O x with Sr 2 IrO 4 interlayer thickness d=5 and 7 nm and in-plane sizes L=10-50 µm. A strontium iridate, Sr 2 IrO 4 , is known as a canted antiferromagnetic insulator at low temperatures and characterized also by the strong spin-orbit interaction due to the impact of the IrO 2 plane. The superconducting critical current density j C ≈ 0.3 A/cm 2 for the case d=7 nm was observed at T=4.2K. The temperature dependences of the superconducting critical current I C (T) and the voltage position on the I-V curve of the gap singularity of the Nb electrode V ∆ (T) show an increase with decreasing temperature and corresponds to the expected BCS behavior of the Nb energy gap ∆ Nb (T). The critical current is very sensitive to the influence of an external magnetic field and reduces twice at an external magnetic field (H≈0.2 Oe for L=40-50 µm) comparable with the earth magnetic field; The magnetic field dependence I C (H) at low H was narrower than the Fraunhofer pattern about 1.5 times. Both the integer and fractional Shapiro steps at voltages V m,n =(m/n)(h/2e)f e were observed under microwave radiation at frequencies f e =38 GHz and f e =50 GHz. Fractional Shapiro steps (m/n=1/2, 3/2) may point on the presence of the second harmonic in the superconducting current-phase relation.The spin-triplet superconducting pairing induced at the interface of a superconductor and a material with the strong spin-orbit interaction (SOI) gives promising opportunities for superconducting spintronics applications [1][2][3]. It has been shown theoretically, that the SOI in a ferromagnet of the superconductor-ferromagnet-superconductor junction can result in a spintriplet pairing [4][5][6][7]. Rashba proximity states in superconducting tunnel junctions, tuning of a magnetization, the proximity-induced triplet superconductivity, and the anomalous Josephson effect have been predicted as well [8][9][10][11][12][13][14][15][16][17]. Coulomb repulsion and Pauli quenching affect the superconducting current in tunnel junction with SOI interlayer but do not destroy the possibility to tune it by changing the strength of the spin-orbit interaction [18][19][20][21]. So, a lot of very