  Flares on the Sun are often associated with ejected plasma: these events are
known as coronal mass ejections (CMEs). These events, although are studied in
detail on the Sun, have only a few dozen known examples on other stars, mainly
detected using the Doppler-shifted absorption/emission features in Balmer lines
and tedious manual analysis. We present a possibility to find stellar CMEs with
the help of high-resolution solar spectra.
