红外辐射

Active galactic nuclei activity in the form of expression in:(1) intense light changes, that is, optical and radio radiation intensity over time, there are Big changes;(2) is very strong luminosity, even more than the Eddington luminosity;(3) significant non-thermal radiation, especially in the infrared region of the non-thermal radiation reached the maximum;(4) a strong movement and a huge gas jet stream.

活动星系核活动的形式表现在：（1）剧烈光变，即光学和射电辐射强度随时间有很大变化；（2）非常强的光度，甚至超过爱丁顿光度；（3）巨大的非热辐射，尤其在红外区的非热辐射达到最大；（4）强烈的气体运动和规模巨大的喷流。

At its core Electrophysics is an engineering company with multi-disciplinary expertise in advanced infrared sensor signal processing, calibration techniques, radiometry, optics, embedded software development, PC application software development, industrial and mechanical design and production tooling.

美国Electrophysics 公司是世界先进的高性能红外相机、便携式测温系统和夜视图像解决方案的开发生产商。另外，该公司还研究图像获取、软件分析以及一系列应用程序所需的特殊附件。Electrophysics 所拥有的技术专家们可以随时帮您解决各方面的问题，尤其精通于红外传感器信号处理、校准技术、辐射线测定、光学、嵌入式软件开发、PC应用软件开发和机械设计等等。

Firstly, the infrared optical system was usually designed to large-sized relative aperture system by reason of the target detected by the system was far, and weak radiant energy. However, the infrared image was suffered from geometric distortions due to wide-angle design of the infrared optical system.

为了获得更多的辐射能量，红外光学系统一般设计为大相对口径系统，这就不可避免的造成光学上像差校正的困难，进而导致红外图像的几何畸变。

Based on the requirement of"infrared image decoy composition"and"infrared hide star shell composition", experiment research and numerical simulation of Mg/PTFE infrared pyrotechnic composition combustion radiation character is studied in this paper.

本文结合"红外成像诱饵剂"及"红外隐身照明剂"课题，对Mg／PTFE红外烟火剂燃烧辐射特性进行了实验研究与数值模拟。

So it is urgent to find a method todetect underground pipeline and its branches conveniently. In order to solve the above problem, based on the fact that the heated petroleumradiates heat to the soil and then the especial temperature distribution will be formedon the ground, this paper reach out a method creatively using the infrared imaging todetect the underground pipeline.

本文的研究内容正是从这一实际需求出发，根据石油在管道中传输时因加热而向周围土壤辐射红外能量，进而在管道上方地表形成特殊的温场分布的特点，创造性地提出了用红外热成像技术来检测埋地输油管道方法，并重点完成了几下几方面工作。

In this study, we reported the detailed gating scheme, a gating module and the status of end-station of infrared microspectroscopy. Utilizing both noise eliminating system and technique of synchrotron-radiation-based FT-IR, we successfully acquired subsequently spectra and spectral images.

在本文中将详细说明此逻辑闸模组机制与红外显微光谱实验站之现况，经由此逻辑闸模组控制和同步辐射傅立叶转换红外显微技术，不但可提供量测样品於中红外光区的分子振动吸收光谱，更可利用样品中不同成分物种之特徵吸收，以建立红外光谱影像。

Because the photospheric temperature of carbon stars are less than 3000K and the temperature of rich-dust envelope formed by the mass loss is lower, and therefore most of the energy from carbon stars are radiated between 1 to 60um range, in which the vibrational and ro-vibrational bands of many molecules also lies, the study of infrared spectra in this wavelength range is very important to reveal chemical compositions, dust formation process, the atmospheric structure and evolutionary status of stars.

碳星光球的有效温度不超过3000K，同时较大的质量损失率形成了富碳的尘埃壳层，以致于它的辐射能量主要集中在1—60μm的红外波段上，并且许多分子的转动振动能谱也集中在红外，因此在红外波段的研究对揭示碳星化学成份及其分布、尘埃形成过程、恒星大气结构和演化状态都有十分重要的意义。

Based on the geological structure conditions of known hot springs and ground thermometric data,the comprehensive remote sensing prediction of geothermal abnormal area was carried out.

地热异常地段，在热红外波段(8~14μm)其热辐射温度较高，利用TM6波段(10.45~12.50μm)和航空热红外扫描图像(光谱波长8~14μm)及航空彩红外图像，选择适宜的波段组合作密度信息的增强处理。

We can calibrate various radiation thermometers and radiation heat flux bolometers, for example, IR-thermometers, IR-tympanic thermometers.

能够进行各种辐射温度计的校正工作，例如辐射高温计，红外温度计和红外耳温计，以及校正一些辐射热流计。

Several unusual properties make this object particular interesting:(1) ultra-luminous near and far infrared (L〓≈10〓L〓, and L〓≈10〓 L〓) emission,(2) very strong optical Fe Ⅱ emission (R〓≈4.35),(3) apparently blueshifted optical Fe Ⅱ multiplets (several hundred km/s),(4) the strongest radio emission among radio-FIR selected NLS1's and extreme Fe Ⅱ emitters,(5) composite Balmer lines with both narrow and broad components (the latter blueshifted by about 1000 km s〓).

我们发现2MASS0153+260为首例超强光学FeⅡ线射电类星体，具有如下极为有趣特征：(1)远红外和近红外光度非常高，L〓≈10〓 L〓且L〓≈10〓 L〓；(2)光学FeⅡ线发射特别强，R4570≈4.35；(3)光学FeⅡ线相对于禁线和氢Balmer线窄成分有明显蓝移，Δυ～4×10〓kms〓；(4)在射电-远红外选NLS1和超强光学FeⅡ线AGN中射电辐射最强；(5)具有复杂的Balmer发射线轮廓，宽成分相对于窄成分和禁线有～1000km s〓的蓝移。

For a big chunk of credit-card losses; the number of filings (and thus charge-off rates) would be rising again, whether

年美国个人破产法的一个改动使得破产登记急速下降，而后引起了信用卡大规模的亏损。

Eph. 4:23 And that you be renewed in the spirit of your mind

弗四23 而在你们心思的灵里得以更新