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Cited article:

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PLASMA PHYSICAL PARAMETERS ALONG CORONAL-MASS-EJECTION-DRIVEN SHOCKS. I. ULTRAVIOLET AND WHITE-LIGHT OBSERVATIONS

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Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. I. Reconciliation of “EIT Waves”, Type II Radio Bursts, and Leading Edges of CMEs

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Energy Storage and Release through the Solar Activity Cycle

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FIRST COMPLETE DETERMINATION OF PLASMA PHYSICAL PARAMETERS ACROSS A CORONAL MASS EJECTION-DRIVEN SHOCK

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Fragmented type II burst emission during CME liftoff

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UV and Radio Observations of the Coronal Shock Associated with the 2002 July 23 Coronal Mass Ejection Event

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Generation of a secondary shock wave during the oblique collision between a current sheet and a fast magnetosonic shock wave

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Ultraviolet spectroscopy of the extended solar corona

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Electromagnetic wave emission during collision between a current sheet and a fast magnetosonic shock associated with coronal mass ejections

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