Search Publications

Time-Dependent Modulation of Cosmic Rays in the Heliosphere
DOI: 10.1007/s11207-013-0445-y Bibcode: 2014SoPh..289.2207M

Ferreira, S. E. S.; Potgieter, M. S.; Manuel, R.

The time-dependent modulation of galactic cosmic rays in the heliosphere is studied by computing intensities using a time-dependent modulation model. By introducing recent theoretical advances in the transport coefficients in the model, computed intensities are compared with Voyager 1, International Monitoring Platform (IMP) 8, and Ulysses proton …

2014 Solar Physics
Ulysses 55
Identification of Interplanetary Coronal Mass Ejections at Ulysses Using Multiple Solar Wind Signatures
DOI: 10.1007/s11207-014-0540-8 Bibcode: 2014SoPh..289.3843R

Richardson, I. G.

Previous studies have discussed the identification of interplanetary coronal mass ejections (ICMEs) near the Earth based on various solar wind signatures. In particular, methods have been developed of identifying regions of anomalously low solar wind proton temperatures (Tp) and plasma compositional anomalies relative to the composition…

2014 Solar Physics
Ulysses 40
Characterization of the Turbulent Magnetic Integral Length in the Solar Wind: From 0.3 to 5 Astronomical Units
DOI: 10.1007/s11207-014-0531-9 Bibcode: 2014SoPh..289.3917R

Dasso, S.; Matthaeus, W. H.; Weygand, J. M. +1 more

The solar wind is a structured and complex system, in which the fields vary strongly over a wide range of spatial and temporal scales. As an example, the turbulent activity in the wind affects the evolution in the heliosphere of the integral turbulent scale or correlation length [λ], usually associated with the breakpoint in the turbulent-energy s…

2014 Solar Physics
Ulysses 29
Solar Wind Electron Strahls Associated with a High-Latitude CME: Ulysses Observations
DOI: 10.1007/s11207-014-0558-y Bibcode: 2014SoPh..289.4239L

Lazar, M.; Poedts, S.; Pomoell, J. +2 more

Counterstreaming beams of electrons are ubiquitous in coronal mass ejections (CMEs) - although their existence is not unanimously accepted as a necessary and/or sufficient signature of these events. We continue the investigation of a high-latitude CME registered by the Ulysses spacecraft on 18 - 19 January 2002 (Dumitrache, Popescu, and Oncica, So…

2014 Solar Physics
Ulysses 11
Two-Way Frequency Fluctuations Observed During Coronal Radio Sounding Experiments
DOI: 10.1007/s11207-013-0417-2 Bibcode: 2014SoPh..289.1715E

Pätzold, M.; Bird, M. K.; Efimov, A. I. +5 more

Coronal radio-sounding experiments were carried out using two-way coherent dual-frequency carrier signals of the ESA spacecraft Rosetta (ROS) in 2006. Frequency measurements recorded at both NASA and ESA tracking stations (sample rate: 1 Hz) are analyzed in this work. Spectral analysis of the S-band, X-band, and differential frequency records has …

2014 Solar Physics
MEx Rosetta Ulysses 5