• Fulltext


        Click here to view fulltext PDF

      Permanent link:

    • Keywords


      DSHA; PSHA; maximum magnitude; rupture characteristics; GMPE; SA; PGA.

    • Abstract


      A seismic hazard map of Kanpur city has been developed considering the region-specific seismotectonic parameters within a 500-km radius by deterministic and probabilistic approaches. The maximum probable earthquake magnitude \textit(Mmax) for each seismic source has been estimated by considering the regional rupture characteristics method and has been compared with the maximum magnitude observed \textit(Mobsmax), \textit(Mobsmax) + 0.5 and Kijko method. The best suitable ground motion prediction equations (GMPE) were selected from 27 applicable GMPEs based on the ‘efficacy test’. Furthermore, different weight factors were assigned to different Mmax values and the selected GMPE to calculate the final hazard value. Peak ground acceleration and spectral acceleration at 0.2 and 1 s were estimated and mapped for worstcase scenario and 2 and 10% probability of exceedance for 50 years. Peak ground acceleration (PGA) showed a variation from 0.04 to 0.36 g for DSHA, from 0.02 to 0.32 g and 0.092 to 0.1525 g for 2 and 10% probability in 50 years, respectively. A normalised site-specific design spectrum has been developed considering three vulnerable sources based on deaggregation at the city center and the results are compared with the recent 2011 Sikkim and 2015 Nepal earthquakes, and the Indian seismic code IS 1893.

    • Author Affiliations


      Anbazhagan P1 2 Ketan Bajaj1 Nairwita Dutta1 Sayed S R Moustafa2 3 Nassir S N Al-Arifi3

      1. Department of Civil Engineering, Indian Institute of Science, Bengaluru 560 012, India.
      2. King Saud University, Riyadh, Saudi Arabia.
      3. National Research Institute of Astronomy and Geophysics (NRIAG), Cairo 11421, Egypt.
    • Dates

  • Journal of Earth System Science | News

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

© 2017-2019 Indian Academy of Sciences, Bengaluru.