Comparative Study of the Three-Dimensional Thermodynamical Structure of the Inner Corona of Solar Minimum Carrington Rotations 1915 and 2081

[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 .