News

CALL FOR PAPERS DECEMBER 2024

IJSAR going to launch new issue Volume 05, Issue 12, December 2024; Open Access; Peer Reviewed Journal; Fast Publication. Please feel free to contact us if you have any questions or comments send email to: editor@scienceijsar.com

IMPACT FACTOR: 6.673

Submission last date: 15th December 2024

Interpretation of aeromagnetic data of Oyo area, Southwesthern Nigeria

×

Error message

  • Notice: Trying to access array offset on value of type int in element_children() (line 6609 of /home1/sciensrd/public_html/scienceijsar.com/includes/common.inc).
  • Notice: Trying to access array offset on value of type int in element_children() (line 6609 of /home1/sciensrd/public_html/scienceijsar.com/includes/common.inc).
  • Deprecated function: implode(): Passing glue string after array is deprecated. Swap the parameters in drupal_get_feeds() (line 394 of /home1/sciensrd/public_html/scienceijsar.com/includes/common.inc).
Author: 
Egbeyale Godwin, B., Ogunseye Titus, T., Adegbenro S. Ajani and Adekunle K. Bello
Page No: 
3579-3587

The study presents aeromagnetic data interpretation which involves the interpretation of aeromagnetic data features. Due to Magnetic properties of the earth crust, aeromagnetic anomalies over Oyo town are evaluated to map the magnetic lineaments and estimate the depth to the basement. The aeromagnetic data, from the study area sheet 241 Oyo, acquired were subjected to various filtering and processing technique which in turn properly displays the magnetic anomalies and magnetic intensities. Butterworth was applied to improve the signal to noise ratio, to reduce magnetic equator to properly position anomalies and to remove grappling effects. Gaussian filter was also applied to remove the regional effects thus leaving only the residual anomalies. Other processing techniques such as Upward continuation of 500m, 1000m, 1500m and 2000m, derivatives in x, y directions, analytic signal to delineate magnetically active zones, averaged power spectrum, Euler Deconvolution. The result shows that the depth to the top of the deepest magnetic source of about 2.3 km, depth to the shallow source ranges from 0.25 to 0.5km The obtained data shows that there is an abundance of positive anomalies that correspond to the migmatite-gneiss complex which is of moderate intensity. Derivatives in x, y and z directions revealed the parallel to sub-parallel lineaments which generally trends NE-SW direction except for major lineament that cuts through the migmatite-gneiss complex which trends in NW-SE direction. All these observations were made from qualitative and quantitative data interpretations, which in turn support magnetic information of the area.

Download PDF: