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[图片,小资料] 大气窗口(大气射电窗口) atmospheric radio window
大气窗口: atmospheric window
大气射电窗口: atmospheric radio window
大气特性: atmospheric characteristics
图1 大气窗口示意图
https://www.zgbk.com/ecph/words?SiteID=1&ID=111847&Type=bkzyb&SubID=94760
最科学、最准确
图2 intro_1-1-jpg.webp
https://smd-cms.nasa.gov/wp-content/uploads/2023/04/intro_1-1-jpg.webp
https://science.nasa.gov/ems/01_intro
频率(波长)范围最宽
图3 x374.jpg
Figure 1.1: Ground-based astronomy is confined to the visible and radio atmospheric windows, wavelength ranges in which the atmosphere is nearly transparent. The radio window is much wider than the visible window when plotted on logarithmic wavelength or frequency scales, so it includes a wide range of astronomical sources and emission mechanisms. Radio astronomers usually measure (and think in terms of) frequencies ν=c/λ instead of wavelengths λ. Thus λ=0.3mm corresponds to ν=1 THz, the highest frequency accessible from the best terrestrial sites. The Earth’s ionosphere reflects radio waves longer than λ~30m (ν~10MHz). Abscissa: Wavelength. Ordinate: Atmospheric transmission. Image Credit: ESA/Hubble (F. Granato).
【机器翻译】图1.1:地面天文学仅限于可见光和射电大气窗口,即大气几乎透明的波长范围。当以对数波长或频率标度绘制时,无线电窗口比可见光窗口宽得多,因此它包括各种天文源和发射机制。射电天文学家通常测量(并考虑)频率ν=c/λ,而不是波长λ。因此,λ=0.3mm对应于ν=1 THz,这是从最佳陆地站点获得的最高频率。地球电离层反射的无线电波长度超过30米(10兆赫)。Abscissa:波长。坐标:大气传输。图片来源:ESA/哈勃(F.Granato)。
https://www.cv.nrao.edu/~sransom/web/x374.jpg
https://www.cv.nrao.edu/~sransom/web/Ch1.html
图4 spectral_bands_marked2_mid.jpg
http://physics.wku.edu/~gibson/radio/bands/spectral_bands_marked2_mid.jpg
http://physics.wku.edu/~gibson/radio/bands/
图5 EMS-Introduction.jpeg
https://smd-prod.s3.amazonaws.com/science-red/s3fs-public/thumbnails/image/EMS-Introduction.jpeg
https://science.nasa.gov/ems/01_intro
图6 applsci-12-10429-g002.webp
https://www.mdpi.com/applsci/applsci-12-10429/article_deploy/html/images/applsci-12-10429-g002.png
https://www.mdpi.com/2076-3417/12/20/10429
图7 The-atmospheric-transmission-windows-from-radio-to-X-ray-wavelengths-Figure-created-by.png
图8 FIGURE 3 Window.jfif
http://employees.oneonta.edu/baumanpr/geosat2/RS-Introduction/FIGURE%203%20Window.JPG
http://employees.oneonta.edu/baumanpr/geosat2/RS-Introduction/RS-Introduction.html
图9 Atmospheric_electromagnetic_transmittance_or_opacity.jpg
图10 Robert-A.-Rohde-as-part-of-the-Global-Warming-Art-project-5-scaled.jpg
The Solar Spectrum. Courtesy of NASA and Geoengineering.global.
太阳光谱。由美国国家航空航天局和地球工程全球公司提供。
https://geoengineering.global/solar-radiation-management/
参考资料:
[1] 2022-12-23,大气窗口/atmospheric window/黄佑然,刘学富撰,黄永锋修订,中国大百科全书,第三版网络版[DB/OL]
https://www.zgbk.com/ecph/words?SiteID=1&ID=533733&Type=bkzyb&SubID=163178
天体辐射中能穿透大气的一些波段。
[2] 2023-11-02,大气窗口/atmospheric window/张永红,郭明,中国大百科全书,第三版网络版[DB/OL]
https://www.zgbk.com/ecph/words?SiteID=1&ID=120171&Type=bkzyb&SubID=115617
太阳光经过大气层时透过率较高的光谱波段。
[3] 2023-06-14,大气窗口/atmospheric window/方圣辉,中国大百科全书,第三版网络版[DB/OL]
https://www.zgbk.com/ecph/words?SiteID=1&ID=111847&Type=bkzyb&SubID=94760
电磁波通过大气层时较少被反射、吸收和散射的透过率高的波段。
[4] 2024-04-29,大气窗口/atmospheric window/戴礼云,胡斯勒图,中国大百科全书,第三版网络版[DB/OL]
https://www.zgbk.com/ecph/words?SiteID=1&ID=745994&Type=bkztb&SubID=1200
天体辐射中能穿透大气的一些波段。
[5] 2023-03-09,大气射电窗口/atmospheric radio window/钱志瀚,中国大百科全书,第三版网络版[DB/OL]
https://www.zgbk.com/ecph/words?SiteID=1&ID=557933&Type=bkzyb&SubID=227638
[6] 2023-10-19,大气特性/atmospheric characteristics/丁雷,陆燕,中国大百科全书,第三版网络版[DB/OL]
https://www.zgbk.com/ecph/words?SiteID=1&ID=569609&Type=bkzyb&SubID=237069
[7] Chapter 1, Introduction, 1.1 An Introduction to Radio Astronomy, Essential Radio Astronomy, James J. Condon and Scott M. Ransom
https://www.cv.nrao.edu/~sransom/web/Ch1.html
1.1.2 Atmospheric Windows
[8] NOAA, 2023-04-10, The Atmospheric Window
https://www.noaa.gov/jetstream/satellites/absorb
[9] Geoengineering.global, advancing the mitigation of Climate Change and Global Warming through Geoengineering education and research
https://geoengineering.global/solar-radiation-management/
[10] RADIO FREQUENCIES FOR SPACE COMMUNICATION, Australian Space Academy
https://www.spaceacademy.net.au/spacelink/radiospace.htm
[11] NASA Earthdata
https://www.earthdata.nasa.gov/
Your Gateway to NASA Earth Observation Data
The Earth Science Data Systems (ESDS) Program provides open access to NASA’s archive of Earth science data, empowering researchers and decision makers to better understand and protect our home planet.
相关链接:
[1] 2024-11-06,[图片,小资料] 地球大气密度、温度随高度的变化
https://blog.sciencenet.cn/blog-107667-1458901.html
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https://blog.sciencenet.cn/blog-107667-1452999.html
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https://blog.sciencenet.cn/blog-107667-1352999.html
[4] 2010-09-01,NASA的大气层照片显示大气的层次
https://blog.sciencenet.cn/blog-107667-358165.html
[5] 2023-09-20,[小资料] 我国近年风能、太阳能分布图
https://blog.sciencenet.cn/blog-107667-1403262.html
[6] 2021-08-15,感谢中国科学院《科学智慧火花》给贴出《高空机翼风筝发电设想》
https://blog.sciencenet.cn/blog-107667-1312669.html
https://idea.cas.cn/zhhh/gcjskxygjs/gcjskxygjs_nydlydljx/info/2021/521690.html
[7] 2022-12-03,往日(16):2015-05-25 的未来的两大安全能源
https://blog.sciencenet.cn/blog-107667-1366389.html
[8] 2022-09-06,[求助,备课,答疑] 关于“能源”的一些名词
https://blog.sciencenet.cn/blog-107667-1354217.html
[9] 2022-08-10,[第125.5个问题,大问题] 人类能源利用中降低“全球变暖”的方法有哪些?
https://blog.sciencenet.cn/blog-107667-1350689.html
[10] 2022-08-09,[大讨论] 人类消耗的能源最终都变成了什么?会不会直接加热大气?
https://blog.sciencenet.cn/blog-107667-1350584.html
[11] 2023-09-19,[小资料] 2012年~2022年我国原油进口来源及对外依存度
https://blog.sciencenet.cn/blog-107667-1403139.html
[12] 2022-07-08,[打听,科普] 为什么有些行星大气风向在不同纬度相反(木星、天王星、海王星)
https://blog.sciencenet.cn/blog-107667-1346438.html
[13] 2020-03-14,[请教] 叶笃正先生大气运动尺度观点的专业级解释
https://blog.sciencenet.cn/blog-107667-1223472.html
[14] 2018-08-12,我们的论文《基于季风和大气压分布的我国风电功率预测研究》刊出
https://blog.sciencenet.cn/blog-107667-1128808.html
[15] 2023-06-26,[笔记,思考] 反射太阳能给地球降温
https://blog.sciencenet.cn/blog-107667-1393089.html
[16] 2022-08-28,[讨论] 平流层反射太阳能,首选的“地球降温”方式?
https://blog.sciencenet.cn/blog-107667-1352999.html
[17] 2022-08-08,[大讨论] 给地球降温的各类奇思妙想
https://blog.sciencenet.cn/blog-107667-1350444.html
[18] 2024-09-16,[小资料,优先权] 天气终于凉快了(月球影响地球温度)
https://blog.sciencenet.cn/blog-107667-1451413.html
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