- SOLAR WIND HELIUM ABUNDANCE AS A FUNCTION OF SPEED AND HELIOGRAPHIC LATITUDE: VARIATION THROUGH A SOLAR CYCLE
- DETERMINING THE MAGNETIC FIELD ORIENTATION OF CORONAL MASS EJECTIONS FROM FARADAY ROTATION
- Wind observations of extreme ion temperature anisotropies in the D. Clack,1,2
- Physics-based tests to identify the accuracy of solar wind ion measurements: A case study with the Wind Faraday Cups
- Langmuir waves upstream of interplanetary shocks: Dependence on shock and plasma parameters
- Space Sci Rev DOI 10.1007/s11214-009-9584-8
- Are periodic solar wind number density structures formed in the solar corona?
- Wind/SWE observations of firehose constraint on solar wind proton temperature anisotropy
- Storm-time distortion of the inner magnetosphere: How severe can it get?
- Planetary and Space Science 52 (2004) 14151421 LOFAR: The potential for solar and space weather studies
- Space Sci Rev (2007) 129: 391419 DOI 10.1007/s11214-007-9153-y
- Geomagnetic disturbances and their relationship to Interplanetary shock parameters
- Heating of the solar wind with electron and proton effects , Steven R. Cranmer
- Hot Solar-Wind Helium: Direct Evidence for Local Heating by Alfven-Cyclotron Dissipation J. C. Kasper*
- Solar wind proton temperature anisotropy: Linear theory and WIND/SWE observations
- Justin Christophe Kasper Curriculum vita
- Major geomagnetic storms (Dst 100 nT) generated by corotating interaction regions
- GCR access to the Moon as measured by the CRaTER instrument on LRO
- The Astrophysical Journal, 659:L65L68, 2007 April 10 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- THE BASTILLE DAY MAGNETIC CLOUDS AND UPSTREAM SHOCKS: NEAR-EARTH INTERPLANETARY OBSERVATIONS
- Electron and proton heating by solar wind turbulence B. Breech,1
- Interferometric Imaging with the 32 Element Murchison Wide-Field Array S. M. ORD,1
- The Astrophysical Journal Letters, 728:L27 (7pp), 2011 February 20 doi:10.1088/2041-8205/728/2/L27 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- DOI 10.1007/s11207-010-9697-y THE SOLAR DYNAMICS OBSERVATORY
- Low-frequency whistler waves and shocklets observed at quasi-perpendicular interplanetary shocks
- TheMurchisonWidefieldArray: Design Overview
- Plasma flows in the heliosheath J. D. Richardson,1
- Solar and interplanetary sources of major geomagnetic storms (Dst 100 nT) during
- FIELD DEPLOYMENT OF PROTOTYPE ANTENNA TILES FOR THE MILEURA WIDEFIELD ARRAY LOW FREQUENCY DEMONSTRATOR
- Constraints on the global structure of magnetic clouds: Transverse size and
- Plasma depletion and mirror waves ahead of interplanetary coronal mass ejections
- Interplanetary coronal mass ejection and ambient interplanetary magnetic field correlations during the Sun-Earth
- A scale-free analysis of magnetic holes at 1 AU M. L. Stevens1
- Waves in Interplanetary Shocks: AWind/WAVES Study L. B. Wilson III, C. Cattell, P. J. Kellogg, K. Goetz, K. Kersten, L. Hanson, and R. MacGregor*
- Journal of Atmospheric and Solar-Terrestrial Physics 70 (2008) 219225 Solar cycle variations of solar wind dynamics and structures
- Correlation between energetic ion enhancements and heliospheric current sheet crossings in the outer heliosphere
- Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock
- Magnetic Fluctuation Power Near Proton Temperature Anisotropy Instability Thresholds in the Solar Wind
- Propagation of the October//November 2003 CMEs through the heliosphere
- Thermodynamic structure of collision-dominated expanding plasma
