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| 1 | Effect of temperature and concentration on nheological properties of ' Kesar' mango juice 显示文摘 | Dak M Verma R C Jaaffrey S N A | 2007 | Journal of Food Engineering2007，80，4： | 1 |
| 2 | Effect of temperature and concentration on rheological properties of 'Kesar' mango juice显示文摘 | Dak M Verrna R C Jaaffrey S N A | 2007 | Journal of Food Engineering2007，80，： | 1 |
| 3 | Effect of temperature and concentration on rheologieal properties of ' Kesar' mango juice显示文摘 | Dak M Verma R C Jaaffrey S N A | | 0，，： | 1 |
| 4 | Effect of temperature and concentration on Rheological properties of 'Kesar' mango juice显示文摘 | Dak M Verma R C Jaaffrey S N A | 2007 | J Food Eng2007，80，4： | 1 |
| 5 | AstroSat observation of GX 5–1: spectral and timing evolution显示文摘We report on the first analysis of an AstroSat observation of the Z-source GX 5–1 on 2017 February 26-27. The hardness-intensity plot reveals that the source traced out the horizontal and normal branches. The 0.8-20 keV spectra from simultaneous SXT and LAXPC data at different locations of the hardness-intensity plot can be described well by disk emission and a thermal Comptonized component. The ratio of the disk flux to the total flux, i.e., the disk flux ratio, increases monotonically along the horizontal branch to the normal one. Thus, the difference between the normal and horizontal branches is that in the normal branch, the disk dominates the flux while in the horizontal one it is the Comptonized component which dominates. The disk flux scales with the inner disk temperature as Tin5.5 and not as Tin4 , suggesting that either the inner radius changes dramatically or that the disk is irradiated by the thermal component changing its hardness factor. The power spectra reveal a quasi-periodic oscillation(QPO) whose frequency changes from 30 Hz to 50 Hz. The frequency is found to correlate well with the disk flux ratio. In the 3-20 keV LAXPC band, the r.m.s. of the QPO increases with energy(r.m.s. ∝ E0.8), while the harder X-rays seem to lag the soft ones with a time-delay of milliseconds. The results suggest that the spectral properties of the source are characterized by the disk flux ratio and that the QPO has its origin in the corona producing the thermal Comptonized component. | Yashpal Bhulla Ranjeev Misra JSYadav SNA Jaaffrey | 2019 | Research in Astronomy and Astrophysics2019，19，8： | 0 |
| 6 | Timing and Spectral Studies of Pulsar EXO2030+375显示文摘我们报导预定的结果并且光谱 X 光脉冲星 EXO2030+375 的分析。观察用预定探索者空间卫星的 Rossi X 光被做。光谱分析为 X 光精力范围 330keV 的流动被执行。比例的相反的数组的 X 光连续统系列能被一个二部件的模型,代表有在更高的精力和 blackbody 的指数的截止的一条幂定律。在大约 6.46.6 keV 的一根铁线也被检测。 | Shubhra Tiwari S. N. A. Jaaffrey Rizwan S. Khan Sushil K. Gandhi Santvana Bapna | 2010 | Chinese Physics Letters2010，27，2： | 0 |
| 7 | Secondary X-Ray Environment in the Lower Atmosphere of the Earth during Monsoon Season over Udaipur City (India) in July-September 2006显示文摘我们在场精力乐队 2 −100 keV 的第二等的 X 光上的研究由灰尘暴风雨,季风飘移和重力的拉在 meteoritic 淋浴上在更低的空气带上的侵入的主要污染物质部件(气体和矿物质) 射出。在地面上,我们采用了 1.5 ×在一个焕发察觉者的 1 英寸 2 NaI 晶体,对精力范围合适第二等的 X 光的 2 −100 keV,比更大的大小的晶体提供更好的精力分辨率。以便消除地球的放射性的背景,察觉者很好在铅(Pb ) 的帮助下在所有方面上被防护容器,除了与在到许可证的顶的一扇小开的窗户仅仅垂直地事件第二等的放射。从从 7 月在时期期间在 Udaipur 城市(印度) 上在季风期间获得到 9 月(2006 ) 的数据分析的结果揭示了在灰尘暴风雨淫液季风云之间的线性关联并且从侵入的污染物质观察了第二等的 X 光放射的光明。当重灰尘和季风云被灰尘暴风雨和季风飘移作为与正常的天相比在 Udaipur 城市上在更低的空气带上时,我们从侵入的污染物质发现了第二等的 X 光的强烈流动。因此,在环境的第二等的 X 光在更低的空气为本地恼人的污染物质部件的调查提供一个工具。 | S. N. A. Jaaffrey Shubhra Tiwari | 2009 | Chinese Physics Letters2009，26，8： | 0 |
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