Dynamics of Food Price Inflation in Eastern Ethiopia: A Meso-Macro Modeling

High inflationary pressure especially in food price has been a top agenda in many developing countries since the last decade as it has been hindering their socioeconomic development. Though Ethiopia is achieving an encouraging economic growth in recent years, the occurrence of galloping inflation mainly since 2005 is retarding its progress and causing high welfare loss. The very step to struggle this problem is documenting the real causes of inflation. So far, there are only few attempts to document the macroeconomic determinants of general inflation in Ethiopia. Specially, empirical works on meso level price dynamics and focus on certain items are scant. This study is, therefore, designed to assess the macro-meso derivers of food price dynamics in Dire Dawa administration and Harari regional state based on qualitative data collected through key informant interview and quantitative monthly data from January, 2001 to September 2012. A result from Vector Error Correction Model (VECM) revealed that, in the long run, money supply, real income and international food and oil price hikes increase domestic food inflation while rise in exchange rate (depreciation or devaluation) was found to decrease inflation. Inflation expectation, smuggling, rise in world oil price and exchange rate are also documented to impact food price inflation of the study area in the short run. Pursuing conservative monetary policy, promoting competitiveness in the market and reducing the cost of making business would help to mitigate the galloping inflation in the study area.Key words: Price Dynamics, Inflation, Error Correction Model, Smuggling JEL Classification: E31, E37, C3

Asteroids in the Inner Solar System II - Observable Properties

This paper presents synthetic observations of long-lived, coorbiting asteroids of Mercury, Venus, the Earth and Mars. Our sample is constructed by taking the limiting semimajor axes, differential longitudes and inclinations for long-lived stability provided by simulations. The intervals are randomly populated with values to create initial conditions. These orbits are re-simulated to check that they are stable and then re-sampled every 2.5 years for 1 million years. The Mercurian sample contains only horseshoe orbits, the Martian sample only tadpoles. For both Venus and the Earth, the greatest concentration of objects on the sky occurs close to the classical Lagrange points at heliocentric ecliptic longitudes of 60 and 300 degrees. The distributions are broad especially if horseshoes are present in the sample. The full-width half maximum (FWHM) in heliocentric longitude for Venus is 325 degrees and for the Earth is 328 degrees. The mean and most common velocity of these coorbiting satellites coincides with the mean motion of the parent planet, but again the spread is wide with a FWHM for Venus of 27.8 arcsec/hr and for the Earth of 21.0 arcsec/hr. For Mars, the greatest concentration on the sky occurs at heliocentric ecliptic latitudes of 12 degrees. The peak of the velocity distribution occurs at 65 arcsec/hr, significantly less than the Martian mean motion, while its FWHM is 32.3 arcsec/hr. The case of Mercury is the hardest of all, as the greatest concentration occurs at heliocentric longitudes close to the Sun.Comment: 16 pages, 11 figures, Monthly Notices (in press). Higher quality figures available at http://www-thphys.physics.ox.ac.uk/users/WynEvans/home.htm

Evolution of the interfacial structure of LaAlO3 on SrTiO3

The evolution of the atomic structure of LaAlO3 grown on SrTiO3 was investigated using surface x-ray diffraction in conjunction with model-independent, phase-retrieval algorithms between two and five monolayers film thickness. A depolarizing buckling is observed between cation and oxygen positions in response to the electric field of polar LaAlO3, which decreases with increasing film thickness. We explain this in terms of competition between elastic strain energy, electrostatic energy, and electronic reconstructions. The findings are qualitatively reproduced by density-functional theory calculations. Significant cationic intermixing across the interface extends approximately three monolayers for all film thicknesses. The interfaces of films thinner than four monolayers therefore extend to the surface, which might affect conductivity

Independent mobility of proteins and lipids in the plasma membrane of Escherichia coli

Biotechnology and Biological Sciences Research Council. Grant Number: BB/E009571, Oxford Centre for Integrative Systems Biology (OCISB), Engineering and Physical Science Research Council, Royal Society, Hertford College Oxfor

Spontaneous Discharge Patterns in Cochlear Spiral Ganglion Cells Prior to the Onset of Hearing in Cats

Spontaneous neural activity has been recorded in the auditory nerve of cats as early as 2 days postnatal (P2 ), yet individual auditory neurons do not respond to ambient sound levels below 90–100 dB SPL until about P10. Significant refinement of the central projections from the spiral ganglion to the cochlear nucleus occurs during this neonatal period. This refinement may be dependent on peripheral spontaneous discharge activity. We recorded from single spiral ganglion cells in kittens aged P3 to P9. The spiral ganglion was accessed via the round window through the spiral lamina. A total of 112 ganglion cells were isolated for study in 9 animals. Spike rates in neonates were very low, ranging from 0.06 to 56 sp/s with a mean of 3.09 +/- 8.24 sp/s. Ganglion cells in neonatal kittens exhibited remarkable repetitive spontaneous bursting discharge patterns. The unusual patterns were evident in the large mean interval coefficient of variation (CVi = 2.9 +/-1.6) and burst index of 5.2 +/- 3.5 across ganglion cells. Spontaneous bursting patterns in these neonatal mammals were similar to those reported for cochlear ganglion cells of the embryonic chicken suggesting this may be a general phenomenon that is common across animal classes. Rhythmic spontaneous discharge of retinal ganglion cells has been shown to be important in the development of central retinotopic projections and normal binocular vision (Shatz, 1996, Proc Natl Acad Sci 93). Bursting rhythms in cochlear ganglion cells may play a similar role in the auditory system during pre-hearing periods. Originally published in Journal of Neurophysiology Vol. 98, No. 4 200