Search Results - "Zurbuchen, T. H"
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Global distribution of the solar wind during solar cycle 23: ACE observations
Published in Geophysical research letters (01-07-2009)“…The composition of the solar wind can be used to determine its origin at the Sun; e.g., solar wind from coronal holes has demonstrably lower charge states than…”
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Topological Evolution of a Fast Magnetic Breakout CME in Three Dimensions
Published in The Astrophysical journal (20-08-2008)“…We present the extension of the magnetic breakout model for CME initiation to a fully three-dimensional, spherical geometry. Given the increased complexity of…”
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3
Spatial distribution of Mercury's flux ropes and reconnection fronts: MESSENGER observations
Published in Journal of geophysical research. Space physics (01-08-2016)“…We perform a statistical study of flux ropes and reconnection fronts based on MErcury Surface, Space ENviroment, GEochemistry, and Ranging (MESSENGER) magnetic…”
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Dynamics of Coronal Hole Boundaries
Published in The Astrophysical journal (10-03-2017)“…Remote and in situ observations strongly imply that the slow solar wind consists of plasma from the hot, closed-field corona that is released onto open…”
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A PROTON-CYCLOTRON WAVE STORM GENERATED BY UNSTABLE PROTON DISTRIBUTION FUNCTIONS IN THE SOLAR WIND
Published in The Astrophysical journal (01-03-2016)“…ABSTRACT We use audification of 0.092 s cadence magnetometer data from the Wind spacecraft to identify waves with amplitudes nT near the ion gyrofrequency…”
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Ion heating resulting from pickup in magnetic reconnection exhausts
Published in Journal of Geophysical Research - Space Physics (01-05-2009)“…The heating of ions downstream of the x‐line during magnetic reconnection is explored using full‐particle simulations, test particle simulations, and analytic…”
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CHARGE STATE EVOLUTION IN THE SOLAR WIND. II. PLASMA CHARGE STATE COMPOSITION IN THE INNER CORONA AND ACCELERATING FAST SOLAR WIND
Published in The Astrophysical journal (10-12-2012)“…In the present work, we calculate the evolution of the charge state distribution within the fast solar wind. We use the temperature, density, and velocity…”
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On the differences in composition between solar energetic particles and solar wind
Published in Space science reviews (01-06-2007)“…Issue Title: The Composition of Matter Although the average composition of solar energetic particles (SEPs) and the bulk solar wind are similar in a number of…”
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Conference Proceeding Journal Article -
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Tracking Solar Active Region Outflow Plasma from Its Source to the Near-Earth Environment
Published in Solar physics (01-10-2014)“…Seeking to establish whether active-region upflow material contributes to the slow solar wind, we examine in detail the plasma upflows from Active Region (AR)…”
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Iron charge state distributions as an indicator of hot ICMEs: Possible sources and temporal and spatial variations during solar maximum
Published in Journal of Geophysical Research - Space Physics (01-01-2004)“…It has been shown that Fe charge states greater than and equal to 16 are often observed in the presence of interplanetary coronal mass ejections (ICMEs) at 1…”
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Coronal Mass Ejection Shock and Sheath Structures Relevant to Particle Acceleration
Published in The Astrophysical journal (01-04-2005)“…Most high-energy solar energetic particles are believed to be accelerated at shock waves driven by coronal mass ejections (CMEs). The acceleration process…”
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FIRST MEASUREMENTS OF THE COMPLETE HEAVY-ION CHARGE STATE DISTRIBUTIONS OF C, O, AND Fe ASSOCIATED WITH INTERPLANETARY CORONAL MASS EJECTIONS
Published in The Astrophysical journal (20-05-2012)“…We present the first analysis of the complete charge state distributions of heavy ions in interplanetary coronal mass ejections (CMEs), from singly charged to…”
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Composition of quasi-stationary solar wind flows from Ulysses/Solar Wind Ion Composition Spectrometer
Published in Journal of Geophysical Research, Washington, DC (01-12-2000)“…Using improved, self‐consistent analysis techniques, we determine the average solar wind charge state and elemental composition of nearly 40 ion species of He,…”
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Interchange Reconnection and Coronal Hole Dynamics
Published in The Astrophysical journal (01-05-2010)“…We investigate the effect of magnetic reconnection between open and closed fields, often referred to as 'interchange' reconnection, on the dynamics and…”
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Distribution and properties of open magnetic flux outside of coronal holes
Published in Journal of Geophysical Research - Space Physics (01-09-2006)“…The open magnetic flux of the Sun, the component of the solar magnetic field that forms the heliospheric magnetic field, is known to be concentrated into…”
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The solar wind composition throughout the solar cycle: A continuum of dynamic states
Published in Geophysical research letters (01-05-2002)“…Variations in the speed and elemental and ionic charge composition of the solar wind are reported throughout the solar cycle, as observed by the SWICS…”
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Observable Properties of the Breakout Model for Coronal Mass Ejections
Published in The Astrophysical journal (10-12-2004)“…We compare the "magnetic breakout" model for coronal mass ejections (CMEs) with observed general properties of CMEs by analyzing in detail recent…”
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Acceleration of Low-Energy Ions at the Termination Shock of the Solar Wind
Published in The Astrophysical journal (10-06-2006)“…The Voyager 1 investigators have reported that the spacecraft crossed the termination shock of the solar wind at 94 AU from the Sun. The intensity of…”
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Internal structure of magnetic clouds: Plasma and composition
Published in Journal of Geophysical Research - Space Physics (01-06-2003)“…A comprehensive analysis of magnetic clouds observed by the Advanced Composition Explorer (ACE) spacecraft from February 1998 to July 2001 is presented. The…”
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Phase-synchronization, energy cascade, and intermittency in solar-wind turbulence
Published in Physical review letters (11-12-2012)“…The energy cascade in solar wind magnetic turbulence is investigated using MESSENGER data in the inner heliosphere. The decomposition of magnetic field time…”
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