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We operate the six German stations of the LOw Frequency ARray as standalonetelescopes to observe more than 100 pulsars every week. To date, we havecollected almost four years of high-quality data at an unprecedented weeklycadence. This allows us to perform a wide variety of analyses aimed atcharacterising the magnetoionic plasma crossed by pulsar radiation. Inparticular, our studies are focused on electron density variations in theinterstellar and interplanetary media, the Galactic and interplanetary magneticfield, scintillation, and extreme scattering events. Here we report the firstresults from our Solar wind monitoring campaign.

The effect of the Solar wind on low-frequency observations of pulsars