Venus Express(金星快車)到底是什麼？
Venus Express 金星快車 - This circumstance led to a long standstill for further space programs to Venus after the first space-based explorations of this planet in the 1970s through the mid-1990s, which was not broken until the launch of ESA's Venus Express (VEX) mission in 2005. [1] These neurons were spatially clustered, exhibited intermittently repeated dVenus expression, and often continued to express Arc-dVenus for approximately two weeks. [2] Experiments involving the radio sounding of solar plasma with signals from the Venus Express and Mars Express spacecraft, which were carried out from October 6 to December 6, 2006, provided data on frequency fluctuations of the radio signals for the western and eastern coronal limbs. [3] In hypothalamic organotypic cultures from the AVP-Venus mice, Venus-labeled AVP neurons in the supraoptic and paraventricular nuclei survived for 1 month, and Venus expression was upregulated by forskolin. [4] The selected CME eruption occurred on the 6th of January 2013 and was encountered by two spacecraft, Venus Express and STEREO--A, which were radially aligned at the time of the CME passage. [5] We will present here several comparisons of the upper atmosphere of Venus between our model results and a selection of aerobraking data from different missions such as Venus Express, Pioneer Venus and Magellan. [6] We focus on an eruption from 6 January 2013 encountered by two radially aligned spacecraft, Venus Express and STEREO-A. [7] We focus on the validation of the model built from a collection of data mostly from Venus Express (2006-2014) experiments and coordinated ground-based telescope campaigns, in the upper mesosphere/lower thermosphere of Venus (80-150 km). [8] Following the co-injection of the piwil1-Venus expression vector and the Tol2 transposase mRNA into fertilized eggs, presumptive transgenic fish were reared. [9] From the early flyby transit of the Mariner 5 spacecraft to the later orbit crossings of the Venera 10, the Pioneer Venus and more recently the Venus Express there has been accumulated evidence of the presence of that transition by the flanks of the Venus wake. [10] We investigate the heavy ion density and velocity in the Venusian upper ionosphere near the North Pole, using the Ion Mass Analyzer, a part of the Analyzer of Space Plasmas and Energetic Atoms 4, together with the magnetic field instruments on Venus Express. [11] In adulthood, however, there was a significant female predominance in the number of Venus expressing neurons in two subnuclei of the dorsolateral BNST, i. [12] Using data from the MESSENGER, Venus Express and ACE spacecraft, we analyze with the superposed epoch technique the profiles of ICME substructures, namely the sheath and the magnetic ejecta. [13] Finally, there is a good agreement between the TEXES results and those obtained in the UV range (SPICAV/Venus Express and UVI/Akatsuki) at a slightly higher altitude. [14] Moreover, ovariectomy resulted in the absence of OXTR-Venus expression in the AVPV, whereas estrogen replacement therapy restored OXTR-Venus expression. [15] In this work, we present a comprehensive catalog of 47 CMEs measured in situ measurements by two or more radially aligned spacecraft (MESSENGER, Venus Express, STEREO or Wind/ACE). [16] 1-μm emissivity was derived using Venus Monitoring Camera (VMC) measurements on board of Venus Express (VEx). [17] We conducted a test with ESA's Venus Express (VEX), to evaluate the performance of the PRIDE technique for this particular application. [18] The atmospheric composition has been studied to some extent with the Pioneer Venus Orbiter mission and the more recent Venus Express, however, the concentration of many species and their isotopic ratios are not yet known with satisfying accuracy. [19] The application of PRIDE for atmospheric studies has been demonstrated by observing ESA's Venus Express (VEX) during multiple Venus occultation events (Bocanegra-Bahamon et al. [20]這種情況導致在 1970 年代至 1990 年代中期對金星進行首次太空探索之後，進一步的金星太空計劃長期停滯不前，直到 2005 年歐空局的金星快車 (VEX) 任務發射才被打破。 [1] 這些神經元在空間上聚集，表現出間歇性重複的 dVenus 表達，並且經常持續表達 Arc-dVenus 大約兩週。 [2] 2006 年 10 月 6 日至 12 月 6 日進行的利用金星快車和火星快車信號對太陽等離子體進行無線電探測的實驗提供了西部和東部日冕肢無線電信號頻率波動的數據。 [3] 在來自 AVP-Venus 小鼠的下丘腦器官培養物中，Venus 標記的視上核和室旁核中的 AVP 神經元存活了 1 個月，並且維納斯表達被毛喉素上調。 [4] 選定的 CME 噴發發生在 2013 年 1 月 6 日，兩艘航天器 Venus Express 和 STEREO--A 在 CME 通過時呈放射狀排列。 [5] </span><span> 我們將在此展示我們的模型結果與來自不同任務（如金星快車、先鋒金星和麥哲倫）的航空制動數據之間的金星高層大氣的幾項比較。 [6] 我們專注於 2013 年 1 月 6 日發生的一次噴發，由兩個徑向對齊的航天器 Venus Express 和 STEREO-A 遭遇。 [7] 我們專注於驗證模型的驗證，該模型主要來自金星快車（2006-2014）實驗和協調的地面望遠鏡活動，在金星上層中間層/下層熱層（80-150 公里）。 [8] 在將 piwil1-Venus 表達載體和 Tol2 轉座酶 mRNA 共同註射到受精卵中後，飼養了假定的轉基因魚。 [9] 從早期的水手 5 號航天器飛越到後來的金星 10 號、先鋒金星和最近的金星快車的軌道穿越，已經積累了金星尾跡兩側存在這種過渡的證據。 [10] 我們使用離子質量分析儀（空間等離子體和高能原子 4 分析儀的一部分）與金星快車上的磁場儀器一起研究北極附近金星上層電離層中的重離子密度和速度。 [11] 然而，在成年期，在背外側 BNST 的兩個亞核中表達金星的神經元數量顯著女性佔優勢，即。 [12] 利用來自信使號、金星快車和 ACE 航天器的數據，我們使用疊加時代技術分析了 ICME 子結構的輪廓，即鞘層和磁性噴射物。 [13] 最後，TEXES 結果與在稍高海拔的 UV 範圍（SPICAV/Venus Express 和 UVI/Akatsuki）中獲得的結果有很好的一致性。 [14] 此外，卵巢切除術導致 AVPV 中沒有 OXTR-Venus 表達，而雌激素替代療法恢復了 OXTR-Venus 表達。 [15] 在這項工作中，我們提供了由兩個或更多徑向對齊的航天器（信使、金星快車、立體聲或 Wind/ACE）現場測量的 47 個 CME 的綜合目錄。 [16] 使用 Venus Express (VEx) 上的 Venus Monitoring Camera (VMC) 測量得出 1-μm 發射率。 [17] 我們使用 ESA 的 Venus Express (VEX) 進行了測試，以評估 PRIDE 技術在此特定應用中的性能。 [18] 先鋒金星軌道飛行器任務和最近的金星快車已經在一定程度上研究了大氣成分，但是，許多物種的濃度及其同位素比尚不能令人滿意的準確度。 [19] 通過在多次金星掩星事件期間觀察歐空局的金星快車 (VEX) 證明了 PRIDE 在大氣研究中的應用（Bocanegra-Bahamon 等人。 [20]
Onboard Venus Express
We test our automatic procedure by applying it to the magnetic field data measured by the FGM onboard Venus Express. [1] More concretely, the Venus Monitoring Camera (VMC) onboard Venus Express orbiter provided the largest and the longest so far set of ultraviolet (UV), visible and near-IR images for investigation of the atmospheric circulation. [2]我們通過將其應用於由 FGM 機載 Venus Express 測量的磁場數據來測試我們的自動程序。 [1] 更具體地說，金星快車軌道器上的金星監測攝像機 (VMC) 提供了迄今為止最大和最長的一組紫外線 (UV)、可見光和近紅外圖像，用於研究大氣環流。 [2]
venus express radio
The Venus Express radio science experiment VeRa provided more than 900 neutral atmospheric profiles between the years 2006 and 2014. [1] Here we validate the current version of the Institut Pierre Simon Laplace (IPSL) Venus GCM, by means of a comparison between the modelled temperature field and that obtained from data by the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) and the Venus Express Radio Science Experiment (VeRa) onboard Venus Express. [2]Venus Express 無線電科學實驗 VeRa 在 2006 年至 2014 年間提供了 900 多個中性大氣剖面。 [1] 在這裡，我們通過比較模擬的溫度場與從可見和紅外熱成像光譜儀 (VIRTIS) 和 Venus Express Radio Science 的數據獲得的溫度場，驗證了 Institut Pierre Simon Laplace (IPSL) Venus GCM 的當前版本Venus Express 上的實驗 (VeRa)。 [2]
venus express spacecraft
The measurements from the Venus Express spacecraft are analyzed for the basic properties of fast forward interplanetary shocks at Venus’s orbit (∼0. [1] Winds derived by a digital tracking technique from UV (365 nm) images captured by the Venus Monitoring Camera onboard the Venus Express spacecraft from 2006 through 2013 were used to study the atmospheric circulation at cloud top level (70±2 km). [2]對金星快車的測量結果進行了分析，以了解金星軌道上快進行星際衝擊的基本特性（~0. [1] 通過數字跟踪技術從 2006 年至 2013 年金星快車上的金星監測相機拍攝的紫外（365 nm）圖像中獲得的風被用於研究雲層頂層（70±2 公里）的大氣環流。 [2]
venus express visible 金星快車可見
Guided by the remarkably consistent morphological appearance of this feature, we have identified at least one previous instance of it in the Venus Express Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) data. [1] In 2010 the ESA Venus Express Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) instrument first observed 1 μm emissivity anomalies over the top and eastern flank of Idunn Mons (46° S; 146° W), a 200 km wide volcano located in Imdr Regio, a volcano-dominated large volcanic rise of Venus. [2]在這一特徵非常一致的形態外觀的指導下，我們在 Venus Express 可見光和紅外熱成像光譜儀 (VIRTIS) 數據中至少發現了一個先前的實例。 [1] 2010 年，歐空局金星快車可見光和紅外熱成像光譜儀 (VIRTIS) 儀器首次在位於 Imdr Regio 的一座 200 公里寬的火山 Idunn Mons（南緯 46°；西經 146°）的頂部和東側觀測到 1 μm 發射率異常，以火山為主的金星大型火山上升。 [2]
venus express observation 金星快車觀測
Latitudinal variations of mode mixtures as interpreted by the M3L coordinates were compared with those in the Venus Express observation-based studies. [1] Here we study the well-structured Venusian IMB with a sudden magnetic field rotation and a sharp magnetosheath plasma decrease using Venus Express observations. [2]將 M3L 坐標解釋的模式混合的緯度變化與 Venus Express 基於觀測的研究中的那些進行了比較。 [1] 在這裡，我們使用 Venus Express 觀測研究了結構良好的金星 IMB，它具有突然的磁場旋轉和急劇的磁鞘等離子體減少。 [2]
venus express space 金星快車空間
We present the detection and characterisation of mesoscale waves on the lower clouds of Venus using images from the Visible Infrared Thermal Imaging Spectrometer (VIRTIS-M) onboard the European Venus Express space mission and from the 2 μm camera (IR2) instrument onboard the Japanese space mission Akatsuki. [1] Our results are consistent with the observation of Venus Express space probe. [2]我們使用來自歐洲金星快車太空任務上的可見紅外熱成像光譜儀 (VIRTIS-M) 和日本太空上的 2 μm 相機 (IR2) 儀器的圖像，展示了金星低層雲中中尺度波的檢測和表徵任務曉。 [1] 我們的結果與金星快車太空探測器的觀測結果一致。 [2]