THE WAVE PROPERTIES OF CORONAL BRIGHT FRONTS OBSERVED USING <i>SDO</i> /AIA
THE WAVE PROPERTIES OF CORONAL BRIGHT FRONTS OBSERVED USING <i>SDO</i> /AIA
Coronal bright fronts (CBFs) are large-scale wavefronts that propagate through the solar corona at hundreds of kilometers per second. While their kinematics have been studied in detail, many questions remain regarding the temporal evolution of their amplitude and pulse width. Here, contemporaneous high cadence, multi-thermal observations of the solar corona …