Deflection and Rotation of CMEs from Active Region 11158

[1]  Merav Opher,et al.  Predicting the Magnetic Field of Earth-impacting CMEs , 2017 .

[2]  A. Vourlidas,et al.  USING ForeCAT DEFLECTIONS AND ROTATIONS TO CONSTRAIN THE EARLY EVOLUTION OF CMEs , 2016, 1606.03460.

[3]  M. Opher,et al.  THE HELIOCENTRIC DISTANCE WHERE THE DEFLECTIONS AND ROTATIONS OF SOLAR CORONAL MASS EJECTIONS OCCUR , 2015, 1509.04948.

[4]  M. L. Mays,et al.  Ensemble Modeling of CMEs Using the WSA–ENLIL+Cone Model , 2015, 1504.04402.

[5]  P. Liewer,et al.  Observations and Analysis of the Non-Radial Propagation of Coronal Mass Ejections Near the Sun , 2015 .

[6]  M. Opher,et al.  CONSTRAINING THE MASSES AND THE NON-RADIAL DRAG COEFFICIENT OF A SOLAR CORONAL MASS EJECTION , 2015, 1503.00664.

[7]  Thuy Mai,et al.  Solar Dynamics Observatory (SDO) , 2015 .

[8]  R. Evans,et al.  GLOBAL TRENDS OF CME DEFLECTIONS BASED ON CME AND SOLAR PARAMETERS , 2014, 1410.4496.

[9]  A. Vourlidas,et al.  INNER HELIOSPHERIC EVOLUTION OF A “STEALTH” CME DERIVED FROM MULTI-VIEW IMAGING AND MULTIPOINT IN SITU OBSERVATIONS. I. PROPAGATION TO 1 AU , 2013, 1311.6895.

[10]  N. Gopalswamy,et al.  Testing the empirical shock arrival model using quadrature observations , 2013, 1310.8510.

[11]  R. Evans,et al.  FORECASTING A CORONAL MASS EJECTION'S ALTERED TRAJECTORY: ForeCAT , 2013, 1307.7603.

[12]  Yang Liu,et al.  INTERPRETING ERUPTIVE BEHAVIOR IN NOAA AR 11158 VIA THE REGION'S MAGNETIC ENERGY AND RELATIVE-HELICITY BUDGETS , 2013, The Astrophysical Journal.

[13]  A. Vourlidas,et al.  Three-Dimensional Evolution of Erupted Flux Ropes from the Sun (2 – 20 R⊙) to 1 AU , 2013, Solar Physics.

[14]  O. Olmedo,et al.  SECONDARY WAVES AND/OR THE “REFLECTION” FROM AND “TRANSMISSION” THROUGH A CORONAL HOLE OF AN EXTREME ULTRAVIOLET WAVE ASSOCIATED WITH THE 2011 FEBRUARY 15 X2.2 FLARE OBSERVED WITH SDO/AIA AND STEREO/EUVI , 2012, 1206.6137.

[15]  B. Anderson,et al.  Remote and in situ observations of an unusual Earth‐directed coronal mass ejection from multiple viewpoints , 2012 .

[16]  T. Török,et al.  3D Reconstruction of a Rotating Erupting Prominence , 2011, 1112.3388.

[17]  C. J. Wolfson,et al.  Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) , 2012 .

[18]  M. Velli,et al.  Origins of Rolling, Twisting, and Non-radial Propagation of Eruptive Solar Events , 2011, 1211.1376.

[19]  N. Srivastava,et al.  Rolling motion in erupting prominences observed by STEREO , 2011 .

[20]  A. Vourlidas,et al.  THE FIRST OBSERVATION OF A RAPIDLY ROTATING CORONAL MASS EJECTION IN THE MIDDLE CORONA , 2011 .

[21]  B. Gui,et al.  Quantitative Analysis of CME Deflections in the Corona , 2011, 1105.3382.

[22]  B. Gui,et al.  Kinematic Evolution of a Slow CME in Corona Viewed by STEREO-B on 8 October 2007 , 2011, 1101.3205.

[23]  C. J. Wolfson,et al.  The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO) , 2011 .

[24]  Hilary V. Cane,et al.  Near-Earth Interplanetary Coronal Mass Ejections During Solar Cycle 23 (1996 – 2009): Catalog and Summary of Properties , 2010 .

[25]  Jackie A. Davies,et al.  OBSERVATIONAL EVIDENCE OF A CORONAL MASS EJECTION DISTORTION DIRECTLY ATTRIBUTABLE TO A STRUCTURED SOLAR WIND , 2010 .

[26]  J. Luhmann,et al.  STEREO observations of interplanetary coronal mass ejections and prominence deflection during solar minimum period , 2009 .

[27]  J. Luhmann,et al.  ROTATION OF CORONAL MASS EJECTIONS DURING ERUPTION , 2009 .

[28]  A. Vourlidas,et al.  Forward Modeling of Coronal Mass Ejections Using STEREO/SECCHI Data , 2009 .

[29]  N. Gopalswamy,et al.  CME interactions with coronal holes and their interplanetary consequences , 2009 .

[30]  A. Vourlidas,et al.  Modeling of Flux Rope Coronal Mass Ejections , 2006 .

[31]  J. Zhang,et al.  A Statistical Study of Main and Residual Accelerations of Coronal Mass Ejections , 2006 .

[32]  R. Skoug,et al.  Magnetic disconnection from the Sun: Observations of a reconnection exhaust in the solar wind at the heliospheric current sheet , 2005 .

[33]  Y. Fan,et al.  Numerical Simulations of Three-dimensional Coronal Magnetic Fields Resulting from the Emergence of Twisted Magnetic Flux Tubes , 2004 .

[34]  V. Bothmer,et al.  On the three-dimensional configuration of coronal mass ejections , 2004 .

[35]  T. Török,et al.  The evolution of twisting coronal magnetic flux tubes , 2003 .

[36]  Stephen L. Keil,et al.  Innovative Telescopes and Instrumentation for Solar Astrophysics , 2003 .

[37]  David F. Elmore,et al.  COR1 inner coronagraph for STEREO-SECCHI , 2003, SPIE Astronomical Telescopes + Instrumentation.

[38]  N. Gopalswamy,et al.  Non-radial motion of eruptive filaments , 2001 .

[39]  R. MacQueen,et al.  The propagation of coronal mass ejection transients , 1986 .

[40]  E. Hildner Mass ejections from the solar corona into interplanetary space , 1977 .

[41]  J. Wilcox,et al.  A model of interplanetary and coronal magnetic fields , 1969 .