High-latitude supergiants: Anomalies in the spectrum of LN Hya in 2010

High-spectral-resolution observations with the Special Astrophysical Observatory 6-m telescope obtained in 2003–2011 are used to study features of the optical spectrum and the velocity field in the atmosphere of the semiregular variable LN Hya in detail. The weak, symmetric, photospheric absorption lines indicate radial-velocity variations from night to night (by as much as 3 km/s), resulting from small pulsations. Peculiarities and profile variations were found for strong lines of FeI, FeII, BaII, SiII, etc. The profiles of these lines were asymmetric: their short-wavelength wings were extended and their cores were either split or distorted by emission. During the 2010 observing season, the position and depth of the Hα absorption component, the intensities of the short- and long-wavelength emission components, and the intensity ratio of the latter components varied from spectrum to spectrum. Weak emission lines of neutral atoms (VI, MnI, CoI, NiI, FeI) appeared in the spectrum of June 1, 2010. These spectral peculiarities, recorded for the first time, suggest that we have detected rapid changes in the physical conditions in the upper atmospheric layers of LN Hya in 2010.