Maheswar Ojha

Dr. Maheswar Ojha

National Geophysical Research Institute, Hyderabad, India
orcid

Research Focus & Metrics

Academic Career Length

20Years (2007-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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8 June 2010 in Journal of Geophysical Research
Verified
Journal Article
Closed access
PDF file
RGRanjana Ghosh
Ranjana Ghosh
KSKalachand Sain
Kalachand Sain
Maheswar OjhaMaheswar Ojha
Maheswar Ojha

1 October 2019 in Marine and Petroleum Geology
Verified
Journal Article
Closed access
UYU.S. Yadav
U.S. Yadav
KSK.M. Shukla
K.M. Shukla
Maheswar OjhaMaheswar Ojha
Maheswar Ojha
PKPushpendra Kumar
Pushpendra Kumar
USUma Shankar
Uma Shankar

1 June 2012 in Journal of the Geological Society of India
Verified
Journal Article
Closed access
PDF file
KSKalachand Sain
Kalachand Sain
Maheswar OjhaMaheswar Ojha
Maheswar Ojha
NSNittala Satyavani
Nittala Satyavani
GRG. A. Ramadass
G. A. Ramadass
TRT. Ramprasad
T. Ramprasad
HGHarsh Gupta
Harsh Gupta

1 December 2009 in Episodes
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Journal Article
Open access
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Maheswar OjhaMaheswar Ojha
Maheswar Ojha
KSKalachand Sain
Kalachand Sain
Maheswar Ojha and Kalachand Sain. Episodes 2009;32:264-70. https://doi.org/10.18814/epiiugs/2009/v32i4/003

1 August 2008 in Marine and Petroleum Geology
Verified
Journal Article
Closed access
Maheswar OjhaMaheswar Ojha
Maheswar Ojha
KSKalachand Sain
Kalachand Sain

1 January 2010 in Geophysics
Verified
Journal Article
Closed access
Maheswar OjhaMaheswar Ojha
Maheswar Ojha
KSKalachand Sain
Kalachand Sain
TMTim MInshull
Tim MInshull
We estimate the saturations of gas hydrate and free gas based on measurements of seismic-reflection amplitude variation with offset (AVO) for a bottom-simulating reflector coupled with rock-physics modeling. When we apply the approach to data from a seismic line in the Makran accretionary prism in the Arabian Sea, the results reveal lateral variations of gas-hydrate and free-gas saturations of 4–29% and 1–7.5%, respectively, depending on the rock-physics model used to relate seismic velocity to saturation. Our approach is simple and easy to implement.