CHANG-ES

Galactic winds play a key role in regulating the evolution of galaxies over cosmic time. In recent years, rays (CR) formation galactic wind has increasingly gained attention. Therefore, we use radio continuum data to analyse ray transport edge-on galaxies. Data from LOFAR Two-metre Sky Survey (LoTSS) release 2 at 144 MHz (HBA) and reprocessed VLA 1.6 GHz (L-band) Continuum Halos Nearby Galaxies - an EVLA (CHANG-ES) enable us increase extent analysed profile significantly (up factor 2) compared previous studies. We compute thermal emission maps using mixture approach H-alpha near infrared data, which is then subtracted yield synchrotron maps. Then compile non-thermal spectral index intensity profiles box integration approach. Lastly, perform 1D modelling. The show evidence that LoTSS are affected by absorption, star forming regions. scale height analysis reveals most equally well fitted with one-component instead twocomponent exponential profile. find bi-modality within our sample. While NGC 3432 4013 have similar heights L-band HBA, low-frequency 891, 4157, 4631 exceed their high-frequency counterpart significantly. CR modelling shows agreement predicted magnetic field strength estimates equipartition measurements. Additionally increasing difference velocities (with disk) between central outer regions