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Titlebook: Solar Electromagnetic Radiation Study for Solar Cycle 22; Proceedings of the S J. M. Pap,C. Fr?hlich,R. K. Ulrich Conference proceedings 19

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發(fā)表于 2025-3-21 19:52:18 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Solar Electromagnetic Radiation Study for Solar Cycle 22
副標(biāo)題Proceedings of the S
編輯J. M. Pap,C. Fr?hlich,R. K. Ulrich
視頻videohttp://file.papertrans.cn/872/871360/871360.mp4
圖書(shū)封面Titlebook: Solar Electromagnetic Radiation Study for Solar Cycle 22; Proceedings of the S J. M. Pap,C. Fr?hlich,R. K. Ulrich Conference proceedings 19
描述Measurements of solar irradiance, both bolometric and atvarious wavelengths, over the last two decades have establishedconclusively that the solar energy flux varies on a wide range of timescales, from minutes to the 11-year solar cycle. The major question ishow the solar variability influences the terrestrial climate. .The .Solar Electromagnetic Radiation Study for Solar Cycle 22.(SOLERS22) is an international research program operating under theauspices of the Solar-Terrestrial Energy Program (STEP) WorkingGroup 1: `The Sun as a Source of Energy and Disturbances‘. STEP issponsored by the Scientific Committee of Solar-TerrestrialPhysics (SCOSTEP) of the International Council of Scientific Unions(ICSU). .The main goal of the SOLERS22 1996 Workshop was to bring theinternational research community together to review the most recentresults obtained from observations, theoretical interpretation,empirical and physical models of the variations in the solar energyflux and their possible impact on climate studies. These questions areessential for researchers and graduate students insolar-terrestrial physics.
出版日期Conference proceedings 1998
關(guān)鍵詞Corona; Orbit; Scale; Solar flare; Solar wind; Sun; Sunspot; Wind; solar
版次1
doihttps://doi.org/10.1007/978-94-011-5000-2
isbn_softcover978-94-010-6099-8
isbn_ebook978-94-011-5000-2
copyrightSpringer Science+Business Media Dordrecht 1998
The information of publication is updating

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,GOME Solar UV/VIS Irradiance Measurements Between 1995 and 1997 — First Results on Proxy Solar Actiservations on Nimbus-7 and covers solar cycles 21 and 22. This paper briefly describes the GOME spectrometer and measurement mode which are relevant to the solar viewing. Preliminary results from the solar irradiance measurements between 1995 and 1997 and comparisons to SSBUV-8 (Shuttle SBUV) in Jan
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Solar UV Activity at Solar Cycle 21 and 22 Minimum from NOAA-9 SBUV/2 Data,riability. Comparisons with contemporaneous data from Nimbus-7 SBUV (1985–1986) and UARS SUSIM (1994–1995) are used to validate the results obtained from the NOAA-9 data. Current short-term UV activity differs from the cycle 21–22 minimum. Continuous 13-day periodicity was observed from September 19
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發(fā)表于 2025-3-22 22:11:46 | 只看該作者
Comparisons of the NOAA-11 SBUV/2, UARS SOLSTICE, and UARS SUSIM Mg II Solar Activity Proxy Indexesespect to both the absolute value and temporal variations of the Mg II index. Periodograms of the three indexes demonstrate comparable solar variation tracking. Between October 1991 and October 1994 predominate power occurs near 27 days, with secondary maxima in the power spectra near 29 and 25 days
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發(fā)表于 2025-3-23 05:22:08 | 只看該作者
Solar Extreme Ultraviolet Irradiance Measurements During Solar Cycle 22,nt of the solar EUV irradiance, because these instruments are calibrated at the National Institute of Standards and Technology (NIST) with a radiometric uncertainty of about 8%. These more accurate sounding-rocket measurements suggest revisions of the previous reference AE-E spectra by as much as a
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