找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: Deep Impact Mission: Looking Beneath the Surface of a Cometary Nucleus; Christopher T. Russell Book 2005 Springer Science+Business Media B

[復(fù)制鏈接]
樓主: 駝峰
31#
發(fā)表于 2025-3-27 00:01:34 | 只看該作者
An Overview of the Instrument Suite for the Deep Impact Mission, crater formation for the Deep Impact mission. The high-resolution instrument (HRI) consists of an ./35 telescope with 10.5mfocal length, and a combined filtered CCD camera and IR spectrometer. The medium-resolution instrument (MRI) consists of an ./17.5 telescope with a 2.1 m focal length feeding a
32#
發(fā)表于 2025-3-27 01:28:01 | 只看該作者
33#
發(fā)表于 2025-3-27 08:00:42 | 只看該作者
The History and Dynamics of Comet 9P/Tempel 1,vations for the seven apparitions beginning in 1967 have been fit with an orbit that includes only radial and transverse nongravitational accelerations that model the rocket-like thrusting introduced by the outgassing of the cometary nucleus. The successful nongravitational acceleration model did no
34#
發(fā)表于 2025-3-27 09:36:15 | 只看該作者
,Deep Impact: Working Properties for the Target Nucleus — Comet 9P/Tempel 1,ttle was known about its physical properties. Efforts were immediately begun to improve this situation by the . Science Team leading to the founding of a worldwide observing campaign (Meech ., ., 2005a). This campaign has already produced a great deal of information on the global properties of the c
35#
發(fā)表于 2025-3-27 13:40:00 | 只看該作者
The Coma of Comet 9P/Tempel 1,ucleus as its component icy volatiles sublimate. Driven mainly by water ice sublimation at surface temperatures . > 200 K, this coma is a gravitationally unbound atmosphere in free adiabatic expansion. Near the nucleus (≤10. km), it is in collisional equilibrium, at larger distances (≥10. km) it is
36#
發(fā)表于 2025-3-27 18:02:48 | 只看該作者
37#
發(fā)表于 2025-3-28 00:47:33 | 只看該作者
38#
發(fā)表于 2025-3-28 05:47:08 | 只看該作者
Impact Cratering Theory and Modeling for the Deep Impact Mission: From Mission Planning to Data Anaegard to the impacting energy, target material, space environment, and extremely low-gravity field. Consequently, impact cratering theory and modeling play an important role in this mission, from initial inception to final data analysis. Experimentally derived impact cratering scaling laws provide u
39#
發(fā)表于 2025-3-28 08:48:53 | 只看該作者
The Deep Impact Earth-Based Campaign, an intensive world-wide observing campaign designed to obtain mission critical information about the target nucleus, including the nucleus size, albedo, rotation rate, rotation state, phase function, and the development of the dust and gas coma. The specific observing schemes used to obtain this in
40#
發(fā)表于 2025-3-28 11:36:07 | 只看該作者
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點(diǎn)評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-9 04:55
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
若尔盖县| 保德县| 聂荣县| 乃东县| 枣阳市| 万宁市| 崇阳县| 桐梓县| 屏东市| 如东县| 霍城县| 平南县| 望江县| 怀来县| 湘阴县| 浠水县| 鄱阳县| 马边| 小金县| 石城县| 枣强县| 昭通市| 民县| 武川县| 晋宁县| 固镇县| 平罗县| 安乡县| 玉林市| 察雅县| 会东县| 新沂市| 石河子市| 商水县| 金秀| 长垣县| 昌吉市| 建湖县| 嵊泗县| 普格县| 武隆县|