AUTOMATED SOLAR FLARE STATISTICS IN SOFT X-RAYS OVER 37 YEARS OF GOES OBSERVATIONS: THE INVARIANCE OF SELF-ORGANIZED CRITICALITY DURING THREE SOLAR CYCLES
暂无分享,去创建一个
[1] The State of Self-organized Criticality of the Sun during the Last Three Solar Cycles. II. Theoretical Model , 2010, 1010.0986.
[2] M. Aschwanden. Irradiance observations of the 1–8 Å solar soft X-ray flux from goes , 1994 .
[3] H. Garcia. Polytropic Indices of Solar Flares , 2001 .
[4] P. Sturrock. Model of the High-Energy Phase of Solar Flares , 1966, Nature.
[5] B. Kliem. Coupled magnetohydrodynamic and kinetic development of current sheets in the solar corona , 1995 .
[6] Steven Christe,et al. Rhessi Microflare Statistics , 2004 .
[7] Size dependence of solar X-ray flare properties , 2005, astro-ph/0505154.
[8] W. Neupert. Intercalibration of Solar Soft X-Ray Broad Band Measurements from SOLRAD 9 through GOES-12 , 2011 .
[9] A. Benz. Radio spikes and the fragmentation of flare energy release , 1985 .
[10] H. Hudson. Solar flares, microflares, nanoflares, and coronal heating , 1991 .
[11] Henrik Jeldtoft Jensen,et al. Self-Organized Criticality , 1998 .
[12] T. Metcalf,et al. A Test of a New Flare Loop Scaling Law Using YOHKOH SXT and GOES Observations , 1996 .
[13] Howard A. Garcia,et al. Temperature and emission measure from goes soft X-ray measurements , 1994 .
[14] Paul Charbonneau,et al. Avalanche models for solar flares (Invited Review) , 2001 .
[15] A. Veronig,et al. Physics of the Neupert Effect: Estimates of the Effects of Source Energy, Mass Transport, and Geometry Using RHESSI and GOES Data , 2005 .
[16] S. White,et al. Updated Expressions for Determining Temperatures and Emission Measures from Goes Soft X-Ray Measurements , 2005 .
[17] E. Lu,et al. Avalanches and the Distribution of Solar Flares , 1991 .
[18] E. Hildner,et al. The NOAA Goes-12 Solar X-Ray Imager (SXI) 2. Performance , 2001 .
[19] P. Bak,et al. Self-organized criticality. , 1988, Physical review. A, General physics.
[20] M. Aschwanden. Physics of the Solar Corona. An Introduction , 2004 .
[21] Markus J. Aschwanden,et al. Self-Organized Criticality in Astrophysics , 2011 .
[22] Brian R. Dennis,et al. Frequency distributions and correlations of solar X-ray flare parameters , 1993 .
[23] Spiro K. Antiochos,et al. The Role of Magnetic Reconnection in Chromospheric Eruptions , 1995 .
[24] Self‐Organized Criticality in Earth Systems , 2003 .
[25] H. Hudson,et al. THE HARD SOLAR X-RAY SPECTRUM OBSERVED FROM THE THIRD ORBITING SOLAR OBSERVATORY. , 1969 .
[26] Per Bak,et al. How Nature Works , 1996 .
[27] M. Aschwanden. The State of Self-organized Criticality of the Sun During the Last Three Solar Cycles. I. Observations , 2010, 1006.4861.
[28] M. Aschwanden,et al. Self-Organized Criticality in Astrophysics: The Statistics of Nonlinear Processes in the Universe , 2011 .
[29] Lawrence Shing,et al. CCD development and characterization for the GOES N and O Solar X-ray Imager , 1999, Optics & Photonics.
[30] James R. Lemen,et al. Characterization of the flight CCD detectors for the GOES N and O solar x-ray imagers , 2004, SPIE Optics + Photonics.
[31] N. Crosby. Frequency distributions: from the sun to the earth , 2011 .
[32] N. Gopalswamy,et al. Different Power-Law Indices in the Frequency Distributions of Flares with and without Coronal Mass Ejections , 2006, astro-ph/0609197.
[33] P. Bornmann. Limits to derived flare properties using estimates for the background fluxes - Examples from GOES , 1990 .
[34] J. Sheinbaum,et al. Nonlinear Processes in Geophysical Fluid Dynamics , 2003 .
[35] S. Freeland,et al. Data Analysis with the SolarSoft System , 1998 .
[36] A. Veronig,et al. A Coronal Thick-Target Interpretation of Two Hard X-Ray Loop Events , 2004 .
[37] M. Shay,et al. Electron acceleration from contracting magnetic islands during reconnection , 2006, Nature.
[38] Henrik Jeldtoft Jensen,et al. Self-Organized Criticality: Emergent Complex Behavior in Physical and Biological Systems , 1998 .
[39] A. Veronig,et al. The Neupert effect and new RHESSI measures of thetotal energy in electrons accelerated in solar flares , 2003 .
[40] Tang,et al. Self-Organized Criticality: An Explanation of 1/f Noise , 2011 .
[41] B. Dennis,et al. The Neupert effect: What can it tell us about the impulsive and gradual phases of solar flares? , 1993 .
[42] J. McTiernan,et al. The Neupert Effect and the Chromospheric Evaporation Model for Solar Flares , 1995 .
[43] M. Güdel. Are Coronae of Magnetically Active Stars Heated by Flares , 1997 .
[44] K. Shibata,et al. Plasmoid-induced-reconnection and fractal reconnection , 2001, astro-ph/0101008.
[45] Markus J. Aschwanden,et al. Flare Plasma Cooling from 30 MK down to 1 MK modeled from Yohkoh, GOES, and TRACE observations during the Bastille Day Event (14 July 2000) , 2001 .
[46] A. Hanslmeier,et al. The solar soft X-ray background flux and its relation to flare occurrence , 2004 .
[47] B. Kliem. Fragmentary energy release due to tearing and coalescence in coronal current sheets , 1990 .
[48] Martin A. Davis,et al. The NOAA Goes-12 Solar X-Ray Imager (SXI) 1. Instrument, Operations, and Data , 2005 .
[49] M. Shimojo,et al. Occurrence Rate of Microflares in an X-Ray-bright Point within an Active Region , 1999 .
[50] T. Sakurai,et al. Thermal and Magnetic Parameters in Solar Flares Derived from GOES X-Ray Light Curves , 2010 .
[51] D. Sornette. Critical Phenomena in Natural Sciences: Chaos, Fractals, Selforganization and Disorder: Concepts and Tools , 2000 .
[52] J. Drake. Characteristics of soft solar X-ray bursts , 1971 .
[53] T. Tajima,et al. Dynamic magnetic x-points , 1981 .
[54] James R. Lemen,et al. The solar x-ray imager for GOES , 2004, SPIE Optics + Photonics.
[55] M. Aschwanden. A statistical fractal-diffusive avalanche model of a slowly-driven self-organized criticality system , 2011, 1112.4859.
[56] J. McTiernan. RHESSI/GOES OBSERVATIONS OF THE NONFLARING SUN FROM 2002 TO 2006 , 2009 .
[57] R. Kreplin,et al. The NRL SOLRAD X-ray detectors: A summary of the observations and a comparison with the SMS/GOES detectors , 1991 .
[58] T. Tajima,et al. Current loop coalescence model of solar flares , 1987 .
[59] B. Rogers,et al. Formation of secondary islands during magnetic reconnection , 2006 .
[60] M. Siarkowski,et al. Relationship between non-thermal electron energy spectra and GOES classes , 2009, 0904.1588.
[61] W. Wagner. Observations of 1–8 Å solar X-ray variability during solar cycle 21 , 1988 .
[62] D. Turcotte,et al. Self-organized criticality , 1999 .
[63] A. Benz,et al. Relations between concurrent hard X-ray sources in solar flares , 2006, astro-ph/0606353.
[64] C. Crannell,et al. Expressions to determine temperatures and emission measures for solar X-ray events from GOES measurements , 1984 .
[65] Stefan Hergarten. Self-Organized Criticality , 2002 .
[66] U. Feldman,et al. The Occurrence Rate of Soft X-Ray Flares as a Function of Solar Activity , 1997 .
[67] H. Garcia. Reconstructing the Thermal and Spatial Form of a Solar Flare from Scaling Laws and Soft X-Ray Measurements , 1998 .
[68] W. Otruba,et al. Temporal aspects and frequency distributions of solar soft X-ray flares , 2002, astro-ph/0207234.