2016
DOI: 10.1016/j.jappgeo.2016.08.005
|View full text |Cite
|
Sign up to set email alerts
|

Mineral magnetic characteristics of the late Quaternary coastal red sands of Bheemuni, East Coast (India)

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1

Citation Types

0
2
0

Year Published

2018
2018
2024
2024

Publication Types

Select...
4

Relationship

1
3

Authors

Journals

citations
Cited by 4 publications
(2 citation statements)
references
References 47 publications
0
2
0
Order By: Relevance
“…The weathering of volcanic rocks in a sub-aerial oxidizing environment alters coarser ferrimagnetic titano-(magnetite) particles into smaller fine superparamagnetic (SP)-SD ferrimagnetic particles and produces secondary iron oxides such as maghemite and hematite through oxidation and structural inversion 21 , 41 . The fine pigmentary hematite particles are often attributed to the red color of the soils and sediments, and can also form through chemical precipitation via hydrolysis during sub-aerial chemical weathering 41 , 42 . The magnetic analysis on clay separates indicates that the hematite is mainly associated with finer fractions in the WRGR red clay, and might have formed from the chemical precipitation during the chemical weathering of the WRGR volcanic rocks.…”
Section: Discussionmentioning
confidence: 99%
“…The weathering of volcanic rocks in a sub-aerial oxidizing environment alters coarser ferrimagnetic titano-(magnetite) particles into smaller fine superparamagnetic (SP)-SD ferrimagnetic particles and produces secondary iron oxides such as maghemite and hematite through oxidation and structural inversion 21 , 41 . The fine pigmentary hematite particles are often attributed to the red color of the soils and sediments, and can also form through chemical precipitation via hydrolysis during sub-aerial chemical weathering 41 , 42 . The magnetic analysis on clay separates indicates that the hematite is mainly associated with finer fractions in the WRGR red clay, and might have formed from the chemical precipitation during the chemical weathering of the WRGR volcanic rocks.…”
Section: Discussionmentioning
confidence: 99%
“…They also appear to have originated from fluvial and coastal dunes and are located about +12 m from the present sea level, indicating the strength of the aeolian processes (Gardner, 1995;Rao et al, 2006). Chronological data from the Indian red dunes suggests that they could have been deposited post LGM (Rao et al, 2006;Srivastava et al, 2016).…”
Section: Pleistocene Coastal Remarks and Evolutionmentioning
confidence: 99%