太阳较差自转130年(1855~1985)的观测和理论研究史的回顾
Look Back on History (130 Years) of Observational and Theoretical Research of Solar Differential Rotation (1855-1985)

DOI: 10.12677/AAS.2013.13007, PP. 45-52

Keywords: 太阳较差自转；观测和理论研究史(1855~1985)；回顾
Solar Differential Rotation, History of the Observational and Theoretical Research (1855-1985), Look Back

Full-Text   Cite this paper   Add to My Lib

Abstract:

本文对太阳较差自转从1855年到1985年130年的观测和理论研究史做了回顾。回顾了天文工作者对太阳较差自转的观测和理论研究结果，其中包括纬向较差自转的表面观测和理论研究，也包括了径向较差自转(内部较差自转)以及产生较差自转的机制，稳定和演化的研究结果。在最后一节中作者还列出了在不同年代一些作者从观测和理论研究给出的太阳的纬向和径向较差自转定律的形式。
The history of observational and theoretical research of solar differential rotation is investigated from 1855 to 1985 year for 130 years. The results given by a lot of authors on this topic are reviewed including solar latitudinal and radial differential rotation and its mechanism, evolution and stability. In the last section, the author listed the formation for the law of solar latitudinal and radial differential rotation given by some astronomical workers from observational and theoretical research in the different era.

References

[1]	Carrington R C. Results of astronomical observations made of the observatory of the University, Durham, 1855.
[2]	Carrington R C. MNRAS, 1859: 13
[3]	Carrington R C. Observation of Solar Spots. London: Williarms and Norgate, 1863: 244.
[4]	Faye H. CR, 1865, 60: 138.
[5]	Sp？rer G. PAG, 1874, 13: 151.
[6]	Maunder A S D. MMRAS, 1905, 65: 813.
[7]	Newall M F. MNRAS, 1922, 82: 110.
[8]	Stom K (外目清秀). PIA, 1927, 3: 317.
[9]	Notuki M (野附诚夫). PPMSJ, 1929, 11: 102.
[10]	Abetti G. HDP, 1929, 4: 162.
[11]	Abetti G. ALA, 1934, 9: 863.
[12]	Newton H W. MNRAS, 1934, 95: 66.
[13]	Becker U. ZA, 1954, 34: 229.
[14]	Kippenhahn R. ApJ, 1963, 173: 309.
[15]	Durner B R. SoPh, 1974, 38: 309.
[16]	Deubner F L, Vazquez M. SoPh, 1975, 43: 87.
[17]	Chostyakov V F. BAICz, 1976, 27: 84.
[18]	Newton H W, Numn M. MNRAS, 1951, 111: 413.
[19]	Ward F. ApJ, 1965, 141: 534; ApJ, 1966, 145: 416.
[20]	Lustig G, Dvorak R. A&A, 1984, 141: 105.
[21]	Howard R, et al. ApJ, 1984, 283: 373.
[22]	Lustig G, Dvorak R. A&A, 1984, 141: 105.
[23]	Balthasar H, et al. SoPh, 1982, 76: 21.
[24]	Ward F. ApJ, 1966, 145: 416.
[25]	Godoli G, Mazzucconi F. SoPh, 1979, 64: 247.
[26]	Balthasar H, Wohl H. A&A, 1980, 92: 111.
[27]	Arèvolo M J, et al. A&A, 1982, 111: 266.
[28]	Howard R, et al. ApJ, 1984, 283: 373.
[29]	Balthesar H, et al. SoPh, 1984, 91: 55.
[30]	Wilsing J. AN, 1888, 119: 311.
[31]	Cheralier S. ApJ, 1910, 32: 388.
[32]	Cheralier S. AnZoC, 1911, 6: 47.
[33]	Wolfer A. VNG, 1896, 41: 100.
[34]	Hale E G. ApJ, 908, 7: 219.
[35]	Kempf P. POPot, 1916, 71: 36.
[36]	Fox P. PYerO, 1921, 3: 67.
[37]	D’azambuja M. AnApm, 1948, 6: 7.
[38]	Duner N C. Upsala: Sur la rotation du Soleil, 1891.
[39]	Duner N C. UGC, 1891, 3: 3.
[40]	Halm J. MNRAS, 1907, 173: 273.
[41]	Halm J. TRSE, 1981, 41: 89.
[42]	Adans W S, Lasby J B. Publications of Carnegie Institution of Washington, 1911: 1.
[43]	Adans W S. Rotation Periods of the Sun, 1911.
[44]	Adans W S. ApJ, 1910, 31: 30.
[45]	S t John C E. ApJ, 1913, 38: 341.
[46]	Schlesinger F. MNRAS, 1944, 104: 94.
[47]	Plaskett J S. ApJ, 1913, 37: 73; 1915, 42: 392.
[48]	Lury R E. JRASC, 1935, 35: 39.
[49]	Evershed J. MNRAS, 1913, 73: 554; 1935, 95: 503.
[50]	Notuki M. PPMSJ, 1930, 12: 264.
[51]	Livingston W C. SoPh, 1969, 29: 448.
[52]	Hansen R T, Hansen S F. SoPh, 1969, 10: 135.
[53]	Simon G W. SoPh, 1972, 1: 8.
[54]	Belvedere G, Godoli G, Smott L. MmSAI, 1972, 43: 637.
[55]	Dupree A K. SoPh, 1973, 33: 452.
[56]	Scherree P H. SoPh, 1972, 26: 15.
[57]	Milasevie K M. CzAS, 1950, 201: 666.
[58]	Schr？ter E H, et al. SoPh, 1975, 42: 3.
[59]	Schr？ter E H, W？hl H. SoPh, 1976, 49: 19.
[60]	Dupree A K, Henze W. SoPh, 1972, 27: 271.
[61]	Simon G W, Noyes R W. SoPh, 1972, 22: 450.
[62]	Liu S J, Kundu R M. SoPh, 1976, 46: 15.
[63]	Antomucci E, et al. SoPh, 1977, 53: 519.
[64]	d’Azambuja M. AnPar, 1948, 6: 1.
[65]	Wagner W J. ApJ, 1975, 198: L141.
[66]	Adams W M. SoPh, 1976, 47: 601.
[67]	Timothy A F, et al. SoPh, 1975, 42: 135.
[68]	Sonodgrass H M. SoPh, 1984, 94: 13. .
[69]	d’Azambuja M. AnApM, 1948, 6: 7.
[70]	Howard R, Har-vey J W. SoPh, 1970, 12: 23.
[71]	Howard R, et al. SoPh, 1980, 66: 167.
[72]	Howard R, et al. SolPh, 1983, 83: 321.
[73]	Scherrer P H, et al. ApJ, 1980, 241: 811.
[74]	LaBotte B J, Howard R. SoPh, 1982a, 75: 161; 1982b, 80: 361.
[75]	Snodgrass H M, et al. SoPh, 1984, 90: 199.
[76]	Pierce A K, Lopresto J C. SoPh, 1984, 93: 155.
[77]	Howard R. ARA&A, 1984, 22: 131.
[78]	Schr？ter E H. SoPh, 1985, 100: 14.
[79]	Wilsing J. AN, 1891, 127: 233.
[80]	Harzer P. ApNr, 1891, 127: 17.
[81]	Wilczinski E J. Hydrodynamische Un-dersuchungen mit Anwendung auf die Theorie des Sonnen Rotation. Berlin: Mayer and Muller, 1897.
[82]	Jeans H. MNRAS, 1926, 85: 328. .
[83]	Rosseland S. ZA, 1930, 1: 138.
[84]	Emden R. ZA, 1936, 12: 233.
[85]	荒川俊秀. 科学, 1940, 10: 82.
[86]	Biermann B L. ZA, 1951, 38: 304.
[87]	Synge J L. MNRAS, 1963, 124: 275.
[88]	Wasiutynsky J. ApNr, 1946, 4: 1.
[89]	Kippenhahn R. MSRSL, 1960, 5: 249.
[90]	Kippenhahn R. ApJ, 1963, 137: 664.
[91]	Sakurai T. PASJ, 1966, 18: 174.
[92]	Plaskett H H. MNRAS, 1966, 131: 407.
[93]	Cocke W J. ApJ, 1967, 150: 1041.
[94]	Roburgh I W. Proc IAU COU on Stellar Rotation, 8-11 Septem- ber 1969: 318-320. Edited by A Slettebak, Columbus: Ohio State Univer-sity.
[95]	Kohler H. SoPh, 1974, 34: 11.
[96]	Durney B R. SoPh, 1973, 23: 3.
[97]	Durney B R. ApJ, 1974, 190: 211.
[98]	Kato S, Nakagawa Y. SoPh, 1969, 10: 476.
[99]	Nickel G H. SoPh, 1969, 10: 472.
[100]	Gierasch P J. ApJ, 1974, 190: 199.
[101]	Gunn R. PhRv, 1930, 35: 635; 1930, 36: 1251; 1931, 37: 283.
[102]	Ferraro V C A. MNRAS, 1937, 97: 458.
[103]	Alfven H. ArMAF, 1943, 29: 1.
[104]	Walèn C. On the Vibratory Rotation of the Sun. Stockholm: Henrik Lindst？hls Bokhandel, 1949.
[105]	Chapman S. MNRAS, 1948, 108: 410
[106]	Lundquist S. ArMAF, 1948, 35: 1.
[107]	Cowling F G. Solar Electro-Dynamics. Chicago: University of Chicago Press, 1953: 31.
[108]	Clark A, Thomas J H, Clark P A. Sci, 1969, 164: 290.
[109]	Schatten K H. SoPh, 1973, 32: 315.
[110]	Howard R. SciAm, 1975, 232: 106.
[111]	Dicka R H. Proc IAU Colloquium on Stellar Rotation, 8-11 September 1969: 289. Edited by A Slettebak, Columbus: Ohio State University.
[112]	李林森. 东北师大学报(自然科学版), 1981, 4: 23.
[113]	Paul H M. GBzG, 1935, 44: 376.
[114]	Парийский H H. О моменме колич？ства уижения Сoлнча в “ВОПРОСЫ KОСMГОHИЙ”, 1955: том 4 edited by И А Н СССР, москва.
[115]	樱井健郎. 日本物理学会志, 1967, 22: 225.
[116]	de Jader C. HDP, 1958, B52: 80.
[117]	戴文赛. 天文学报, 1960, 8: 1.
[118]	Dicke R H. ApJ, 1967, 149: 121.
[119]	Dicke R H. Sci, 1974, 184: 419.
[120]	Schatten K H. NZJS, 1973, 16: 659. Ap&SS, 1975, 34: 467; ApJ, 1977, 216: 650.
[121]	Rood R T, Vlrich R R. Natur, 1974, 252: 366.
[122]	Demarque P, Mengel J. Natur, 1973, 246: 33.
[123]	Roxbuvgh I W. Natur, 1974, 252: 209; MNRAS, 1975, 170: 35.
[124]	杉本一郎. 科学, 1974, 44: 544.
[125]	Dicke R H. Natur, 1964, 202: 432.
[126]	Goldreich P, Schubert G. ApI, 1967, 150: 571.
[127]	Goldreich P, Schubert G. ApJ, 1968, 154: 1005.
[128]	Sakurai T. PASJ, 1972, 24: 153.
[129]	Sakurai T. MNRAS, 1975, 171: 35.
[130]	Durney B R. Proc IAU, 1976, 71: 243-295.

Full-Text