Edit
Edit may refer to:
See also
Edit (album)
Edit is the sixth album by vocalist Mark Stewart, released on March 28, 2008 through Crippled Dick Hot Wax!.
Accolades
Track listing
Personnel
References
External links
Edit (Regina Spektor song)
"Edit" is an Anti-folk/Indie rock song from Anti-folk singer Regina Spektor, released in the summer of 2006 on the album Begin to Hope. The line "You don't have no Doctor Robert/You don't have no Uncle Albert" references the Beatles' song "Doctor Robert" as well as Paul and Linda McCartney's 1979 hit "Uncle Albert". "Edit" was covered by British anti-folk band The Red Army.
Inflation
In economics, inflation is a sustained increase in the general price level of goods and services in an economy over a period of time. When the price level rises, each unit of currency buys fewer goods and services. Consequently, inflation reflects a reduction in the purchasing power per unit of money – a loss of real value in the medium of exchange and unit of account within the economy. A chief measure of price inflation is the inflation rate, the annualized percentage change in a general price index, usually the consumer price index, over time. The opposite of inflation is deflation.
Inflation affects an economy in various positive and negative ways. Negative effects of inflation include an increase in the opportunity cost of holding money, uncertainty over future inflation which may discourage investment and savings, and if inflation were rapid enough, shortages of goods as consumers begin hoarding out of concern that prices will increase in the future. Positive effects include reducing the real burden of public and private debt, keeping nominal interest rates above zero so that central banks can adjust interest rates to stabilize the economy, and reducing unemployment due to nominal wage rigidity.
Inflation (cosmology)
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation is a theory of exponential expansion of space in the early universe. The inflationary epoch lasted from 10−36 seconds after the Big Bang to sometime between 10−33 and 10−32 seconds. Following the inflationary period, the Universe continues to expand, but at a less rapid rate.
Inflation theory was developed in the early 1980s. It explains the origin of the large-scale structure of the cosmos. Quantum fluctuations in the microscopic inflationary region, magnified to cosmic size, become the seeds for the growth of structure in the Universe (see galaxy formation and evolution and structure formation). Many physicists also believe that inflation explains why the Universe appears to be the same in all directions (isotropic), why the cosmic microwave background radiation is distributed evenly, why the Universe is flat, and why no magnetic monopoles have been observed.
While the detailed particle physics mechanism responsible for inflation is not known, the basic picture makes a number of predictions that have been confirmed by observation. The hypothetical field thought to be responsible for inflation is called the inflaton.
Monetary inflation
Monetary inflation is a sustained increase in the money supply of a country (or currency area). Depending on many factors, especially public expectations, the fundamental state and development of the economy, and the transmission mechanism, it is likely to result in price inflation, which is usually just called "inflation", which is a rise in the general level of prices of goods and services.
There is general agreement among economists that there is a causal relationship between monetary inflation and price inflation. But there is neither a common view about the theoretical exact mechanisms and relationships, nor about how to measure it exactly in reality. This relationship is also constantly changing, within a larger complex economic system. So there is a great deal of debate on the issues involved, such as how to measure the monetary base and price inflation, how to measure the effect of public expectations, how to judge the effect of financial innovations on the transmission mechanisms, and how much factors like the velocity of money affect the relationship. Thus there are different views on what could be the best targets and tools in monetary policy.
River Dee, Galloway
The River Dee (Scottish Gaelic: Dè / Uisge Dhè), in south-west Scotland, flows from its source in Loch Dee amongst the Galloway Hills, firstly to Clatteringshaws Loch, then into Loch Ken, where it joins the Water of Ken. From there, the Dee flows 15 miles (24 km) southwards to Kirkcudbright, and into Kirkcudbright Bay to reach the Solway. The distance is just over 38 miles (61 km) in total. Together with its tributaries, the Dee's total catchment area is over 400 square miles (1,000 km2).
The river is dammed at Tongland, two miles (3 km) upriver from Kirkcudbright. This was constructed as part of the Galloway hydro-electric power scheme in the 1930s. Also at this site is Tongland Bridge, built in 1806 by Thomas Telford.
The ruins of Threave Castle stand on an island on the lower part of the Dee.
In Ptolemy's 2nd century work Geography it is recorded as Dēoúa. This form represents a development of Proto-Indo-European *deiueh2- 'a goddess', which occurs in many Celtic river-names.
