Modeling the solar energetic particle events in closed structures of interplanetary magnetic field

Journal of Geophysical Research: Space Physics

Volumn 110, Issue A12, 2005, Pages

  Kocharov, L ^a,b   Kovaltsov, G A ^a,b   Torsti, J ^a   Huttunen Heikinmaa, K ^a  

^a UNIVERSITY OF TURKU   (Finland)

^b IOFFE INSTITUTE   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33845796479     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2005JA011082     Document Type: Article

References (30)

1. Bieber, J. W., W. Dröge, P. A. Evenson, R. Pyle, D. Ruffolo, U. Pinsook, P. Tooprakai, M. Rujiwarodom, T. Khumlumlert, and S. Krucker (2002), Energetic particle observations during the 2000 July 14 solar event, Astrophys. J., 567, 622-634.
2. Burlaga, L. F., R. M. Skoug, C. W. Smith, D. F. Webb, T. H. Zurbuchen, and A. Reinard (2001), Fast ejecta during the ascending phase of solar cycle 23: ACE observations, 1998-1999, J. Geophys. Res., 106, 20,957-20,978.
3. Daibog, E. I., Yu. I. Logachev, S. Kahler, and K. Kecskeméty (2003), Statistical properties of SEP event flux declines, Adv. Space Res., 32(12), 2655-2660.
4. Forbush, S. E. (1938), On world-wide changes in cosmic-ray intensity, Phys. Rev., 54, 975-988.
5. Forman, M. A. (1971), Convection-dominated transport of solar cosmic rays, J. Geophys. Res., 76, 759-767.
6. Gosling, J. T., D. N. Baker, S. J. Bame, W. C. Feldman, R. D. Zwickl, and E. J. Smith (1987), Bidirectional solar wind electron heat flux events, J. Geophys. Res., 92, 8519-8535.
7. Kallenrode, M.-B. (2001), Shock as a black box: 2. Effects of adiabatic deceleration and convection included, J. Geophys. Res., 106, 24,989-25,003.
8. Kocharov, L., R. Vainio, J. Torsti, and G. A. Kovaltsov (1998), Adiabatic deceleration of solar energetic particles as deduced from Monte Carlo simulations of interplanetary transport, Solar Phys., 182, 195-215.
9. Kocharov, L., G. A. Kovaltsov, J. Torsti, A. Anttila, and T. Sahla (2003), Modeling the propagation of solar energetic particles in corotating compression regions of solar wind, J. Geophys. Res., 108(A11), 1404, doi: 10.1029/2003JA009928.
10. Kocharov, L., M. Lytova, R. Vainio, T. Laitinen, and J. Torsti (2005), Modeling the shock aftermath source of energetic particles in solar corona, Astrophys. J., 620, 1052-1068.
11. Lee, M. A. (2000), Acceleration of energetic particles on the Sun, in the heliosphere and in the galaxy, in Acceleration and Transport of Energetic Particles Observed in the Heliosphere, edited by R. A. Mewaldt et al., AIP Conf. Proc., 528, 3-18.
12. Lockwood, J. A. (1971), Forbush decreases in the cosmic radiation, Space Sci. Rev., 12, 658-715.
13. Neugebauer, M., and R. Goldstein (1997), Particle and field signatures of coronal mass ejections in the solar wind, in Coronal Mass Ejections, Geophys. Monogr. Ser., vol. 99, edited by N. Crooker, J. A. Joselyn, and J. Feynman, pp. 245-251, AGU, Washington, D. C.
14. Palmer, I. D. (1982), Transport coefficients of low-energy cosmic rays in interplanetary space, Rev. Geophys., 20, 335-351.
15. Parker, E. N. (1958), Dynamics of the interplanetary gas and magnetic fields, Astrophys. J., 128, 664-676.
16. Parker, E. N. (1965), The passage of energetic charged particles through interplanetary space, Planet. Space Sci., 13, 9-49.
17. Richardson, I. G., and H. V. Cane (1996), Particle flows observed in ejecta during solar event onsets and their implication for the magnetic field topology, J. Geophys. Res., 101, 27,521-27,532.
18. Richardson, I. G., V. M. Dvomikov, V. E. Sdobnov, and H. V. Cane (2000), Bidirectional particle flows at cosmic ray and lower (~1 MeV) energies and their association with interplanetary coronal mass ejections/ejecta, J. Geophys. Res., 105, 12,579-12,592.
19. Ruffolo, D. (1995), Effect of adiabatic deceleration on the focused transport of solar cosmic rays, Astrophys. J., 442, 861-874.
20. Sarris, E. T., and O. E. Malandraki (2003), Dependence of the decay phase of solar energetic electron events on the large-scale IMF structure: ACE observations, Geophys. Res. Lett., 50(21), 2079, doi:10.1029/2003GL017921.
21. Shodhan, S., et al. (2000), Counterstreaming electrons in magnetic clouds, J. Geophys. Res., 105, 27,261-27,268.
22. + enhancement within a coronal mass ejection in the solar wind, Geophys. Res. Lett., 26, 161-164.
23. Toptygin, I. N. (1985), Cosmic Rays in Interplanetary Magnetic Fields, Geophys. and Astrophys. Monogr., vol. 27, 387 pp., Springer, New York.
24. Torsti, J., et al. (1995), Energetic particle experiment ERNE, Sol. Phys., 162, 505-531.
25. Torsti, J., E. Riihonen, and L. Kocharov (2004), The 1998 May 2-3 magnetic cloud: An interplanetary "highway" for solar energetic particles observed with SOHO/EK.NE, Astrophys. J., 600, L83-L86.
26. Tranquille, C., T. R. Sanderson, R. G. Marsden, K.-P. Wenzel, and E. J. Smith (1987), Properties of a large-scale interplanetary loop structure as deduced from low-energy proton anisotropy and magnetic field measurements, J. Geophys. Res., 92, 6-14.
27. Vainio, R., and T. Laitinen (2001), The relation between cyclotron heating and energetic particles on open coronal field lines, Astron. Astrophys., 371, 738-747.
28. Vandas, M., D. Odstrčil, and S. Watari (2002), Three-dimensional MHD simulation of a loop-like magnetic cloud in the solar wind, J. Geophys. Res., 107(A9), 1236, doi:10.1029/2001JA005068.
29. Zank, G. P., W. K. M. Rice, and C. C. Wu (2000), Particle acceleration and coronal mass ejection driven shocks: A theoretical model, J. Geophys. Res., 105, 25,079-25,095.
30. Zhang, M., J. R. Jokipii, and R. B. McKibben (2003), Perpendicular transport of solar energetic particles in heliospheric magnetic fields, Astro-phys. J., 595, 493-499.