Colonial violence and civilising utopias in the French and British empires: the Morant Bay Rebellion (1865) and the Insurrection of the South (1870)

Debates on the relevance of repatriation of indigenous human remains are water under the bridge today. Yet, a genuine will for dialogue to work through colonial violence is found lacking in the European public sphere. Looking at local remembrance of the Majimaji War (1905–7) in the south of Tanzania and a German–Tanzanian theatre production, it seems that the spectre of colonial headhunting stands at the heart of claims for repatriation and acknowledgement of this anti-colonial movement. The missing head of Ngoni leader Songea Mbano haunts the future of German–Tanzanian relations in heritage and culture. By staging the act of post-mortem dismemberment and foregrounding the perspective of descendants, the theatre production Maji Maji Flava offers an honest proposal for dealing with stories of sheer colonial violence in transnational memory.

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Presidential Republicanism in the South, 1960

The Journal of Politics ◽

10.1017/s002238160001656x ◽

1962 ◽

Vol 24 (2) ◽

pp. 303-322 ◽

Cited By ~ 3

Author(s):

Bernard Cosman

Keyword(s):

The South

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Long-term Cyclic Variations of Prominences, Green and Red Coronae over Solar Cycles

International Astronomical Union Colloquium ◽

10.1017/s0252921100064496 ◽

2000 ◽

Vol 179 ◽

pp. 201-204

Author(s):

Vojtech Rušin ◽

Milan Minarovjech ◽

Milan Rybanský

Keyword(s):

Emission Lines ◽

High Latitudes ◽

Green Line ◽

Solar Cycles ◽

The South ◽

Coronal Emission ◽

Local Maxima ◽

The North ◽

Cyclic Variations

AbstractLong-term cyclic variations in the distribution of prominences and intensities of green (530.3 nm) and red (637.4 nm) coronal emission lines over solar cycles 18–23 are presented. Polar prominence branches will reach the poles at different epochs in cycle 23: the north branch at the beginning in 2002 and the south branch a year later (2003), respectively. The local maxima of intensities in the green line show both poleward- and equatorward-migrating branches. The poleward branches will reach the poles around cycle maxima like prominences, while the equatorward branches show a duration of 18 years and will end in cycle minima (2007). The red corona shows mostly equatorward branches. The possibility that these branches begin to develop at high latitudes in the preceding cycles cannot be excluded.

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