Theoretical models for the electromagnetic launching of astrophysical jets have long indicated that this process should generate helical magnetic fields. which should then propagate outward with the jet plasma. Polarization observations of jets are key for testing this idea. since they provide direct information about the magnetic field structures in the synchrotron-emitting radio jets. https://parisnaturalfoodes.shop/product-category/aloe-vera-lip-balm/