Density distribution in the Earth

Author(s):  
E. D. Williamson ◽  
L. H. Adams
2018 ◽  
Vol 8 (1) ◽  
pp. 14-17 ◽  
Author(s):  
L.E. Sjöberg ◽  
M.S.S. Joud

Abstract In 1962 A. Bjerhammar introduced the method of analytical continuation in physical geodesy, implying that surface gravity anomalies are downward continued into the topographic masses down to an internal sphere (the Bjerhammar sphere). The method also includes analytical upward continuation of the potential to the surface of the Earth to obtain the quasigeoid. One can show that also the common remove-compute-restore technique for geoid determination includes an analytical continuation as long as the complete density distribution of the topography is not known. The analytical continuation implies that the downward continued gravity anomaly and/or potential are/is in error by the so-called topographic bias, which was postulated by a simple formula of L E Sjöberg in 2007. Here we will numerically test the postulated formula by comparing it with the bias obtained by analytical downward continuation of the external potential of a homogeneous ellipsoid to an inner sphere. The result shows that the postulated formula holds: At the equator of the ellipsoid, where the external potential is downward continued 21 km, the computed and postulated topographic biases agree to less than a millimetre (when the potential is scaled to the unit of metre).


1986 ◽  
Vol 87 (1) ◽  
pp. 123-141 ◽  
Author(s):  
F. Sansò ◽  
R. Barzaghi ◽  
C. C. Tscherning

Science ◽  
1968 ◽  
Vol 160 (3826) ◽  
pp. 442-442
Author(s):  
F. Press

2011 ◽  
Vol 29 (12) ◽  
pp. 2211-2217 ◽  
Author(s):  
J. H. Zoennchen ◽  
J. J. Bailey ◽  
U. Nass ◽  
M. Gruntman ◽  
H. J. Fahr ◽  
...  

Abstract. Terrestrial exospheric atomic hydrogen (H) resonantly scatters solar Lyman-α (121.567 nm) radiation, observed as the glow of the H-geocorona. The Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS) satellites are equiped with two Lyman-α line-of-sight Detectors (LADs) each. Since during the past solar minimum conditions the relevant solar control parameters practically did not vary, we are using LAD data between June and September 2008 to create a time averaged hydrogen geocorona model representative for these solar minimum conditions. In this averaged model we assume that the H-geocorona is longitudinally symmetric with respect to the earth-sun line. We find a 3-dimensional H-density distribution in the range from 3 to 8 earth radii which with some caution can also be extrapolated to larger distances. For lower geocentric distances than 3 earth radii a best fitting r-dependent Chamberlain (1963)-like model is adapted. Main findings are larger than conventionally expected H-densities at heights above 5 RE and a pronounced day-to-night side H-density asymmetry. The H-geocorona presented here should serve as a reference H-atmosphere for the earth during solar minimum conditions.


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