| 摘要 |
astrophysical measurements, applicable for research of the structure and dynamics of magnetic fields in the solar atmosphere. SUBSTANCE: the intensity of luminous radiation is measured simultaneously in the section of superposition of spectral component &phis;rbl in blue Èbl and red Èrl wings of the spectral line, as well as in the section of continuous spectrum Èc that is closest to the line. The magnetic field strength is calculated by formula: , where kH-calibration factor. EFFECT: provided simultaneous measurement of the longitudinal magnetic field strength and the beam velocity only per exposition, which considerably weakens the action of atmospheric instabilities and reduces the time of observations. 2 dwg
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