scholarly journals S/words versus S/words: A Bidirectional Reading of the Post/colonial Fictions

sjesr ◽  
2021 ◽  
Vol 4 (1) ◽  
pp. 247-256
Author(s):  
Saleem Akhtar Khan ◽  
Muhammad Ehsan ◽  
Nasar Iqbal

The article explicates the polemical schema of the novels produced by the British and the Indian writers apropos the historical event of the anticolonial rebellion/ revolution (1857). Grounded in the idea of creating a dialogue between the colonial and counter discursive texts, the research invokes Richard Lane’s bidirectional approach to explain how conflictual political visions trigger the skewed versions of the great defiance. The novelists of both nations have produced prolific fictional yields to represent the epic event. However, keeping in mind the scope of the study, the researchers have delimited their focus upon two of the representative novels, one for each nation: Louis Tracy’s The Red Year: A Story of the Indian Mutiny (1907) for the English version and Basavaraj Naikar’s The Sun behind the Cloud (2001) for the Indian one. Each of the novels voices the sloganized rhetoric of the respective nation while narrating the colossal clash, that is, Tracy portrays the mutiny as nefarious recalcitrance of the Indian rebels to disrupt the civilizational program and Naikar presents it as an auspicious act of defiance against the exploitative encroachment of the usurpers. A comparison has been drawn between the ideology-ridden discursive patterns of both the belligerent narratives and an intriguing concatenation of the diametric contrasts has been identified. The essential argument of the article is entrenched in the postcolonial and the new historicist notions vis-à-vis the chequered nature of the textual narratives and politicized parlance of the discursive records of the historical happenings.

Ramus ◽  
1982 ◽  
Vol 11 (1) ◽  
pp. 48-56 ◽  
Author(s):  
J. G. MacQueen

Somebody mentioned your fate, Heraclitus, and he brought me to a tear; and I remembered how often we both made the sun sink in conversation. But you, my guest-friend from Halicarnassus, have, I suppose, been ashes for a very long time. But your nightingales are alive, on which Hades, plunderer of all things, will not lay his hand.This epigram of Callimachus is one of the best known poems in Classical literature, but it suffers more than most from the misfortune of having to live permanently in the shadow of its own translation. It may no longer be the case that every schoolboy knows ‘They told me, Heraclitus, they told me you were dead’, but it is certainly true that Cory's English version is much more widely known, and much more widely quoted, than Callimachus's Greek original. One result of this has been that a good deal of attention has often been given to comparing the two poems, but little time has been spent on examining the Callimachus as a poem in itself in an effort to see what its virtues are. One may occasionally find a few remarks on the restraint or simplicity of the Greek, as opposed to the English, or a note suggesting that Heraclitus of Halicarnassus, the poet to whom the verses are addressed, wrote a volume of verse the title of which was actuallyAēdones(‘Nightingales’) — hence the ‘nightingales’ of the second last line. Occasionally a commentator will go a little further. K. J. Mckay for instance remarks: ‘The high respect in which this epigram is held is fully justified. The way in which the thoughts spill over their barriers in the first four lines, the magic ofkatedusamen(suggestive of a communion of uncommon power), the skilful location of key thoughts (teon moron, katedusamen, aēdones), the pathos of an unknown grave and an abiding grief cannot but move us. Above all, the suggestion of unfathomable sorrow.’


Author(s):  
David Woolf Marks

This chapter presents a sermon unusual for David Woolf Marks, as a response to a specific historical event. The background to this address was the outbreak of violence on the Indian subcontinent in May 1857, soon called the ‘Indian Mutiny’. The chapter compares the content of Marks' sermon to that of the Christian preachers of the day. Conversely, it shows how Marks emphasizes a theme that is understandably missing from the Christian preachers, who took it for granted: solidarity with Christian neighbours and the patriotism of the Jews of Britain. The other polemical thrust of the sermon is the reference to ‘whatever opinions we may entertain with respect to the causes which have produced this serious rebellion’. And throughout the text, there are passages that reveal the rhetorical power for which Marks was known.


Author(s):  
Dr. Ghada Fayez Abu-Enein

This research delves within the novel Men in the Sun by Ghassan Kanafani, in order to analyze the effect of colonialism on the Palestinian identity. Following what happened to the characters that are presented in the novel after colonization; these characters resemble and present different segments of the Palestinian. This research also includes a deep description of the harsh circumstances that faced each character. Firstly, this research starts with the analysis of each character individually. Secondly, it shows the mutual suffering between all characters. Finally, it ends with the tragic end of all characters. Return to Haifa is also another work for Kanafani. It discusses the conflict that rises within the soul of the colonized as a result of colonialism. This is the focal point for both works. The theory of post-colonialism is the most prominent theory in works of Kanafani. Post-colonial theory describes what happens to the refugees after colonization.


1966 ◽  
Vol 24 ◽  
pp. 40-43
Author(s):  
O. C. Wilson ◽  
A. Skumanich

Evidence previously presented by one of the authors (1) suggests strongly that chromospheric activity decreases with age in main sequence stars. This tentative conclusion rests principally upon a comparison of the members of large clusters (Hyades, Praesepe, Pleiades) with non-cluster objects in the general field, including the Sun. It is at least conceivable, however, that cluster and non-cluster stars might differ in some fundamental fashion which could influence the degree of chromospheric activity, and that the observed differences in chromospheric activity would then be attributable to the circumstances of stellar origin rather than to age.


1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1997 ◽  
Vol 161 ◽  
pp. 761-776 ◽  
Author(s):  
Claudio Maccone

AbstractSETI from space is currently envisaged in three ways: i) by large space antennas orbiting the Earth that could be used for both VLBI and SETI (VSOP and RadioAstron missions), ii) by a radiotelescope inside the Saha far side Moon crater and an Earth-link antenna on the Mare Smythii near side plain. Such SETIMOON mission would require no astronaut work since a Tether, deployed in Moon orbit until the two antennas landed softly, would also be the cable connecting them. Alternatively, a data relay satellite orbiting the Earth-Moon Lagrangian pointL2would avoid the Earthlink antenna, iii) by a large space antenna put at the foci of the Sun gravitational lens: 1) for electromagnetic waves, the minimal focal distance is 550 Astronomical Units (AU) or 14 times beyond Pluto. One could use the huge radio magnifications of sources aligned to the Sun and spacecraft; 2) for gravitational waves and neutrinos, the focus lies between 22.45 and 29.59 AU (Uranus and Neptune orbits), with a flight time of less than 30 years. Two new space missions, of SETI interest if ET’s use neutrinos for communications, are proposed.


1997 ◽  
Vol 161 ◽  
pp. 707-709 ◽  
Author(s):  
Jun Jugaku ◽  
Shiro Nishimura

AbstractWe continued our search for partial (incomplete) Dyson spheres associated with 50 solar-type stars (spectral classes F, G, and K) within 25 pc of the Sun. No candidate objects were found.


2000 ◽  
Vol 179 ◽  
pp. 263-264
Author(s):  
K. Sundara Raman ◽  
K. B. Ramesh ◽  
R. Selvendran ◽  
P. S. M. Aleem ◽  
K. M. Hiremath

Extended AbstractWe have examined the morphological properties of a sigmoid associated with an SXR (soft X-ray) flare. The sigmoid is cospatial with the EUV (extreme ultra violet) images and in the optical part lies along an S-shaped Hαfilament. The photoheliogram shows flux emergence within an existingδtype sunspot which has caused the rotation of the umbrae giving rise to the sigmoidal brightening.It is now widely accepted that flares derive their energy from the magnetic fields of the active regions and coronal levels are considered to be the flare sites. But still a satisfactory understanding of the flare processes has not been achieved because of the difficulties encountered to predict and estimate the probability of flare eruptions. The convection flows and vortices below the photosphere transport and concentrate magnetic field, which subsequently appear as active regions in the photosphere (Rust & Kumar 1994 and the references therein). Successive emergence of magnetic flux, twist the field, creating flare productive magnetic shear and has been studied by many authors (Sundara Ramanet al.1998 and the references therein). Hence, it is considered that the flare is powered by the energy stored in the twisted magnetic flux tubes (Kurokawa 1996 and the references therein). Rust & Kumar (1996) named the S-shaped bright coronal loops that appear in soft X-rays as ‘Sigmoids’ and concluded that this S-shaped distortion is due to the twist developed in the magnetic field lines. These transient sigmoidal features tell a great deal about unstable coronal magnetic fields, as these regions are more likely to be eruptive (Canfieldet al.1999). As the magnetic fields of the active regions are deep rooted in the Sun, the twist developed in the subphotospheric flux tube penetrates the photosphere and extends in to the corona. Thus, it is essentially favourable for the subphotospheric twist to unwind the twist and transmit it through the photosphere to the corona. Therefore, it becomes essential to make complete observational descriptions of a flare from the magnetic field changes that are taking place in different atmospheric levels of the Sun, to pin down the energy storage and conversion process that trigger the flare phenomena.


2000 ◽  
Vol 179 ◽  
pp. 193-196
Author(s):  
V. I. Makarov ◽  
A. G. Tlatov

AbstractA possible scenario of polar magnetic field reversal of the Sun during the Maunder Minimum (1645–1715) is discussed using data of magnetic field reversals of the Sun for 1880–1991 and the14Ccontent variations in the bi-annual rings of the pine-trees in 1600–1730 yrs.


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