First Results From the SCM Search?Coil Magnetometer on Parker Solar Probe

Parker Solar Probe is the first mission to probe in situ innermost heliosphere, revealing an exceptionally dynamic and structured outer solar corona. Its payload includes a search-coil magnetometer (SCM) that measures up three components of fluctuating magnetic field between 3 Hz 1 MHz. After more than years operation, SCM has revealed multitude different wave phenomena wind. Here we present overview some discoveries made so far. These include oblique sunward propagating whistler waves are important for their interaction with energetic electrons, observation signature associated escaping electrons during dust impacts, component slow extraordinary modes type III radio burst events, more. This study focuses on major observations date, including description instrument lessons learned.