oblateness
- oblateness的基本解释
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扁率
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扁圆形
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扁球形
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The oblateness tends to decrease since the formation of the earth.
地球的扁率自形成以来总体趋势在减小。
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The change of oblateness in individual geological periods is needed to determine the change of the earth's shape.
为了确定地球形状的变化需要了解各个地质历史时期其扁率的变化。
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The effects of air drag and oblateness of the earth on relative orbit were derived by simulations under different conditions.
从动力学出发在考虑大气阻力和地球扁率的情况下推导出详细的航天器相对运动方程表达式。
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Using the data of inclination, radius and mass of disc galaxies, the mass density and oblateness of 93 disc galaxies have been obtained.
盘星系的质量密度在研究星系的结构和演化时,星系的质量密度是一个重要的物理量。
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The oblateness in each time can be calculated according to the conjectured change of the radius, the quality and the angular velocity.
通过推测地球的半径、质量和角速度的变化量,计算出地球各个时期的扁率。
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oblateness:扁率
oblate spherold 扁球体 | oblateness 扁率 | obligatory point 约束体
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oblateness:扁率;扁圆形
oblate 扁圆形的 | oblateness 扁率;扁圆形 | Oblatinella 扁球粉属
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oblateness:椭圆
Plane geometry 平面几何 | Oblateness 椭圆 | Parallelogram 平行四边形
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oblateness:扁圆形
oblateness 扁率 | oblateness 扁圆形 | oblatenessspheroidicity 扁球形
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polar oblateness:极向扁率
polar night 极夜 | polar oblateness 极向扁率 | polar path [地]极轨线
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