  The perplexing mystery of what maintains the solar coronal temperature at
about a million K, while the visible disc of the Sun is only at 5800 K, has
been a long standing problem in solar physics. A recent study by Mondal(2020)
has provided the first evidence for the presence of numerous ubiquitous
impulsive emissions at low radio frequencies from the quiet sun regions, which
could hold the key to solving this mystery. These features occur at rates of
about five hundred events per minute, and their strength is only a few percent
of the background steady emission. One of the next steps for exploring the
feasibility of this resolution to the coronal heating problem is to understand
the morphology of these emissions. To meet this objective we have developed a
technique based on an unsupervised machine learning approach for characterising
the morphology of these impulsive emissions. Here we present the results of
application of this technique to over 8000 images spanning 70 minutes of data
in which about 34,500 features could robustly be characterised as 2D elliptical
Gaussians.
