magnetic splitting fâqeš-e meqnâtisi Fr.: dédoublement magnétique A process whereby the (internal) → magnetic field of a star modifies the → pulsations by lifting some of its degeneracy. Instead of just one pulsation frequency, a multiplet of frequencies is then observed. This effect was proposed as a possible explanation for the observed frequency pattern of → Beta Cephei. In practice, the magnetic splitting is difficult to observe, because of the very small expected frequency difference between the peaks. However, when unaccounted for, it may lead to a wrong mode identification. The current best candidate to detect magnetic splitting is → HD 43317, since this star displays two close frequency patterns (Buysschaert et al., 2017, astro-ph/1709.02619). |
splitting fâqeš Fr.: clivage, fissure, rupture The act or instance of being split or causing something to split. → splitting of energy level. Verbal noun of → split. |
splitting of energy level fâqeš-e tarâz-e kâruž Fr.: dédoublement d'un niveau d'énergie The splitting of a single atomic level into a group of closely spaced levels when the substance producing the single line is subjected to a uniform magnetic field. → Zeeman effect; → Stark effect. → spliting; → energy level. |