Presumed guilty: how the Jews were blamed for the death of Jesus

Title: Presumed guilty: how the Jews were blamed for the death of Jesus. Author: Tomson, Peter J Presumed guilty xiv, 146 p. Publisher: Zoetermeer, Netherlands : Uitgeverij Meinema ; Minneapolis : Fortress, 2005

Introducing the Bible

Title: Introducing the Bible. Author: Drane, John Introducing the Bible 730 p. Publisher: Minneapolis : Fortress Pr, 2005

The Passion of Gibson: evaluating a recent interpretation of Christ\u27s suffering and death in light of the New Testament

Passion of the Christ Publisher: [S.l.] : Icon Film Distribution, 2004

Alfven-wave dissipation: A support mechanism for quiescent prominences

High resolution filtergrams or spectrograms of the main body of quiescent prominences often show a very vivid dynamical picture that cannot be reconciled with static models. Even if large differences exist between individual prominences in this respect, at least parts of the prominence are usually found to be in a 'choppy', turbulent state. Evidence for systematic flows are found in local regions in the prominence and also in the transition zone in the surroundings. These two regions are probably decoupled magnetically. Alfven waves are generally believed to be responsible for the heating in the upper chromosphere and corona (Hollweg 1986). Since evidence for the presence of Alfven-waves has also been found in the solar wind field, it is highly probable that such waves are generated in the convection zone of the sun and propagated outwards in the solar atmosphere wherever a proper magnetic field is present to carry the waves. The most basic magnetic formations in the solar atmosphere are simple loops. They occur all over the solar surface and cover a large range of magnetic field strengths. Loops with the strongest magnetic fields are found in active regions. It is to be expected that the Alfven-wave flux which is channelled into the loops from below, could show considerable variation both with heliocentric latitude, with time and locally between neighbouring loops. What happens when a magnetic loop is exposed to the appropriate Alfven-wave flux required to heat the upper solar atmosphere is examined

Bisimple monogenic orthodox semigroups

We give a complete description of the structure of all bisimple orthodox semigroups generated by two mutually inverse elements