Large solar event of September 29, 1989: Ten years after

Space Science Reviews

Volumn 91, Issue 3-4, 2000, Pages 615-715

  Miroshnichenko, L I ^a,b   De Koning, C A ^c   Perez Enriquez, R ^a,d  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^b PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

^c UNIVERSITY OF DELAWARE   (United States)

^d CENTRO DE FÍSICA APLICADA Y TECNOLOGÍA AVANZADA   (Mexico)

Author keywords

[No Author keywords available]

Indexed keywords

PROTON;

ACCELERATION; ARTICLE; COSMIC RADIATION; ENERGY; GAMMA RADIATION; SOLAR RADIATION; STATISTICAL MODEL; X RAY;

EID: 0033831107     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1005279108725     Document Type: Article

References (235)

1. The effects of solar flares on single event upset rates
2. Search for neutrinos from solar flares with the Mont Blanc Detector
3. Atmospheric attenuation length for relativistic solar protons
4. Mean attenuation length for solar protons of 29 September 1989
5. The ground level enhancement of September 29, 1989
6. Worldwide solar flare associated increase of cosmic ray intensity on September 29, 1989
7. Evidence for prolonged acceleration based on a detailed analysis of the long-duration solar gamma-ray flare on June 15, 1991
8. Powerful solar proton events at the onset of cycle 22
9. The ground level comic ray event of September 29, 1989, as recorded by the Rome detectors
10. Preliminary analysis of the 29 September 1989 solar flare on the basis of data from the kover instrument at the baksan neutrino observatory
11. Analysis of the data of the baksan underground scintillation telescope registered during the solar flare of September 29, 1989
12. 29 September 1989 GLE (Ground Level Enhancement) at baksan air shower array (BASA)
13. Short-term increases of muon intensity at baksan underground scintillation telescope correlated with solar flares?
14. Short-Term bursts of muon intensity at the baksan underground scintillation telescope correlated with solar flares
15. The ground level solar cosmic ray enhancements in 1989-1990
16. Magnetospheric effects in cosmic rays during forbush-decreases
17. The features of the ground level increase of cosmic ray intensity on September 29, 1989
18. Peculiarities of ground level increase in solar cosmic rays on 29 September 1989 according to neutron monitor data
19. The features of the ground level increase of cosmic ray intensity on September 29, 1989
20. Proton spectra of the four remarkable GLE in the 22nd solar cycle
21. Dynamics of radiation conditions on the path of the MIR space station at the time of the 29 Septqmber 1989 solar proton event
22. Investigation of radiation conditions on the MIR station during the September 29, 1989, solar proton event: Results from the lyulin dosimeter-radiometer
23. Transient phenomena in the energetic behind-the-limb solar flare of September 29, 1989, Proc. of the IAU Colloq. No. 154, January 1995 Pune, India
24. Focusing anisotropy of solar cosmic rays
25. A barrage of relativistic solar particle events
26. Determination of energy spectra for the large solar particle events of 1989
27. Proton and electron mean free paths: The palmer consensus revisited
28. Injection characteristics of energetic particles on the sun during GLE
29. Energetic particles in the solar wind: Propagation, acceleration and moodulation
30. Investigation of acceleration and propagation of solar cosmic rays in wide energy region (10 MeV-1000 GeV) generated during 56 flares
31. Post-Eruption particle acceleration in the corona: A possible contribution to solar cosmic rays
32. Yohkoh data on CME-flare relationships and post-eruption magnetic reconnection in the corona
33. The role of coronal mass ejections and post-eruption energy release in solar high-energy phenomena
34. Some features of the post-eruption energy release in the solar corona
35. Evolution of our understanding of solar flare particle acceleration: (1942-1995)
36. Prompt injection of relativistic protons from the September 1, 1971 solar flare
37. Solar flare gamma-ray emission and energetic particle in space
38. Injection onsets of ~2 GeV protons, ~1 MeV electrons, and ~100 keV electrons in solar cosmic ray flares
39. On the origin of gamma-ray emission from the behind-the-limb flare on 29 September 1989
40. On cosmic-ray cut-off terminology
41. The response of los cerrillos detectors to the 1989/1990 GLE events
42. Cosmic ray intensity increase observed on September 29, 1989: The chilean neutron monitor data
43. The GLE of 29 September 1989
44. The effect of near-earth IMF structure on the modeling of ground level enhancements
45. Observations related to the acceleration, injection, and interplanetary propagation of energetic protons during the solar cosmic ray event of February 16, 1984
46. The GLE of September 29, 1989: Analysis of the pitch angle distribution I
47. The GLE of September 29, 1989: Analysis of the pitch angle distribution II
48. Diffusion analysis of the GLE (Ground Level Enhancement) of September 29, 1989
49. X-ray aspects of the high energy solar physics workshop: Rapporteur paper I
50. Determination of the ionic charge states of SEPs using the University of Chicago IMP-8 instrument
51. Solar cosmic rays
52. Comments on the origins of coronal mass ejections
53. Relativistic solar cosmic rays
54. The ground level enhancements of 1989 September 29 and October 22
55. Analysis of cosmic ray pitch angle anisotropy during the forbush-effect in June 1972 by the method of spectrographic global survey
56. A spectrographic global survey technique for studying cosmic-ray distribution function variations and the planetary system of geomagnetic cutoff rigidities
57. The GLE of 29 September 1989: Time variations of the cosmic-ray rigidity spectrum
58. The GLE of 29 September 1989: Time variations in angular distribution of different-energy particles
59. Time variations of the cosmic ray distribution function during a solar proton event of September 29, 1989
60. The effect of adiabatic focusing upon charged-particle propagation in random magnetic fields
61. Non-Diffusive propagation of cosmic rays in the solar system and in extragalactic radio sources
62. Propagation of charged particle pulses immediately after injection
63. Shock acceleration of electrons and ions in solar flares
64. Neutrino generation during the flares at visible and invisible sides of the solar disk
65. Anisotropy of solar cosmic rays at different ejection regimes of energetic particles
66. Solar cosmic ray transport under anisotropic injection
67. The GLE of May 24, 1990: Kinetic approach to anisotropic event
68. On the propagation and diffusion of solar protons
69. Cosmic ray flares between August and October 1989
70. Solar cosmic ray flare on September 29, 1989, by data of the yakutsk array complex
71. Solar cosmic rays
72. Aspects of combining models of the Earth's internal and external magnetic field
73. Grund-Level enhancement database: An update
74. Compilation and distribution of relativistic solar proton data
75. The solar flare myth
76. 4He ratios for March and June 1991 SEP events
77. Upper cutoff of high energy solar protons
78. Solar proton event: Influence on stratospheric ozone
79. Solar flare neutron production and the angular dependence of the capture gamma-ray emission
80. Detection of 0.5-15 GeV protons on 29 September 1989 at Australian stations
81. The 29 September 1989 solar cosmic ray event as observed by Australian stations
82. Association between coronal mass ejections and solar energetic proton events
83. Injection profiles of solar energetic particles as functions of coronal mass ejection heights
84. Temporal variations of shock-accelerated proton/alpha ratios at E ≥ 100 MeV/nucleon in a large solar energetic particle event
85. On taking into account the barometric effect of the neutron component during cosmic ray flares
86. On the possibility of observation of extremely high-energy particles by the baksan underground scintillation telescope during solar flares
87. Extremely high-energy solar protons by the data of baksan underground scintillation telescope
88. On a search for the extremely high-energy particles from the sun by the baksan underground scintillation telescope data
89. Intensity of protons with energy above 500 GeV during GLEs
90. Intensity of protons with the energy above 500 GeV during solar flares
91. Muon bursts at the baksan underground scintillation telescope during energetic solar phenomena
92. Ozone 'Mini-Holes' initiated by solar protons in the northern and southern polar caps
93. Cosmogenic nuclei, solar neutrinos, neutrons and gamma-rays
94. Solar thermonuclear and flare neutrinos
95. Solar flare neutrinos
96. Solar proton intensity magnitudes of large flares in fall 1989 observed at synchronous orbit
97. Generation and propagation of high-energy solar cosmic rays in the 29 September 1989 event according to the data of the Global Neutron Monitor Network
98. Upper limit of the energy spectrum for solar cosmic rays
99. High energy particle generation during the solar flares
100. Production of neutrinos in solar flares
101. On the origin of solar protons of extremely high energies: Signatures of the post-eruptive acceleration in the corona
102. The exceptional cosmic ray burst of September 29, 1989, as indicated by data from the Yakutsk Array Complex
103. Quasiperiodic variations and terrestrial environments
104. Solar particle production
105. Non-thermal processes in large solar flares
106. Relativistic acceleration of protons in reconnecting current sheets of solar flares
107. An extended analysis of the September 1989 cosmic ray ground level enhancement
108. 3He-rich solar flares
109. The observation of a 'Negative Burst' with high spatial resolution
110. Solar particles and processes
111. Gamma rays from pion decay: Evidence for long-term trapping of particles in solar flares
112. Particle acceleration in solar flares
113. A circuit model for filament eruption and two-ribbon flares
114. Unique series of increases in cosmic ray intensity due to solar flares
115. Muon telescope observations of the solar flare ground level event of 29 September 1989
116. The cosmic-ray flare effect. I. Some new methods of analysis
117. Much ado about nothing
118. On the absolute fluxes of particles accelerated at the sun on February 23, 1956
119. On conditions of the spectrum formation for Solar Cosmic Rays near the earth and in the source
120. Investigations of Solar Cosmic Rays
121. Cyclic variations and sporadic fluctuations of Solar Cosmic Rays
122. Generation and transport of Solar Cosmic Rays
123. Acceleration parameters and particle spectrum dynamics in Solar Flares
124. On the ultimate capabilities of particle accelerators on the sun
125. Empirical model for the upper limit spectrum for solar cosmic rays at the earth's orbit
126. Energetic particles in extended coronal structures: Acceleration scenario with two sources
127. Numerical solution of inverse problem for the restoration of source spectrum of solar cosmic rays
128. Relativistic protons near the sun on September 29, 1989
129. Two relativistic solar proton components in some SPEs
130. On the formation of relativistic particle beams in extended coronal structures: I. Evidence for two separate sources of solar cosmic rays
131. On the formation of relativistic particle beams in extended coronal structures: II. Two source model for solar cosmic rays
132. On the formation of relativistic particle fluxes in extended coronal structures
133. Relativistic protons near the sun on September 29, 1989
134. Relativistic protons near the sun on September 29 and October 22, 1989: Pitch angle distributions and ejection functions
135. Energy spectra of accelerated solar protons from different sources: I. Reconstruction and properties of source spectrum
136. Space distribution and rigidity spectrum of solar particles of the GLE observed on 29 September 1989
137. Motion of solar cosmic rays in the coronal magnetic field
138. Release of solar cosmic rays from the corona: Rayleigh-Taylor instability and reconnection
139. Solar protons in the 22nd cycle of solar activity
140. The October 22, 1989, solar cosmic ray event measured at geosynchronous orbit
141. Coronal transport of solar flare particles
142. Spectrum of accelerated particles in solar proton events with a prompt component
143. The spectrum of accelerated particles in solar proton events with a prompt component
144. An electromagnetic model of solar flare
145. Theoretical models for high energy solar flare emissions
146. Implications of solar flare charge particles, gamma ray and neutron observations: Rapporteur paper ii for the high energy solar physics workshop
147. Nuclear processes and accelerated particles in solar flares
148. Solar gamma rays
149. On the origin of the pion-decay radiation in the 1982 June 3 solar flare
150. Acceleration in solar flares: Interacting particles versus interplanetary particles
151. Non-thermal particles in the interplanetary medium
152. The dark side of the solar flare myth
153. Energetic particles from solar flares and coronal mass ejections
154. The spatial distribution of particles accelerated by coronal mass ejection-driven shocks
155. The great solar energetic particle events of 1989 observed from geosynchronous orbit
156. Response of the middle atmosphere to the solar proton events of August-December, 1989
157. Coronal transport of solar flare protons
158. Dynamics of an auroral low ionospheric fringe at geophysical disturbances on 29 September 1989
159. Prompt arrival of solar energetic particles from Far Eastern events: The role of large-scale interplanetary magnetic field structure
160. Propagation of coherent pulses of solar cosmic rays
161. Solar flares and collisions between current-carrying loops
162. A solar flare type increase in cosmic rays at low latitudes
163. GOES observations of energetic protons E > 685 MeV: Ground-Level events from October 1983 to July 1992
164. Fast azimuthal transport of solar cosmic rays via a coronal magnetic bottle
165. Evidence for very high-energy solar particle production
166. Solar cosmic rays, 1960-1989
167. The evaluation of cutoff rigidities and reentrant albedo calculations for Palestine, Dallas, and Midland, Texas
168. Possible evidences for a rigidity-dependent release of relativistic protons from the solar corona
169. A summary of major solar proton events
170. Solar proton events - Review and status
171. Recent and historical solar proton events
172. Solar proton events: History, statistics and predictions
173. Significant proton events of solar cycle 22 and a comparison with events of previous solar cycles
174. Unusual intensity-time profiles of ground-level solar proton events
175. Dual acceleration and/or release of relativistic solar cosmic rays
176. Possible ground-level measurements of solar neutron decay protons during the 19 October 1989 solar cosmic ray event
177. Review of ground-level solar cosmic ray enhancements during the 22nd solar cycle
178. Ozone 'Miniholes' initiated by energetic solar protons
179. High-latitude ozone 'Miniholes' and solar protons
180. Protons in solar flares
181. Solar cosmic rays
182. Solar proton events during the past three solar cycles
183. Probable pitch angle distribution and spectra of the 23 February 1956 solar cosmic ray event
184. A comparison of the magnitude of the 29 September 1989 high energy event with solar cycle 17, 18 and 19 events
185. Unusual aspects of the ground-level cosmic ray event of 7/8 December 1982
186. Solar cosmic rays on 29 September 1989: An analysis using the world-wide network of cosmic ray stations
187. Magnetically driven coronal transients
188. Reconnection and acceleration to high energies in flares
189. The solar proton flare of 29 September 1989 as recorded South African neutrons monitors
190. Coronal and interplanetary transport of solar flare protons from the ground level event of 29 September 1989
191. Ground-Level solar flare proton event recorded by the sanae neutron monitor since 1966
192. Relativistic solar proton events
193. On 'the Solar Flare Myth' postulated by gosling
194. The September 29, 1989 ground-level event observed at high rigidity
195. Observation of high energy solar particles on September 29, 1989, by neutron monitors with high time resolution
196. Radiation dose measurements on board the station MIR during solar proton flares in September-October 1989
197. Estimation of transport parameters for the solar cosmic ray events in 1989
198. Search for peculiarities in the flux profiles of GLEs in 1989
199. Estimation of high-energy solar particle-transport parameters during the GLEs in 1989
200. Measurement of the radiation dose on the MIR station during solar proton events in September-October, 1989
201. The mean ionic charge state of solar energetic Fe ions above 200 MeV per nucleon
202. Observation of very high energy solar heavy ions from IMP-8
203. High energy solar Fe ions in the 29 September 1989 ground level event
204. Characteristics of generation and transport of solar protons during the event of September 29, 1989
205. The GLE of September 29, 1989 study by computations and experimental data analysis
206. Short-Term SCR intensity variations during GLE
207. Search for peculiarities of proton events in solar cycle 22 from ground based observations
208. Large ground-level events in solar cycle 22 and some peculiarities of relativistic proton acceleration
209. Peculiarities of anisotropy during ground level events of the 22nd cycle of solar activity
210. Generation and propagation characteristics of relativistic solar protons during the GLE of September 29, 1989
211. Proton energy spectrum and source parameters of the September 29, 1989 event
212. Evidence for a spatially extended component of gamma rays from solar flares
213. The solar maximum mission atlas of gamma ray flares
214. Intercomparison of neutron monitors during solar-flare increases
215. Complex features of the GLE of September 29, 1989
216. What is the condition for fast magnetic reconnection?