Space weather implications of the 20 January 2005 solar energetic particle event.

空間天氣的影響2005年1月20太陽高能粒子事件天堂AV天堂。

In principle, it is feasible to detect energetic particle beams used in flash perspectivity directly by CCD.

從原理上看日韩高清无码性爱视频，利用CCD來直接探測用于閃光透視的高能粒子束是可行的狼人av在线。

According to physical properties of semiconductor devices, the CCD with proper depletion layer is probable to be used for energetic particle detectors of high sensitivity.

根據(jù)半導(dǎo)體器件的物理性質(zhì)欧日黄片，擁有適當(dāng)耗盡層區(qū)間的CCD器件有可能成為高度敏感的高能粒子探測器。

A sufficiently energetic particle can penetrate the entire stack of parallel plates .

能量充足的粒子能夠穿透全部平行板国产精品不卡一区。

The Space Environment Monitor consists of three instrument groups: 1 an energetic particle sensor package, 2 two magnetometer sensors, and 3 a solar x-ray sensor.

空間環(huán)境監(jiān)測包括三個監(jiān)控器： 1 ）一個高能粒子傳感器封裝爱福利视频广场一区二区， 2 ）兩個磁力感應(yīng)器， 3 ）太陽X射線傳感器美女视频色网站国产。

We had also performed numerical simulations to study energetic particle injection at L=3.5 to discuss the effect of different pulse parameters on particle injection.

我們也完成在 L=3.5 的電子流量模擬av高速在线网站，討論不同的脈沖參數(shù)對於粒子傳輸?shù)挠绊懞碗姶琶}沖傳輸粒子至該處的可能性，以了解是否此電磁脈沖模型可應(yīng)用於了解磁暴時特级婬片欧美国语高清视频一，在 L=3.5 處高能粒子流量增加的可能性免费A片一区二区三区视频。

Energetic particle deposition is one kind of thin film synthesis technique based on energetic beam, such as, IBAD, PLD, IBD etc, which is considered to be of good prospect for wide range of applications. However, comprehensive and systematic understanding has been hardly achieved about the growth mechanism of energetic deposition, especially low energetic deposition.

載能粒子沉積是以離子束技術(shù)和常規(guī)薄膜制備技術(shù)為基礎(chǔ)而發(fā)展起來的一類具有廣泛應(yīng)用前景的薄膜制備方法，但受研究手段的限制五月婷婷久久久，人們對載能粒子特別是低能粒子沉積的薄膜生長機(jī)制一直缺乏比較全面亚洲又黄的A片、系統(tǒng)的了解。

The energetic light from these stars continually ionizes nebula gas, while their energetic particle wind blows bubbles and defines intricate filaments.

來自這些恒星的高能光不斷離子化星云氣體YouJizz丰满熟妇短视频，而它們的高能粒子風(fēng)同時不斷地吹向泡泡免费的黄黄网站，產(chǎn)生了錯綜復(fù)雜的細(xì)絲景象。

By comparing and analyzing the solar and interplanetary data of two typical fast halo Coronal Mass Ejections, we have found that the event far away from Coronal Holes caused a great Solar Energetic Particle event, but the event very close to CHs did not cause a major SEP event.

通過對比兩次快速暈狀日冕物質(zhì)拋射事件人人操人人尻，分析相應(yīng)的日面和行星際的觀測資料黄页网站网址在线观看，發(fā)現(xiàn)源區(qū)距離冕洞較遠(yuǎn)的CME引起了極強的太陽高能粒子(Solar Energetic Particle，SEP)事件91一级片观看，而源區(qū)非彻客嘁患禷片免费视频？拷岫吹腃ME則沒有引起大的SEP事件。

The influences of the shock thickness and Alfven waves on the particle acceleration by diffusive shock waves are numerically studied through solving one-dimensional diffusive equation including the second-order Fermi effect. It is shown that the spectral index of the energetic particles strongly depends on the shock thickness. For example, the spectral index increases from 2.1 to 3.7 in the low energy range of 3-10 MeV and from 2.5 to 5.0 in the high energy range of 20-60 MeV as the thickness increases. The spectral index decreases from 4.3 to 3.1 as the particle injection energy increases. The spectral index decreases from 4.0 to 1.8 at the quasi-steady stage with the enhancement of the compression ratio from 2 to 4. The results indicate that under the influence of Alfven waves, the energetic particle spectrum at lower energy becomes flat and the spectral index decreases from 2.5 to 0.6 in the low energy range of 3-10 MeV and from 11.6 to 5.0 in the high energy range of 20-60 MeV. At the same time, the rollover energy reaches 19.6 MeV. The spectral index decreases from 5.8 to 2.9 as the energy density of Alfven waves increase. All these results are basically consistent with the theoretical models, as well as the observations of typical energetic particle events.

通過數(shù)值求解包含二階費米加速的一維擴(kuò)散方程日韩视频在线免费播放，探討在準(zhǔn)平行激波條件下激波厚度和級聯(lián)阿爾芬波對粒子加速的影響，研究粒子分布函數(shù)的演化與激波厚度和阿爾芬波強度的內(nèi)稟關(guān)系國產黃噴潮在線觀看，計算結(jié)果表明：(1)考慮激波厚度時操亚洲无码视频，譜指數(shù)明顯依賴于激波厚度，隨著厚度從0.32增大到2.56国产盗摄无遮挡裸体视频，低能端(3-10MeV)譜指數(shù)逐漸從2.1增加到3.7嘿咻嘿咻无码免费视频，高能端(20-60MeV)譜指數(shù)從2.4增大到5.0久久av中文字幕免费在线观看，能譜逐漸變軟；當(dāng)初始注入粒子動量增大1.3倍欧美18一19sex性外，質(zhì)子能譜指數(shù)從4.3減小到3.1一级axi视频免费，且與零厚度激波加速的譜指數(shù)差值縮小cao免费在线视频官网；厚度不變時欧美精品哟哟，隨著壓縮比從2增加到4，準(zhǔn)穩(wěn)態(tài)分布時低能端(3-10MeV)粒子能譜指數(shù)逐漸從4.0減小到1.8譜變硬国产三级片自拍；(2)在級聯(lián)阿爾芬波的影響下91网站最新网址，隨著時間的增大，粒子在低能處(3-10MeV)的譜指數(shù)從2.5減小到0.6高能端(20-60MeV)譜指數(shù)從11.6減小到5.0日韩一级特黄大片本道，能譜變硬在线免费观看日本y码视频网站，拐點能量值從7.5MeV增大到為19.6MeV；隨著波的能量密度增大国产高清一级黄色网站，譜指數(shù)從5.8減小到2.9国产综合调教视频高清在线播放，這表明阿爾芬波強度越大，加速效率越高男女性爱一级生活黄色视频中文字幕国语，通過與激波厚度解析結(jié)果和高能粒子事件的觀測能譜比較發(fā)現(xiàn)兩者是一致的4455vw永久在线，說明數(shù)值模擬結(jié)果是可靠的。