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Tidal disruption events (TDEs) around super massive black holes (SMBHs) are apotential laboratory to study super-Eddington accretion disks and sometimesresult in powerful jets or outflows which may shine in the radio and submillimeter bands. In this work, we model the thermal synchrotron emission ofjets from general relativistic radiation magneto-hydrodynamics (GRRMHD)simulations of a BH accretion disk/jet system which assumes the TDE resulted ina magnetized accretion disk around a BH accreting at $\sim 12-25$ times theEddington accretion rate. Through synthetic observations with the NextGeneration Event Horizon Telescope (ngEHT) and an image reconstructionanalysis, we demonstrate that TDE jets may provide compelling targets, withinthe context of the models explored in this work. In particular, we find thatjets launched by a SANE super-Eddington disk around a spin $a_*=0.9$ reach thengEHT detection threshold at large distances (up to 100 Mpc in this work). Atwo-temperature plasma in the jet or weaker jets, such as a spin $a_*=0$ model,requires a much closer distance as we demonstrate detection at 10 Mpc forlimiting cases of $a_*=0,\,\mathcal{R}=1$ or $a_*=0.9,\, \mathcal{R}=20$. Wealso demonstrate that TDE jets may appear as superluminal sources if the BH israpidly rotating and the jet is viewed nearly face on.

Modeling Reconstructed Images of Jets Launched by SANE Super-Eddington Accretion Flows Around SMBHs with the ngEHT