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Temperature diagnostics for carbon IV ion by using a collision model in the solar transition region

For spectral diagnostics of temperature in the solar transition region, by using a semi-classical method, we calculate the collision strengths for the dipole transition of carbon IV 2S1/2-2P1/2 and 2S1/2-2P3/2, and we discuss the Maxwellian-averaged collision strengths for a wide temperature region. Then, based on the Maxwellian-averaged collision strengths, we discuss the spectral diagnostic of temperature in the solar transition region and obtain the temperature T = 1.7 × 105 K for the carbon IV ion in that region, which is in good agreement with the predicted temperature range of 1.0 × 105 K to 2.0 × 105 K. This calculation will be significant for spectral diagnostics in the solar transition region.