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| 1 | Effect of zinc and manganese on the uptake of nitrogen in tea shoot显示文摘 | DEV CHOUDHURY M N BORDOLOR A K SHARMA P K | 1989 | Two and a Bud1989，36，12： | 1 |
| 2 | Role of chlorophylls, amino acidsand sugars in tea显示文摘 | Dev Choudhury M N Bajaj K L | 1980 | Two and a Bud1980，，27： | 1 |
| 3 | Sorption behaviour of lanthanum(III),neodymium(IlI),terbi-um(III),thorium(IV)and uranium(VI)on amberlite XAD-4 resin functionalized with bicine ligands显示文摘 | DEV K PATHAK R RAO G N | | 0，，： | 1 |
| 4 | Biochemical changes during withering of tea shoots显示文摘 | Dev Choudhury M N Bajaj K L | 1980 | Two and a Bud1980，27，1： | 1 |
| 5 | X-ray standing wave and reflectometrie characterization of multilayer structures 显示文摘 | GHOSE S K DEV B N | 2001 | Physical Review B2001，63，24： | 1 |
| 6 | Role of chlorophylls, amino acids and sugars in tea显示文摘 | Dev Choudhury M N Bajaj K L | 1980 | Two and a Bud1980，27，1： | 1 |
| 7 | Impact of Visual Impairment on Vision-Specific Quality of Life among Older Adults Living in Nursing Home显示文摘 | Dev M K Paudel N Joshi N D | 2014 | Curr Eye Res2014，39，3： | 1 |
| 8 | Sorption behaviour of lanthanum(Ⅲ),neodymium(Ⅲ),terbium(Ⅲ),thorium(Ⅳ) and uranium(Ⅵ) on Amberlite XAD-4 resin functionalized with bicine ligands显示文摘 | Pathak R Rao G N | 1999 | Talanta1999，48，3： | 1 |
| 9 | Dry Valley streams in Antarctica: Ecosystems waiting for water显示文摘 | Diane M M Dev K N Alexander S A | 1999 | Bioscience1999，49，12： | 1 |
| 10 | K-P-Burgers equation in negative ion-rich relativistic dusty plasma including the effect of kinematic viscosity显示文摘The stationary solution is obtained for the K–P–Burgers equation that describes the nonlinear propagations of dust ion acoustic waves in a multi-component, collisionless, un-magnetized relativistic dusty plasma consisting of electrons, positive and negative ions in the presence of charged massive dust grains. Here, the Kadomtsev–Petviashvili(K–P) equation, threedimensional(3D) Burgers equation, and K–P–Burgers equations are derived by using the reductive perturbation method including the effects of viscosity of plasma fluid, thermal energy, ion density, and ion temperature on the structure of a dust ion acoustic shock wave(DIASW). The K–P equation predictes the existences of stationary small amplitude solitary wave,whereas the K–P–Burgers equation in the weakly relativistic regime describes the evolution of shock-like structures in such a multi-ion dusty plasma. | A N Dev M K Deka J Sarma D Saikia N C Adhikary | 2016 | Chinese Physics B2016，25，10： | 0 |
| 11 | Characteristics of dust acoustic waves in dissipative dusty plasma in the presence of trapped electrons显示文摘The formation and propagation of nonlinear dust acoustic waves(DAWs) as solitary and solitary/shock waves in an unmagnetized, homogeneous, dissipative and collisionless dusty plasma comprising negatively charged micron sized dust grains in the presence of free and trapped electrons with singly charged non-thermal positive ions is discussed in detail. The evolution characteristics of the solitary and shock waves are studied by deriving a modified Korteweg–de Vries–Burgers(mKdV–Burgers) equation using the reductive perturbation method. The mKdV–Burgers equation is solved considering the presence(absence) of dissipation. In the absence of dissipation the system admits a solitary wave solution, whereas in the presence of dissipation the system admits shock waves(both monotonic and oscillatory) as well as a combination of solitary and shock wave solutions. Standard methods of solving the evolution equation of shock(solitary) waves are used. The results are discussed numerically using standard values of plasma parameters. The findings may be useful for better understanding of formation and propagation of waves in astrophysical plasma. | Ranjit K KALITA Manoj K DEKA Apul N DEV Jnanjyoti SARMA | 2017 | Plasma Science and Technology2017，19，5： | 0 |
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