EMIC waves observed at geosynchronous orbit under quiet geomagnetic conditions ( <i>Kp</i>  ≤ 1)

<jats:title>Abstract</jats:title> <jats:p> We statistically study the local time distribution of the helium band electromagnetic ion cyclotron (EMIC) waves observed at geosynchronous orbit when geomagnetic activity was low ( <jats:italic>K</jats:italic> <jats:italic>p</jats:italic> ≤ 1). In order to identify the geosynchronous EMIC waves, we use high time resolution magnetic field data acquired from GOES 10, 11, and 12 over a 2 year period from 2007 and 2008 and examine the local time distribution of EMIC wave events. Unlike previous studies, which reported high EMIC wave occurrence in the postnoon sector with a peak around 1500–1600 magnetic local time (MLT) during magnetically disturbed times (i.e., storm and/or substorm), we observed that quiet time EMIC waves mostly occur in a region from morning (∼0600 MLT) to afternoon (∼1600 MLT) with a peak around 1100–1200 MLT. To investigate whether the quiet time EMIC wave occurrence has a causal relationship with magnetospheric convection enhancement or solar wind dynamic pressure variations, we performed a superposed epoch analysis of solar wind parameters (solar wind speed, density, dynamic pressure, and interplanetary magnetic field <jats:italic>B</jats:italic> <jats:sub> <jats:italic>z</jats:italic> </jats:sub> ) and geomagnetic indices ( <jats:italic>A</jats:italic> <jats:italic>E</jats:italic> and <jats:italic>S</jats:italic> <jats:italic>Y</jats:italic> <jats:italic>M</jats:italic> ‐ <jats:italic>H</jats:italic> ). From the superposed epoch analysis we found that solar wind dynamic pressure variation is a more important parameter than <jats:italic>A</jats:italic> <jats:italic>E</jats:italic> and <jats:italic>S</jats:italic> <jats:italic>Y</jats:italic> <jats:italic>M</jats:italic> ‐ <jats:italic>H</jats:italic> for quiet time EMIC wave occurrence. </jats:p>