Mudflow Flooding Simulation and Solution Proposal in a Valley in the South of Peru

Andrés V. Pérez; Reyna Huancara; Flor Cutire; Nataly Perez; Anai Perez

doi:10.2495/ei-v4-n3-262-275

Mudflow Flooding Simulation and Solution Proposal in a Valley in the South of Peru

International Journal of Environmental Impacts Management Mitigation and Recovery ◽

10.2495/ei-v4-n3-262-275 ◽

2021 ◽

Vol 4 (3) ◽

pp. 262-275

Author(s):

Andrés V. Pérez ◽

Reyna Huancara ◽

Flor Cutire ◽

Nataly Perez ◽

Anai Perez

Keyword(s):

The South

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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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