  We compile the catalog of Hvar Observatory solar observations in the time
period corresponding to regular digitally stored chromospheric and photospheric
observations 2010-2019. We make basic characterisation of observed phenomena
and compare them to catalogs which are based on full disc solar images. We
compile a catalog of observed ARs consisting of 1100 entries, where each AR is
classified according to McIntosh and Mt Wilson classifications. We find that
HVAR observations are biased towards more frequently observing more complex ARs
and observing them in longer time periods, likely related to the small FOV not
encompassing the whole solar disc. In H$\alpha$ observations we catalog
conspicuous filaments/prominences and flares. We characterise filaments
according to their location, chirality (if possible) and eruptive signatures.
Analysis of the eruptive filaments reveals a slight bias in HVAR catalog
towards observation of partial eruptions, possibly related to the observers
tendency to observe filament which already showed some activity. In the flare
catalog we focus on their observed eruptive signatures (loops or ribbons) and
their shape. In addition, we associate them to GOES soft X-ray flares to
determine their corresponding class. We find that HVAR observations seem biased
towards more frequently observing stronger flares and observing them in longer
time periods. We demonstrate the feasibility of the catalog on a case study of
the flare detected on 2 August 2011 in HVAR H$\alpha$ observations and related
Sun-to-Earth phenomena. Through flare-CME-ICME association we demonstrate the
agreement of remote and in situ properties. The data used for this study, as
well as the catalog, are made publicly available.
