Europlanet Graz, 1-2 June Gerald Duma Central Institute for Meteorology and Geodynamics Vienna, Austria AN ELECTROMAGNETIC PROCESS REGULATES EARTHQUAKE ACTIVITY Workshop Earthquakes: Ground-based and Space Observations
Europlanet Graz, 1-2 June Studies performed 10-year research pogramme Several cooperations in Europe, Asia, America Effect verified for many earthquake zones worldwide Plausible interpretation and model
Europlanet Graz, 1-2 June Observations (1996) – daily range AUSTRIA M 2.5, Geomagnetic Observatory
Europlanet Graz, 1-2 June Duma, Vilardo (INGV), 1998 Geomagnetic Observatory Observations (1997) – daily range Mt. VESUVIUS volcanic eqs, area 10 x 10 km, 1.8 M 3.1, , 1400 events
Europlanet Graz, 1-2 June A seismic daily cycle Aristoteles Pliny the Elder, 79 A.D. eruption of Mt.Vesuvius Tams, 1926 Conrad, 1932 Shimshoni, 1972 Lipovics, 2000, 2005 Schekotov & Molchanov, 2005 Poorly investigated in recent decades, no interpretation given yet
Europlanet Graz, 1-2 June A seismic daily cycle 3 sub-periods 20th century AUSTRIA M 2.5 May 31 – June 18, 1997 Earthquake swarm in Austria, region IMST
Europlanet Graz, 1-2 June A seismic daily cycle Observed in many main seismic regions Earthquakes M 5 and M 6 A very powerful geodynamic process acting!
Europlanet Graz, 1-2 June Geomagnetic Observatory Obs WIK, comp N ‚ secular variation‘ AUSTRIA M 3.1 (Io 5°) Observations (1996) – long term
Europlanet Graz, 1-2 June Mechanism, models? Dependence on Local Time Process related to sun A mechanism which penetrates the whole Earth‘s lithosphere Tides ? No! High energy mechanism Can a few nT influence tectonic performance?
Europlanet Graz, 1-2 June The electromagnetic model Geomagnetic variations in a conductive lithosphere Maxwell‘s equations (E-H) ‚Telluric currents‘ associated with all natural geomagnetic variations (frequency range from min – solar cycle)
Europlanet Graz, 1-2 June The electromagnetic model Telluric currents and forces F = e. [ v e. B ] F... mechanic force vector e... electron charge v e... velocity vector B... magnetic field vector ‚Lorentz force‘ F B veve e
Europlanet Graz, 1-2 June The electromagnetic model Magnetic observatories monitor: H(t) ~ I H (t) ~ F V (t) vertical force
Europlanet Graz, 1-2 June The electromagnetic model r P1 P2 I2 ≠ I1 Regional mechanic moment, torque Tr
Europlanet Graz, 1-2 June The electromagnetic model The gradient of H(t) reflects the change of regional torque Tr(t) (azimuth Az) Torque axis P
Europlanet Graz, 1-2 June Energy – diurnal variation T = MM x H A large scale current field, covering 1/3 of the northern Earth‘s hemisphere The dayside Sq induced lithospheric current vortex (Chapman, Bartels, 1940; Matsushita, 1968)
Europlanet Graz, 1-2 June Energy – diurnal variation The mechanic moment of Sq for a single loop (Duma, Ruzhin, 2003) The example demonstrates: The deformation energy provided to the lithosphere by a single current loop, radius 1500 km and current 10 kA, is equivalent to the energy of an earthquake M 5,1.
Europlanet Graz, 1-2 June Energy – diurnal variation 60% of total moment concentrates in a 30° segment H I
Europlanet Graz, 1-2 June Modelling the electromagnetic effect Data for H(lat,long) to compute gradient Daily variation: hourly mean values Model of Sq telluric current vortex Regional observatory data (lat i, long i ) Long term: annual mean values Retrieved from IGRF, (grid data) Regional observatory data (lat i, long i )
Europlanet Graz, 1-2 June Case studies – Regions AustriaTaiwan CaliforniaBaikal region
Europlanet Graz, 1-2 June Case studies – Austria (M ≥ 3.2, Gradient H – N10W) Gradient H from IGRF10 ( ) Diurnal range Long term Gradient H from Sq-Model
Europlanet Graz, 1-2 June Case studies – Taiwan (M ≥ 5, Gradient H – N55E) Gradient H from IGRF10 ( ) Diurnal range Long term Gradient H from Sq-Model
Europlanet Graz, 1-2 June Case studies – Baikal area (M ≥ 5, Gradient H – N00E) Gradient H from IGRF10 ( ) Diurnal range Long term Gradient H from Sq-Model
Europlanet Graz, 1-2 June Case studies – California (M ≥ 6, Gradient H – N30E) Gradient H from IGRF10 ( ) Diurnal range Long term Gradient H from Sq-Model
Europlanet Graz, 1-2 June Case study – earthquakes – , M 5 S-ITALY IONIAN IS AEGEAN
Europlanet Graz, 1-2 June Case study – earthquakes IONIAN ISLANDS Seismic activity – Local Time M – 1989 (25 yrs, PDE) 1990 – 2003 (14 yrs, PDE) – M 5 n = 11 (PDE) Gradient H (N85E)
Europlanet Graz, 1-2 June Case study – earthquakes – 1980 (72 yrs, INGV) – M 5 n = 4 (PDE) – M 4.5 n = 11 (PDE) S-ITALY Seismic activity – Local Time M 5
Europlanet Graz, 1-2 June Case study – earthquakes Aegean Sea – M 5 n = 5 (PDE) Crete Aegean Sea vs. Crete Seismic activity – Local Time M – M 5 n = 4 (PDE) Aegean Sea / Strongest events : UT= lat=36.31° long=23.21° d=66 km M=6.7
Europlanet Graz, 1-2 June Case study – earthquakes Aegean M 4, n = 956 (NOA) Ionian Is M 4, n = 237 (NOA) Gradient H from IGRF10 AEGEAN vs. IONIAN IS Seismic activity – long term M 4
Europlanet Graz, 1-2 June Case study – earthquakes Ionian Is M 5, n = 36 (NOA) S-Italy M 5, n = 57 (INGV+PDE) S-ITALY vs. IONIAN IS Seismic activity – long term M 5
Europlanet Graz, 1-2 June Novel aspects External sources – causing geomagnetic variations - strongly influence seismic activity (trigger) Origins: solar radiation, ionosphere, Sq ; magnetic dynamo Answer to daily rhythm of seismic activity (LT) Monitoring the process: easy by geomagnetic observatories Predictability: systematic diurnal, seasonal, secular variations (IGRF 2010) Not yet investigated: influence of magnetic storms Faster monitoring of variations by space observations ?
Europlanet Graz, 1-2 June Observations (1997) – long term Duma, Vilardo (INGV), 1998 n: annual number of eqs M 1.8, sf: annual number of solar flares (10 3 ) Duma, Vilardo (INGV), 1998 Mt. VESUVIUS volcanic eqs, area 10 x 10 km, 1.8 M 3.1, , 1400 events
Europlanet Graz, 1-2 June Tectonic settings & faulting mechanisms in Greece (Dewey et al., 1973 / A. Tzanis, UOA, 2003)
Europlanet Graz, 1-2 June Model of Sq telluric current vortex Fits observed Sq-variations at observatories Computes grad H(LT)
Europlanet Graz, 1-2 June H – current density
Europlanet Graz, 1-2 June The electromagnetic model Magnetic observatories monitor horizontal force Fh C (t)
Europlanet Graz, 1-2 June Energy – diurnal variation Sq: solar controlled, heating, ionization, tides (Chapman, Bartels, 1940)