Coronal Mass Ejections from the Same Active Region Cluster: Two Different Perspectives

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

[2]  A. Vourlidas,et al.  Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum , 2014, Solar Physics.

[3]  A. Vourlidas,et al.  Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum , 2014 .

[4]  K. Reardon,et al.  H\alpha\ spectroscopy and multiwavelength imaging of a solar flare caused by filament eruption , 2014, 1405.2194.

[5]  P. Démoulin,et al.  Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events , 2013, 1312.3359.

[6]  M. Aschwanden,et al.  The Association of Solar Flares with Coronal Mass Ejections During the Extended Solar Minimum , 2013, 1308.1465.

[7]  J. Zhang,et al.  A STUDY OF FAST FLARELESS CORONAL MASS EJECTIONS , 2013, 1307.0166.

[8]  Richard A. Harrison,et al.  Stealth Coronal Mass Ejections: A Perspective , 2013 .

[9]  A. Vourlidas,et al.  How Many CMEs Have Flux Ropes? Deciphering the Signatures of Shocks, Flux Ropes, and Prominences in Coronagraph Observations of CMEs , 2012, 1207.1599.

[10]  T. Howard,et al.  Coronal Mass Ejections: Observations , 2012 .

[11]  T. Howard,et al.  THE THOMSON SURFACE. I. REALITY AND MYTH , 2012 .

[12]  Jason P. Byrne,et al.  AUTOMATIC DETECTION AND TRACKING OF CORONAL MASS EJECTIONS. II. MULTISCALE FILTERING OF CORONAGRAPH IMAGES , 2012, 1207.6125.

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

[14]  A. Vourlidas,et al.  CME reconstruction: Pre-STEREO and STEREO era , 2011 .

[15]  J. T. Hoeksema,et al.  Earth-Affecting Solar Causes Observatory (EASCO): A potential International Living with a Star Mission from Sun-Earth L5 , 2011 .

[16]  B. Gui,et al.  Statistical study of coronal mass ejection source locations: Understanding CMEs viewed in coronagraphs , 2011, 1101.0641.

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

[18]  A. Vourlidas,et al.  DETERMINING THE AZIMUTHAL PROPERTIES OF CORONAL MASS EJECTIONS FROM MULTI-SPACECRAFT REMOTE-SENSING OBSERVATIONS WITH STEREO SECCHI , 2010, 1004.0945.

[19]  Matthew West,et al.  On the 3-D reconstruction of Coronal Mass Ejections using coronagraph data , 2010 .

[20]  Angelos Vourlidas,et al.  NO TRACE LEFT BEHIND: STEREO OBSERVATION OF A CORONAL MASS EJECTION WITHOUT LOW CORONAL SIGNATURES , 2009, 0905.2583.

[21]  Yannick Boursier,et al.  The ARTEMIS Catalog of LASCO Coronal Mass Ejections , 2009 .

[22]  M. Temmer,et al.  CME Projection Effects Studied with STEREO/COR and SOHO/LASCO , 2009 .

[23]  E. Christian,et al.  The STEREO Mission: An Introduction , 2008 .

[24]  H. Wechsler,et al.  Automatic Detection and Tracking of Coronal Mass Ejections in Coronagraph Time Series , 2008 .

[25]  D. Nandy,et al.  Kinematic properties of solar coronal mass ejections: Correction for projection effects in spacecraft coronagraph measurements , 2008 .

[26]  E. Robbrecht,et al.  Automated recognition of coronal mass ejections (CMEs) in near-real-time data , 2008 .

[27]  B. Vršnak,et al.  Projection effects in coronal mass ejections , 2007 .

[28]  H. Hudson,et al.  Multi-Wavelength Observations of CMEs and Associated Phenomena , 2006 .

[29]  N. Gopalswamy,et al.  Are halo coronal mass ejections special events , 2006 .

[30]  A. Vourlidas,et al.  The Proper Treatment of Coronal Mass Ejection Brightness: A New Methodology and Implications for Observations , 2006 .

[31]  W. Gonzalez,et al.  The association of coronal mass ejections with their effects near the Earth , 2005 .

[32]  V. Bothmer,et al.  Geometrical Properties of Coronal Mass Ejections , 2004, Proceedings of the International Astronomical Union.

[33]  J. Davila,et al.  Three-Dimensional Polarimetric Imaging of Coronal Mass Ejections , 2004, Science.

[34]  N. Gopalswamy,et al.  A catalog of white light coronal mass ejections observed by the SOHO spacecraft , 2004 .

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

[36]  L. Ofman,et al.  Cone model for halo CMEs: Application to space weather forecasting , 2004 .

[37]  N. Gopalswamy,et al.  A New Method for Estimating Widths, Velocities, and Source Location of Halo Coronal Mass Ejections , 2003 .

[38]  M. Andrews The Front-to-Back Asymmetry of Coronal Emission , 2002 .

[39]  W. Liu,et al.  Determination of geometrical and kinematical properties of halo coronal mass ejections using the cone model , 2002 .

[40]  C. J. Wolfson,et al.  Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) , 2000, SPIE Optics + Photonics.

[41]  B. Low,et al.  Three‐dimensional and twisted: An MHD interpretation of on‐disk observational characteristics of coronal mass ejections , 2000 .

[42]  R. Howard,et al.  LASCO and EIT Observations of Helical Structure in Coronal Mass Ejections , 1999 .

[43]  P. Démoulin,et al.  QUASI-SEPARATRIX LAYERS IN SOLAR FLARES. II. OBSERVED MAGNETIC CONFIGURATIONS , 1997 .

[44]  E. Priest,et al.  Quasi-Separatrix layers in solar flares. I. Method. , 1996 .

[45]  P. Lamy,et al.  The Large Angle Spectroscopic Coronagraph (LASCO) , 1995 .

[46]  V. Domingo,et al.  The SOHO mission: An overview , 1995 .

[47]  A. Hundhausen,et al.  Sizes and locations of coronal mass ejections - SMM observations from 1980 and 1984-1989 , 1993 .

[48]  J. Gosling Coronal mass ejections: The link between solar and geomagnetic activity* , 1993 .

[49]  D. Webb Erupting prominences and the geometry of coronal mass ejections , 1988 .

[50]  F. Crifo,et al.  Coronal transients: Loop or bubble? , 1983 .

[51]  R. Howard,et al.  The observation of a coronal transient directed at earth , 1982 .

[52]  R. MacQueen,et al.  Mass ejections from the Sun: A view from Skylab , 1974 .

[53]  R. Tousey,et al.  Preliminary Results from the NRL/ATM Instruments from Skylab SL/2 , 1974 .

[54]  H. W. Babcock The Sun's General Magnetic Field , 1956, Nature.

[55]  P. Morrison,et al.  Solar Origin of Cosmic-Ray Time Variations , 1956 .

[56]  Faculteit der Wiskunde en Natuurwetenschappen,et al.  The amount of Polarization by Interstellar Grains. , 1950 .

[57]  F. A. Lindemann LXX. Note on the theory of magnetic storms , 1919 .

[58]  R. C. Carrington Description of a Singular Appearance seen in the Sun on September 1, 1859 , 1859 .