Rychlostní pole v erupcích byla odvozena použitím spekter z MSDP. Teoretické profily čar byly spočteny pomocí na základě non-LTE metody přenosu záření. (cs)
Using the MSDP spectra, the velocity fields in flares were derived. Theoretical line profiles were computed using the non-LTE radiative-transfer technique.
Using the MSDP spectra, the velocity fields in flares were derived. Theoretical line profiles were computed using the non-LTE radiative-transfer technique. (en)