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12篇 您的检索式：作者名="Ghezelbash A"

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		题名	作者	年代	出处	被引量
	1	Solventless Synthesis of Cop-per Sulfide Nanorods by Thermolysis of a Single SourceThiolate-Derived Precursor显示文摘	Larsen T.H Sigman M.B Jr Ghezelbash A Doty R.C Korgel.B.A		0，，：	1
	2	Solventless Syn-thesis of Monodisperse Cu2S Nanorods,Nanodisks,andNanoplatelets显示文摘	Sigman M.B Jr Ghezelbash A Hanrath T Saunders A E Lee F Korgel B.A_		0，，：	1
	3	Vortices in de Sitter spacetimes显示文摘	Ghezelbash A M Mann R B	2002	Phys Lett2002，537，2：	1
	4	Synthesis of germanium nanocrystals in high temperature supercritical fluid solvents显示文摘	Lu X Ziegler K J Ghezelbash A	2004	Nano Lett2004，4，5：	1
	5	Sol-ventless Synthesis of Nickel Sulfide Nanorods and Trian-gular Nanoprisms显示文摘	Ghezelbash A Sigman M.B Jr Korgel B.A		0，，：	1
	6	Solventless Synthesis of Copper Sulfide Nanorods by Thermolysis of a Single Source Thiolate-Derived Precursor 显示文摘	] Larsen T H Sigman M Ghezelbash A	2003	J Am Chem Soc2003，125，19：	1
	7	Co- lumnar self-assembly of colloidal nanodisks 显示文摘	Saunders A E Ghezelbash A Smilgies D M	2006	Nano let- ters2006，6，12：	1
	8	显示文摘	Ghezelbash A Korgel B A	2005	Langmuir2005，21，：	1
	9	Solvent- less synthesis of monodisperse Cu2 S nanorods, nanodisks and nanoplatelets显示文摘	Sigman Jr M B Ghezelbash A Hanrath T	2003	Journal of the American Chemical Society2003，125，16：	1
	10	Solventless synthesis of monodisperse Cu2S nanorods, nanodisks, and nanoplatetets 显示文摘	SIGMAN M B GHEZELBASH A HANRATH T	2003	J Am Chem Soc2003，125，16：	1
	11	Nickel sulfide and copper sulfide nanocrystal synthesis and polymorphism 显示文摘	GHEZELBASH A KORGEL B A	2005	Lang- muir2005，21，21：	1
	12	Assessing Doppler velocities of Rankin Inlet F-region echoes显示文摘Doppler velocities observed by the Rankin Inlet (RKN) PolarDARN radar are assessed with a focus on data in the beams oriented roughly along the magnetic meridian. Hourly scatter plots for every month are built. They are shown to vary widely, with median values showing very clear magnetic local time variation with maximum magnitude during pre-noon and pre-midnight hours. The histograms contain a significant amount of very small velocity data that dominates at farther ranges and during the daytime. Near noon data show generally antisunward flows but at large ranges/magnetic latitudes and very close to noon, sunward flows occur for periods of positive IMF B z . The reverse flows are stronger during spring equinox. The velocity magnitude was found to depend linearly on the IMF B z and interplanetary electric field. Velocities are often found to be smaller than those expected from the statistical convection model of Ruohoniemi and Greenwald-1996.	Alexander V Koustov Kale Colville Robyn A D Fiori Mohsen Ghezelbash	2013	Advances in Polar Science2013，24，1：	0

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