Hydrogen Lyα and Lyβ Radiances and Profiles in Polar Coronal Holes

TitreHydrogen Lyα and Lyβ Radiances and Profiles in Polar Coronal Holes
Type de publicationJournal Article
Year of Publication2009
AuteursTian, H., Teriaca L., Curdt W., and Vial J.-C.
JournalAstrophysical Journal Letters
Date PublishedOct

The hydrogen Lyα plays a dominant role in the radiative energy transport in the lower transition region, and is important for the studies of transition-region structure as well as solar wind origin. We investigate the Lyα profiles obtained by the Solar Ultraviolet Measurement of Emitted Radiation spectrograph on the Solar and Heliospheric Observatory spacecraft in coronal holes and the quiet Sun. In a subset of these observations, the H I Lyβ, Si III, and O VI lines were also (quasi-)simultaneously recorded. We find that the distances between the two peaks of Lyα profiles are larger in coronal holes than in the quiet Sun, indicating a larger opacity in coronal holes. This difference might result from the different magnetic structures or the different radiation fields in the two regions. Most of the Lyβ profiles in the coronal hole have a stronger blue peak, in contrast to those in quiet-Sun regions while in both regions the Lyα profiles are stronger in the blue peak. Although the asymmetries are likely to be produced by differential flows in the solar atmosphere, their detailed formation processes are still unclear. The radiance ratio between Lyα and Lyβ decreases toward the limb in the coronal hole, which might be due to the different opacity of the two lines. We also find that the radiance distributions of the four lines are set by a combined effect of limb brightening and the different emission level between coronal holes and the quiet Sun.