The proper treatment of coronal mass ejection brightness : A new methodology and implications for observationsVOURLIDAS, Angelos; HOWARD, Russell A.The Astrophysical journal. 2006, Vol 642, Num 2, pp 1216-1221, issn 0004-637X, 6 p., 1Article

A new technique for deriving prominence mass from SOHO/EIT Fe XII (19.5 nanometers) absorption featuresGILBERT, Holly R; HOLZER, Thomas E; MACQUEEN, R. M et al.The Astrophysical journal. 2005, Vol 618, Num 1, pp 524-536, issn 0004-637X, 13 p., 1Article

On the origins of solar EIT wavesCLIVER, E. W; LAURENZA, M; STORINI, M et al.The Astrophysical journal. 2005, Vol 631, Num 1, pp 604-611, issn 0004-637X, 8 p., 1Article

THE BRIGHTNESS OF DENSITY STRUCTURES AT LARGE SOLAR ELONGATION ANGLES : WHAT IS BEING OBSERVED BY STEREO SECCHI?LUGAZ, N; VOURLIDAS, A; ROUSSEV, I. I et al.The Astrophysical journal. 2008, Vol 684, Num 2, issn 0004-637X, L111-L114, 2Article

Comparison of interplanetary cme charge state composition with CME-associated flare magnitudeREINARD, A.The Astrophysical journal. 2005, Vol 620, Num 1, pp 501-505, issn 0004-637X, 5 p., 1Article

THE RELATIONSHIP BETWEEN CORONAL DIMMING AND CORONAL MASS EJECTION PROPERTIESREINARD, A. A; BIESECKER, D. A.The Astrophysical journal. 2009, Vol 705, Num 1, pp 914-919, issn 0004-637X, 6 p., 1Article

CORONAL MASS EJECTION-ASSOCIATED CORONAL DIMMINGSREINARD, A. A; BIESECKER, D. A.The Astrophysical journal. 2008, Vol 674, Num 1, pp 576-585, issn 0004-637X, 10 p., 1Article

QUANTITATIVE MEASUREMENTS OF CORONAL MASS EJECTION-DRIVEN SHOCKS FROM LASCO OBSERVATIONSONTIVEROS, Veronica; VOURLIDAS, Angelos.The Astrophysical journal. 2009, Vol 693, Num 1, pp 267-275, issn 0004-637X, 9 p., 1Article

Global coronal mass ejectionsZHUKOVI, Andrei N; VESELOYSKY, Igor S.The Astrophysical journal. 2007, Vol 664, Num 2, issn 0004-637X, L131-L134, 2Article

Solar cycle variation of real cme latitudesWENBIN SONG; XUESHANG FENG; YANQI HU et al.The Astrophysical journal. 2007, Vol 667, Num 1, issn 0004-637X, L101-L104, 2Article

Multialtitude observations of a coronal jet during the third Whole Sun Month CampaignKO, Y.-K; RAYMOND, J. C; MASON, H. E et al.The Astrophysical journal. 2005, Vol 623, Num 1, pp 519-539, issn 0004-637X, 21 p., 1Article

A POSSIBLE DETECTION OF A FAST-MODE EXTREME ULTRAVIOLET WAVE ASSOCIATED WITH A MINI CORONAL MASS EJECTION OBSERVED BY THE SOLAR DYNAMICS OBSERVATORYRUISHENG ZHENG; YUNCHUN JIANG; JUNCHAO HONG et al.The Astrophysical journal. 2011, Vol 739, Num 2, issn 0004-637X, L39.1-L39.7, 2Article

A STUDY OF THE BUILD-UP, INITIATION, AND ACCELERATION OF 2008 APRIL 26 CORONAL MASS EJECTION OBSERVED BY STEREOCHENG, X; DING, M. D; ZHANG, J et al.The Astrophysical journal. 2010, Vol 712, Num 2, pp 1302-1310, issn 0004-637X, 9 p., 1Article

TRACKING STREAMER BLOBS INTO THE HELIOSPHERESHEELEY, N. R; ROUILLARD, A. P.The Astrophysical journal. 2010, Vol 715, Num 1, pp 300-309, issn 0004-637X, 10 p., 1Article

A comprehensive study of the initiation and early evolution of a coronal mass ejection from ultraviolet and white-light dataBEMPORAD, A; RAYMOND, J; POLETTO, G et al.The Astrophysical journal. 2007, Vol 655, Num 1, pp 576-590, issn 0004-637X, 15 p., 1Article

First direct observation of the interaction between a comet and a coronal mass ejection leading to a complete plasma tail disconnectionVOURLIDAS, Angelos; DAVIS, Chris J; EYLES, Chris J et al.The Astrophysical journal. 2007, Vol 668, Num 1, issn 0004-637X, L79-L82, 2Article

The width of a solar coronal mass ejection and the source of the driving magnetic explosion : A test of the standard scenario for cme productionMOORE, Ronald L; STERLING, Alphonse C; SUESS, Steven T et al.The Astrophysical journal. 2007, Vol 668, Num 2, pp 1221-1231, issn 0004-637X, 11 p., 1Article

Theoretical predictions of X-ray and extreme-UV flare emissions using a loss-of-equilibrium model of solar eruptionsREEVES, Katharine K; WARREN, Harry P; FORBES, Terry G et al.The Astrophysical journal. 2007, Vol 668, Num 2, pp 1210-1220, issn 0004-637X, 11 p., 1Article

Force balance analysis of a coronal magnetic flux rope in equilibrium or eruptionCHEN, Y; LI, G. O; HU, Y. Q et al.The Astrophysical journal. 2006, Vol 649, Num 2, pp 1093-1099, issn 0004-637X, 7 p., 1Article

Impact of major coronal mass ejections on geospace during 2005 september 7-13YUMING WANG; XIANGHUI XUE; CHENGLONG SHEN et al.The Astrophysical journal. 2006, Vol 646, Num 1, pp 625-633, issn 0004-637X, 9 p., 1Article

The calm before the storm : The link between quiescent cavities and coronal mass ejectionsGIBSON, S. E; FOSTER, D; BURKEPILE, J et al.The Astrophysical journal. 2006, Vol 641, Num 1, pp 590-605, issn 0004-637X, 16 p., 1Article

The flux-rope scaling of the acceleration of coronal mass ejections and eruptive prominencesCHEN, J; MARQUE, C; VOURLIDAS, A et al.The Astrophysical journal. 2006, Vol 649, Num 1, pp 452-463, issn 0004-637X, 12 p., 1Article

Three-dimensional structure of coronal mass ejections from LASCO polarization measurementsDERE, Kenneth P; WANG, Dennis; HOWARD, Russell et al.The Astrophysical journal. 2005, Vol 620, Num 2, pp L119-L122, issn 0004-637X, 2Article

Arrival time of halo coronal mass ejections in the vicinity of the EarthMICHALEK, G; GOPALSWAMY, N; LARA, A et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 423, Num 2, pp 729-736, issn 0004-6361, 8 p.Article

IMPULSIVE ACCELERATION OF CORONAL MASS EJECTIONS. I. STATISTICS AND CORONAL MASS EJECTION SOURCE REGION CHARACTERISTICSBEIN, B. M; BERKEBILE-STOISER, S; VERONIG, A. M et al.The Astrophysical journal. 2011, Vol 738, Num 2, issn 0004-637X, 738191.1-738191.14, 1Article