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IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy (S) - IASPEI - International Association of Seismology and Physics of the Earth's Interior JSS017 Oral Presentation 2371 Thinning of hot indian lithosphere : causes and consequences Dr. O.P. Pandey Theoritical Geophysics National Geophysical Research Institute (NGRI) IASPEI Indian shield is unique and differs considerably from other stable areas of the earth. It has remained dynamic since at least late Archeans due to a number of long sustained tectonothermal events which repeatedly rejuvenated and remobilized the entire lithosphere. The continued reactivation over such a long period of time, which continues even now is not evident elsewhere. About two decades back, a preliminary attempt was made to study the thermal regime of the Indian lithosphere using the then available meager heat flow data set, which indicated the possibility of a quite thin and warm lithosphere beneath Indian shield. Since then, there has been a dramatic increase in heat flow numbers as well as new geological and geophysical informations. Consequently, the crustal structure is now better understood warranting a fresh look over the Indian shields thermal regime. Present study validates the presence of a thin lithosphere (average ~ 105 km compared to 250-300 km in similar terrains elsewhere) and a quite warm Moho with an average temperature close to 600oC beneath Indian cratonic shield. Thinning of the lithosphere has now been confirmed by recent multimode surface waveform tomographic and other geophysical studies. Beneath many of the late Archean segments, heat flow from the mantle exceeds 30 mW/m2. An interesting inference which emerges from this study is that beneath certain ancient cratons, where gravity bias is distinctly positive, Moho temperatures and mantle heat flow reaches as high as 800oC and 45 mW/m2 respectively with depth to the asthenosphere at only 65 km. It is felt that the long sustained reactivation may have led to the enrichment of lithophilic/radioactive elements at shallow mantle levels, which made it buoyant and fertile, thereby allowing for a thinner and weaker lithosphere. Such an order of thinning would result into the underlying lithosphere being subjected to a much higher insitu temperatures leading to sustained regional uplifting and exhumation of deeper crustal layers, which now appears to be so prevalent in the Indian shield. It may not be just a coincidence that almost all the catastrophic/damaging earthquakes which occurred since 1618 lie either on uplifted blocks or on their escarpment edges. Keywords: lithospheric thinning, mantle heatflow, moho temperatures
IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy (S) - IASPEI - International Association of Seismology and Physics of the Earth's Interior JSS017 Oral Presentation 2372 Characterising the influence of latent heat effects on GST history Prof. Christoph Clauser Applied Geophysics RWTH Aachen University IASPEI Darius Mottaghy In moderate and high latitudes, the signature in borehole temperatures due to past surface temperature variations can be significantly influenced by latent heat liberated or consumed by freezing or thawing pore water, respectively. The magnitude of the effect depends on several parameters, most important porosity, but also the present-day and past ground surface temperature (GST), and basal heat flow. Depending on the depth of available borehole temperatures, we studied the impact on short term GST history inversions, as well as long term histories as far back as to the last glaciation. The influence of different parameters is investigated by generating a number of synthetic temperature logs and inverting them for ground surface temperature histories by a regularised Tikhonov inversion scheme. To this end we used a simple step forcing function. These simulations are performed both with and without latent heat effects. Regarding long-term GST history reconstructions and in view of possible corrections applied to inversions which neglect the latent heat effect, we find the difference between present-day and glaciation temperatures useful to quantify this effect. To illustrate possible corrections, we plot the dependence of this temperature difference (as a function of the latent heat effect) versus porosity, basal heat flow, present-day and past GST. Depending on parameter combination and present-day surface temperature, the neglect of freezing and thawing processes results in an overestimation of the postglacial warming of up to 4 K. We also studied the impact of the latent heat effect on GST history inversions on shorter time scales. Using a simplified, synthetic model for the temperature variations within the last 1000 years, we find that amplitude and duration of the cool period of the Little Ice Age and the recent warming are not large enough to cause a significant influence of the latent heat effect. However, neglect of this effect results in a clearly deteriorated timing. Keywords: paleoclimate, borehole temperature, inversion
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IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy<br />
(S) - <strong>IASPEI</strong> - International Association of Seismology and Physics of the Earth's<br />
Interior<br />
JSS017 Oral Presentation 2371<br />
Thinning of hot indian lithosphere : causes and consequences<br />
Dr. O.P. Pandey<br />
Theoritical Geophysics National Geophysical Research Institute (NGRI) <strong>IASPEI</strong><br />
Indian shield is unique and differs considerably from other stable areas of the earth. It has remained<br />
dynamic since at least late Archeans due to a number of long sustained tectonothermal events which<br />
repeatedly rejuvenated and remobilized the entire lithosphere. The continued reactivation over such a<br />
long period of time, which continues even now is not evident elsewhere. About two decades back, a<br />
preliminary attempt was made to study the thermal regime of the Indian lithosphere using the then<br />
available meager heat flow data set, which indicated the possibility of a quite thin and warm lithosphere<br />
beneath Indian shield. Since then, there has been a dramatic increase in heat flow numbers as well as<br />
new geological and geophysical informations. Consequently, the crustal structure is now better<br />
understood warranting a fresh look over the Indian shields thermal regime. Present study validates the<br />
presence of a thin lithosphere (average ~ 105 km compared to 250-300 km in similar terrains<br />
elsewhere) and a quite warm Moho with an average temperature close to 600oC beneath Indian<br />
cratonic shield. Thinning of the lithosphere has now been confirmed by recent multimode surface<br />
waveform tomographic and other geophysical studies. Beneath many of the late Archean segments,<br />
heat flow from the mantle exceeds 30 mW/m2. An interesting inference which emerges from this study<br />
is that beneath certain ancient cratons, where gravity bias is distinctly positive, Moho temperatures and<br />
mantle heat flow reaches as high as 800oC and 45 mW/m2 respectively with depth to the<br />
asthenosphere at only 65 km. It is felt that the long sustained reactivation may have led to the<br />
enrichment of lithophilic/radioactive elements at shallow mantle levels, which made it buoyant and<br />
fertile, thereby allowing for a thinner and weaker lithosphere. Such an order of thinning would result<br />
into the underlying lithosphere being subjected to a much higher insitu temperatures leading to<br />
sustained regional uplifting and exhumation of deeper crustal layers, which now appears to be so<br />
prevalent in the Indian shield. It may not be just a coincidence that almost all the<br />
catastrophic/damaging earthquakes which occurred since 1618 lie either on uplifted blocks or on their<br />
escarpment edges.<br />
Keywords: lithospheric thinning, mantle heatflow, moho temperatures