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Narrow Coronal Mass EjectionsH. R. Gilbert, P. S. McIntosh, R. M. MacQueen et al.|The Astrophysical Journal|2001Cited by 52
A New Technique for Deriving Prominence Mass from<i>SOHO</i>/EIT Fe<scp>xii</scp>(19.5 Nanometers) Absorption FeaturesH. R. Gilbert, R. M. MacQueen, T. E. Holzer|The Astrophysical Journal|2004Cited by 34
Application of a New Technique for Deriving Prominence Mass from<i>SOHO</i>EIT Fe<scp>xii</scp>(19.5 nm) Absorption FeaturesH. R. Gilbert, R. M. MacQueen, Lauren E. Falco et al.|The Astrophysical Journal|2006Cited by 32
Solar Coronal Brightness Changes and Mass Ejections during Solar Cycle 22R. M. MacQueen, Kate Spence, J. Burkepile et al.|The Astrophysical Journal|2001Cited by 18