Japan Geoscience Union Meeting 2014

Presentation information

International Session (Oral)

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

[P-EM09_29PM1] VarSITI - Variability of the Sun and Its Terrestrial Impact

Tue. Apr 29, 2014 2:15 PM - 4:00 PM 501 (5F)

Convener:*Kazuo Shiokawa(Solar-Terrestrial Environment Laboratory, Nagoya University), Taro Sakao(Institute of Space and Astronautical Science Japan Aerospace Exploration Agency), Toshihiko Hirooka(Department of Earth and Planetary Scinences, Kyushu University), Chair:Shin Suzuki(Solar-Terrestrial Environment Laboratory, Nagoya University), Mitsumu K. Ejiri(National Institute of Polar Research)

2:45 PM - 3:00 PM

[PEM09-38] Observations and modeling studies for understanding atmospheric responses to unusual solar activities

*Hitoshi FUJIWARA1, Yasunobu MIYOSHI2, Hidekatsu JIN3, Hiroyuki SHINAGAWA3, Satonori NOZAWA4, Yasunobu OGAWA5, Ryuho KATAOKA5 (1.Faculty of Science and Technology, Seikei University, 2.Department of Earth and Planetary Sciences, Faculty of Sciences, Kyushu University, 3.National Institute of Information and Communications Technology, 4.Solar Terrestrial Environment Laboratory, Nagoya University, 5.National Institute of Polar Research)

Keywords:thermosphere, ionosphere, middle atmosphere, GCM, radar, aeronomy

As pointed out by many researchers, the recent solar activities are very unusual; the solar activity during the last minimum in 2008-2009 was extremely low and that during the next maximum of sunspot cycle 24 shows much lower activities compared with the previous two solar maximums in cycle 22 and 23. In order to understand the complex system of the Earth's middle and upper atmosphere, these solar activities will give us important information and/or good opportunities for searching the basic states of the system both from the observations and GCM simulations. Comprehensive studies by observations from space, ground-based ones, and numerical simulations will enable us to understand the polar mesosphere, thermosphere, and ionosphere quantitatively. In order to understand variations of the polar ionosphere from the solar minimum to maximum periods, we have made EISCAT experiments in January 2011, March, 2012, and March 2013. For example, ionospheric variations were observed during solar flare and CME events on March 12, 2012. These EISCAT data clearly show an example of the solar wind, magnetosphere, and ionosphere coupling. In addition to the EISCAT observations, we have also investigated variations of the polar thermosphere during periods of significant solar activities from GCM simulations. In this presentation, we will introduce our research activities mainly related to the "Role Of the Sun and the Middle atmosphere/thermosphere/ionosphere In Climate (ROSMIC)" project in VarSITI.