PROBLEMS OF GEOCOSMOS

More documents

Recommendations

Info

Proceedings of the 7th International Conference "Problems of Geocosmos" (St. Petersburg, Russia, 26-30 May 2008) Fig. 3. a - dynamics of the sliding Hurst exponent (H) for solar (SSN H) and magnetospheric (AP H) activity, b - dynamics of cumulative deviation from the average Hurst exponent for solar (i SSN H) and magnetospheric (i AP H) activity, c - dynamics of cumulative deviation from the average of solar activity chaotic component (i SSN_Ch M). We observe the feature of dynamics of chaotic component of solar and magnetospheric activity around 1960 year. Analysis: Ap – Temperature. We see some high correlation between dynamics of cumulative deviation from the average of chaotic components for all meteorological stations. Fig. 4a shows data for three stations only. Data of the other three stations have similar dynamics. Fig. 4. a - dynamics of cumulative deviation from the average (Hurst exponent) for air temperature i Т H, b - dynamics of sliding average amplitudes Ap and T, c - dynamics of cumulative deviation from the average amplitudes Ap and T. 357
Proceedings of the 7th International Conference "Problems of Geocosmos" (St. Petersburg, Russia, 26-30 May 2008) Also we see feature in dynamics of chaotic component of temperature: its sharp declining begins in area of 1960 (Fig. 4a). Simultaneously we see an appearance of correlation between an average amplitude of Ap-index and T near 1960 year (Fig.4b and Fig.4c).). We see low correlation till 1960 and after 1960 high correlation (see also Fig. 5b) What happens? What has occurred in dynamics of geospheres (correlation between magnetosphere activity and air temperature after 1960)? How this phenomenon can be explained? Correlation in dynamics of the fractal dimensions of the investigated series was found. Feature near 1960 year in dynamics of the Sun activity chaotic component and the magnetospheric activity also was found. The dynamics of the air temperature does not correlate with dynamics of the magnetosphere activity till 1960 and high correlation is observed after 1960. First hypothesis: The change of a spectral structure (Hurst exponent) and burst of amplitude of chaotic mode of the Sun activity was near 1960. It has led to change of the geospheres dynamics character. The phenomenon can be interpreted as the noise induced phase transition in the Earth’s system. Second hypothesis: The technogenic influence on geospheres connected with a significant intensification of nuclear tests and the beginning of a space age has sharply increased in area of 1960. There is other possible reason of effect of correlation changes between temperature and magnetic field in this situation, namely, influence of the anthropogenous factor. Analysis: other geospheres. We find the features in dynamics of parameters of other geospheres in area of 1960 (Fig. 5 and Fig. 6). We used our results (Fig. 5b and Fig. 5c) and the published information (data, plots) for an illustration of the phenomenon 1960. We have changed appearance of some plots in comparison with originals, but have not changed their information. We see features in other geospheres dynamics in area 1960 year (Fig. 5 and Fig. 6). Fig. 5. a - global nuclear testing [npc.sarov.ru/issues/testing.html], b - correlation coefficient Ccor between average amplitude of Ap-index and T, c - global seismic activity M > 6, d - parameter of chaos in E-layer of ionosphere [Givishvili and Leschenko, 1998] 358
Page 1 and 2:
Saint-Petersburg State University P
Page 3 and 4:
Proc. of the 7th Intern. Conf. "Pro
Page 5 and 6:
Page 7 and 8:
Page 9 and 10:
Page 11 and 12:
Î�ÒÙ×�ØØ��Ñ��Ò
Page 13 and 14:
Proceedings of the 7th Internationa
Page 15 and 16:
��ÒÓÛÐ��Ñ�ÒØ
Page 17 and 18:
Page 19 and 20:
Page 21 and 22:
Page 23 and 24:
Page 25 and 26:
Page 27 and 28:
Page 29 and 30:
Page 31 and 32:
Page 33 and 34:
Page 35 and 36:
(the first number), two three-lette
Page 37 and 38:
Page 39 and 40:
Page 41 and 42:
Page 43 and 44:
Page 45 and 46:
Page 47 and 48:
vertical fields. The vertical field
Page 49 and 50:
Page 51 and 52:
Page 53 and 54:
Page 55 and 56:
Page 57 and 58:
Page 59 and 60:
Page 61 and 62:
Page 63 and 64:
Page 65 and 66:
Page 67 and 68:
Page 69 and 70:
Page 71 and 72:
Page 73 and 74:
Page 75 and 76:
Page 77 and 78:
Page 79 and 80:
Page 81 and 82:
Page 83 and 84:
Page 85 and 86:
Page 87 and 88:
Page 89 and 90:
Page 91 and 92:
Page 93 and 94:
Page 95 and 96:
Page 97 and 98:
Page 99 and 100:
Page 101 and 102:
Page 103 and 104:
Page 105 and 106:
Page 107 and 108:
Page 109 and 110:
Page 111 and 112:
Page 113 and 114:
Page 115 and 116:
Page 117 and 118:
Page 119 and 120:
Page 121 and 122:
Page 123 and 124:
Page 125 and 126:
Page 127 and 128:
Page 129 and 130:
Page 131 and 132:
Page 133 and 134:
Page 135 and 136:
Page 137 and 138:
Page 139 and 140:
Page 141 and 142:
Page 143 and 144:
Page 145 and 146:
Page 147 and 148:
Page 149 and 150:
Page 151 and 152:
Page 153 and 154:
Page 155 and 156:
Page 157 and 158:
Page 159 and 160:
Page 161 and 162:
Page 163 and 164:
Page 165 and 166:
Page 167 and 168:
Page 169 and 170:
Page 171 and 172:
90 60 30 0 -30 -60 Proceedings of t
Page 173 and 174:
Page 175 and 176:
Page 177 and 178:
Page 179 and 180:
Page 181 and 182:
Page 183 and 184:
Page 185 and 186:
Page 187 and 188:
Page 189 and 190:
Page 191 and 192:
Page 193 and 194:
Page 195 and 196:
Page 197 and 198:
Page 199 and 200:
Page 201 and 202:
Page 203 and 204:
Page 205 and 206:
Page 207 and 208:
Page 209 and 210:
Page 211 and 212:
Page 213 and 214:
Page 215 and 216:
Page 217 and 218:
Page 219 and 220:
Page 221 and 222:
Page 223 and 224:
Page 225 and 226:
Page 227 and 228:
Page 229 and 230:
Page 231 and 232:
Page 233 and 234:
Page 235 and 236:
Page 237 and 238:
Page 239 and 240:
Page 241 and 242:
a Proceedings of the 7th Internatio
Page 243 and 244:
Page 245 and 246:
Page 247 and 248:
Page 249 and 250:
Page 251 and 252:
Page 253 and 254:
Page 255 and 256:
Page 257 and 258:
Page 259 and 260:
Page 261 and 262:
Page 263 and 264:
Page 265 and 266:
Page 267 and 268:
Page 269 and 270:
Page 271 and 272:
Page 273 and 274:
Page 275 and 276:
Introduction ON THE NATURE OF PLASM
Page 277 and 278:
Page 279 and 280:
Page 281 and 282:
Page 283 and 284:
Page 285 and 286:
Page 287 and 288:
Page 289 and 290:
Page 291 and 292:
Page 293 and 294:
Page 295 and 296:
Page 297 and 298:
Page 299 and 300:
Page 301 and 302:
Page 303 and 304:
Page 305 and 306:
Page 307 and 308:
Page 309 and 310:
Vy Here index j =1,2 characterizes,
Page 311 and 312:
Jy Proceedings of the 7th Internati
Page 313 and 314:
Page 315 and 316: Proceedings of the 7th Internationa
Page 337 and 338: Fig. 3. Dependence of 1D interpreta
Page 365: Proceedings of the 7th Internationa
Page 417 and 418:
Page 419 and 420:
Page 421 and 422:
Page 423 and 424:
Page 425 and 426:
Page 427 and 428:
Page 429 and 430:
Page 431 and 432:
Page 433 and 434:
Page 435 and 436:
Page 437 and 438:
Page 439 and 440:
Page 441 and 442:
Page 443 and 444:
Page 445 and 446:
Page 447 and 448:
Page 449 and 450:
Page 451 and 452:
Page 453 and 454:
Page 455 and 456:
Page 457 and 458:
Page 459 and 460:
Page 461 and 462:
Page 463 and 464:
Page 465 and 466:
Page 467 and 468:
Page 469:
Page 476 and 477:
Page 478 and 479:
Page 480 and 481:
Page 482 and 483:
Page 484 and 485:
Page 486 and 487:
Page 488 and 489:
Page 490 and 491:
Page 492 and 493:
Page 494 and 495:
2. Burlaga & Klein method. The main
Page 496 and 497:
Page 498 and 499:
Page 500 and 501:
Page 502 and 503:
Page 504 and 505:
show all

PROBLEMS OF GEOCOSMOS

Create successful ePaper yourself

Delete template?

Save as template?