Interpretation of the cross-correlation function of ACE and STEREO solar wind velocities using a global MHD Model

Journal of Geophysical Research: Space Physics

Volumn 115, Issue 11, 2010, Pages

  Riley, Pete ^a   Luhmann, J ^b   Opitz, A ^c   Linker, J A ^a   Mikic, Z ^a  

^a Predictive Science   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c IRAP   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 78649265931     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2010JA015717     Document Type: Article

References (45)

1. Detman, T. R., M. Dryer, T. Yeh, S. M. Han, and S. T. Wu (1991), A time-dependent, three-dimensional MHD numerical study of interplanetary magnetic draping around plasmoids in the solar wind, J. Geophys. Res., 96(A6), 9531-9540, doi:10.1029/91JA00443.
2. Dryer, M., Z. K. Smith, E. J. Smith, J. D. Mihalov, J. H. Wolfe, R. S. Stei-nolfson, and S. T. Wu (1978), Dynamic MHD modeling of solar wind corotating stream interaction regions observed by Pioneer 10 and 11, J. Geophys. Res., 83(A9), 4347-4352, doi:10.1029/JA083iA09p04347.
3. Endler, F. (1971), Wechselwirkung zwischen Sonnenwind und koronalen Magnetfeldern, Mitteilungen Astron. Gesellschaft Hamburg, 30, 136.
4. Galvin, A. B., et al. (2008), The Plasma and Suprathermal Ion Composition (PLASTIC) investigation on the STEREO observatories, Space Sci. Rev., 136, 437-486, doi:10.1007/s11214-007-9296-x.
5. Gosling, J. T., and S. J. Bame (1972), Solar-wind speed variations 1964-1967: An autocorrelation analysis, J. Geophys. Res., 77(1), 12-26, doi:10.1029/JA077i001p00012.
6. Gosling, J. T., J. R. Asbridge, S. J. Bame, and W. C. Feldman (1976), Solar wind speed variations: 1962-1974, J. Geophys. Res., 81(28), 5061-5070, doi:10.1029/JA081i028p05061.
7. Lee, C. O., et al. (2008), Manifestations of solar differential rotation in the solar wind: An update, Eos Trans. AGU, 89, Spring Meet. Suppl., Abstract SH31A-02.
8. Linker, J. A., and Z. Mikic (1997), Extending coronal models to earth orbit, in Coronal Mass Ejections, edited by N. Crooker, J. Joselyn, and J. Feynmann, p. 269, AGU, Washington, D. C.
9. Linker, J. A., G. van Hoven, and D. D. Schnack (1990), A three-dimensional simulation of a coronal streamer, Geophys. Res. Lett., 17(13), 2281-2284, doi:10.1029/GL017i013p02281.
10. Linker, J. A., et al. (1999), Magnetohydrodynamic modeling of the solar corona during whole Sun month, J. Geophys. Res., 104(A5), 9809-9830, doi:10.1029/1998JA900159.
11. Linker, J. A., R. Lionello, Z. Mikic, and T. Amari (2001), Magnetohydro-dynamic modeling of prominence formation within a helmet streamer, J. Geophys. Res., 106(A11), 25,165-25,175, doi:10.1029/2000JA004020.
12. Lionello, R., Z. Mikic, and J. A. Linker (1999), Stability of algorithms for waves with large flows, J. Comput. Phys., 152(1), 346-358.
13. Lionello, R., J. A. Linker, and Z. Mikic (2001), Including the transition region in models of the large-scale solar corona, Astrophys. J., 546(1), 542-551.
14. Lionello, R., J. A. Linker, and Z. Mikic (2009), Multispectral emission of the sun during the first whole Sun month: Magnetohydrodynamic simulations, Astrophys. J., 690, 902-912, doi:10.1088/0004-637X/690/1/902.
15. Manchester, W. B., A. J. Ridley, T. I. Gombosi, and D. L. Dezeeuw (2006), Modeling the Sun-to-Earth propagation of a very fast CME, Adv. Space Res., 38, 253-262, doi:10.1016/j.asr.2005.09.044. (Pubitemid 44537544)
16. McComas, D. J., S. J. Bame, P. Barker, W. C. Feldman, J. L. Phillips, P. Riley, and J. W. Griffee (1998), Solar wind electron proton alpha monitor (swepam) for the advanced composition explorer, Space Sci. Rev., 86(1-4), 563-612.
17. Mikic, Z., and J. A. Linker (1994), Disruption of coronal magnetic field arcades, Astrophys. J., 430, 898-912. (Pubitemid 24973652)
18. Mikic, Z., J. A. Linker, and J. A. Colborn (1996), An MHD Model of the solar corona and solar wind, BAAS, 28, 868.
19. Mikic, Z., J. A. Linker, D. D. Schnack, R. Lionello, and A. Tarditi (1999), Magnetohydrodynamic modeling of the global solar corona, Phys. Plasmas, 6(5), 2217-2224.
20. Mikic, Z., J. A. Linker, R. Lionello, and P. Riley (2002), Predicting the structure of the solar corona during the December 4, 2002 total solar eclipse, Eos Trans AGU, 83(47), Fall Meet. Abstract SH52A-0468.
21. Mikic, Z., J. A. Linker, R. Lionello, P. Riley, and V. Titov (2007), Predicting the structure of the solar corona for the total solar eclipse of March 29, 2006, in Solar and Stellar Physics Through Eclipses, Astron. Soc. Pac. Conf. Ser, vol. 370, edited by O. Demircan, S. O. Selam, and B. Albayrak, pp. 299, Side, Turkey.
22. Odstrcil, D. (1994), Interactions of solar wind streams and related small structures, J. Geophys. Res., 99(A9), 17,653-17,671, doi:10.1029/94JA01225.
23. Odstrcil, D., J. A. Linker, R. Lionello, Z. Mikic, P. Riley, V. J. Pizzo, and J. G. Luhmann (2002), Merging of coronal and heliospheric numerical 2-d mhd models, J. Geophys. Res., 107(A12), 1493, doi:10.1029/2002JA009334.
24. Odstrcil, D., V. J. Pizzo, J. A. Linker, P. Riley, R. Lionello, and Z. Mikic (2004), Initial coupling of coronal and heliospheric numerical magneto-hydrodynamic codes, J. Atmos. Sol.-Terr. Phys., 66, 1311-1320.
25. Opitz, A., et al. (2009), Temporal evolution of the solar wind bulk velocity at solar minimum by correlating the STEREO A and B PLASTIC measurements, Sol. Phys., 256, 365-377, doi:10.1007/s11207-008-9304-7.
26. Paularena, K. I., G. N. Zastenker, A. J. Lazarus, and P. A. Dalin (1998), Solar wind plasma correlations between IMP 8, INTERBALL-1, and WIND, J. Geophys. Res., 103(A7), 14,601-14,618, doi:10.1029/98JA00660.
27. Pizzo, V. (1978), A three-dimensional model of corotating streams in the solar wind: I. Theoretical foundations, J. Geophys. Res., 83(A12), 5563-5572, doi:10.1029/JA083iA12p05563.
28. Pneuman, G. W., and R. A. Kopp (1971), Gas-magnetic field interactions in the solar corona, Sol. Phys., 18, 258-270.
29. Podesta, J. J., A. B. Galvin, and C. J. Farrugia (2008), Correlation length of large-scale solar wind velocity fluctuations measured tangent to the Earth's orbit: First results from Stereo, J. Geophys. Res., 113, A09104, doi:10.1029/2007JA012865.
30. Richardson, J. D., F. Dashevskiy, and K. I. Paularena (1998), Solar wind plasma correlations between L1 and Earth, J. Geophys. Res., 103(A7), 14,619-14,630, doi:10.1029/98JA00675.
31. Riley, P. (2007), Modeling corotating interaction regions: From the Sun to 1 AU, J. Atmos. Sol.-Terr. Phys., 69, 32-42, doi:10.1016/j. jastp. 2006.06.008.
32. Riley, P., J. T. Gosling, L. A. Weiss, and V. J. Pizzo (1996), The tilts of corotating interaction regions at midheliographic latitudes, J. Geophys. Res., 101(A11), 24,349-24,357, doi:10.1029/96JA02447.
33. Riley, P., J. A. Linker, and Z. Mikic (2001a), An empirically driven global MHD model of the corona and inner heliosphere, J. Geophys. Res., 106(A8), 15,889-15,901, doi:10.1029/2000JA000121.
34. Riley, P., J. A. Linker, Z. Mikic, and R. Lionello (2001b), Mhd modeling of the solar corona and inner heliosphere: Comparison with observations, in Space Weather, Geophys. Monogr. Ser., vol. 125, edited by P. Song, H. J. Singer, and G. L. Siscoe, p. 159, AGU, Washington, D. C.
35. Riley, P., J. A. Linker, and Z. Mikic (2002), Modeling the heliospheric current sheet: Solar cycle variations, J. Geophys. Res., 107(A7), 1136, doi:10.1029/2001JA000299.
36. Riley, P., Z. Mikic, and J. A. Linker (2003), Dynamical evolution of the inner heliosphere approaching solar activity maximum: Interpreting ulysses observations using a global mhd model, Ann. Geophys., 21(6), 1347-1357.
37. Riley, P., R. Lionello, Z. Mikic, J. Linker, E. Clark, J. Lin, and Y.-K. Ko (2007), "Bursty" reconnection following solar eruptions: MHD simulations and comparison with observations, Astrophys. J., 655, 591-597, doi:10.1086/509913.
38. Rouillard, A. P., et al. (2009), A multispacecraft analysis of a small-scale transient entrained by solar wind streams, Sol. Phys., 256, 307-326, doi:10.1007/s11207-009-9329-6.
39. Roussev, I.I., T. I. Gombosi, I. V. Sokolov, M. Velli, W. Manchester, D. L. DeZeeuw, P. Liewer, G. Tóth, and J. Luhmann (2003), A three-dimensional model of the solar wind incorporating solar magnetogram observations, Astrophys. J. Lett, 595(1), L57-L61.
40. Smith, Z., and M. Dryer (1990), Mhd study of temporal and spatial evolution of simulated interplanetary shocks in the ecliptic-plane within 1 au, Sol. Phys., 129, 387-405.
41. Snodgrass, H. B. (1983), Magnetic rotation of the solar photosphere, Astrophys. J., 270, 288-299, doi:10.1086/161121.
42. Steinolfson, R. S., S. T. Suess, and S. T. Wu (1982), The steady global corona, Astrophys. J., 255, 730-742, doi:10.1086/159872.
43. Stone, E. C, A. M. Frandsen, R. A. Mewaldt, E. R. Christian, D. Margolies, J. F. Ormes, and F. Snow (1998), The advanced composition explorer, Space Sci. Rev., 86, 1-22, doi:10.1023/A:1005082526237.
44. Usmanov, A. V. (1993), A global numerical 3-D MHD model of the solar wind, Sol. Phys., 146, 377-396, doi:10.1007/BF00662021.
45. Usmanov, A. V. (1996), A global 3-d mhd solar wind model with Alfven waves, Int. Solar Wind Conf., 382, 141-144.