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Northern Hemisphere (NH) ozone flux to be significantly larger (approximately 24\%) than that calculated in the Southern<br />

Hemisphere (SH) during the year 2000. This diagnostic method makes it possible to separate dynamical aspects of transport<br />

from the seasonal cycle of ozone in the lowermost stratosphere and explain the hemispheric difference in the ozone flux. The<br />

SH total horizontal area of exchange is equal to or slightly greater than the area of exchange in the NH throughout an annual<br />

cycle. The mean changes in potential vorticity of parcels near the tropopause are also similar or slightly greater in the SH,<br />

suggesting that NH and SH downward total mass transport to the troposphere are comparable. These results imply that the<br />

greater NH ozone flux is mostly due to the amount of ozone available for exchange rather than net hemispheric dynamical<br />

differences near the tropopause level.<br />

Author<br />

Northern Hemisphere; Ozone; Southern Hemisphere; Tropopause; Wind (Meteorology)<br />

20030025440 NASA Goddard Space Flight Center, Greenbelt, MD, USA<br />

Co-Seismic Mass Dislocation and its Effect on Earth’s Rotation and Gravity<br />

Chao, B. F.; Gross, R. S.; January 2002; 1 pp.; In English; IERS Workshop on Combination Research and Global Geophysical<br />

Fluids, 18-21 Nov. 2002, Munich, Germany; No Copyright; Avail: Other Sources; Abstract Only<br />

Mantle processes often involve large-scale mass transport, ranging from mantle convection, tectonic motions, glacial<br />

isostatic adjustment, to tides, atmospheric and oceanic loadings, volcanism and seismicity. On very short time scale of less<br />

than an hour, co-seismic event, apart from the shaking that is the earthquake, leaves behind permanent (step-function-like)<br />

dislocations in the crust and mantle. This redistribution of mass changes the Earth’s inertia tensor (and hence Earth’s rotation<br />

in both length-of-day and polar motion), and the gravity field (in terms of spherical harmonic Stokes coefficients). The<br />

question is whether these effects are large enough to be of any significance. In this paper we report updated calculation results<br />

based on Chao & Gross (1987). The calculation uses the normal mode summation scheme, applied to nearly twenty thousand<br />

major earthquakes that occurred during 1976-2002, according to source mechanism solutions given by the Harvard Central<br />

Moment Tensor catalog. Compared to the truly large ones earlier in the century, the earthquakes we study are individually all<br />

too small to have left any discernible signature in geodetic records of Earth rotation or global gravity field. However, their<br />

collective effects continue to exhibit an extremely strong statistical tendencies. For example, earthquakes conspire to decrease<br />

J2 and J22 while shortening LOD, resulting in a rounder and more compact Earth. Strong tendency is also seen in the<br />

earthquakes trying to nudge the Earth rotation pole towards approximately 140 degrees E, roughly opposite to the observed<br />

polar drift direction. The geophysical significance and implications will be further studied.<br />

Author<br />

Earth Rotation; Gravitation; Seismology; Volcanology; Geophysics; Earth Mantle<br />

20030025661 NASA Goddard Space Flight Center, Greenbelt, MD, USA<br />

Time-Variable Gravity from Space: Quarter Century of Observations, Mysteries, and Prospects<br />

Chao, Benjamin F.; [2003]; 1 pp.; In English; Workshop on GPS Meteorology: Ground-Based and Space-Borne Applications,<br />

14-17 Jan. 2003, Tsukuba, Japan; No Copyright; Avail: Other Sources; Abstract Only<br />

Any large mass transport in the Earth system produces changes in the gravity field. Via the space geodetic technique of<br />

satellite-laser ranging in the last quarter century, the Earth’s dynamic oblateness J2 (the lowest-degree harmonic component<br />

of the gravity field) has been observed to undergo a slight decrease -- until around 1998, when it switched quite suddenly to<br />

an increase trend which has continued to date. The secular decrease in J2 has long been attributed primarily to the post-glacial<br />

rebound in the mantle; the present increase signifies an even larger change in global mass distribution whose J2 effect<br />

overshadows that of the post-glacial rebound, at least over interannual timescales. Intriguing evidences have been found in the<br />

ocean water distribution, especially in the extratropical Pacific basins, that may be responsible for this J2 change. New<br />

techniques based on satellite-to-satellite tracking will yield greatly improved observations for time-variable gravity, with much<br />

higher precision and spatial resolution (i.e., much higher harmonic degrees). The most important example is the GRACE<br />

mission launched in March 2002, following the success of the CHAMP mission. In addition, although less precise than<br />

GRACE, the GPS/Meteorology constellation mission COSMIC, with 6 mini-satellites to be launched in late 2005, is expected<br />

to provide continued and complementary time-variable gravity observations. Such observations are becoming a new and<br />

powerful tool for remote sensing of geophysical fluid processes that involve larger-scale mass transports.<br />

Author<br />

Earth Gravitation; Gravitational Fields; Satellite Laser Ranging; Mass Distribution; Gravity Anomalies; Mass Transfer<br />

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