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An analysis of the energy spectra of cosmic rays and particularly the precisedata from the AMS-02 experiment support the view about the important role ofthe Local Bubble in the nearby interstellar medium. It is suggested that thebulk of cosmic rays below about 200 GV of rigidity (momentum/charge ratio)comes from the modest number of supernova remnants in the Local Bubble whichappear to have occurred some $10^6$ years ago and contributed to its formation.At higher rigidities the contribution from a 'Local Source', a single supernovaremnant generated some $10^5$ years ago seems to dominate up to, at least 1000GV.

The Local Bubble in the interstellar medium and the origin of the low energy cosmic rays