Stranded marine debris on the touristic beaches in the south of Bali Island, Indonesia: The spatiotemporal abundance and characteristic

2021 ◽  
Vol 173 ◽  
pp. 113026
Author(s):  
Yulianto Suteja ◽  
Agus Saleh Atmadipoera ◽  
Etty Riani ◽  
I Wayan Nurjaya ◽  
Dwiyoga Nugroho ◽  
...  
Keyword(s):  
2009 ◽  
Vol 58 (9) ◽  
pp. 1347-1355 ◽  
Author(s):  
Elodie Martinez ◽  
Keitapu Maamaatuaiahutapu ◽  
Vincent Taillandier

2022 ◽  
Vol 174 ◽  
pp. 113281
Author(s):  
Félix Ayala ◽  
Karen Castillo-Morales ◽  
Susana Cárdenas-Alayza
Keyword(s):  

2018 ◽  
Vol 137 ◽  
pp. 180-184 ◽  
Author(s):  
Ryan Andrades ◽  
Robson G. Santos ◽  
Jean-Christophe Joyeux ◽  
David Chelazzi ◽  
Alessandra Cincinelli ◽  
...  

2017 ◽  
Vol 122 (1-2) ◽  
pp. 420-425 ◽  
Author(s):  
Pablo Denuncio ◽  
María Agustina Mandiola ◽  
Sofía Belén Pérez Salles ◽  
Rodrigo Machado ◽  
Paulo H. Ott ◽  
...  

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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