日本地球惑星科学連合2016年大会

講演情報

ポスター発表

セッション記号 S (固体地球科学) » S-GD 測地学

[S-GD22] 重力・ジオイド

2016年5月22日(日) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*西島 潤(九州大学大学院 工学研究院 地球資源システム工学部門)、青山 雄一(国立極地研究所)

17:15 〜 18:30

[SGD22-P04] 昭和基地超伝導重力計で観測された東南極の積雪増加とチャンドラー極運動の減衰

*青山 雄一1土井 浩一郎1渋谷 和雄1池田 博2早河 秀章1 (1.国立極地研究所、2.筑波大学研究基盤総合センター低温部門)

キーワード:超伝導重力計、東南極の積雪増加

Continuous gravimetric observations have been made with three successive generations of superconducting gravimeter (SG) over 20 years at Syowa Station (39.6E, 69.0S), Dronning Maud Land (DML), East Antarctica. The third-generation SG, OSG#058, was installed in January 2010. Five years of OSG#058 data from January 2010 to January 2015 were of high quality, with no missing data and with no step-like noise. So we could examine the long-period gravity variation precisely. Non-tidal gravity variations derived from the OSG#058 data showed significant correlation with the accumulated snow depth observed at Syowa Station. We inferred the gravitational effect of the accumulated snow mass (ASME) detected by OSG#058. Moreover, the accumulated snow depth at Syowa Station was found to represent heavy snowfall (the snow accumulation) in a broad region in DML, which was estimated from the Gravity Recovery and Climate Experiment (GRACE) satellite gravity data. Such snow accumulation around Syowa Station was detectable by OSG#058. A gravitational response to the Chandler wobble (CW) was deduced from the OSG#058 non-tidal gravity variations after correcting the ASME. The observed response agreed roughly with the predicted response in both amplitude and phase. We also found that recent CW weakened and its period gradually decreased. We will discuss the relation between the heavy snowfall in DML and the weakening of CW, which were observed with OSG#058.