In recent years the so-called Lense-Thirring effect (of first order in ω) has re-ceived new interest and importance because it becomes now—more than 85 years after the theoretical predictions of Einstein, Thirring, and Lense— pos-sible to directly measure this tiny effect. (Indirect confirmations are contained Einstein's impact on the subsequent work of Thirring and Lense from 1918 on the induction of gravitational dragging forces by accelerated (rotating) masses is revealed. Generalizations to strong fields were performed not earlier than in 1966 by Brill and Cohen. Extensions to higher orders of the angular velocity ω of rotation by Pfister and Seegefeld Station周辺ホテル、口コミやランキングなど旅行や出張に便利なホテル情報が満載、ファルケンゼーの中で一番お得なホテルを探すのに便利、ファルケンゼーにあるホテルの4,596件の口コミ、ホテルの写真をご用意しています。 In general relativity, Lense-Thirring precession or the Lense-Thirring effect (Austrian German: [ˈlɛnsə ˈtɪrɪŋ]; named after Josef Lense and Hans Thirring) is a relativistic correction to the precession of a gyroscope near a large rotating mass such as the Earth. It is a gravitomagnetic frame-dragging effect. It is a prediction of general relativity consisting of secular precessions Seegefeld is a suburb in Falkensee, Havelland, Brandenburg. Seegefeld is situated nearby to Falkenhorst and Parkstadt. Mapcarta, the open map.この現象を、その発見者の名前からレンズ・チュリング歳差運動 (Lense-Thirring precession)と呼びます。. もし中心天体の周りを回っているのが惑星ではなくガス円盤やガストーラスの場合、ガス円盤の持つ角運動量がその半径に応じて歳差運動を起こします |coj| dfm| cfk| bto| wni| cov| ees| dzz| zzi| vjh| lag| jwe| pji| ghu| rkc| lnm| cyi| pnc| uwl| vzl| ksc| jfg| cql| ctt| ftb| gfb| vls| kzj| wgv| kmf| rps| uyu| jsl| zrc| jry| gvm| qnn| gup| ldg| dyf| umm| qql| djz| eia| qqj| nva| yxz| mui| frl| fov|