The DOI matches its Crossref record; 317 of the 317 references it cites were found in a registry or an index.
Energetic Particles and Corotating Interaction Regions in the Solar Wind
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“As the stream interaction regions also form roughly along the IMF lines (Richardson 2004), Mars and Earth observe the CIR structure at the same time around these days.”
From Radiation environment for future human exploration on the surface of Mars: the current understanding based on MSL/RAD dose measurements (2021) · cites this paper as Richardson 2004
Citations
Cites
Dynamics of the Interplanetary Gas and Magnetic Fields.
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Interplanetary Dynamical Processes
PARKER, E. N., Marshak, R. E., & Johnson, G. (1964) · Physics Today · doi:10.1063/1.3051487 · Cited by 1,189
A coronal hole and its identification as the source of a high velocity solar wind stream
Krieger, A. S., Timothy, A. F., & Roelof, E. C. (1973) · Solar Physics · doi:10.1007/bf00150828 · Cited by 794
Proton and electron mean free paths: The Palmer consensus revisited
Bieber, J. W., Matthaeus, W. H., Smith, C. W., et al. (1994) · The Astrophysical Journal · doi:10.1086/173559 · Cited by 724
Coronal holes and high‐speed wind streams
Zirker, J. B. (1977) · Reviews of Geophysics · doi:10.1029/rg015i003p00257 · Cited by 687
Quasi-stationary corotating structure in the interplanetary medium
Wilcox, J. M., & Ness, N. F. (1965) · Journal of Geophysical Research Atmospheres · doi:10.1029/jz070i023p05793 · Cited by 550
Steiger, R. V., Schwadron, N. A., Fisk, L. A., et al. (2000) · Journal of Geophysical Research Atmospheres · doi:10.1029/1999ja000358 · Cited by 534
Smith, E. J., & Wolfe, J. H. (1976) · Geophysical Research Letters · doi:10.1029/gl003i003p00137 · Cited by 509
Research works printed but not linked: 18
- Bieber, J. W.: 1998, ‘Remarks on the Diffusion Tensor in the Heliosphere’, Space Sci. Rev. 83, 336.
- Dietrich, W. F. and Simpson, J. A.: 1985, ‘Elemental Abundance Differences Between Nuclei Accelerated in CIR Shocks and Flares’, Proc. 19th Int. Cosmic Ray Conf. 4, 277.
- Dvornikov, V.M., Sdobnov, V. E. and Sergeev, A. V.: 1983, ‘Analysis of Cosmic Ray Pitch-Angle Anisotropy During Forbush-Effect in June 1972 by the Method of Spectrographical Global Survey’, Proc. 18th Int. Cosmic Ray Conf. 3, 249.
- Forbush, S. E.: 1993, in Van Allen, J. A. (ed.), Cosmic Rays, the Sun and Geomagnetism: The Works of Scott E. Forbush, American Geophysical Union, Washington, D.C.
- King, J. H.: 1979, Interplanetary Medium Data Book, Supplement 1, 1975–1978, NSSDC/WDC-A 79–08, Natl. Space Sci. Data Center, Greenbelt, Maryland, USA.
- Kunow, H., Wibberenz, G. et al.: 1977b, ‘Simultaneous Observations of Cosmic Ray Particles in a Corotating Interplanetary Structure at Different Solar Distances Between 0.3 and 1 AU’, Proc. 15th Int. Cosmic Ray Conf. 3, 227.
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- Richardson, I. G.: 1983, Spacecraft Observations at 1 AU of Low Energy Ions in Co-rotating Solar Wind Streams. Ph.D. thesis, Imperial College of Science and Technology, University of London.
- Richardson, I. G. and Hynds, R. J.: 1990, ‘Spectra of > 35 keV Ions in Corotating Ion Enhancements at 1 AU: ISEE-3/ICE EPAS Observations’, Proc. 21st Int. Cosmic Ray Conf. 5, 337.
- Richardson, I. G., Cane, H. V. and Wibberenz, G.: 2001, ‘Recurrent Cosmic Ray Modulations at Solar Minimum and Solar Maximum’, Proc. 27th Int. Cosmic Ray Conf. 9, 3597.
- Richardson, I. G., Barbier, L. M., Reames, D. V. and von Rosenvinge, T. T.: 1993, ‘MeV/n Ions Associated Corotating High-Speed Solar Wind Streams at ≤ 1 AU During 1978 to 1986’, Proc. 22nd Int. Cosmic Ray Conf. 3, 288.
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- Zirker, J. B. (ed.): 1977, Coronal Holes and High Speed Wind Streams, Skylab Solar Workshop, Colorado University Press, Boulder, CO.
Cited by
Sorted by citations
Witasse, O., Sánchez‐Cano, B., Mays, M. L., Kajdič, P., Opgenoorth, H., Elliott, H. A., Richardson, I. G., Zouganelis, I., Zender, J., Wimmer‐Schweingruber, R. F., et al. (2017) · Journal of Geophysical Research: Space Physics · doi:10.1002/2017ja023884 · Cited by 126
Self-citationGuo, J., Zeitlin, C., Wimmer-Schweingruber, R. F., Hassler, D. M., Ehresmann, B., Rafkin, S., Freiherr von Forstner, J. L., Khaksarighiri, S., Liu, W., & Wang, Y. (2021) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-021-00136-5 · Cited by 73
“…the GCR flux can also be altered temporarily in the form of Forbush decreases (Forbush 1937; Lockwood 1971) by transient heliospheric structures with enhanced magnetic fields such as interplanetary coronal mass ejections (ICMEs, Cane 2000) and stream interaction regions (SIRs, Richardson 2004).”
BackgroundMelkumyan, A. A., Belov, A. V., Abunina, M. A., Abunin, A. A., Eroshenko, E. A., Yanke, V. G., & Oleneva, V. A. (2019) · Advances in Space Research · doi:10.1016/j.asr.2018.10.009 · Cited by 33
Directionality of the Martian Surface Radiation and Derivation of the Upward Albedo Radiation
Guo, J., Khaksarighiri, S., Wimmer‐Schweingruber, R. F., Hassler, D. M., Ehresmann, B., Zeitlin, C., Löffler, S., Matthiä, D., Berger, T., Reitz, G., et al. (2021) · Geophysical Research Letters · doi:10.1029/2021gl093912 · Cited by 14
“GCR flux in the heliosphere can be modulated by the recurrent heliospheric structures, called corotating interaction regions (CIRs), which often appear during the declining phase of a solar cycle (e.g.., Crooker et al., 1999; Richardson, 2004).”
BackgroundGuo, J., S. O. E. A. S. S., F. Wimmer-Schweingruber, R., Dumbovicx, M., Heber, B., Wang, Y., C. A. O. S. C. F. E. I. C. P., I. O. E. A. A. P., & H. O. (2020) · Earth and Planetary Physics · doi:10.26464/epp2020007 · Cited by 6
Metadata
- Authors
- Richardson, I. G.
- Affiliations
- Goddard Space Flight Center (US)
- Corresponding author
- Richardson, Ian G.
- ORCID
- Richardson, Ian G.
- Venue
- Space Science Reviews
- Published
- 2004-04
- Volume
- 111
- Issue
- 3-4
- Pages
- 267-376
- ISSN
- 0038-6308 (ISSN-L)
- 1572-9672
- OpenAlex
- W2033867944
- Semantic Scholar
- e785f1c37707950adde9ccbeadb8a8657538b605
- Cited by
- 263
- References
- 317
- Citations by year
- 2026: 11 · 2025: 15 · 2024: 25 · 2023: 16 · 2022: 19 · 2021: 25 · 2020: 20 · 2019: 22 · 2018: 15 · 2017: 9 · 2016: 11 · 2015: 5 · 2014: 8 · 2013: 9 · 2012: 10
- FWCI
- 2.75
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- Locations
- Space Science Reviews (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Solar and Space Plasma Dynamics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Ionosphere and magnetosphere dynamics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
- Keywords
- corotating interaction regions, solar wind, energetic particles, galactic cosmic ray modulation, Jovian electrons, ion acceleration, coronal holes, high-speed solar wind streams, neutron monitor
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- Richardson, I. G. (2004). Energetic Particles and Corotating Interaction Regions in the Solar Wind. Space Science Reviews. https://doi.org/10.1023/b%3Aspac.0000032689.52830.3e
