Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets

We present observations of recurrent active region coronal jets and derive their thermal non-thermal properties, by studying the physical properties plasma simultaneously at base footpoint, along outflow jets. The sample analyzed solar were observed SDO-AIA in Extreme Ultraviolet RHESSI X-Ray domain. main parameters: temperature, density, energy flux contributions, etc. are calculated using multiple inversion techniques to obtain differential emission measure from extreme-ultraviolet filtergrams. underlying models assessed, limitations applicability scrutinized. Complementarily, we perform source reconstruction spectral analysis higher further assess structure identify properties. discuss a peculiar penumbral magnetic reconnection site, which previously identified as ``Coronal Geyser''. Evidence supporting cool hot emission, is presented for subset geyser These found be energetically stronger than polar counterparts, but find potential influence on heliospheric energetics dynamics limited. scrutinize whether does fit erupting microflare picture, finding that our peak flaring times can only explained combination models. This geysers provides new information observational constraints applicable theoretical modeling