STATISTICAL PROPERTIES OF SUPER-HOT SOLAR FLARES
暂无分享,去创建一个
[1] D. Longcope,et al. A MODEL FOR THE ORIGIN OF HIGH DENSITY IN LOOPTOP X-RAY SOURCES , 2011, 1107.2441.
[2] J. Brown,et al. Nonsolar astronomy with the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) , 2003, SPIE Astronomical Telescopes + Instrumentation.
[3] Alphonse C. Sterling,et al. Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond , 1998 .
[4] J. McTiernan. RHESSI/GOES OBSERVATIONS OF THE NONFLARING SUN FROM 2002 TO 2006 , 2009 .
[5] T. Kosugi,et al. Energy Release and Particle Acceleration in Solar Flares with Respect to Flaring Magnetic Loops , 1998 .
[6] R. Lin,et al. The super-hot thermal component in the decay phase of solar flares , 1985 .
[7] Kevin C. Hurley,et al. A new component of hard X-rays in solar flares , 1981 .
[8] Lindsay Glesener,et al. MEASUREMENTS OF THE CORONAL ACCELERATION REGION OF A SOLAR FLARE , 2010 .
[9] J. Lemen,et al. Intercomparison of flare observations with two SMM spectrometers: BCS and HXIS , 1988 .
[10] S. Krucker,et al. RHESSI Microflare Statistics. II. X-Ray Imaging, Spectroscopy, and Energy Distributions , 2007, 0712.2544.
[11] Brian R. Dennis,et al. THE THERMAL PROPERTIES OF SOLAR FLARES OVER THREE SOLAR CYCLES USING GOES X-RAY OBSERVATIONS , 2012, 1206.1005.
[12] M. Carlsson,et al. Radiative Hydrodynamic Models of the Optical and Ultraviolet Emission from Solar Flares , 2005, astro-ph/0507335.
[13] W. E. Behring,et al. Electron Temperature, Emission Measure, and X-Ray Flux in A2 to X2 X-Ray Class Solar Flares , 1996 .
[14] Peter R. Young,et al. CHIANTI—An Atomic Database for Emission Lines. VII. New Data for X-Rays and Other Improvements , 2006 .
[15] S. White,et al. Preflare Nonthermal Emission Observed in Microwaves and Hard X-Rays , 2006 .
[16] J. Qiu,et al. A Quantitative Model of Energy Release and Heating by Time-dependent, Localized Reconnection in a Flare with Thermal Loop-top X-ray Source , 2010, 1106.3572.
[17] A. Hanslmeier,et al. Investigation of the Neupert effect in solar flares. I. Statistical properties and the evaporation model , 2002, astro-ph/0207217.
[18] D. A. Landis,et al. The RHESSI Spectrometer , 2002 .
[19] H. Warren,et al. OBSERVATIONS OF THERMAL FLARE PLASMA WITH THE EUV VARIABILITY EXPERIMENT , 2012, 1211.1875.
[20] M. Kundu,et al. Strong Magnetic Fields and Inhomogeneity in the Solar Corona , 1991 .
[21] M. Aschwanden,et al. The RHESSI Imaging Concept , 2002 .
[22] J. Dubau,et al. Yohkoh observations of Fe XXVI X-ray line emission from solar flares , 1996 .
[23] M. Temmer,et al. An Observational Overview of Solar Flares , 2011, 1109.5932.
[24] P. McIntosh,et al. High-temperature flares observed in broadband soft X-rays , 1991 .
[25] Haimin Wang,et al. Observations of the Failed Eruption of a Filament , 2003 .
[26] A. Caspi,et al. RHESSI LINE AND CONTINUUM OBSERVATIONS OF SUPER-HOT FLARE PLASMA , 2010, 1105.2839.
[27] J. McTiernan,et al. The Solar Flare Soft X-Ray Differential Emission Measure and the Neupert Effect at Different Temperatures , 1999 .
[28] M. Aschwanden,et al. Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares , 2011, 1109.6496.
[29] W. Neupert. COMPARISON OF SOLAR X-RAY LINE EMISSION WITH MICROWAVE EMISSION DURING FLARES. , 1968 .
[30] B. Dennis,et al. The Neupert effect: What can it tell us about the impulsive and gradual phases of solar flares? , 1993 .
[31] R. Canfield,et al. Flare loop radiative hydrodynamics. V - Response to thick-target heating. VI - Chromospheric evaporation due to heating by nonthermal electrons. VII - Dynamics of the thick-target heated chromosphere , 1985 .
[32] Size dependence of solar X-ray flare properties , 2005, astro-ph/0505154.