The sources of isolated ultrashort light pulses are highly requested in modern ultrafast and attosecond science. Even though some experiments with isolated attosecond pulses (APs) have already been demonstrated [1], such light sources are still quite unique and not easily available while trains of APs are routinely produced in so called high-harmonics generation experiments. Regardless of the generation mechanisms deep understanding and characterisation of these pulse trains is an essential step towards routine generation of isolated attosecond pulses.

© 2019 IEEE

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