Temporal aspects and frequency distributions of solar soft X-ray flares
暂无分享,去创建一个
W. Otruba | M. Temmer | M. Messerotti | A. Hanslmeier | A. Veronig | A. Hanslmeier | M. Temmer | A. Veronig | M. Messerotti | W. Otruba
[1] R. Rosner,et al. Erratum: Cosmic Flare Transients: Constraints upon Models for Energy Storage and Release Derived from the Event Frequency Distribution , 1978 .
[2] Ester Antonucci,et al. The energetics of chromospheric evaporation in solar flares , 1984 .
[3] Säm Krucker,et al. Energy Distribution of Heating Processes in the Quiet Solar Corona , 1998 .
[4] R. Wilson. On the variation of the sun's X ray background flux and its relation to the sun's flaring rate, energetic event rate, and the solar cycle , 1993 .
[5] J. Culhane,et al. Solar X-ray bursts at energies less than 10 keV observed with OSO-4 , 1970 .
[6] Timothy S. Bastian,et al. X-Ray Network Flares of the Quiet Sun , 1997 .
[7] W. Otruba,et al. Statistical analysis of solar H-alpha flares , 2001 .
[8] W. E. Behring,et al. Electron Temperature, Emission Measure, and X-Ray Flux in A2 to X2 X-Ray Class Solar Flares , 1996 .
[9] J. McTiernan,et al. The Solar Flare Soft X-Ray Differential Emission Measure and the Neupert Effect at Different Temperatures , 1999 .
[10] E. Parker. Nanoflares and the solar X-ray corona , 1988 .
[11] H. Garcia. Thermal-Spatial Analysis of Medium and Large Solar Flares, 1976 to 1996 , 2000 .
[12] B. Dennis,et al. The Neupert effect: What can it tell us about the impulsive and gradual phases of solar flares? , 1993 .
[13] H. Hudson. Solar flares, microflares, nanoflares, and coronal heating , 1991 .
[14] R. Thomas,et al. Solar soft X-rays and solar activity , 1969 .
[15] H. Hudson,et al. Observations of solar X-ray bursts in the energy range 5–15 keV , 1974 .
[16] J. McTiernan,et al. The Neupert Effect and the Chromospheric Evaporation Model for Solar Flares , 1995 .
[17] On the reliability of peak-flux distributions, with an application to solar flares , 2001, astro-ph/0106158.
[18] John C. Brown,et al. The deduction of energy spectra of non-thermal electrons in flares from the observed dynamic spectra of hard X-ray bursts , 1971 .
[19] R. Canfield,et al. Flare Loop Radiative Hydrodynamics - Part Six - Chromospheric Evaporation due to Heating by Nonthermal Electrons , 1985 .
[20] P. Jupp,et al. Statistical Analysis of the Energy Distribution of Nanoflares in the Quiet Sun , 2000 .
[21] W. Neupert. COMPARISON OF SOLAR X-RAY LINE EMISSION WITH MICROWAVE EMISSION DURING FLARES. , 1968 .
[22] Howard A. Garcia,et al. Temperature and emission measure from goes soft X-ray measurements , 1994 .
[23] E. Lu,et al. Avalanches and the Distribution of Solar Flares , 1991 .
[24] J. McTiernan,et al. The Distribution of Flare Parameters and Implications for Coronal Heating , 1993 .
[25] U. Feldman,et al. The Occurrence Rate of Soft X-Ray Flares as a Function of Solar Activity , 1997 .
[26] Alphonse C. Sterling,et al. Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond , 1998 .
[27] James M. McTiernan,et al. Solar flares and avalanches in driven dissipative systems , 1993 .
[28] M. Wheatland. DO SOLAR FLARES EXHIBIT AN INTERVAL–SIZE RELATIONSHIP? , 2000 .
[29] H. Hudson,et al. NOAA 7978: The Last Best Old-Cycle Region? , 1998 .
[30] J. Drake. Characteristics of soft solar X-ray bursts , 1971 .
[31] Brian R. Dennis,et al. Frequency distributions and correlations of solar X-ray flare parameters , 1993 .
[32] Brian R. Dennis,et al. Logistic Avalanche Processes, Elementary Time Structures, and Frequency Distributions in Solar Flares , 1998 .
[33] Bernhard Haisch,et al. The Many Faces of the Sun : A Summary of the Results from NASA's Solar Maximum Mission , 1999 .