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SKA's large field of view and high sensitivity at low frequencies willprovide almost a complete coverage of the very early rising phase ofextragalactic and Galactic transients which undergo a flare or outburst due toan abrupt accretion onto either supermassive (such as tidal disruption events,TDEs) or stellar mass black hole transients (such as black hole LMXB) , whentheir broadband emission is supposed to be jet-dominated at low luminosities,allowing SKA to be the first facility to make source discoveries and to sendout alerts for follow-up ground or space observations as compared with thesensitivity of future X-ray wide-field-view monitoring. On the other hand, dueto extremely large rate-of-change in the mass accretion rate during the risingphase of TDE flares or transient outbursts, SKA will be able to cover anextremely large range of the mass accretion rate as well as its rate-of-changenot accessible with observations in persistent black hole systems, which willshape our understanding of disk-jet coupling in accreting black holes in thenon-stationary accretion regimes.

Early Phase Detection and Coverage of Extragalactic and Galactic Black Hole X-ray Transients with the SKA