標(biāo)題: Titlebook: Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere; Eric Quémerais,Martin Snow,Roger-Maurice Bonnet Book 2013 [打印本頁] 作者: 搖尾乞憐 時(shí)間: 2025-3-21 16:24
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere影響因子(影響力)
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere影響因子(影響力)學(xué)科排名
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere網(wǎng)絡(luò)公開度
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere被引頻次
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere被引頻次學(xué)科排名
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere年度引用
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere年度引用學(xué)科排名
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere讀者反饋
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere讀者反饋學(xué)科排名
作者: Extemporize 時(shí)間: 2025-3-21 23:42
ISSI Scientific Report Serieshttp://image.papertrans.cn/d/image/240271.jpg作者: Detoxification 時(shí)間: 2025-3-22 03:53
Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere978-1-4614-6384-9Series ISSN 2946-1278 Series E-ISSN 2946-1286 作者: 用樹皮 時(shí)間: 2025-3-22 07:59
Theoretical Foundations of the Welfare State accuracy that can be achieved, and review the different sources of emissions that can be used in that range, i.e. the interplanetary background, stars, and solar system bodies such as planets, moons, and comets. As most of the work presented here is based on comparisons with older datasets obtained作者: 動(dòng)脈 時(shí)間: 2025-3-22 10:57
Summarized Findings and Conclusionhe atoms penetrate through the region of the solar wind (SW) interaction with the local interstellar medium (LISM). In the interaction region the atoms can exchange charge with both solar wind and interstellar protons disturbed in the SW/LISM interaction region. Charge exchange results in a disturba作者: 簡潔 時(shí)間: 2025-3-22 16:14 作者: 簡潔 時(shí)間: 2025-3-22 19:34 作者: 發(fā)起 時(shí)間: 2025-3-23 01:08
Beschreibung deutscher Unternehmen in China,planetary Lyman-. data obtained in 2009–2011 on the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft mission, daily all-sky Lyman-. maps were generated for use by the Lunar Reconnaissance Orbiter (LRO) LAMP Lyman-Alpha Mapping Project (LAMP) experiment. These mode作者: Abominate 時(shí)間: 2025-3-23 04:14
Beschreibung deutscher Unternehmen in China,olet spectrograph on the New Horizons spacecraft (the first new such data from outside the orbit of Saturn since the Voyager spacecraft). The observations consist of 6. ×360. great-circle swaths on the sky, centered on the ecliptic direction λ = 51. 3., . = 44. 8., which passes within ～ 33. of the u作者: 聽寫 時(shí)間: 2025-3-23 05:35
,Auff?lligkeiten in H?ufigkeitsverteilungen, the ultraviolet (115–300 nm). Prior to launch, it was calibrated at the SURF-III synchrotron. Spectra from the International Ultraviolet Explorer (IUE) corrected to the white dwarf flux scale are in good agreement with SOLSTICE observations, validating the two completely independent methods of cali作者: 策略 時(shí)間: 2025-3-23 12:03
,Auff?lligkeiten in H?ufigkeitsverteilungen,majority of the previous work on characterizing the lunar reflectance has been in the visible part of the spectrum using ground-based lunar images. The SOLar-STellar Irradiance Comparison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) can be used to extend the lunar spec作者: 皮薩 時(shí)間: 2025-3-23 17:00
Begriff der Wahrscheinlichkeit,ison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) both made observations of comet 17P/Holmes at Lyman-α wavelengths. The intent of these observations was to compare the calibration of SWAN and SOLSTICE, rather than to study the properties of comets. The two datasets re作者: epidermis 時(shí)間: 2025-3-23 19:10
https://doi.org/10.1007/978-1-4614-6384-9Lyman-alpha Comet Holmes; Lyman-alpha Models; Modeling Interplanetary Background; Moon Irradiance; UV Sp作者: Defraud 時(shí)間: 2025-3-24 01:21 作者: 輕彈 時(shí)間: 2025-3-24 03:14 作者: gout109 時(shí)間: 2025-3-24 08:22
Theoretical Foundations of the Welfare Stated by the two ultraviolet (UV) spectrometers on Voyager 1 and Voyager 2 with models and other more recent datasets shows that it is indeed necessary to derive new calibration factors for these two instruments.作者: FLAX 時(shí)間: 2025-3-24 12:50 作者: 無可非議 時(shí)間: 2025-3-24 18:12
,Auff?lligkeiten in H?ufigkeitsverteilungen,llar observations. Since only a handful of stars in the IUE archive have been converted to the white dwarf scale and many of them are relatively faint, the SOLSTICE catalog of bright stars can be an extremely useful resource for inflight calibration of ultraviolet spectrographs.作者: 善辯 時(shí)間: 2025-3-24 20:03 作者: 種族被根除 時(shí)間: 2025-3-25 00:59
New Horizons Cruise Observations of Lyman-, Emissions from the Interplanetary Mediuml simulations, although the brightness of interplanetary Lyman-. emissions falls off more slowly than expected with radial distance from the Sun. The ratio of Lyman-./Lyman-. brightnesses in the interplanetary medium agrees well with previous measurements by the Voyager ultraviolet spectrometers.作者: 節(jié)約 時(shí)間: 2025-3-25 06:05 作者: 碎片 時(shí)間: 2025-3-25 10:02 作者: auxiliary 時(shí)間: 2025-3-25 14:14
Thirty Years of Interplanetary Background Data: A Global Viewion factors derived here are significantly different from the values published by Hall (Ultraviolet resonance radiation and the structure of the heliosphere. Dissertation, University of Arizona, 1992).作者: obsession 時(shí)間: 2025-3-25 16:48
Lyman-α Observations of Comet Holmes from SORCE SOLSTICE and SOHO SWANquire significant processing to remove interplanetary and geocoronal backgrounds which increased the uncertainty of the result. However, both instruments measured similar Lyman-α irradiances, confirming their calibration agreement.作者: 青春期 時(shí)間: 2025-3-25 20:03 作者: FATAL 時(shí)間: 2025-3-26 03:02 作者: Eeg332 時(shí)間: 2025-3-26 06:47 作者: Binge-Drinking 時(shí)間: 2025-3-26 09:17
Distribution of Interstellar Hydrogen Atoms in the Heliosphere and Backscattered Solar Lyman-αhe atoms penetrate through the region of the solar wind (SW) interaction with the local interstellar medium (LISM). In the interaction region the atoms can exchange charge with both solar wind and interstellar protons disturbed in the SW/LISM interaction region. Charge exchange results in a disturba作者: 糾纏,纏繞 時(shí)間: 2025-3-26 14:21
Solar Parameters for Modeling the Interplanetary Backgroundn Bern, Switzerland was to establish a photometric cross-calibration of various UV and extreme ultraviolet (EUV) heliospheric observations. Realization of this goal required a credible and up-to-date model of the spatial distribution of neutral interstellar hydrogen in the heliosphere, and to that e作者: 遺忘 時(shí)間: 2025-3-26 18:39 作者: 財(cái)產(chǎn) 時(shí)間: 2025-3-26 23:14 作者: Coeval 時(shí)間: 2025-3-27 02:44 作者: Figate 時(shí)間: 2025-3-27 08:28 作者: Radiation 時(shí)間: 2025-3-27 10:04
Absolute Ultraviolet Irradiance of the Moon from the LASP Lunar Albedo Measurement and Analysis frommajority of the previous work on characterizing the lunar reflectance has been in the visible part of the spectrum using ground-based lunar images. The SOLar-STellar Irradiance Comparison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) can be used to extend the lunar spec作者: Conflagration 時(shí)間: 2025-3-27 13:38
Lyman-α Observations of Comet Holmes from SORCE SOLSTICE and SOHO SWANison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) both made observations of comet 17P/Holmes at Lyman-α wavelengths. The intent of these observations was to compare the calibration of SWAN and SOLSTICE, rather than to study the properties of comets. The two datasets re作者: MUTE 時(shí)間: 2025-3-27 21:13
Book 2013ackground is presented as well. This work also includes comparisons of older datasets with current ones.? This raises the question of the consistency of the existing datasets. Previous experiments have been calibrated independently and comparison of the datasets may lead to inconsistencies. The auth作者: 放牧 時(shí)間: 2025-3-28 01:40 作者: Macronutrients 時(shí)間: 2025-3-28 05:52 作者: Homocystinuria 時(shí)間: 2025-3-28 08:34
Lyman-, Models for LRO LAMP from MESSENGER MASCS and SOHO SWAN Data represents a failure of the model or a decline in sensitivity in SWAN in 2010 and 2011. MESSENGER MASCS and SOHO SWAN Lyman-. calibrations systematically differ in comparison with the model, with MASCS reporting Lyman-. values some 30 % lower than SWAN.作者: Modify 時(shí)間: 2025-3-28 12:46 作者: Gnrh670 時(shí)間: 2025-3-28 16:25 作者: 大漩渦 時(shí)間: 2025-3-28 19:03 作者: conspicuous 時(shí)間: 2025-3-28 23:55 作者: 反應(yīng) 時(shí)間: 2025-3-29 06:12 作者: 一再遛 時(shí)間: 2025-3-29 08:46 作者: 我沒有命令 時(shí)間: 2025-3-29 13:00 作者: 突襲 時(shí)間: 2025-3-29 16:06
https://doi.org/10.1007/978-3-642-66997-2 zu erforschen, welche die Kosten eines Betriebes bestimmen (Kosteneinflu?gr??en), und die Zusammenh?nge, welche zwischen diesen Gr??en und der H?he der Kosten bestehen, zu ergründen und zu erkl?ren. In diesem Sinne ist die vorliegende Arbeit eine kostentheoretische Untersuchung.
