Reconnaissance geophysical studies of the geothermal system in southern Raft River Valley, Idaho

Geophysics ◽  
1978 ◽  
Vol 43 (7) ◽  
pp. 1470-1484 ◽  
Author(s):  
Don R. Mabey ◽  
Donald B. Hoover ◽  
James E. O’Donnell ◽  
Carol W. Wilson

Gravity, aeromagnetic, and telluric current surveys in the southern Raft River have been used to infer the structure and the general lithology underlying the valley. The gravity data indicate the approximate thickness of the Cenozoic rocks and location of the larger normal faults, and the aeromagnetic data indicate the extent of the major Cenozoic volcanic units. The relative ellipse area contour map compiled from the telluric current survey generally conforms to the gravity map except for lower values in the area of the geothermal system. An area of low apparent resistivity values defined by the audiomagnetotelluric (AMT) survey appears to outline the extent of the geothermal reservoir even though the reservoir is deeper than the penetration of the survey. Self‐potential anomalies relate to near surface hydrology. The Raft River Valley is underlain by about 2 km of Cenozoic rock, most of which is Tertiary sediments of the Salt Lake formation. On the west side of the valley the Tertiary rocks appear to be separated from the underlying Precambrian basement by a low angle fault along which the Tertiary rocks have slid off a buried basement dome. Subsequent normal faults displace both the basement surface and the Tertiary beds. The geothermal system occurs where these north‐trending faults intersect a poorly understood northeast‐trending zone that may be a basement shear zone. Apparently deep circulating water at a temperature of about 150°C rises in the area of this intersection and then spreads laterally in porous zones near the base of the Tertiary rocks to form the geothermal reservoir. Upward leakage from the reservoir produces shallower effects that were measured by the AMT survey.

Author(s):  
Changjiang Zhou ◽  
Jianghai Xia ◽  
Jingyin Pang ◽  
Feng Cheng ◽  
Xinhua Chen ◽  
...  

2014 ◽  
Vol 644-650 ◽  
pp. 2670-2673
Author(s):  
Jun Wang ◽  
Xiao Hong Meng ◽  
Fang Li ◽  
Jun Jie Zhou

With the continuing growth in influence of near surface geophysics, the research of the subsurface structure is of great significance. Geophysical imaging is one of the efficient computer tools that can be applied. This paper utilize the inversion of potential field data to do the subsurface imaging. Here, gravity data and magnetic data are inverted together with structural coupled inversion algorithm. The subspace (model space) is divided into a set of rectangular cells by an orthogonal 2D mesh and assume a constant property (density and magnetic susceptibility) value within each cell. The inversion matrix equation is solved as an unconstrained optimization problem with conjugate gradient method (CG). This imaging method is applied to synthetic data for typical models of gravity and magnetic anomalies and is tested on field data.


2021 ◽  
Vol 48 (2) ◽  
pp. 273-284
Author(s):  
A. M. Plyusnin ◽  
A. V. Ukraintsev ◽  
M. K. Chernyavskii ◽  
E. G. Peryazeva ◽  
N. A. Angakhaeva
Keyword(s):  

First Break ◽  
2008 ◽  
Vol 26 (10) ◽  
Author(s):  
D. Colombo ◽  
M. Cogan ◽  
S. Hallinan ◽  
M. Mantovani ◽  
M. Virgilio ◽  
...  

Geothermics ◽  
2020 ◽  
Vol 85 ◽  
pp. 101795
Author(s):  
Justus Maithya ◽  
Yasuhiro Fujimitsu ◽  
Jun Nishijima

The variations in speed of the orbiting Apollo spacecraft as observed from Earth-based radiometric data have provided a direct measure of the local gravitational field. The gravity data were used to infer mass distributions that relate to topography in varying degrees. The mascons exist as mass excesses in topographic lows in all the near-side ringed basins and are best represented as near surface disks with excess loads of 800 kg/cm2. Large 100 km size craters like Langrenus, Theophilus, and Copernicus have mass deficits that are consistent with the craters’ volumes. Both of these results imply a relatively rigid surface layer that allowed little isostatic adjustment over lunar time. However, the Apennine mountains, presumably formed at the time of the Imbrium impact event, reveal only a small gravitational anomaly compared to their topographic size. This suggests that at this era the Moon was more plastic and isostatically compensated. By using the orbital element history of the subsatellites, the first realistic far-side field has been determined. The far-side ringed basins are mass deficits consistent with the lack of maria filling. The 2 km centre-ofgravity offset from the geometric centre implies a thicker far-side crust that possibly prevented far-side maria flooding. The homogeneity parameter (C/MR2) is near that of a homogeneous sphere having possibly a small core with a slight density increase towards its centre.


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