检索结果-南通市图书馆

第十五届国际光伏科学与工程大会

作者： Sumita Mukhopadhyay Romyani Goswami swati ray Energy Research Unit Indian Association for the Cultivation ofScienceJadavpurKolkata 700 032.India

Transition from amorphous to microcrystalline phase in silicon film has been realised at high power-pressure varying the hydrogen dilution in RFPECVD system. At the transition region the dark conductivity of the film is (σ) ～2.67×10 Scm with its activation energy (E) of～480meV. IR vibrational spectra have shown low microstructural defects in the films compared to films deposited at low power-pressure. Bonded H-content changes from 15.6% to 5.6% in the transition region. The material deserves high promise to be used as intrinsic layers in solar cells.

关键词： RFPECVD Transition FTIR

来源： cnki会议评论

在线全文

cnki会议

学校读者我要写书评

暂无评论

Voltage-controlled NiO/ZnO p–n heterojunction diode: a new approach towards selective VOC sensing

引用

Microsystems & Nanoengineering 2020年第1期6卷 894-902页

作者： Sayan Dey swati Nag Sumita Santra Samit Kumar ray Prasanta Kumar Guha Department of Electronics&Electrical Communication Engineering Indian Institute of TechnologyKharagpur 721302India Department of Electrical Engineering National Institute of TechnologyAgartala 99046India Department of Physics Indian Institute of TechnologyKharagpur 721302India Department of Physics Belda CollegeBelda 721424India S N Bose National Centre for Basic Sciences Kolkata 700106India

Metal oxide resistive gas sensors suffer from poor selectivity that restricts their practical *** sensor arrays are used to improve selectivity which increased the system ***,we have proposed a novel NiO/ZnO-based p–n junction single-diode device for selective sensing of several volatile organic compounds(VOCs)simultaneously by tuning bias *** operating voltage was varied between 3 and 5 volts to achieve selective sensing of 2-propanol(19.1 times for 95ppm with response and recovery times of 70 s and 55s respectively‚at 3 volts),toluene(20.1 times for 95 ppm with response and recovery times of 100 s and 60 s respectively,at 4 volts),and formaldehyde(11.2 times for 95 ppm with response and recovery times of 88 s and 54s respectively,at 5 volts).A probable mechanism of the tunable selectivity with operating bias voltage due to increase in surface carriers with increasing voltage was hence put ***,this device may play an important role to develop future selective multiple VOC sensor thereby replacing standard sensor arrays.

关键词： selectivity hence thereby

来源：

维普期刊数据库评论

在线全文

维普期刊数据库

学校读者我要写书评

暂无评论

A multiwavelength view of the ISM in the merger remnant galaxy Fornax A

引用

Research in Astronomy and Astrophysics 2013年第8期13卷 885-898页

作者： swati Pralhadrao Deshmukh Bhagorao Tukaram Tate Nilkanth Dattatray Vagshette Sheo Kumar Pandey Madhav Khushalrao Patil Department of Physics Institute of Science Department of Physics Balbhim Arts Science and Commerce College School of Physical Sciences Swami Ramanand Teerth Marathwada University School of Studies in Physics & Astrophysics Pandit Ravishankar Shukla University

We present multi-wavelength imagery of the merger remnant galaxy NGC 1316 with an objective to study the dust content and its association with the other phases of the interstellar medium. Color-index maps as well as extinction maps derived for this galaxy reveal an intricate and complex dust morphology in NGC 1316, i.e. there is a prominent lane in the inner part, while at about 6-7 kpc it apparently takes the form of an arc-like pattern extending along the northeast direction. In addition to this, several other dust clumps and knots are also evident in this galaxy. The dust emission mapped using Spitzer data at 8 μm indicates even more complex morphological structures of the dust in NGC 1316. The extinction curve derived over the optical to near-IR bands closely follows the standard Galactic curve, suggesting similar properties of the dust grains. The dust content of NGC 1316, estimated from optical extinction, is ,- 2.13 × 10^5 M⊙. This is a lower limit compared to that estimated using the IRAS flux densities of ,-5.17× 10^6 M⊙ and the flux densities at 24, 70 and 160 p.m from MIPS ,-3.2× 10^7 M⊙. High resolution Chandra observations of this merger remnant system have provided an unprecedented view of the complex nature exhibited by the distribution of hot gas in NGC 1316, which closely matches the morphology of ionized gas and to some extent also the dust. X-ray color-color plots for the resolved sources within the optical D25 extent of NGC 1316 have enabled us to separate them into different classes.

关键词： galaxies individual (NGC 1316) - galaxies: ISM - X-rays: ISM - (ISM:) dust - extinction - galaxies: elliptical and lenticular, cD

来源：

维普期刊数据库

同方期刊数据库评论

在线全文

学校读者我要写书评

暂无评论

欢迎您,

建议与咨询留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

时间限定

文献类型

馆藏选择

核心期刊

语言

文献类型

帮助

文字说明：

检索规则说明：

检索范例：

分类表

所选分类

限定检索结果

文献类型

馆藏范围

日期分布

学科分类号

主题

机构

作者

语言

在线全文

在线全文

在线全文

请选择保存的检索档案：

请选择收藏分类：

通借通还

欢迎您,

建议与咨询 留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

时间限定

文献类型

馆藏选择

核心期刊

语言

文献类型

帮助

文字说明：

检索规则说明：

检索范例：

分类表

所选分类

限定检索结果

文献类型

馆藏范围

日期分布

学科分类号

主题

机构

作者

语言

在线全文

在线全文

在线全文

请选择保存的检索档案： 新增检索档案 确定 取消

请选择收藏分类： 新增自定义分类 确定 取消

通借通还

建议与咨询留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

请选择保存的检索档案：

请选择收藏分类：