Saint Paul’s doctrine of sin

St. Paul sees sin both as 'prenomic’ ("in. the world before the law was given" Rom.5.13) and as revealed by the law. The law was meant to "make alive" (Gal.3.21), but Paul came to see that the law reveals man's inability to fulfil God's, demand, and, in fact, energises 'prenomic' sin, making it '.transgression’. This realisation does not affect Paul's estimate, of-the law; rather, the law's failure, to fulfil its function in man is explained by the fact that man, as flesh, is "sold under sin" (Rom.7.14). The flesh is not inherently sinful, but is dominated by the power of sin. "All have sinned" (Rom.3.23) and sin is essentially one, though three, forms of sin are to be found in Paul's, thought. 'Prenomic' sin is a dominant feature of human activity or living which distinguishes it as resulting in alienation from God. This conception is made concrete in two directions. Firstly, transgression, which requires the context of the law, has the elements of defiance of God's demand and subjective guilt. Secondly, sin personalised is the hidden power of sin, which holds man in slavery. St. Paul is not so much concerned, with the origin of sin as with its consequences of alienation from God, 'more sin’ and death. It is as God reveals himself in the work of Christ and the gift of the Spirit that sin is revealed; it is in the revelation of Christ that God’s purpose of faith is made known and man's failure to fulfil God's purpose is revealed. The Christian though Christ has condemned sin in the flesh (Rom.8.3), has to contend with the fact that he is still in the flesh, as he awaits the full outworking of God's action in Christ in the resurrection of the dead

Temporal evolution of velocity structures in the solar wind

Generally poor correlations were obtained of solar wind flow speed measurements at one point in the ecliptic plane with measurements at the same point 28 days (one solar rotation) earlier or with measurements at other points in the ecliptic plane separated by 50 deg or more in solar longitude. This is evidence that either the flow speed is a very sensitive function of solar latitude or that temporal processes typically alter the speed of the wind emanating from particular solar regions on a time scale of about 4 days. From a measure of the persistence of the flow speed at the orbit of the earth, it appears that the temporal explanation is more likely to be the correct one

People Like Me Don’t Belong in Places Like This. Creating and Developing a Community of Learners beyond the Prison Gates

It is widely accepted that individuals with criminal convictions experience multiple disadvantage and deprivation, and, as a result, are considered least likely to progress to higher education (Unlock, 2018). The risk-adverse nature of higher education application processes further compound such disadvantage, even though there is no evidence to suggest that screening for criminal convictions increase campus safety (Centre for Community Alternatives, 2010). Drawing upon ethnographic data, the discussion critically reflects upon the development of one situated Learning Together initiative based within a University in the north-west of England. In doing so, the discussion highlights a series of emerging opportunities and competing contradictions that span over three key developmental areas: creation, progress and maintenance. We anticipate that the findings will go some way in opening up a wider debate about the sustainability of initiatives that seek to create dynamic educational partnerships between the higher education sector and criminal justice system more broadly

Complex small-scale structure in the infrared extinction towards the Galactic Centre

A high level of complex structure, or ``granularity'', has been observed in the distribution of infrared-obscuring material towards the Galactic Centre (GC), with a characteristic scale of 5arcsec - 15arcsec, corresponding to 0.2 - 0.6pc at a GC distance of 8.5kpc. This structure has been observed in ISAAC images which have a resolution of 0.6arcsec, significantly higher than that of previous studies of the GC. We have discovered granularity throughout the GC survey region, which covers an area of 1.6deg x 0.8deg in longitude and latitude respectively (300pc x 120pc at 8.5kpc) centred on Sgr A*. This granularity is variable over the whole region, with some areas exhibiting highly structured extinction in one or more wavebands and other areas displaying no structure and a uniform stellar distribution in all wavebands. The granularity does not appear to correspond to longitude, latitude or radial distance from Sgr A*. We find that regions exhibiting high granularity are strongly associated with high stellar reddening.Comment: 5 pages, 3 figures, accepted for publication in ApJ

Solar cycle variation of real CME latitudes

With the assumption of radial motion and uniform longitudinal distribution of coronal mass ejections (CMEs), we propose a method to eliminate projection effects from the apparent observed CME latitude distribution. This method has been applied to SOHO LASCO data from 1996 January to 2006 December. As a result, we find that the real CME latitude distribution had the following characteristics: (1) High-latitude CMEs ($\theta>60^{\circ}$ where $\theta$ is the latitude) constituted 3% of all CMEs and mainly occurred during the time when the polar magnetic fields reversed sign. The latitudinal drift of the high-latitude CMEs was correlated with that of the heliospheric current sheet. (2) 4% of all CMEs occurred in the range $45^{\circ}\leq\theta\leq60^{\circ}$. These mid-latitude CMEs occurred primarily in 2000, near the middle of 2002 and in 2005, respectively, forming a prominent three-peak structure; (3) The highest occurrence probability of low-latitude ($\theta< 45^{\circ}$) CMEs was at the minimum and during the declining phase of the solar cycle. However, the highest occurrence rate of low-latitude CMEs was at the maximum and during the declining phase of the solar cycle. The latitudinal evolution of low-latitude CMEs did not follow the Sp\"{o}rer sunspot law, which suggests that many CMEs originated outside of active regions.Comment: 4 pages, 4 figures, accepted by ApJ Lette

Multiple spacecraft observations of interplanetary shocks: Characteristics of the upstream ULF turbulence

All interplanetary shocks observed by ISEE-3 and either ISEE-1 or ISEE-2 or both in 1978 and 1979 are examined for evidence of upstream waves. In order to characterize the properties of these shocks it is necessary to determine accurate shock normals. An overdetermined set of equations were inverted to obtain shock normals, velocities and error estimates for all these shocks. Tests of the method indicate it is quite reliable. Using these normals the Mach number and angle were between the interplanetary magnetic field and the shock normal for each shock. The upstream waves were separated into two classes: whistler mode precursors which occur at low Mach numbers and upstream turbulence whose amplitude at Mach numbers greater than 1.5 is controlled by the angle of the field to the shock normal. The former waves are right hand circularly polarized and quite monochromatic. The latter waves are more linearly polarized and have a broadband featureless spectrum

The Magellanic system X-ray sources

Using archival X-ray data from the second XMM-Newton serendipitous source catalogue, we present comparative analysis of the overall population of X-ray sources in the Large and Small Magellanic Clouds. We see a difference between the characteristics of the brighter sources in the two populations in the X-ray band. Utilising flux measurements in different energy bands we are able to sort the X-ray sources based on similarities to other previously identified and classified objects. In this manner we are able to identify the probable nature of some of the unknown objects, identifying a number of possible X-ray binaries and Super Soft Sources.Comment: 4 pages, 2 figures. Poster to appear in proceedings of IAU Symposium 256, The Magellanic System: Stars, Gas, and Galaxies. Keele Univeristy, U

Can Streamer Blobs prevent the Buildup of the Interplanetetary Magnetic Field?

Coronal Mass Ejections continuously drag closed magnetic field lines away from the Sun, adding new flux to the interplanetary magnetic field (IMF). We propose that the outward-moving blobs that have been observed in helmet streamers are evidence of ongoing, small-scale reconnection in streamer current sheets, which may play an important role in the prevention of an indefinite buildup of the IMF. Reconnection between two open field lines from both sides of a streamer current sheet creates a new closed field line, which becomes part of the helmet, and a disconnected field line, which moves outward. The blobs are formed by plasma from the streamer that is swept up in the trough of the outward moving field line. We show that this mechanism is supported by observations from SOHO/LASCO. Additionally, we propose a thorough statistical study to quantify the contribution of blob formation to the reduction of the IMF, and indicate how this mechanism may be verified by observations with SOHO/UVCS and the proposed NASA STEREO and ESA Polar Orbiter missions.Comment: 7 pages, 2 figures; accepted by The Astrophysical Journal Letters; uses AASTe