The DOI matches its Crossref record; 218 of the 218 references it cites were found in a registry or an index.
Solar wind stream interaction regions throughout the heliosphere
Open accessAbstract
This paper focuses on the interactions between the fast solar wind from coronal holes and the intervening slower solar wind, leading to the creation of stream interaction regions that corotate with the Sun and may persist for many solar rotations. Stream interaction regions have been observed near 1 AU, in the inner heliosphere (at $$\sim 0.3$$ –1 AU) by the Helios spacecraft, in the outer and distant heliosphere by the Pioneer 10 and 11 and Voyager 1 and 2 spacecraft, and out of the ecliptic by Ulysses, and these observations are reviewed. Stream interaction regions accelerate energetic particles, modulate the intensity of Galactic cosmic rays and generate enhanced geomagnetic activity. The remote detection of interaction regions using interplanetary scintillation and white-light imaging, and MHD modeling of interaction regions will also be discussed.
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Cites
Interplanetary Magnetic Field and the Auroral Zones
Dungey, J. W. (1961) · Physical Review Letters · doi:10.1103/physrevlett.6.47 · Cited by 4,254
Dynamics of the Interplanetary Gas and Magnetic Fields.
Parker, E. N. (1958) · The Astrophysical Journal · doi:10.1086/146579 · Cited by 3,643
Large-amplitude Alfvén waves in the interplanetary medium, 2
Belcher, J. W., & Davis, L. (1971) · Journal of Geophysical Research Atmospheres · doi:10.1029/ja076i016p03534 · Cited by 1,933
Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI)
Howard, R. A., Moses, J. D., Vourlidas, A., Newmark, J. S., Socker, D. G., Plunkett, S. P., Korendyke, C. M., Cook, J. W., Hurley, A., Davila, J. M., et al. (2008) · Space Science Reviews · doi:10.1007/s11214-008-9341-4 · Cited by 1,784
Existence of Electromagnetic-Hydrodynamic Waves
ALFVÉN, H. (1942) · Nature · doi:10.1038/150405d0 · Cited by 1,746
The STEREO Mission: An Introduction
Kaiser, M. L., Kucera, T. A., Davila, J. M., St. Cyr, O. C., Guhathakurta, M., & Christian, E. (2008) · Space Science Reviews · doi:10.1007/s11214-007-9277-0 · Cited by 1,674
The passage of energetic charged particles through interplanetary space
Parker, E. N. (1965) · Planetary and Space Science · doi:10.1016/0032-0633(65)90131-5 · Cited by 1,607
Interplanetary dynamical processes
Chamberlain, J. W. (1964) · Planetary and Space Science · doi:10.1016/0032-0633(64)90147-3 · Cited by 1,339
A model of interplanetary and coronal magnetic fields
Schatten, K. H., Wilcox, J. M., & Ness, N. F. (1969) · Solar Physics · doi:10.1007/bf00146478 · Cited by 1,211
Interplanetary Dynamical Processes
PARKER, E. N., Marshak, R. E., & Johnson, G. (1964) · Physics Today · doi:10.1063/1.3051487 · Cited by 1,200
Cited by
Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium
Rankin, J. S., Bindi, V., Bykov, A. M., Cummings, A. C., Della Torre, S., Florinski, V., Heber, B., Potgieter, M. S., Stone, E. C., & Zhang, M. (2022) · Space Science Reviews · doi:10.1007/s11214-022-00912-4 · Cited by 53
Properties of Stream Interactions and Their Associated Shocks near 1.52 au: MAVEN Observations
Huang, H., Guo, J., Wang, Z., Lin, H., Zheng, J., Cui, J., Xu, X., Wang, Y., Feng, X., Wei, Y., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab25e9 · Cited by 25
Properties of stream interaction regions at Earth and Mars during the declining phase of SC 24
Geyer, P., Temmer, M., Guo, J., & Heinemann, S. G. (2021) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202040162 · Cited by 18
Metadata
- Authors
- Richardson, I. G.
- Venue
- Living Reviews in Solar Physics
- Published
- 2018-01-26
- Volume
- 15
- Issue
- 1
- Pages
- 1-1
- ISSN
- 1614-4961 (ISSN-L)
- 2367-3648
- OpenAlex
- W2785379947
- Cited by
- 367
- References
- 218
- FWCI
- 17.35
- Type
- journal article
- Language
- en
- Open access
- diamond
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