Source: http://www.netess.ru/3astronomy/20757-2-dinamika-prostranstvennoe-raspredelenie-solnechnih-kosmicheskih-luchey-geliosfere.php
Timestamp: 2019-04-22 03:19:39+00:00

Document:
5. Струминский А.Б. (2010a). Источник солнечных протонов: температура вспышечной плазмы и моменты инжекции. CD-rom. ВККЛ-2010. М: НИИ ЯФ МГУ, 2010.
6. Струминский А.Б. (2010b) Наблюдения радиоизлучения на частоте 245 МГц как индикатор нового режима ускорения электронов и нагрева плазмы // Труды Всероссийской ежегодной конференции по физике Солнца, солнечная и солнечно земная физика-2010 / Под ред. А.В. Степанова и Ю.А. Наговицина, СПб, ГАО РАН, 2010. С. 425-428.
7. Aushev V., Antonova, V., Belov A., Eroshenko E., Kryakunova O., Struminsky A.
(1999). Search for Solar Neutron Events in Alma-Ata NM Data // 26th ICRC, Salt Lake City, Utah, USA, 1999. V. 6. P. 50-53.
8. Struminsky A. and Kohno T. (1993). Peculiarities of Solar Proton Spectra in Stratosphere and Geostationary Orbit on 2-3 November 1992 // 23rd ICRC, Calgary, Canada, 1993. V. 3. P. 5-9.
9. Struminsky A., M. Matsuoka and Takakhashi K. (1994). Evidence of Additional Production of High Energy Neutrons During the Solar Flare on 1991 June 4 // Proc. of Kofu Symposium. Kofu, Japan. NRO Report. 1994. N. 360. P. 405-409.
10. Belov A., Chertok I., Struminsky A. (1995) Time Evolution of Solar Proton Energetic Spectra at the Earth orbit and Possibility of Multi-Step Particle Acceleration // 24th ICRC. Rome, Italy. 1995. V. 4. P. 127-130.
11. Struminsky A., Belov A. (1997) Neutron Monitor Sensitivity to Primary Protons below 3 GV Derived from Data of Ground Level Events // 25th ICRC. Durban, South Africa. 1997. V.1. P. 201-204.
12. Struminsky A. (2001a) Forbush decrease on October 20-22, 1989: solar protons, interplanetary and magnetospheric variations // 27th ICRC. Hamburg, Germany.
2001. V. 9. P. 3558-3561.
13. Struminsky A. and Lal M. (2001b) Magnetospheric currents and variations of cutoff rigidities on October 20, 1989 // 27th ICRC. Hamburg, Germany. 2001. V. 10.
14. Struminsky A. (2003a). Interacting and Escaping 100 MeV Solar Protons as observed on 11 and 15 June 1991 // 28th ICRC. Tsukuba, Japan. 2003. V. 6.
15. Struminsky A. (2003b) Prolonged Release of 100 MeV Solar Protons in the GLE Events of 1997-2002 // 28th ICRC. Tsukuba, Japan, 2003. V. 6. P. 3317-3320.
16. Struminsky A. (2003c) On Accuracy of Solar Cosmic Ray Anisotropy and Intensity Deduced from NM Data // 28th ICRC. Tsukuba, Japan, 2003. V. 6. P. 3419-3422.
17. Struminsky A. (2005a). Three modes of particle propagation in the heliosphere // 29th ICRC. Pune, India, 2005. CD-rom.
18. Struminsky A. (2005b). On Possibility of Prolonged Two Step Production of High Energy Neutrons during the Solar Flare on 28 October 2003 // 29th ICRC. Pune, India, 2005. CD-rom.
19. Struminsky A., (2005c). Variations of solar proton spectrum during the ground level enhancement of 2005 January 20 // 29th ICRC. Pune, India, 2005. CD-rom.
20. Struminsky A. (2006). Enhancements of 200-2000 MeV proton intensity observed by KET/ULYSSES in 1997-2005 // Proceedings 20th ECRS. Lisbon, Portugal, 2006, CD-rom.
21. Struminsky A., B. Heber, R. Gomez-Herrero, A. Klassen (2008). Modulation of Proton Fluxes at ~5AU during the Largest SEP Events of 2005 // 30th ICRC. Merida, Mexico. 2008. N 1. P. 131-134.
22. Heber B., Struminsky A., I. Zimovets, and et al. (2008). Observations of the December 2006 Particle Events at High Latitudes with the KET aboard ULYSSES // 30th ICRC. Merida, Mexico, 2008. N 1. P. 217-220.
23. Struminsky A. and Zimovets I. (2008). Time Scales of Hard X-ray and Radio Emissions of Large Proton Flares. // 30th ICRC. Merida, Mexico, 2008. N 1. P. 7-10.
24. Struminsky A. and I. Zimovets (2009). On estimates of first solar proton arrival // In Proc. 21st ECRS / Eds. P. Kyraly, K. Kudela, M. Stehlik, A.W. Wolfendale, printed by VIENALA s.r.o., Koshice, Slovakia, 2009. P. 237-241.
25. Struminsky A., Zimovets I., Heber B. and Klassen A. (2009) The role of large scale solar magnetic field for distribution of SEP in the 3D heliosphere // 31st ICRC. Lodz, Poland, 2009. CD-rom.
26. Struminsky A. (2011). Relative Timing of Electron Acceleration and Proton Release in X-class Solar Events // 32nd ICRC. Beijing, China, 2011. CD-rom. Paper 0132.
СПИСОК ЛИТЕРАТУРЫ Базилевская Г.А., Свиржевская А.К. (2008). Приход первых релятивистских протонов и условия в солнечной короне // Геомагнетизм и Аэрономия. 2008. Т. 48.
Любимов Г.П. Радиационные пояса Солнца Космические (2002). // Исследования. 2002. Т. 40. № 6. С. 565.
Allafort A., et al. (2011). Long-lived solar -ray emission during 2011 March 7 to detected by Fermi-LAT // 32nd ICRC. Beijing, China, 2011. Paper 0683.
Cane H. et al. (2010). A study of solar energetic particle events of 1997–2006: Their composition and associations // JGR. 2010. V. 115. No A08101.10.1029/2009JA014848.
Cliver E. (2009). History of research on solar energetic particle (SEP) events: the evolving paradigm // In Proc. IAU Symposium, 2009. V. 257. P. 401.
Dalla S. et al. (2003a). Properties of high heliolatitude solar energetic particle events and constraints on models of acceleration and propagation // Geophys. Res. L.
2003. V. 30. N. 19. P. 8035.
.Dalla S., et al. (2003b). Delay in solar energetic particle onsets at high heliographic latitudes // Ann. Geophysicae. 2003. V. 21. P. 1267.
Observations from 1 to 72 AU // 26th ICRC. Uta, USA, 1999. V. 6. P. 328.
Feldman U. (1990). The beam-driven chromospheric evaporation model of solar flares - A model not supported by observations from nonimpulsive large flares // ApJ.
1990. V. 364. P. 322.
Frost K. and Dennis B. (1971). Evidence from Hard X-Rays for Two-Stage Particle Acceleration in a Solar Flare // ApJ. 1971. V. 165. P. 655.
Gosling J.T.(1993). The solar flare myth // JGR. 1993. V. 98. P. 18937.
et al. (2004). INTEGRAL/SPI Observation of the 2003 Oct 28 Solar Flare // In Proc. of the 5th INTEGRAL Workshop. ESA SP-552.
Hamilton D.C. (1981). Dynamics of solar cosmic ray events - Processes at large heliocentric distances /much greater than 1 AU // JASR. 1981. V. 1. P. 25.
Kahler S. et al. (1980). Primary energy release // In Solar Flares / Edited by P. A.
Sturrock, Colorado associated University Press, Boulder, Colorado, 1980. P. 83.
Kallenrode M.B. (2003). Current views on impulsive and gradual solar energetic particle events // J. of Physics G: Nuclear and Particle Physics. 2003. V. 29. N. 5.
Klecker B. et al. (2006). Energetic Particle Observations // Space Sci. Rev. 2006.
Coronal Acceleration versus Shock Wave Acceleration // Space Sci. Rev. 2001. V. 95.
Lario D. et al. (2004a). Low-energy particle response to CMEs during the Ulysses solar maximum northern polar passage // JGR. 2004. V. 109. P. A01107.
Lario D. et al. (2004b). Heliospheric energetic particle observations by the Cassini spacecraft: Correlation with 1 AU observations // JGR. 2004. V. 109. P. A09S02.
Lario D.and Decker R.B. (2001). Re-examination of the October 20, 1989 ESP event // 27th ICRC, Hamburg, Germany, 2001. CD-rom.
Lario D. and Decker R.B. (2002). The energetic storm particle event of October 20, 1989 // GRL. 2002. V. 29. N. 10. P. 1393.
Neupert W.M. (1968). Comparison of Solar X-Ray Line Emission with Microwave Emission during Flares // ApJ. 1968. V. 153. P. L59.
McKibben R.B. et al. (2003). Ulysses COSPIN observations of cosmic rays and solar energetic particles from the South Pole to the North Pole of the Sun during solar maximum // Ann. Geophysicae. 2003. V. 21. P. 1217.
Murphy R. and Share G. (1993). OSSE Observations of the 4 June 1991 Solar Flare // 23rd ICRC. Calgary, Canada, 1993. V. 3. P. 99.
Palmer I.D. (1982). Transport coefficients of low-energy cosmic rays in interplanetary space // Rev. of Geophys. and Space Physics. 1982. V. 20. P. 335.
Mandzhavidze, N. et al. (1993). Acceleration in solar flares: Interacting particles versus interplanetary particles // JASR. 1993. V. 13. No 9. P. 275.
Ramaty R. and Mandzhavidze N. (1994). Theoretical models for high-energy solar flare emissions // In High-energy solar phenomena-A new era of spacecraft measurements. AIP Conference Proceedings. 1994. V. 294. P. 26.
Reames D.V. (2009). Solar Energetic-Particle Release Times in Historic Ground Level Events // ApJ. 2009. V. 706. P. 844.
Reames D.V. (1999). Particle acceleration at the Sun and in the heliosphere // Space Sci. Rev. 1999. V. 90. N 3. P. 413.
Reams D.V. et al. (1997).Spatial and Temporal Invariance in the Spectra of Energetic Particles in Gradual Solar Events // ApJ. V. 491. P. 414.
Ryan J.M. (2000). Long-Duration Solar Gamma-Ray Flares // Space Sci. Rev.
2000. V. 93. P. 581.
Simpson A. et al. (1992). The ULYSSES Cosmic Ray and Solar Particle Investigation // A&A Suppl. Ser. 1992. V. 92. P. 365.
Takakhashi K. et al. (1991) Observation of Solar Neutrons by Mt. Norikura Neutron Monitor During a Period of Solar Cycle 22 // 22nd ICRC. Dublin, Ireland, 1991. V. 3. P. 37.
Tylka A. et al. (2005) Shock Geometry, Seed Populations, and the Origin of Variable Elemental Composition at High Energies in Large Gradual Solar Particle Events // ApJ. 2005. V. 625. P. 474.
Zhang M. et al. (2003) Perpendicular transport of solar energetic particles in Heliospheric magnetic fields // ApJ. 2003. V. 595. P. 493.
Ротапринт ИКИ РАН 117997, Москва, Профсоюзная ул., 84/ 055(02) Подписано к печати 12.10.2011_ Заказ 2260 Формат 70х108/32 Тираж 100 2,0 уч.-изд.л..

References: V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V. 
 V.