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Comparison of Observations at ACE and Ulysses with Enlil Model Results: Stream Interaction Regions During Carrington Rotations 2016 - 2018
DOI: 10.1007/s11207-011-9858-7 Bibcode: 2011SoPh..273..179J

Luhmann, J. G.; Russell, C. T.; Jian, L. K. +6 more

During the latitudinal alignment in 2004, ACE and Ulysses encountered two stream interaction regions (SIRs) each Carrington rotation from 2016 to 2018, at 1 and 5.4 AU, respectively. More SIR-driven shocks were observed at 5.4 AU than at 1 AU. Three small SIRs at 1 AU merged to form a strong SIR at 5.4 AU. We compare the Enlil model results with s…

2011 Solar Physics
Ulysses 60
Large-Scale Variation of Solar Wind Electron Properties from Quasi-Thermal Noise Spectroscopy: Ulysses Measurements
DOI: 10.1007/s11207-011-9797-3 Bibcode: 2011SoPh..271..141L

Issautier, K.; Meyer-Vernet, N.; Hoang, S. +1 more

The transport of energy in space plasmas, especially in the solar wind, is far from being understood. Measuring the temperature of the electrons and their non-thermal properties is essential to understand the transport properties in collisionless plasmas. Quasi-thermal noise spectroscopy is a reliable tool for measuring the electron temperature ac…

2011 Solar Physics
Ulysses 36
Simulation of the Unusual Solar Minimum with 3D SIP-CESE MHD Model by Comparison with Multi-Satellite Observations
DOI: 10.1007/s11207-011-9785-7 Bibcode: 2011SoPh..271...91Y

Wu, S. T.; Feng, Xueshang; Zhang, Shaohua +2 more

The observations both near the Sun and in the heliosphere during the activity minimum between solar cycles 23 and 24 exhibit different phenomena from those typical of the previous solar minima. In this paper, we have chosen Carrington rotation 2070 in 2008 to investigate the properties of the background solar wind by using the three-dimensional (3…

2011 Solar Physics
SOHO Ulysses 26
Tracking a Ulysses High-latitude ICME Event Back to Its Solar Origins
DOI: 10.1007/s11207-011-9811-9 Bibcode: 2011SoPh..272..137D

Dumitrache, C.; Popescu, N. A.; Oncica, A.

High-latitude interplanetary mass ejections (ICMEs) observed beyond 1 AU are not studied very often. They are useful for improving our understanding of the 3D heliosphere. As there are only few such events registered by the Ulysses spacecraft, the task of detecting their solar counterparts is a challenge, especially during high solar activity peri…

2011 Solar Physics
SOHO Ulysses 4