THERMAL CYCLOTRON RADIATION FROM A HOT CORONAL LOOP WITH HELICAL MAGNETIC-FIELD

The spectral and polarization properties of thermal cyclotron radio em ission from a hot coronal loop with a current along the axis are compu ted. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components b eing of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute v alue along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight r esults in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhan ced radio emission at those harmonics which are optically thin (for ex ample, s=4). These cannot be observed in models with the commonly empl oyed magnetic field configuration (longitudinal along the loop axis). We show that the frequency spectrum of thermal cyclotron radiation fro m a hot coronal loop with a helical magnetic field differs from that o f the standard s-component source (with smooth frequency characteristi cs and polarization corresponding to e-mode) in that plenty of fine st ructures (line-like features and cut-offs) are present and the o-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in th e model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be assoc iated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of loc al sources testifying to the presence of a helical magnetic field.