Popery, Arbitrary Government, and War, 1670–8

2021 ◽  
pp. 38-53
Author(s):  
Hannah Smith

This chapter examines Charles II’s political and military problems during the Third Anglo-Dutch War as he once again attempted a policy of religious toleration. With the country at war, Charles was confronted with the dilemma of appointing a commander for his army and with the problem of how to discipline this newly increased force. But even more difficult was his relationship with parliament, which was intensely suspicious of the army. Parliament remained deeply concerned that the army had been infiltrated by Catholics. Moreover, parliament continued to be apprehensive of Charles’s plans for his army, particularly when the army was enlarged to fight a war with France in 1678.

2013 ◽  
Vol 10 (2) ◽  
pp. 261-291 ◽  
Author(s):  
ARASH ABIZADEH

What motivated an absolutist Erastian who rejected religious freedom, defended uniform public worship, and deemed the public expression of disagreement a catalyst for war to endorse a movement known to history as the champion of toleration, religion's freedom from coercion, and separation of church and state? At least three factors motivated Hobbes's 1651 endorsement of Independency: the Erastianism of Cromwellian Independency, the influence of the politique tradition, and, paradoxically, the contribution of early modern practices of toleration to maintaining the public sphere's religious uniformity. The third factor illustrates how a key function of the emerging private sphere in the early modern period was to protect uniformity, rather than diversity; it also shows that what was novel was not so much the public/private distinction itself, but the separation of two previously conflated dimensions of publicity—visibility and representativeness—that enabled early modern Europeans to envisage modes of worship out in the open, yet still private.


Author(s):  
Ross Carroll

The relaxing of censorship in Britain at the turn of the eighteenth-century led to an explosion of satires, caricatures, and comic hoaxes. This new vogue for ridicule unleashed moral panic and prompted warnings that it would corrupt public debate. But ridicule also had vocal defenders who saw it as a means to expose hypocrisy, unsettle the arrogant, and deflate the powerful. This book examines how leading thinkers of the period searched for a humane form of ridicule, one that served the causes of religious toleration, the abolition of the slave trade, and the dismantling of patriarchal power. It brings to life a tumultuous age in which the place of ridicule in public life was subjected to unparalleled scrutiny. It shows how the Third Earl of Shaftesbury, far from accepting ridicule as an unfortunate byproduct of free public debate, refashioned it into a check on pretension and authority. The book examines how David Hume, Mary Wollstonecraft, and others who came after Shaftesbury debated the value of ridicule in the fight against intolerance, fanaticism, and hubris. Casting Enlightenment Britain in an entirely new light, the book demonstrates how the Age of Reason was also an Age of Ridicule, and speaks to our current anxieties about the lack of civility in public debate.


1913 ◽  
Vol 6 (4) ◽  
pp. 397-406
Author(s):  
Charles William Eliot

Churches in the great religions have been allies of all ancient governments and most modern ones. The Emperor of Japan was believed to have, and in the popular mind still has, intimate relations with the heavenly powers. He used to be held in a seclusion suitable for this peculiar relationship to Deity. The Emperor of China for thousands of years under various dynasties was a high priest, whose offerings and prayers were peculiarly acceptable to Deity, and frequently procured for his people good seedtimes and good harvests, although he sometimes failed to avert pestilences, droughts, floods, and famines. The Indian castes are family clans and trades-unions with strong religious sanctions. The Koran contains the foundations of civil law as well as of ecclesiastical, and the Sultan claims succession to the religious as well as to the civil authority of the Caliphs. Under the feudal system there was a chaplain in every great noble's house, and the king ruled “by the grace of God,” and by the same grace transmitted his office to his son. Both Napoleon the Great and Napoleon the Little claimed as Emperor the support of the Church; but Napoleon the Third never seemed to see the extraordinary pathos in the formula he used so much, “By the grace of God and the national will Emperor of the French.” The French Revolution tried to divorce civil government from religion, but failed to do so. National established churches supported by the state exist all over Europe, although their tenure is frail in several European countries. The American Republic has carried into practice complete religious toleration and complete separation of church and state; but every now and then some one proposes to bridge the gap between church and state by a phrase such as “Vox populi, vox Dei,” or to “recognize” the Divine Immanence by inserting the word God in the Constitution.


This introductory chapter provides an overview of the book's main themes. This book is an anthology of significant writings on religion and politics from the colonial period to recent times. Rather than offering a comprehensive prescription for our public life, it presents an extended conversation. Although this volume covers a wide range of subjects, it returns throughout to three interrelated themes, common problems that persist across historical eras. The first theme deals with the scope of religious freedom and religious toleration, values inextricably linked to the First Amendment's religion clauses. The second addresses religion's role as an ethical compass for public life. The third major center of gravity, which intermingles with the first two, is about the character of the American nation.


1978 ◽  
Vol 29 (1) ◽  
pp. 51-73
Author(s):  
G. M. Ditchfield

It is widely accepted among historians that the House of Lords in the eighteenth century was an obstacle to religious change. Its unfriendly mien appears to be confirmed by the fate of several Quaker tithe bills and Dissenting petitions. Despite the passage of limited relief acts for Roman Catholics and Dissenters in 1778 and 1779 respectively, it was unusual for such legislation to be well received, or even to find a sponsor, in that chamber. Yet, in the summer of 1789 the House of Lords and that House alone witnessed what has been a neglected episode in ecclesiastical and political history. This was the attempt by the third earl Stanhope to amend the law concerning religious toleration. Although admittedly far from an exception to the rule in the way in which it was greeted by the peers, it has received scant notice from modern historians of toleration. Stanhope himself, of course, has become known to the historically minded as one of the celebrated eccentrics of the period; the image of ‘Citizen Stanhope’ the defender of the French Revolution and the ‘minority of one’ is unlikely to be effaced. Accordingly such discussion as there has been of the earl's bill has tended to emphasise Stanhope's personal idiosyncrasies and peculiar brand of aristocratic radicalism rather than the detailed provisions of the measure.


1967 ◽  
Vol 31 ◽  
pp. 177-179
Author(s):  
W. W. Shane

In the course of several 21-cm observing programmes being carried out by the Leiden Observatory with the 25-meter telescope at Dwingeloo, a fairly complete, though inhomogeneous, survey of the regionl11= 0° to 66° at low galactic latitudes is becoming available. The essential data on this survey are presented in Table 1. Oort (1967) has given a preliminary report on the first and third investigations. The third is discussed briefly by Kerr in his introductory lecture on the galactic centre region (Paper 42). Burton (1966) has published provisional results of the fifth investigation, and I have discussed the sixth in Paper 19. All of the observations listed in the table have been completed, but we plan to extend investigation 3 to a much finer grid of positions.


1966 ◽  
Vol 25 ◽  
pp. 227-229 ◽  
Author(s):  
D. Brouwer

The paper presents a summary of the results obtained by C. J. Cohen and E. C. Hubbard, who established by numerical integration that a resonance relation exists between the orbits of Neptune and Pluto. The problem may be explored further by approximating the motion of Pluto by that of a particle with negligible mass in the three-dimensional (circular) restricted problem. The mass of Pluto and the eccentricity of Neptune's orbit are ignored in this approximation. Significant features of the problem appear to be the presence of two critical arguments and the possibility that the orbit may be related to a periodic orbit of the third kind.


1988 ◽  
Vol 102 ◽  
pp. 79-81
Author(s):  
A. Goldberg ◽  
S.D. Bloom

AbstractClosed expressions for the first, second, and (in some cases) the third moment of atomic transition arrays now exist. Recently a method has been developed for getting to very high moments (up to the 12th and beyond) in cases where a “collective” state-vector (i.e. a state-vector containing the entire electric dipole strength) can be created from each eigenstate in the parent configuration. Both of these approaches give exact results. Herein we describe astatistical(or Monte Carlo) approach which requires onlyonerepresentative state-vector |RV> for the entire parent manifold to get estimates of transition moments of high order. The representation is achieved through the random amplitudes associated with each basis vector making up |RV>. This also gives rise to the dispersion characterizing the method, which has been applied to a system (in the M shell) with≈250,000 lines where we have calculated up to the 5th moment. It turns out that the dispersion in the moments decreases with the size of the manifold, making its application to very big systems statistically advantageous. A discussion of the method and these dispersion characteristics will be presented.


Author(s):  
Zhifeng Shao

A small electron probe has many applications in many fields and in the case of the STEM, the probe size essentially determines the ultimate resolution. However, there are many difficulties in obtaining a very small probe.Spherical aberration is one of them and all existing probe forming systems have non-zero spherical aberration. The ultimate probe radius is given byδ = 0.43Csl/4ƛ3/4where ƛ is the electron wave length and it is apparent that δ decreases only slowly with decreasing Cs. Scherzer pointed out that the third order aberration coefficient always has the same sign regardless of the field distribution, provided only that the fields have cylindrical symmetry, are independent of time and no space charge is present. To overcome this problem, he proposed a corrector consisting of octupoles and quadrupoles.


Author(s):  
Oktay Arda ◽  
Ulkü Noyan ◽  
Selgçk Yilmaz ◽  
Mustafa Taşyürekli ◽  
İsmail Seçkin ◽  
...  

Turkish dermatologist, H. Beheet described the disease as recurrent triad of iritis, oral aphthous lesions and genital ulceration. Auto immune disease is the recent focus on the unknown etiology which is still being discussed. Among the other immunosupressive drugs, CyA included in it's treatment newly. One of the important side effects of this drug is gingival hyperplasia which has a direct relation with the presence of teeth and periodontal tissue. We are interested in the ultrastructure of immunocompetent target cells that were affected by CyA in BD.Three groups arranged in each having 5 patients with BD. Control group was the first and didn’t have CyA treatment. Patients who had CyA, but didn’t show gingival hyperplasia assembled the second group. The ones displaying gingival hyperplasia following CyA therapy formed the third group. GMC of control group and their granules are shown in FIG. 1,2,3. GMC of the second group presented initiation of supplementary cellular activity and possible maturing functional changes with the signs of increased number of mitochondria and accumulation of numerous dense cored granules next to few normal ones, FIG. 4,5,6.


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