Kwon, Y, Zhang, J, Gomez-Herrero, R, Dresing, N, Riley, P

    Published in The Astrophysical journal (10-12-2014)
    “…We investigate the solar phenomena associated with the origin of the solar energetic particle (SEP) event observed on 2013 April 11 by a number of spacecraft…”
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    Modeling the 2012 May 17 Solar Energetic Particle Event Using the AWSoM and iPATH Models by Li, Gang, Jin, Meng, Ding, Zheyi, Bruno, A., de Nolfo, G. A., Randol, B. M., Mays, L., Ryan, J., Lario, D.

    Published in The Astrophysical journal (01-10-2021)
    “…Abstract We model the 2012 May 17 solar energetic particle event by combining the AWSoM and iPATH codes. Using this combined approach, we investigate particle…”
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    LONGITUDINAL PROPERTIES OF A WIDESPREAD SOLAR ENERGETIC PARTICLE EVENT ON 2014 FEBRUARY 25: EVOLUTION OF THE ASSOCIATED CME SHOCK by Lario, D., Kwon, R.-Y., Vourlidas, A., Raouafi, N. E., Haggerty, D. K., Ho, G. C., Anderson, B. J., Papaioannou, A., Gómez-Herrero, R., Dresing, N., Riley, P.

    Published in The Astrophysical journal (01-03-2016)
    “…ABSTRACT We investigate the solar phenomena associated with the origin of the solar energetic particle (SEP) event observed on 2014 February 25 by a number of…”
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    Heavy-ion Acceleration in 3He-rich Solar Energetic Particle Events: New Insights from Solar Orbiter by Mason, G. M., Roth, I., Nitta, N. V., Bučík, R., Lario, D., Ho, G. C., Allen, R. C., Kouloumvakos, A., Wimmer-Schweingruber, R. F., Rodriguez-Pacheco, J.

    Published in The Astrophysical journal (01-11-2023)
    “…We present Solar Orbiter energetic particle observations of two 3He-rich events with features more clearly observed than in prior studies. The event of 2022…”
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    On the Seed Population of Solar Energetic Particles in the Inner Heliosphere by Wijsen, N., Li, G., Ding, Z., Lario, D., Poedts, S., Filwett, R. J., Allen, R. C., Dayeh, M. A.

    “…Particles measured in large gradual solar energetic particle events are believed to be predominantly accelerated at shocks driven by coronal mass ejections…”
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    CIRCUMSOLAR ENERGETIC PARTICLE DISTRIBUTION ON 2011 NOVEMBER 3 by Gomez-Herrero, R, Dresing, N, Klassen, A, Heber, B, Lario, D, Agueda, N, Malandraki, O E, Blanco, J J, Rodriguez-Pacheco, J, Banjac, S

    Published in The Astrophysical journal (20-01-2015)
    “…Late on 2011 November 3, STEREO-A, STEREO-B, MESSENGER, and near-Earth spacecraft observed an energetic particle flux enhancement. Based on the analysis of in…”
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    Time‐dependent magnetohydrodynamic simulations of the inner heliosphere by Merkin, V. G., Lyon, J. G., Lario, D., Arge, C. N., Henney, C. J.

    “…This paper presents results from a simulation study exploring heliospheric consequences of time‐dependent changes at the Sun. We selected a 2 month period in…”
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    The Extended Field-aligned Suprathermal Proton Beam and Long-lasting Trapped Energetic Particle Population Observed Upstream of a Transient Interplanetary Shock by Lario, D., Richardson, I. G., Wilson III, L. B., Berger, L., Jian, L. K., Trotta, D.

    Published in The Astrophysical journal (01-02-2022)
    “…The properties of the suprathermal particle distributions observed upstream of interplanetary shocks depend not only on the properties of the shocks but also…”
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    LONGITUDINAL AND RADIAL DEPENDENCE OF SOLAR ENERGETIC PARTICLE PEAK INTENSITIES: STEREO , ACE , SOHO , GOES , AND MESSENGER OBSERVATIONS by Lario, D, Aran, A, Gomez-Herrero, R, Dresing, N, Heber, B, Ho, G C, Decker, R B, Roelof, E C

    Published in The Astrophysical journal (10-04-2013)
    “…Simultaneous measurements of solar energetic particle (SEP) events by two or more of the spacecraft located near 1 AU during the rising phase of solar cycle 24…”
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    RELEASE HISTORY AND TRANSPORT PARAMETERS OF RELATIVISTIC SOLAR ELECTRONS INFERRED FROM NEAR-THE-SUN IN SITU OBSERVATIONS by Agueda, N., Lario, D.

    Published in The Astrophysical journal (01-10-2016)
    “…ABSTRACT We study four consecutive 300-800 keV electron events observed on 1980 May 28 by Helios-1, when the spacecraft was located at 0.31 au from the Sun. We…”
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    On the Link between the Release of Solar Energetic Particles Measured at Widespread Heliolongitudes and the Properties of the Associated Coronal Shocks by Lario, D., Kwon, R.-Y., Riley, P., Raouafi, N. E.

    Published in The Astrophysical journal (01-10-2017)
    “…Under the paradigm that the main agents in the acceleration of solar energetic particles (SEPs) are shocks initially driven by coronal mass ejections, we…”
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    Particle acceleration at perpendicular shock waves: Model and observations by Zank, G. P., Li, Gang, Florinski, V., Hu, Qiang, Lario, D., Smith, C. W.

    “…On the basis of a recently developed nonlinear guiding center theory for the perpendicular spatial diffusion coefficient κ⊥ used to describe the transport of…”
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