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Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments

机译:太阳动力学观测台(sDO)的极端紫外线可变性实验(EVE):科学目标,仪器设计,数据产品和模型开发概述

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摘要

The highly variable solar extreme ultraviolet (EUV) radiation is the major energy input to the Earth’s upper atmosphere, strongly impacting the geospace environment, affecting satellite operations, communications, and navigation. The Extreme ultraviolet Variability Experiment (EVE) onboard 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 (ten seconds), and accuracy (20%). EVE includes several irradiance instruments: The Multiple EUV Grating Spectrographs (MEGS)-A is a grazing-incidence spectrograph that measures the solar EUV irradiance in the 5 to 37 nm range with 0.1-nm resolution, and the MEGS-B is a normal-incidence, dual-pass spectrograph that measures the solar EUV irradiance in the 35 to 105 nm range with 0.1-nm resolution. To provide MEGS in-flight calibration, the EUV SpectroPhotometer (ESP) measures the solar EUV irradiance in broadbands between 0.1 and 39 nm, and a MEGS-Photometer measures the Sun’s bright hydrogen emission at 121.6 nm. The EVE data products include a near real-time space-weather product (Level 0C), which provides the solar EUV irradiance in specific bands and also spectra in 0.1-nm intervals with a cadence of one minute and with a time delay of less than 15 minutes. The EVE higher-level products are Level 2 with the solar EUV irradiance at higher time cadence (0.25 seconds for photometers and ten seconds for spectrographs) and Level 3 with averages of the solar irradiance over a day and over each one-hour period. The EVE team also plans to advance existing models of solar EUV irradiance and to operationally use the EVE measurements in models of Earth’s ionosphere and thermosphere. Improved understanding of the evolution of solar flares and extending the various models to incorporate solar flare events are high priorities for the EVE team.
机译:高度可变的太阳极端紫外线(EUV)辐射是输入到地球高层大气的主要能量,对地球空间环境产生了巨大影响,影响了卫星的运行,通信和导航。 NASA太阳动力天文台(SDO)上的极端紫外线变异性实验(EVE)将以前所未有的光谱分辨率(0.1 nm),时间节奏(十秒)和准确性(20%)测量从0.1至105 nm的太阳EUV辐照度。 EVE包括几种辐照仪器:多重EUV光栅光谱仪(MEGS)-A是掠入射光谱仪,可测量5至37 nm范围内的太阳EUV辐照度,分辨率为0.1 nm,而MEGS-B是普通的-入射双通光谱仪,可测量35至105 nm范围内的太阳EUV辐照度,分辨率为0.1 nm。为了提供MEGS的飞行中校准,EUV分光光度计(ESP)可以测量0.1至39 nm之间宽带中的太阳EUV辐照度,而MEGS光度计可以测量121.6 nm处太阳的明亮氢辐射。 EVE数据产品包括近乎实时的空间天气产品(0C级),该产品可提供特定频段的太阳EUV辐照度,以及0.1 nm间隔的光谱,节奏为一分钟,时延小于1分钟。 15分钟。 EVE较高级别的产品具有2级,其太阳EUV辐照度具有较高的时间节奏(光度计为0.25秒,光谱仪为10秒),以及3级,具有一天和每个小时的平均太阳辐照度。 EVE小组还计划推进现有的太阳EUV辐照度模型,并在地球电离层和热层模型中实际使用EVE测量。 EVE团队非常重视对太阳耀斑演变的理解,并扩展各种模型以纳入太阳耀斑事件。

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