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THE EUV VARIABILITY EXPERIMENT (EVE) ON THE SOLAR DYNAMICS HE OBSERVATORY (SDO): SCIENCE PLAN AND INSTRUMENT OVERVIEW

机译:EUV变异实验(EVE)在太阳能动力学的天文台(SDO):科学计划和仪器概述

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The highly variable solar extreme ultraviolet (EUV) radiation is the major energy input into the Earth’s upper atmosphere and thus impacts the geospace environment that affects satellite operations, commun communications, and navigation. The Extreme ications, ultraviolet Variability Experiment (EVE) aboard the NASA Solar Dynamics Observatory (SDO) will measure the solar EUV irradiance from 0.1 to 105 nm with unprecedented spectral resolution (0.1 nm), temporal cadence (10 s sec), and accuracy (20%). The ec), EVE program will provide solar EUV irradiance data for the NASA Living With the Star (LWS) program, including near real real-time data products to be used in operational atmospheric models that specify the space environment and to a assist in forecasting for space ssist weather operations. The EVE program is expected to make significant progress towards real understanding of the physics of the solar EUV irradiance variations on time scales from flares to the solar cycle. Additional informati information about the EVE program can be found at on http://lasp.colorado.edu/eve/ eve/.
机译:高度变化的太阳能极端紫外(EUV)辐射是进入地球高层大气的主要能量,从而影响了影响卫星操作,通信和导航的地球合区环境。 NASA太阳能动力学天文台(SDO)的极端近期,紫外变化实验(EVE)将以前所未有的光谱分辨率(0.1nm),时间焦点(10 s sec)和精度来测量0.1至105nm的太阳能EUV辐照度。 20%)。 EC),EVE程序将为与星空(LWS)程序为居的NASA提供太阳能EUV辐照度数据,包括近实际的实时数据产品,以用于指定空间环境和辅助预测的运行大气模型空间SSIST天气运营。预计前夕计划将对真实理解对太阳循环到太阳循环的时间尺度的太阳能EUV辐照度变化的物理学进行了重大进展。有关eve程序的其他信息可以在http://lasp.colorado.edu/eve/ eve /。

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