參考文獻 |
[1] Aschwanden 2010arXiv1003.0122A
[2] Aschwanden, M. J. 2010, The state of Self-Organized Criticality of the Sun During the Last Three Solar Cycles.ⅠObservations, Solar Physics 274, 119-129
[3] Bak, P., Tang, C., & Wiesenfeld, K. 1987, Self-organized criticality – An explanation of 1/f noise, Physical Review Lett. 59/27,381-384
[4] Bak, P., Tang, C., & Wiesenfeld, K. 1988, Self-organized criticality, pp.364-374
[5] Barclay, T., Still, M., Jenkins, J. M., & et al. 2012, Serendipitous Kepler observations of a background dwarf nova of SU UMa type, MNRAS, 422, 1219
[6] Barning, F. J. M. 1963, The numerical analysis of the light-curve of 12 Lacertae, Bulletin of the Astronomical Institutes of the Netherlands, Vol. 17, p.22
[7] Basri, G., Borucki, W. J., & Koch, D. 2005, The Kepler Mission: A wide-field transit search for terrestrial planets, New Astronomy Reviews, v. 49, iss. 7-9, p. 478-485
[8] Basri G., Romos-Stierle, F., Soto., K., & et al. 2008, The Kepler Mission: Terrestrial Extrasolar Planets and Stellar Activity, ASPC, 384, 281
[9] Basri, G., Walkowicz, L. M., Batalha, N., & et al. 2011, Photometric Variability in Kepler Target Stars. II. An Overview of Amplitude, Periodicity, and Rotation in First Quarter Data, AJ, 141, Issue 1, article id. 20.8 pp
[10] Basri, G., Walkowicz, L. M., & Reiners, A. 2013, Comparison of Kepler Photometric Variability with the Sun on Different Timescales, The Astrophysical Journal, Volume 769, Issue 1, article id. 37, 20 pp.
[11] Benz, A. O., & Güdel, M. 2010, Physical Processes in Magnetically Driven Flares on the Sun, Stars, and Young Stellar Objects, Annual Review of Astronomy and Astrophysics, vol. 48, p.241-287
[12] Borucki, W.J., Koch, D., Basri, G., & et al. 2010, Kepler Planet-Detection Mission: Introduction and First Results, Science, Volume 327, Issue 5968, pp. 977-
[13] Bray, R. J., & Loughhead R. E. 1964, Sunspots, The International Astrophysics Series, London: Chapman & Hall
[14] Carrington, R. C. 1860, Monthly Notices of the Royal Astronomical Society, vol. 20, p.13
[15] Cliver, E. W. 1983, Secondary peaks in solar microwave outbursts, Solar Physics, vol. 84, April 1983, p. 347-359
[16] Dennis, B.R. 1985, Solar hard X-ray bursts, Solar Physics, vol. 100, Oct. 1985, p. 465-490
[17] Fröhlich, H.- E., Frasca, A., Catanzaro, G., & et al. 2012, Magnetic activity and differential rotation in the young Sun-like stars KIC 7985370 and KIC 7765135, Astronomy & Astrophysics, Volume 543, id.A146, 16 pp
[18] Gershberg, R. E. 2005, Solar-Type Activity in Main-Sequence Stars, Solar-Type Activity in Main-Sequence Stars, Astronomy and Astrophysics Library. ISBN 978-3-540-21244-7
[19] Gilliland, R. L., Jenkins, J. M., Borucki, W. J., & et al. 2010, Initial Characteristics of Kepler Short Cadence Data, The Astrophysical Journal Letters, Volume 713, Issue 2, pp. L160-L163
[20] Gizis, J. E., Burgasser, A. J., Berger, E. & et al. 2013, Kepler Monitoring of an L Dwarf I. The Photometric Period and White Light Flares, The Astrophysical Journal, Volume 779, Issue 2, article id. 172, 14 pp
[21] Hale, G. E., Ellerman, F., Nicholson, S. B., & et al. 1919, The Magnetic Polarity of Sun-Spots, Astrophysical Journal, vol. 49, p.153
[22] Hawley, S. L., & Pettersen, B., R. 1991, The great flare of 1985 April 12 on AD Leonis, Astrophysical Journal, Part 1, vol. 378, Sept. 10, 1991, p. 725-741
[23] Hoge, E. R, 1947, The Great Sunspot Group of March and April, 1947, Publications of the Astronomical Society of the Pacific, Vol. 59, No. 348, p.109
[24] Huber, D., Aguirre, V. S., Matthews, J. M., & et al. 2014, Revised Stellar Properties of Kepler Targets for the Quarter 1-16 Transit Detection Run, The Astrophysical Journal Supplement, Volume 211, Issue 1, article id. 2, 18 pp
[25] Kasting, J. F., Whitmire, D. P., & Reynolds, R. T. 1993, Habitable Zones around Main Sequence Stars, Icarus, Volume 101, Issue 1, p. 108-128
[26] Kinemuchi, K., Barclay, T., Fanelli, M., & et al. 2012, Demystifying Kepler Data: A Primer for Systematic Artifact Mitigation, Publications of the Astronomical Society of the Pacific, Volume 124, issue 919, pp.963-984
[27] Kiraga, M., & Stępień, K. 2011, Age-Rotation-Activity Relations for M Dwarf Stars, Acta Astronomica, Vol. 57, pp.149-172
[28] Kopp, G., Lawrence, G., & Rottman, G. 2005, The Total Irradiance Monitor (TIM): Science Results, Solar Physics, Volume 230, Issue 1-2, pp. 129-139
[29] Kopp, R. A., & Pneuman, G. W. 1976, Magnetic reconnection in the corona and the loop prominence phenomenon, Solar Physics, vol. 50, Sept.-Oct. 1976, p. 85-98
[30] Kowalski, A. F., Hawley, S. L., Holtzman, J. A. 2010, A White Light Megaflare on the dM4.5e Star YZ CMi, The Astrophysical Journal Letters, Volume 714, Issue 1, pp. L98-L102
[31] Kretzschmar, M. 2011, The Sun as a star: observations of white-light flares, Astronomy & Astrophysics, Volume 530, id.A84, 7 pp
[32] Krucker, S., & Lin, R. P. 2000, On the solar release of Energetic Particles detected at 1 AU, Acceleration and transport of energetic particles observed in the heliosphere: ACE 2000 Symposium. AIP Conference Proceedings, Volume 528, pp. 87-90
[33] Künzel, H. 1960, Die Flare-Häufigkeit in Fleckengruppen unterschiedlicher Klasse und magnetischer Struktur, Astronomische Nachrichten, volume 285, p.271
[34] Lanza, A. F., Aigrain, S., Messina, S., & et al. 2009, Photospheric activity and rotation of the planet-hosting star CoRoT-4a, Astronomy and Astrophysics, Volume 506, Issue 1, 2009, pp.255-262
[35] Lin, R. P., Schwartz, R. A., Kane, S. R., & et al. 1984, Solar hard X-ray microflares, Astrophysical Journal, Part 1, vol. 283, Aug. 1, 1984, p. 421-425
[36] Lomb, N. R. 1976, Least-squares frequency analysis of unequally spaced data, Astrophysics and Space Science, vol. 39, Feb. 1976, p. 447-462
[37] Loomis, E. 1861, The great auroral exhibition of August 28th to September 4th 1859, Am. J. Sci. Arts, Second Series. 28, 32, 71–84, 318-335
[38] Lu, E. T, & Hamilton, R. J. 1991, Avalanches and the Distribution of Solar Flares, Bulletin of the American Astronomical Society, Vol. 23, p.1044
[39] Maehara, H., Shibayama, T., Notsu, S., & et al. 2012, Superflares on solar-type stars, Nature, Volume 485, Issue 7399, pp. 478-481
[40] Matthews, S. A., van Driel-Gesztelyi, L., Hudson, H. S. & et al. 2003, A catalogue of white-light flares observed by Yohkoh, Astronomy and Astrophysics, v.409, p.1107-1125
[41] Martínez Oliveros, J.-C., Hudson, H. S., Hurford, G. J., & et al. 2012, The Height of a White-light Flare and Its Hard X-Ray Sources, The Astrophysical Journal Letters, Volume 753, Issue 2, article id. L26, 5 pp.
[42] McIntosh, P. S. 1990, The classification of sunspot groups, Solar Physics, vol. 125, Feb. 1990, p. 251-267
[43] McQuillan, A., Aigrain, S., & Mazeh, T. 2013, Measuring the rotation period distribution of field M dwarfs with Kepler, Monthly Notices of the Royal Astronomical Society, Volume 432, Issue 2, p.1203-1216
[44] Mikkel, N. L., Hans, K., Jørgen C.-D., & et al. 2014, Detection of ℓ = 4 and ℓ = 5 Modes in 12 Years of Solar VIRGO-SPM Data—Tests on Kepler Observations of 16 Cyg A and B, The Astrophysical Journal, Volume 782, Issue 1
[45] Neupert, W. M. 1968, Comparison of Solar X-Ray Line Emission with Microwave Emission during Flares, Astrophysical Journal, vol. 153, p.L59
[46] Noyes, R.W. 1985, Stellar analogs of solar magnetic activity, SoPh, 100, 385
[47] Noyes, R. W., Weiss, N. O., & Vaughan, A. H. 1984, The relation between stellar rotation rate and activity cycle periods, Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 287, Dec. 15, 1984, p. 769-773
[48] Osten, R. A. 2012, Probing Magnetic Mysteries with Stellar Flares, New Horizons in Time-Domain Astronomy, Proceedings of the International Astronomical Union, IAU Symposium, Volume 285, p. 137-137
[49] Palla, F. & Stahler, S. W. 1999, Star Formation in the Orion Nebula Cluster, The Astrophysical Journal, Volume 525, Issue 2, pp. 772-783
[50] Pallavicini, R., Golub, L., Rosner, R., & et al. 1981, Relations among stellar X-ray emission observed from Einstein, stellar rotation and bolometric luminosity, Astrophysical Journal, Part 1, vol. 248, Aug. 15, 1981, p. 279-290
[51] Patty, S. R., & Hagyard, M. J. 1986, Delta-configurations - Flare activity and magnetic-field structure, Solar Physics (ISSN 0038-0938), vol. 103, Jan. 1986, p. 111-128.
[52] Pinsonneault, M. H., An, D., Molenda-Żakowicz, J., & et al. 2013, A Revised Effective Temperature Scale for the Kepler Input Catalog, The Astrophysical Journal Supplement, Volume 199, Issue 2, article id. 30, 22 pp
[53] Pizzolato, N., Maggio, A., Micela, G., & et al. 2003, The stellar activity-rotation relationship revisited: Dependence of saturated and non-saturated X-ray emission regimes on stellar mass for late-type dwarfs, Astronomy and Astrophysics, v.397, p.147-157
[54] Rauer, H., Catala, C., Aerts, C., & et al. 2013, The PLATO 2.0 Mission, eprint arXiv:1310.0696
[55] Reinhold, T., Reiners, A., & Basri, G. 2013 Rotation and differential rotation of active Kepler stars, Astronomy & Astrophysics, Volume 560, id.A4, 19 pp
[56] Roettenbacher, R. M., Monnier, J. D., Harmon, R. O., & et al. 2013, Imaging Starspot Evolution on Kepler Target KIC 5110407 Using Light-Curve Inversion, ApJ, 767, 60
[57] Roy, J.-R., 1977, The north-south distribution of major solar flare events, sunspot magnetic classes and sunspot areas /1955-1974/, Solar Physics, vol. 52, Apr. 1977, p. 53-61
[58] Rust, D. M., 1972, Flares and Changing Magnetic Fields, Solar Physics, Volume 25, Issue 1, pp.141-157
[59] Sammis, I., Tang, F., & Zirin, H. 2000, The Dependence of Large Flare Occurrence on the Magnetic Structure of Sunspots, The Astrophysical Journal, Volume 540, Issue 1, pp. 583-587
[60] Scargle, J. D. 1982, Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data, Astrophysical Journal, Part 1, vol. 263, Dec. 15, 1982, p. 835-853
[61] Schaefer, B. E., King, J. R., & Deliyannis, C. P. 2000, Superflares on Ordinary Solar-Type Stars, The Astrophysical Journal, Volume 529, Issue 2, pp. 1026-1030
[62] Schaefer, B. E. 1989, A Very Low Luminosity Star with a Very Large Amplitude Flare, Bulletin of the American Astronomical Society, Vol. 21, p.1222
[63] Severny, A. B. 1969, Solar flares and magnetic fields, Solar Flares and Space Research, Proceedings of a Symposium, held on the occasion of the 11th Plenary Meeting of the Committee on Space Research, held in Tokyo, Japan, May 9-11, 1968. Edited by C. de Jager and Z. Svestka. Amsterdam: North-Holland Publication Co., 1969., p.38
[64] Shakhovskaya, N. I. 1989, Stellar flare statistics - Physical consequences, Solar Physics, vol. 121, no. 1-2, 1989, p. 375-386; Discussion, p. 496.
[65] Shibata, K., Masuda, S., Shimojo, M., & et al. 1995, Hot-Plasma Ejections Associated with Compact-Loop Solar Flares, Astrophysical Journal Letters v.451, p.L83
[66] Shibayama, T., Maehara, H., Notsu, S., & et al. 2013, Superflares on Solar-type Stars Observed with Kepler. I. Statistical Properties of Superflares, The Astrophysical Journal Supplement, Volume 209, Issue 1, article id. 5, 13 pp
[67] Skumanich, A. 1972, Time Scales for CA II Emission Decay, Rotational Braking, and Lithium Depletion, Astrophysical Journal, vol. 171, p.565
[68] Spiegel, E. A. & Zahn, J. P. 1992, The solar tachocline, Astronomy and Astrophysics, vol. 265, no. 1, p. 106-114
[69] Stark, C. C., Boss, A. P., Weinberger, A. J., & et al. 2013, A Search for Exozodiacal Clouds with Kepler, ApJ, 764, 195
[70] Still, M., & Barclay, T. 2012, Astrophysics Source Code Library, 8004
[71] Švestka, Z. 1971, Solar Particle Events, Philosophical Transactions for the Royal Society of London. Series A, Mathematical and Physical Sciences, Volume 270, Issue 1202, pp. 157-165
[72] Tsurutani, B.T., Gonzalez, W.D., Lakhina G.S., & Alex, S. 2003, The extreme magnetic storm of 1–2 September 1859, J. Geophys. Res., 108, 1268, SSH 1-1,
[73] Tanaka, K. 1991, Studies on a very flare-active delta group - Peculiar delta SPOT evolution and inferred subsurface magnetic rope structure, Solar Physics (ISSN 0038-0938), vol. 136, Nov. 1991, p. 133-149
[74] Vaughan, A. H., Preston, G. W., Baliunas, S. L., & et al. 1981, Stellar rotation in lower main-sequence stars measured from time variations in H and K emission-line fluxes. I - Initial results, Astrophysical Journal, Part 1, vol. 250, Nov. 1, 1981, p. 276-283
[75] Walkowicz, L. M., & Basri, G. S., 2013, Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars, Monthly Notices of the Royal Astronomical Society, Volume 436, Issue 2, p.1883-1895
[76] Walkowicz, L. M., Basri, G., Batalha, N., & et al. 2011, White-light Flares on Cool Stars in the Kepler Quarter 1 Data, The Astronomical Journal, Volume 141, Issue 2, article id. 50, 9 pp
[77] Wang, L., Lin, R. P., Krucker, S., & et al. 2006, Evidence for double injections in scatter-free solar impulsive electron events, Geophysical Research Letters, Volume 33, Issue 3, CiteID L03106
[78] Warwick, C. S. 1966, Sunspot Configurations and Proton Flares, Astrophysical Journal, vol. 145, p.215
[79] Watanabe, K., Krucker, S., Hudson, H., & et al. 2010, G-band and Hard X-ray Emissions of the 2006 December 14 Flare Observed by Hinode/SOT and Rhessi, The Astrophysical Journal, Volume 715, Issue 1, pp. 651-655
[80] Zhang, H. 1995, Formation of magnetic shear and an electric current system in an emerging flux region, Astronomy and Astrophysics, v.304, p.541
[81] Zhou, A. H., Li, J. P., & Wang, X. D. 2011, A Study of a New Increasing Submillimeter Spectral Component of an X28 Solar Flare, The Astrophysical Journal, Volume 727, Issue 1, article id. 42, 5 pp |