Comparative Study of the Three-Dimensional Thermodynamical Structure of the Inner Corona of Solar Minimum Carrington Rotations 1915 and 2081
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[1] Peter R. Young,et al. CHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite Lines , 2019, The Astrophysical Journal Supplement Series.
[2] R. Frazin,et al. Effect of stray light correction of extreme-ultraviolet solar images in tomography , 2017 .
[3] R. Chastain,et al. THE CORONAL LOOP INVENTORY PROJECT: EXPANDED ANALYSIS AND RESULTS , 2016, 1705.09360.
[4] J. Byers,et al. Sparse Bayesian Inference and the Temperature Structure of the Solar Corona , 2016, 1610.05972.
[5] S. Cranmer,et al. EXPLAINING INVERTED-TEMPERATURE LOOPS IN THE QUIET SOLAR CORONA WITH MAGNETOHYDRODYNAMIC WAVE-MODE CONVERSION , 2016, 1608.04398.
[6] C. Schrijver,et al. THERMAL DIAGNOSTICS WITH THE ATMOSPHERIC IMAGING ASSEMBLY ON BOARD THE SOLAR DYNAMICS OBSERVATORY: A VALIDATED METHOD FOR DIFFERENTIAL EMISSION MEASURE INVERSIONS , 2015, 1504.03258.
[7] R. Frazin,et al. MULTIMODAL DIFFERENTIAL EMISSION MEASURE IN THE SOLAR CORONA , 2015, 1503.02473.
[8] A. M. V'asquez. Seeing The Solar Corona in Three Dimensions , 2015, 1503.02238.
[9] R. Frazin,et al. A STEADY-STATE PICTURE OF SOLAR WIND ACCELERATION AND CHARGE STATE COMPOSITION DERIVED FROM A GLOBAL WAVE-DRIVEN MHD MODEL , 2014, 1412.8288.
[10] R. Frazin,et al. Time-dependent tomographic reconstruction of the solar corona , 2014, Astron. Comput..
[11] P. Lamy,et al. Comparing the solar minima of cycles 22/23 and 23/24: The view from LASCO white light coronal images , 2014 .
[12] T. Gombosi,et al. ALFVÉN WAVE SOLAR MODEL (AWSoM): CORONAL HEATING , 2013, 1311.4093.
[13] G. Zanna. The multi-thermal emission in solar active regions , 2013 .
[14] R. Frazin,et al. EVOLUTION OF THE GLOBAL TEMPERATURE STRUCTURE OF THE SOLAR CORONA DURING THE MINIMUM BETWEEN SOLAR CYCLES 23 AND 24 , 2013 .
[15] H. Mason,et al. CHIANTI—AN ATOMIC DATABASE FOR EMISSION LINES. XIII. SOFT X-RAY IMPROVEMENTS AND OTHER CHANGES , 2013 .
[16] R. Frazin,et al. NEWLY DISCOVERED GLOBAL TEMPERATURE STRUCTURES IN THE QUIET SUN AT SOLAR MINIMUM , 2012, 1207.6661.
[17] Russell J. Hewett,et al. Intercomparison of the LASCO-C2, SECCHI-COR1, SECCHI-COR2, and Mk4 Coronagraphs , 2012 .
[18] P. Martens,et al. FAST DIFFERENTIAL EMISSION MEASURE INVERSION OF SOLAR CORONAL DATA , 2012, 1204.6306.
[19] R. Frazin,et al. A GLOBAL TWO-TEMPERATURE CORONA AND INNER HELIOSPHERE MODEL: A COMPREHENSIVE VALIDATION STUDY , 2012 .
[20] E. Kontar,et al. Differential Emission Measures from the Regularized Inversion of Hinode and SDO data , 2012, 1201.2642.
[21] A. Gilbert,et al. THE FIRST STRAY LIGHT CORRECTED EXTREME-ULTRAVIOLET IMAGES OF SOLAR CORONAL HOLES , 2011, 1110.3052.
[22] Bart van der Holst,et al. OBTAINING POTENTIAL FIELD SOLUTIONS WITH SPHERICAL HARMONICS AND FINITE DIFFERENCES , 2011, 1104.5672.
[23] M. Aschwanden,et al. SOLAR CORONA LOOP STUDIES WITH THE ATMOSPHERIC IMAGING ASSEMBLY. I. CROSS-SECTIONAL TEMPERATURE STRUCTURE , 2011, 1103.0228.
[24] R. Frazin,et al. The WHI Corona from Differential Emission Measure Tomography , 2011 .
[25] R. Frazin,et al. A DATA-DRIVEN, TWO-TEMPERATURE SOLAR WIND MODEL WITH ALFVÉN WAVES , 2010 .
[26] R. Frazin,et al. THE SOLAR MINIMUM CORONA FROM DIFFERENTIAL EMISSION MEASURE TOMOGRAPHY , 2010, 1012.5953.
[27] Farzad Kamalabadi,et al. Dynamic Three-Dimensional Tomography of the Solar Corona , 2010 .
[28] Farzad Kamalabadi,et al. QUANTITATIVE, THREE-DIMENSIONAL ANALYSIS OF THE GLOBAL CORONA WITH MULTI-SPACECRAFT DIFFERENTIAL EMISSION MEASURE TOMOGRAPHY , 2009 .
[29] F. Kamalabadi,et al. 3D Temperatures and Densities of the Solar Corona via Multi-Spacecraft EUV Tomography: Analysis of Prominence Cavities , 2009 .
[30] S. Suess,et al. Stagnation Flow in Thin Streamer Boundaries , 2005 .
[31] J. Raymond,et al. The Effect of Proton Temperature Anisotropy on the Solar Minimum Corona and Wind , 2003, astro-ph/0310846.
[32] M. Aschwanden,et al. Analytical Approximations to Hydrostatic Solutions and Scaling Laws of Coronal Loops , 2002 .
[33] Richard A. Frazin,et al. Tomography of the Solar Corona. II. Robust, Regularized, Positive Estimation of the Three-dimensional Electron Density Distribution from LASCO-C2 Polarized White-Light Images , 2002 .
[34] U. Feldman,et al. CHIANTI—An Atomic Database for Emission Lines. V. Comparison with an Isothermal Spectrum Observed with SUMER , 2002 .
[35] R. Frazin. Tomography of the Solar Corona. I. A Robust, Regularized, Positive Estimation Method , 2000 .
[36] U. Feldman,et al. Properties of Quiet-Sun Coronal Plasmas at Distances of 1.03 ⩽ R☉ ⩽ 1.50 along the Solar Equatorial Plane , 1999 .
[37] D. Biesecker,et al. Solar minimum streamer densities and temperatures using Whole Sun Month coordinated data sets , 1999 .
[38] J. T. Hoeksema,et al. Synoptic Sun during the first Whole Sun Month Campaign: August 10 to September 8, 1996 , 1999 .
[39] G. Naletto,et al. Physical Structure of a Coronal Streamer in the Closed-Field Region as Observed from UVCS/SOHO and SXT/Yohkoh , 1998 .
[40] V. Kashyap,et al. Markov-Chain Monte Carlo Reconstruction of Emission Measure Distributions: Application to Solar Extreme-Ultraviolet Spectra , 1998 .
[41] P. Lamy,et al. Origin of Streamer Material in the Outer Corona , 1998 .
[42] S. Suess,et al. Volumetric heating in coronal streamers , 1996 .
[43] H. Gursky,et al. The potential for plasma diagnostics from stellar extreme-ultraviolet observations , 1992 .
[44] P. Sen. Estimates of the Regression Coefficient Based on Kendall's Tau , 1968 .
[45] R. Rosner,et al. Closed coronal structures. II. generalized hydrostatic model , 1981 .
[46] R. Michael Perry,et al. On determining the electron density distribution of the solar corona from K-coronameter data , 1972 .