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To study some characteristics of the interstellar medium, observational dataof pulsars with large Faraday rotation values (|RM|> 300 rad / m2) were used.It was suggested and justified that large |RM| values can be due to thecontribution of the regions with increased electron concentration, projected onthe pulsar. Most likely these are the HII regions, dark nebulae and molecularclouds. In these objects the magnetic field can be oriented in the direction ofa large-scale field of the Galaxy, or simply is a deformed extension of thegalactic field. It was shown that the Galactic distribution of rotationmeasures of pulsars with |RM|> 300rad / m2 corresponds to the circular model ofthe magnetic field of the Galaxy, with the counter-clockwise direction of themagnetic field in the galactocentric circle 5 kpc <R <7 kpc.

On the magnetic field inside the solar circle of the Galaxy: On the  possibility of investigation some of characteristics of the interstellar  medium with using of pulsars with large Faraday rotation values