找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問(wèn)微社區(qū)

打印 上一主題 下一主題

Titlebook: Atmospheric Optics; Nikolai B. Divari (Chairman) Book 1970 Consultants Bureau, New York 1970 optics

[復(fù)制鏈接]
樓主: 可樂(lè)
11#
發(fā)表于 2025-3-23 11:42:59 | 只看該作者
The Height of the Twilight Ray,on of the sinking of the sun. This was first demonstrated by V. G. Fesenkov [1] and later examined in detail by N. M. Shtaude [2]. The thickness of the layer that determines the main flow of scattered radiation is not great, so in the first approximation the layer is often replaced by a single ray (
12#
發(fā)表于 2025-3-23 16:16:21 | 只看該作者
Evaluating the Dust Component of the Upper Atmosphere by the Twilight Method,ndard atmospheres, summarizing the results of studies of structure and composition, give densities, pressures, temperatures, molecular weights, and other structural parameters up to very high altitudes for a great variety of geophysical conditions: time of day, season, solar cycle, etc. Other atmosp
13#
發(fā)表于 2025-3-23 19:24:58 | 只看該作者
14#
發(fā)表于 2025-3-23 23:27:41 | 只看該作者
15#
發(fā)表于 2025-3-24 03:10:15 | 只看該作者
16#
發(fā)表于 2025-3-24 07:03:43 | 只看該作者
Funktionen von mehreren Ver?nderlichenOptical instability of the earth’s atmosphere impairs the quality of photographs of astronomical objects. One method of improving image quality is to photograph during periods of relative atmospheric quiet.
17#
發(fā)表于 2025-3-24 13:11:10 | 只看該作者
https://doi.org/10.1007/978-3-0348-4119-1Studies of atmospheric transmittance and scattered-light intensity make it possible to establish relationships among certain optical parameters. These relationships can then be used in solving a number of applied problems.
18#
發(fā)表于 2025-3-24 15:23:54 | 只看該作者
https://doi.org/10.1007/978-3-8348-2340-3The brightness of the sky on the solar almucantar is chiefly determined by the following parameters [1, 2]: the solar zenith distance z., the optical thickness of the atmosphere .. and the albedo of the underlying surface q, and it is greatly dependent upon the form of the scattering indicatrix.
19#
發(fā)表于 2025-3-24 21:11:47 | 只看該作者
Konstruktion analytischer Funktionen,Twilight phenomena are very complex, since the brightness observed at any point in the sky is the sum of the brightnesses of the primary twilight segment and of higher-order scattering, to which, when the sun has sunk sufficiently below the horizon, we must add the background of the night sky — primarily zodiacal light.
20#
發(fā)表于 2025-3-24 23:49:53 | 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(ài)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(píng) 投稿經(jīng)驗(yàn)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(guó)際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-15 05:06
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
昭苏县| 安远县| 信丰县| 洛南县| 枣庄市| 新河县| 泾阳县| 唐河县| 虹口区| 绵竹市| 延川县| 阳高县| 绍兴市| 蒙自县| 嘉峪关市| 星子县| 宁明县| 噶尔县| 平远县| 山东| 金寨县| 云梦县| 博野县| 临江市| 广东省| 张掖市| 合阳县| 郴州市| 开原市| 长葛市| 郓城县| 招远市| 炎陵县| 霍山县| 子长县| 辰溪县| 万载县| 宜丰县| 灵丘县| 白水县| 闵行区|