Evangelical Journeys:Choice and Change in a Northern Irish Religious Subculture

This book draws on interview material with more than 100 evangelicals. We ask why do people born into the same religious community turn out so differently? We tell the stories of pro-life DUP picketers, liberal peace-campaigning ministers, housewives afraid of the devil, students deconstructing their faith and atheists mortified by their religious past. We explore why people have chosen to go in one religious direction or another, and how their religious journeys have unfolded.

Ulster Says Maybe: The Restructuring of Evangelical Politics in Northern Ireland

The recent electoral triumphs of the Democratic Unionist Party (DUP) have stimulated debate about the role of fundamentalist or ‘traditional evangelical’ Protestantism within the party and in Northern Irish politics. This paper argues that a significant restructuring of evangelical politics is taking place, one that is interest group‐centred rather than DUP‐centred. This process has been facilitated by changes in the structure of civil society. Traditional evangelical interest groups are ‘reframing’ their political projects in surprising new ways: abandoning Calvinist conceptions of church and state, using discourses of marginalisation and discrimination, and focusing on ‘moral’ issues. These subtle shifts in rhetoric constitute an acceptance of the post‐Belfast Agreement order. Rather than the tired, ‘Ulster Says No’ politics of the past, evangelicals are speaking out with a pragmatic ‘maybe’. This move parallels and reinforces the DUP’s ideological shifts, and provides an extra‐party platform for evangelicals to impact politics.

Mechanisms for mhd poynting flux generation in simulations of solar photospheric magnetoconvection

We investigate the generation mechanisms of MHD Poynting flux in the magnetized solar photosphere. Using radiative MHD modeling of the solar photosphere with initial magnetic configurations that differ in their field strength and geometry, we show the presence of two different mechanisms for MHD Poynting flux generation in simulations of solar photospheric magnetoconvection. The weaker mechanism is connected to vertical transport of weak horizontal magnetic fields in the convectively stable layers of the upper photosphere, while the stronger is the production of Poynting flux in strongly magnetized intergranular lanes experiencing horizontal vortex motions. These mechanisms may be responsible for the energy transport from the solar convection zone to the higher layers of the solar atmosphere.