Coupled Hydromagnetic Wave Excitation and Ion Acceleration at an Evolving Coronal/Interplanetary Shock

By Martin A. Lee. 2005

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In Astronomy and Astrophysics

Citations in the corpus

Heavy-Ion Elemental Abundances in Large Solar Energetic Particle Events and Their Implications for the Seed Population (2006, background): “Furthermore, such mechanisms can only deplete the abundances of heavier ions like Fe with respect to O (e.g., see Ellison & Ramaty 1985; Lee 2005; Channok et al. 2005) and therefore cannot account for the systematic M/Q-dependent enhancements in the heavy-ion abundances that span more than an order…”
A Model for Spectral and Compositional Variability at High Energies in Large, Gradual Solar Particle Events (2006, background): “Lee (2005a) derived the explicit dependence of the shock-accelerated spectrum’s rollover energy on Bn, the angle between the upstream magnetic field vectorB and the shock-normaln.”
The Two Sources of Solar Energetic Particles (2012, background): “Lee (2005) finds that the limit varies as E-1 and the simpler theory of Sandroos and Vainio (2009) gives p-1.”
Dynamics of the Earth’s Particle Radiation Environment (2009, methodology): “This idea has so far been applied to a coupled system of energetic protons and Alfvén waves (Ng and Reames 1994, 2008; Rice et al. 2003; Vainio 2003; Lee 2005; Vainio and Laitinen 2007; Vainio and Laitinen 2008) and modeling efforts show that non-linear models that include the dynamics of coronal…”
STEREO IMPACT Investigation Goals, Measurements, and Data Products Overview (2008, unknown): “Nevertheless, theoretical analyses suggest that as protons stream away from the shock they generate Alfven waves that trap the particles that follow, causing efficient acceleration to higher energies (Lee 1983, 2005).”
PROPAGATION OF SOLAR ENERGETIC PARTICLES IN THREE-DIMENSIONAL INTERPLANETARY MAGNETIC FIELDS (2009, methodology): “There are a large number of papers dealing with various aspects of SEP acceleration (see Lee 2005 and references therein).”
Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation (2016, background): “DSA comprises first-order Fermi acceleration when applied to shocks that move along the magnetic field (parallel shocks), and shock-drift acceleration when applied to shocks that move nearly normal to the magnetic field (quasi-perpendicular shocks) (e.g., Lee 2005).”
The Solar Probe Plus Mission: Humanity’s First Visit to Our Star (2016, background): “But in the sheath adjacent to and upstream of a shock, particles streaming along B can excite high intensities of gyro-resonant waves, which in turn scatter the particles in pitch angle and produce the small scattering mean free paths essential for shock acceleration (Lee 2005).”
SOLAR RELEASE TIMES OF ENERGETIC PARTICLES IN GROUND-LEVEL EVENTS (2009, background): “GLEs appear to be extreme examples of large “gradual” SEP events in which ions are accelerated by shock waves driven out from the Sun by coronal mass ejections (CMEs) (see reviews Reames 1990, 1995, 1999, 2002; Kahler 1992, 1994, 2001; Gosling 1993; Lee 1997, 2005; Tylka 2001; Tylka et al. 2005).”
Stochastic Acceleration by Turbulence (2012, background): “Possible generation by some instability due to accelerated particles has been suggested and some details have been worked out by Lee (2005), but this problem is not fully resolved as observations of shocks in the solar wind do not always show presence of any turbulence in the upstream region. when…”