scholarly journals The Lahars of the South-East slope of Mount Cameroon: geological study, economic interest and impacts of their exploitation on the environment

Author(s):  
Joseph Legrand TCHOP ◽  
Victor METANG ◽  
Jacques DİLİ-RAKE ◽  
Gaelle NANA ◽  
Pauline WOKWENMENDAM NGUET ◽  
...  
OALib ◽  
2019 ◽  
Vol 06 (04) ◽  
pp. 1-22
Author(s):  
Richard Ayuk Akoachere ◽  
Edwin Ngwene Etone ◽  
Roy Lyonga Mbua ◽  
Marcelle Pami Ngassam ◽  
Simon Ngomba Longonje ◽  
...  

2017 ◽  
Vol 09 (12) ◽  
pp. 1526-1546
Author(s):  
Anatole E. Djieto Lordon ◽  
Christopher M. Agyingi ◽  
Veronica E. Manga ◽  
Nenita N. Bukalo ◽  
Etienne T. Beka

1977 ◽  
Vol 81 ◽  
pp. 15-33
Author(s):  
F Ulff-Møller

In the area between Hammers Dal and Gieseckes Dal on north-west Disko (fig. 10) several native iron bearing intrusions have been found over the years (Münther, 1952, 1973; Pedersen, 1975a). Most of these intrusions were formed at shallow depths as volcanic necks of.iron-bearing, highly contaminated intermediate rocks, which probably served as feeders for the lavas of the Niaqússat member ofthe Maligât Formation (Pedersen, 1975a). In addition a series of interconnected subvolcanic intrusions of a very unusual type - the Hammers Dal Complex (Pedersen, 1975a) - were found in 1972 in the south-facing slopes of Hammers Dal extending a few kilometres towards the north-north-wesl (fig. 11 and Plate 2). Nickel and copper-bearing pyrrhotite mineralization was associated with the wall rock of the intrusions and cumu.late zones of native iron were found in the intllJsions themelves. As these were of potential economic interest a detailed investigation of the complex was desirable. [A preliminary description of the Hammer Dal Complex has aiready been given by Ulff-Møller (1975)].


1962 ◽  
Vol 24 (2) ◽  
pp. 303-322 ◽  
Author(s):  
Bernard Cosman
Keyword(s):  

2000 ◽  
Vol 179 ◽  
pp. 201-204
Author(s):  
Vojtech Rušin ◽  
Milan Minarovjech ◽  
Milan Rybanský

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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