Multi-viewpoint Coronal Mass Ejection Catalog Based on STEREO COR2 Observations
暂无分享,去创建一个
Angelos Vourlidas | Guillermo Stenborg | Alisson Dal Lago | A. Vourlidas | G. Stenborg | A. D. Lago | L. Balmaceda | L. A. Balmaceda | A. Lago
[1] A. Thernisien. IMPLEMENTATION OF THE GRADUATED CYLINDRICAL SHELL MODEL FOR THE THREE-DIMENSIONAL RECONSTRUCTION OF CORONAL MASS EJECTIONS , 2011 .
[2] Angelos Vourlidas,et al. Tracking of Coronal White-Light Events by Texture , 2010 .
[3] Yuming Wang,et al. Full halo coronal mass ejections: Do we need to correct the projection effect in terms of velocity? , 2013, 1303.4059.
[4] D. Berghmans,et al. Validation of CME Detection Software (CACTus) by Means of Simulated Data, and Analysis of Projection Effects on CME Velocity Measurements , 2011 .
[5] H. Wechsler,et al. Automatic Detection and Tracking of Coronal Mass Ejections in Coronagraph Time Series , 2008 .
[6] N. Gopalswamy,et al. A catalog of white light coronal mass ejections observed by the SOHO spacecraft , 2004 .
[7] A. Vourlidas. The flux rope nature of coronal mass ejections , 2014 .
[8] Russell A. Howard,et al. Coronal mass ejections - 1979-1981 , 1985 .
[9] J. Luhmann,et al. A model for stealth coronal mass ejections , 2016, 1612.08323.
[10] 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.
[11] Jie Zhang,et al. ARE HALO-LIKE SOLAR CORONAL MASS EJECTIONS MERELY A MATTER OF GEOMETRIC PROJECTION EFFECTS? , 2015 .
[12] A. Vourlidas. Mission to the Sun‐Earth L5 Lagrangian Point: An Optimal Platform for Space Weather Research , 2015 .
[13] S. Wu,et al. Direct Detection of a Coronal Mass Ejection-Associated Shock in Large Angle and Spectrometric Coronagraph Experiment White-Light Images , 2003 .
[14] Y.-M. Wang,et al. IS SOLAR CYCLE 24 PRODUCING MORE CORONAL MASS EJECTIONS THAN CYCLE 23? , 2014 .
[15] E. Christian,et al. The STEREO Mission: An Introduction , 2008 .
[16] A. Hundhausen,et al. Role of projection effects on solar coronal mass ejection properties: 1. A study of CMEs associated with limb activity , 2004 .
[17] C. J. Wolfson,et al. Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) , 2008 .
[18] T. Howard,et al. Interplanetary coronal mass ejections that are undetected by solar coronagraphs , 2008 .
[19] S. Antiochos,et al. A MODEL FOR SOLAR POLAR JETS , 2009 .
[20] Yannick Boursier,et al. Automatic detection of coronal mass ejections on LASCO-C2 synoptic maps , 2005, SPIE Optics + Photonics.
[21] V. Bothmer,et al. On the three-dimensional configuration of coronal mass ejections , 2004 .
[22] H. Morgan,et al. ERUPTING FILAMENTS WITH LARGE ENCLOSING FLUX TUBES AS SOURCES OF HIGH-MASS THREE-PART CMEs, AND ERUPTING FILAMENTS IN THE ABSENCE OF ENCLOSING FLUX TUBES AS SOURCES OF LOW-MASS UNSTRUCTURED CMEs , 2015, 1606.03278.
[23] A. Vourlidas,et al. Three-Dimensional Properties of Coronal Mass Ejections from STEREO/SECCHI Observations , 2012 .
[24] A. Vourlidas,et al. COMPREHENSIVE ANALYSIS OF CORONAL MASS EJECTION MASS AND ENERGY PROPERTIES OVER A FULL SOLAR CYCLE , 2010, 1008.3737.
[25] Yannick Boursier,et al. The ARTEMIS Catalog of LASCO Coronal Mass Ejections , 2009 .
[26] Yannick Boursier,et al. ARTEMIS II: A Second-Generation Catalog of LASCO Coronal Mass Ejections Including Mass and Kinetic Energy , 2013 .
[27] H. Morgan,et al. JETS, CORONAL “PUFFS,” AND A SLOW CORONAL MASS EJECTION CAUSED BY AN OPPOSITE-POLARITY REGION WITHIN AN ACTIVE REGION FOOTPOINT , 2016 .
[28] L. P. Karakatsanis,et al. THE MAJOR GEOEFFECTIVE SOLAR ERUPTIONS OF 2012 MARCH 7: COMPREHENSIVE SUN-TO-EARTH ANALYSIS , 2016 .
[29] T. Howard,et al. Coronal Mass Ejections: Observations , 2012 .
[30] A. Vourlidas,et al. STEREO SECCHI Stereoscopic Observations Constraining the Initiation of Polar Coronal Jets , 2008, 0804.4862.
[31] M. Temmer,et al. CME Projection Effects Studied with STEREO/COR and SOHO/LASCO , 2009 .
[32] S. Lepri,et al. DIRECT OBSERVATIONAL EVIDENCE OF FILAMENT MATERIAL WITHIN INTERPLANETARY CORONAL MASS EJECTIONS , 2010 .
[33] P. Lamy,et al. The Large Angle Spectroscopic Coronagraph (LASCO) , 1995 .
[34] Dieter Schmitt,et al. Does the butterfly diagram indicate a solar flux-transport dynamo? , 2004 .
[35] Jason P. Byrne,et al. AUTOMATIC DETECTION AND TRACKING OF CORONAL MASS EJECTIONS. II. MULTISCALE FILTERING OF CORONAGRAPH IMAGES , 2012, 1207.6125.
[36] D. Webb,et al. MLSO Mark III K-Coronameter Observations of the CME Rate from 1989 – 1996 , 2015 .
[37] Russell A. Howard,et al. The SOHO/LASCO CME Catalog , 2009 .
[38] A. Hundhausen,et al. Sizes and locations of coronal mass ejections - SMM observations from 1980 and 1984-1989 , 1993 .
[39] P. Hess,et al. Comparing Automatic CME Detections in Multiple LASCO and SECCHI Catalogs , 2017 .
[40] M. Linton,et al. IMAGING PROMINENCE ERUPTIONS OUT TO 1 AU , 2015, 1512.06748.
[41] E. Robbrecht,et al. AUTOMATED LASCO CME CATALOG FOR SOLAR CYCLE 23: ARE CMEs SCALE INVARIANT? , 2008, 0810.1252.
[42] Russell A. Howard,et al. The solar cycle variation of coronal mass ejections and the solar wind mass flux , 1994 .
[43] H. Morgan,et al. Automated detection of coronal mass ejections in three-dimensions using multi-viewpoint observations , 2016, 1612.04560.
[44] A. Vourlidas,et al. USING MULTIPLE-VIEWPOINT OBSERVATIONS TO DETERMINE THE INTERACTION OF THREE CORONAL MASS EJECTIONS OBSERVED ON 2012 MARCH 5 , 2015 .
[45] S. Cranmer,et al. Ultraviolet spectroscopy of the extended solar corona , 2006 .
[46] Guillermo Stenborg,et al. Pseudo-automatic characterization of the morphological and kinematical properties of coronal mass ejections using a texture-based technique , 2013 .
[47] Russell J. Hewett,et al. Intercomparison of the LASCO-C2, SECCHI-COR1, SECCHI-COR2, and Mk4 Coronagraphs , 2012 .