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Cited article:

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Generation of low-frequency magnetic field disturbances in coronal loops by proton and electron beams

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Kinematics and Physics of Celestial Bodies 26 (2) 62 (2010)
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Reappraising Transition Region Line Widths in Light of Recent Alfvén Wave Discoveries

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Preferential Perpendicular Heating of Coronal Hole Minor Ions by the Fermi Mechanism

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The Astrophysical Journal 668 (1) 546 (2007)
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Broadening of Resonantly Scattered Ultraviolet Emission Lines by Coronal Hole Outflows

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The Astrophysical Journal 660 (2) 1660 (2007)
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Drivers of the solar wind: then and now

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Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 364 (1839) 505 (2006)
https://doi.org/10.1098/rsta.2005.1713

On the behavior of O+5 in coronal holes: Importance of sunward propagating waves

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Journal of Geophysical Research: Space Physics 111 (A12) (2006)
https://doi.org/10.1029/2006JA011917

Recurrent Magnetic Storms: Corotating Solar Wind Streams

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Line broadening of EUV lines across the Solar limb: A spicule contribution?

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Astronomy & Astrophysics 431 (3) L17 (2005)
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Astrophysics in 2004

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Publications of the Astronomical Society of the Pacific 117 (830) 311 (2005)
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