Japan Geoscience Union Meeting 2015

Presentation information


Symbol P (Space and Planetary Sciences) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM27] Physics and Chemistry in the Atmosphere and Ionosphere

Tue. May 26, 2015 6:15 PM - 7:30 PM Convention Hall (2F)

Convener:*Yuichi Otsuka(Solar-Terrestrial Environment Laboratory, Nagoya University), Takuya Tsugawa(National Institute of Information and Communications Technology), Seiji Kawamura(National Institute of Information and Communications Technology)

6:15 PM - 7:30 PM

[PEM27-P21] An observation of sodium twilight airglow using a Fabry-Perot imager

*Hidehiko SUZUKI1, Hideyuki TAKAHASHI2, Makoto TAGUCHI2 (1.Meiji university, 2.Rikkyo university)

Keywords:twilight airglow, mesosphere, thermosphere, metallic layer, Fabry-Perot

The mesosphere and lower thermosphere (MLT) region is thought as a key region to solve a mechanism of the global change in the Earth's atmospheric system. Atomic metal layers which are maintained by ablation of meteors in the MLT region are known as a precious tracer to investigate chemistry and dynamics of the upper atmosphere [Williams, 2002]. For example, resonance scatter lidars tuned for wavelengths of various metal species are widely used to infer the winds and temperature in the MLT region [Plane, 2003]. However, there are still many ambiguities in knowledge about a horizontal structure and a seasonal variability of the metal layers. Therefore, a twilight airglow is focused on as a tracer to investigate horizontal structures of the metal layers in the MLT region in this study. The twilight airglow is luminous phenomenon which is caused by a resonance scattering of the metallic atoms in the MLT region illuminated by solar irradiance. This emission is effectively detectable in twilight time under a suitable geometric condition among the Sun, the metal layers, and a ground-based observer [e.g. Chamberlein, 1961]. Unlike a resonance scattering lidar, an emission from a metallic atom layer occurs simultaneously in a horizontally spread area, because a light source of the emission is solar irradiance in a case of twilight airglow. Thus, it is possible to deduce a horizontal distribution of metallic atoms from twilight airglow observations by using a sensitive and narrow band imaging device with a wide field of view. The Fabry-Perot interferometric imager (FPI) of the National Institute of Polar Research (NIPR) is one of instruments which satisfy these requirements. In this study results of a test observation of sodium twilight airglow, which is one of the strongest emissions in twilight, using the FPI at NIPR are presented, and future possibilities for study of a horizontal structure of metallic atom distribution in the MLT region using the FPI are discussed.