THREE-DIMENSIONAL EVOLUTION OF SOLAR WIND DURING SOLAR CYCLES 22–24

作者: P. K. Manoharan

DOI: 10.1088/0004-637X/751/2/128

关键词: Solar cycle 22Solar maximumSolar cycle 23PhysicsCoronal holeSolar minimumSolar cycleAtmospheric sciencesHeliospheric current sheetCoronal mass ejection

摘要: This paper presents an analysis of three-dimensional evolution solar wind density turbulence and speed at various levels activity between cycles 22 24. The data used in this study have been obtained from the interplanetary scintillation (IPS) measurements made Ooty Radio Telescope, operating 327 MHz. Results show that (1) on average, there was a downward trend maximum cycle to deep minimum phase 23; (2) scattering diameter corona around Sun shrunk steadily toward Sun, starting 2003 smallest size deepest minimum, it corresponded reduction ~50% phases (3) latitudinal distribution significantly different minima 23. At 22, when underlying magnetic field simple nearly dipole nature, high-speed streams were observed poles ~30° latitudes both hemispheres. In contrast, long-decay 23, sources poles, accordance with weak polar fields, occupied narrow latitude belts ~60° latitudes. Moreover, agreement large amplitude heliospheric current sheet, low-speed prevailed low- mid-latitude regions heliosphere. (4) transition 23 24, high close equator extended equatorial-to-mid-latitude regions. above results comparison Ulysses other situ suggest source has changed globally, important implication supply mass energy space reduced prolonged period low activity. IPS are consistent onset growth middle 2009. However, width northern almost disappeared indicates ascending reached hemisphere Sun. southern part hemisphere, yet develop and/or increase.

参考文章(52)
P. Fox, P. McIntosh, P. R. Wilson, Coronal Holes and the Polar Field Reversals Solar Physics. ,vol. 177, pp. 375- 393 ,(1998) , 10.1023/A:1004939014025
A. J. Lazarus, The Day the Solar Wind Almost Disappeared Science. ,vol. 287, pp. 2172- 2173 ,(2000) , 10.1126/SCIENCE.287.5461.2172
S. R. Cranmer, J. T. Hoeksema, J. L. Kohl, SOHO-23: Understanding a Peculiar Solar Minimum SOHO-23: Understanding a Peculiar Solar Minimum. ,vol. 428, ,(2010)
S. Ananthakrishnan, P. K. Manoharan, Determination of solar-wind velocities using single-station measurements of interplanetary scintillation. Monthly Notices of the Royal Astronomical Society. ,vol. 244, pp. 691- 695 ,(1990)
M. Tokumaru, M. Kojima, K. Fujiki, K. Maruyama, Y. Maruyama, H. Ito, T. Iju, A newly developed UHF radiotelescope for interplanetary scintillation observations: Solar Wind Imaging Facility Radio Science. ,vol. 46, ,(2011) , 10.1029/2011RS004694
Masayoshi Kojima, Ken-ichi Fujiki, Masaya Hirano, Munetoshi Tokumaru, Tomoaki Ohmi, Kazuyuki Hakamada, Solar Wind Properties from IPS Observations ASSL. ,vol. 317, pp. 147- 178 ,(2004) , 10.1007/978-1-4020-2831-1_6
Li-Jia Liu, Xi-Zhen Zhang, Jian-Bin Li, P. K Manoharan, Zhi-Yong Liu, Bo Peng, Observations of interplanetary scintillation with a single-station mode at Urumqi Research in Astronomy and Astrophysics. ,vol. 10, pp. 577- 586 ,(2010) , 10.1088/1674-4527/10/6/007
K. Asai, M. Kojima, M. Tokumaru, A. Yokobe, B. V. Jackson, P. L. Hick, P. K. Manoharan, Heliospheric tomography using interplanetary scintillation observations: 3. Correlation between speed and electron density fluctuations in the solar wind Journal of Geophysical Research: Space Physics. ,vol. 103, pp. 1991- 2001 ,(1998) , 10.1029/97JA02750
C. O. Lee, J. G. Luhmann, X. P. Zhao, Y. Liu, P. Riley, C. N. Arge, C. T. Russell, I. de Pater, Effects of the Weak Polar Fields of Solar Cycle 23: Investigation Using OMNI for the STEREO Mission Period Solar Physics. ,vol. 256, pp. 345- 363 ,(2009) , 10.1007/S11207-009-9345-6
M. SCHUBIGER, H. A. SCHNEIDERMAN, Nuclear Transplantation in Drosophila melanogaster Nature. ,vol. 230, pp. 185- 186 ,(1971) , 10.1038/230185A0