Journal of Geoscience and Environment Protection, 2014, 2, 99-107
Published Online June 2014 in SciRes. http://www.scirp.org/journal/gep
How to cite this paper: Li, Z. X. et al. (2014). Some Mass Migration Underground Found in Beijing Area. Journal of Geo-
science and Environment Protection, 2, 99-107. http://dx.doi.org/10.4236/gep.2014.23014
Some Mass Migration Underground Found
in Beijing Area
Zheng Xin Li1,2, Jin Song Ping1,2, Yong Zhang Yang1,2, Alexander Gusev1
1Key Laboratory of Lunar and Deep Space, National Astronomical Observatories, Chinese Academy of Sciences,
2Center of Astrodynamic Research, Shanghai Astronomical Observatory, Chinese Academy of Sciences,
Email: email@example.com, firstname.lastname@example.org
Received April 2014
The relationship between the change of a local gravity field and the mass migration underground
is discussed by means of using a point-source disturbed body as a substitute for the mass migra-
tion underground. Some significant local gravity field changes in Beijing area have been found,
from which the three parameters of the disturbed bodies, location, depth and mass, have been de-
rived successfully from the observations of a gravimetric network. In order to determine the
depth of a body, a new approach is suggested in which the gravity change difference is used in-
stead of the gravity change itself. The mass of a disturbing body has been estimated properly. As-
tronomical PZT is suggested for this kind of survey. The results provide us a picture of the under-
ground mass migration with which the gravity changes on the ground surface may be interpreted
in a better way. This additional information may be useful in seismological studies.
Component, Underground Mass Migration, Gravity Field, Earthquake, PZT
Gravity change and earthquake (Barnes, 1966), or furthermore, the relationship among gravity change, under-
ground mass migration and earthquake (Chen et al., 1979), is an interesting but unsolved problem for many
years (Chen et al., 2002). The China Beijing-Tianjin-Tangsh an-Zhangjiakou (BTTZ) gravimetric network was
established in 1980’s (Chen et al., 2002), and its observational data have been used heavily in studying the
problem (Gu et al., 1998; Kuo et al., 1993; Kuo et al., 1999; Jia et al., 1998; Li et al., 2001; Jia et al., 2006). Due
to the incompleteness of the network, which is based on the observations of relative gravimeter, the image of the
relationship among the gravity change, underground mass migration and earthquake is still not clear (Chen et al.,
The purpose of the paper is to find a new approach to study the problem. A point-source underground dis-
turbed body (UDB) is used to describe the underground mass migration and its relation to the gravity change on
ground is discussed. Some significant local gravity field changes (LGFC) have been found in Beijing area from
Z. X. Li et al.
which the related UDBs are studied. The three parameters of a UDB (location, depth and mass) are derived by a
new approach, including a special order to calculate them. First measure the location, second the depth, third the
mass; and then use the difference of gravity change in depth calculation instead of using the gravity change itself;
and the mass estimation is the last step. It is hoping that the results will be helpful in understanding the problems
mentioned above, as well as the related studies in seismology.
Assume a mass migration, limited both in depth and size, has taken place underground during a time period and
makes the local gravity field change. We use a point-source disturbed body underground, which is able to make
the same gravity field change, to describe it, and try to determine its three parameters: location, depth (H) and
An observer on ground, whose horizontal distance is D to the body site, will thus observe a gravity vector
change with module of Δg = GM/S2 (G-gravity constant), pointing to the body with distance of S (S = (D2 +
H2)1/2). A gravimeter observes the vertical element while the horizontal one can be deduced from the observa-
tion of an astronomical instrument. The vector is expressed by the following two elements in a vertical plane
(Zhang et al., 2002):
The vertical element is read as:
gv g/ /HS GMHS
The horizontal element, or the deflection of the vertical (DOV) is read as:
gh g/ /DS GMDS
The two unknowns of the underground disturbed body, the H and M, may be determined by the Δgv, as well
as the Δgh, observed at separate places to which the distances Ds are known.
Instead of using the Δgv, or Δgh, itself directly, the ratio of them at two sites, No.1 and 2, may be used as an
assumed “observation” Kv, or Kh, and use one of the following equations to calculate the unknown H:
gv gv//SSDHD H=∆ ∆==++Kv
() ()( )
ghgh// /( H/())DDSSDDDD H=∆ ∆=×=×++
in which, D1 and D2 are the known horizontal distances of the two observational sites.
The differential of Δgv may also be used in such a determination, which is derived as:
d / dgv3/3/gh
DGMDH SHS∆ =−=−×∆
thus we have:
gh d/dgvD∆= ×∆Khv
- 1/3/SH= ×Khv
The ratio Kdv of two Δgv differentials can be expressed as the following:
( )( )()()
d/dgv /d/dgv//DDDD SS= ∆∆=×Kdv
() () ()
d/dgv /d/dgv//DDDDDHD H= ∆∆=×++
from which the depth of the disturbed body (H) may also be calculated.
Having the H, the mass of the disturbed body M may then be calculated by the following equation but in term
of its ratio to Earth mass (ME):
from the Δgv
/gv/ g//MMSH SR=∆×∗
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from the Δgh
/gh / g//MMSD SR=∆×∗
in which RE is the Earth radius (6371 km), g0 is the gravity on ground (use g0 = 981 Gal), and ME = 5.9742 ×
In Figure 1, the maximum observed Δgv, while observer is just upside the body, is used as the unit (100%) in
showing the Δgv, Δgh and d/dD (Δgv); their horizontal distance to the body site is count by unit of H. It can be
seen that Δgh has a peak (38%) at the distance of 0.7H and becomes the same as the Δgv (36%) at distance of H,
then decreasing to less than 5% when D > 5H. If we use 5% as a standard of gathering observations with enough
sense, we may see that the area of meaningful Δgh observations (4.3H) is larger than that of the Δgv (2.5 H).
Khv (see Equation (7)) is also shown in Figure 1, but with a different scale, which varies within −8.66 to −0.33
while −5 < D < 5.
3. BTTZ Gravimetric Network and the Local Gravity Field Change
The BTTZ gravimetric network (Figure 2) is located in north China and has more than hundred network points,
2 - 4 batch repeated observations per year, high precision of observations, and its continuation since 1987 (Chen
et al., 2002; Li et al., 2005), are making it an appropriate place to study the problem of underground mass mi-
LaCoste & Romberg G model gravimeter are used in relative measurement between two neighboring network
points with precision of about ±7 ~ 10 micro Gal (Li et al., 2001). In addition, absolute gravimeter has also been
performed from time to time at some network points in order to connect the observations of different batches
together (Jia et al., 2006). Processing a batch observations, which have been completed in a short time, by the
National Standard (Liu et al., 1991) and takes their average time as the observational epoch of the batch; then
together, 46 batches of observations, which covers the period of 1987.25-1998.67, are reduced together in a
treatment, in which the possible drift of a gravimeter, the movement of some network points etc., have been de-
termined and corrected and an adjustment is done afterwards in order to combine the whole data set in a ho-
mogenous way in a time-space domain. Detail of this special treatment can be found in (Li et al., 2000).
Being gridded over the 5˚ (longitude) × 2˚ (latitude) area (Figure 2) to give 61 × 25 smoothed values, each of
the 46 batch gravity results is now considered as observations of the gravity field at its observational epoch.
From these 46 batch results, relative change of gravity field during the time of any two observational epochs
can be derived with which the existence of a LGFC, being related to an underground mass migration, is checked.
Quite the same as reported (Li et al., 2009), the LGFCs found are usually in pair, having almost the same shape
and size but opposite in sign, and usually related to the timing of an earthquake in the area (Li et al., 2009; Li et
al., 2011). Figure 3 shows two pairs of them: the LGFC(1)-LGFC(2) and the LGFC(3)-LGFC(4), of which the
correlation coefficients are –0.67 and –0.89 respectively.
It appears that the timing of these two pair LFGC results is related to the two earthquakes in the region (see
Figure 2), thus the LGFC(1) and LGFC(3) are called the LGFC before the earthquake, while the other two, the
LGFC(2) and LGFC(4), as the ones after the earthquake.
From Figure 3 the existence of a LGFC, which is related to an underground mass migration, is evident since
their magnitude of a signal is 30 - 50 micro Gal, several times the standard observational error of a measurement
(±7 - 10 micro Gal) which connects the middle network point and its neighboring points around, although hav-
ing some distortion in comparing to the standard one in Figure 1. Their flat top (see figures), having somewhat
reduced the signal size, is caused by a cutting of the figure at the middle network point (see figures above),
while the unbalance of the two sides of a signal is due to the measuring error between the middle network point
and those around. In the lower figures, displacement of the LGFC signal’s base line (dash-dot line) away from
the namely “zero” of gravity change is apparent (10 to 40 micro Gal), it is due to the limitation of the BTTZ
network which uses only relative gravimeter in batch observations. In such a case, a batch result is connected to
a special point of the BTTZ network where an absolute gravimeter is installed and operates all the time in order
to maintain an absolute reference for gravity measuring, but the connection between this special point and that
of any other points of the batch is measured by relative gravimeter observation. The displacement shown in the
figures is the accumulation of the observational errors related. Since the standard error of an observation is ±7 ~
10 micro Gal or so, its accumulation attains the magnitude of 10 - 40 micro Gal is quite possible in
Z. X. Li et al.
Figure 1. Relation of Δgv, Δgh, d/dD(Δgv) and Khv.
Figure 2. BTTZ gravimetric network, LGFC found, and the two earthquakes (M5.0: 1995.76; M4.6: 1998.29).
Z. X. Li et al.
Figure 3. Two pairs of LGFC result (unit of contour: micro Gal; ⊕-network point) and their W-E vertical sections (below).
practice, since the middle network point of a LGFC result is away from the special point for a distance of several
4. Determining an Underground Disturbed Body
As mentioned above, a point-source underground disturbed body (UDB) is used in the study to describe the un-
derground mass migration during a time period. A UDB determination means to measure its three parameters
from its related LGFC: location, depth and mass. With a contour map of the LGFC (Figure 3), it is easy to find
its location, even by eyes for example. To be more precise, one may use the vertical sections of a contour map to
do so. Its depth (H) is now suggested to use a new approach to calculate it (Equation (9)), instead of the Equa-
tion (3), since the gravity reference is already deviated from the real one (see Fig u re 3).
We use the LGFC (1) (1995.42-1995.67) as an example to show the detail of an H determination. Its vertical
section of 5′interval at latitude 40.17˚ and the gravity change difference of 1′ interval are shown in Figure 4 top
left image. The 16 points (83rd - 98th) of the time series of the latter (Figure 4 top right image) are now taking
part into the calculation. The detail of part of the calculation, related to the points (86th - 91st), is presented in
Table 1. Among these 6 points, the 89th is considered as the “No.1” (distance D1) in Equation (9) whiles the
other ones as the “No.2” (distance D2). Calculate one by one the ratio Kdv of the five points in considering the
89th as 100% (see the 3rd line of the table), together with their D2 (4th line), the five results of the depth H (5th
line) are obtained by the equation (9). There are 16 points taken part in the calculation, but two of them, the 83rd
and 88th, are used as reference points in the calculation. The derived 14 H results are now showing in Figure 4
middle right image. Their average is 15.75 ± 1.47 (km), which is the final result of the depth determination.
With the location established and the depth determined, now is the time that the mass can be calculated by the
observed gravity change at any point of which the distance D is known (see Equation (10)). Other points can be
calculated as well (see Figure 4 lower left image). An assumed correction (−10 micro Gal) is added to the de-
rived gravity values (see Figure 4 lower left image), which is due to the incompleteness of data mentioned
above. Altogether 7 of these corrected gravity change values have been used in the mass calculation; the results
are shown by the solid line in Figure 4 lower right image.
In order to have an estimation on the possible influence of using this assumed correction (−10 micro Gal), two
other corrections (−15 and −5 micro Gal) have also been used. The two dotted lines (upper and lower) represent
the results while −15 and −5 micro Gal is used accordingly. Although we are not sure of the exact amount of the
mass, the two dotted lines are telling us something about the possible range of its dispersion (Figure 4 below
right image). Due to the limit density of the network points, the actual observed maximum gravity changes are
usually reduced in size (see the four Figure 3 lower images), consequently the derived mass result would proba-
bly be under estimated. Considering the above points, it might be better to say that it is an estimation of the mass,
Z. X. Li et al.
Figure 4. Calculation of the depth (H) and the mass (M) in the case of LGFC(1).
Table 1. Calculating the depth (H) by the ratio K dv .
Point No. 86 87 88 89 90 91
gv) (micro Gal) 2.2041 2.6179 2.8343 2.8535 2.6752 2.3403
Kdv 1.2946 1.0900 1.0067 1.0000 1.0666 1.2193
D (km) 4.42 5.84 7.26 8.68 10.40 11.52
H (k m) 16.98 16.68 16.29 ------- 14.84 13.96
Average of the 14 determinations (km) 15.75 ± 1.47 (km)
which is of the order of about 0.3 × 10−12 (unit: Earth mass).
The depth and the mass derived from the other three LGFC results have also been obtained. A summary of
them together is given in Table 2.
In order to use gravity observations to study seismological phenomena in Beijing area, whether or not there is
real detectable mass migration underground in practice is one of the important problems to be studied.
The purpose of the paper is to show evidence that there are significant LGFC in the area, and it is possible to
describe the related mass migration (depth: several to 20 km; mass: of the order of 0.3 × 10−12 Earth mass) by
means of a point-source disturbed body. It is also possible to determine or estimate its three parameters (location,
depth and mass) in using appropriate approach.
As a first step of the study, we concentrate ourselves mainly on the mass migration of which the depth is less
than 20 km. In such a case, the problem can be discussed in a simplest way, considering the ground as a flat
plane. Hoping that the formulae used and the results obtained will be easier to be understood and accepted by
In the study one understands better the importance of a gravimetric network used, especially the density of its
network points. It can be seen in the contour maps (Figure 3) that the derived LGFC signal depends very much
on its distance to the nearest network point. Since a LGFC signal will reduce its size to only 36% at the distance
of the UDB depth H (see Figure 1), one may believe that other than the two pair LGFCs reported here, there
will be quite some other ones in Beijing area that cannot be detected by the network.
Rather than using gravity data directly, here an intermediate observable, the deflection of the vertical Δgh is
used in the approach. Local DOV not only can be estimated from gravity variation, but also can be observed by
optical astrometric method. It can substitute gravity survey if the deflection of the vertical is measured with
Z. X. Li et al.
higher accuracy and higher frequency. At the IAU General Assembly, Buenos Aires 1991, the Commission 19
of Rotation of the Earth made a decision of Application of Optical Astrometry Time and Latitude Programms,
that optical astrometric data previously used to measure the rotation of the Earth had been shown to measure the
variations in the deflection of the vertical, that the collected astrometric data contain valuable information on
star positions including radio stars, and recommended that optical astrometric data continue to be collected in
order to investigate the possibility of deriving long-term variations in the deflection of the vertical. In such a
situation, Li et al. (2005) succeeded in observing the longitudinal component of DOV at Beijing with the accu-
racy better than 0.05 seconds of arc, which can be corresponded to the variation of DOV derived from the grav-
ity surveys made at the network along Beijing.
For the optical astrometric technique, the Photographic Zenith Tube (PZT, see Figure 5) has played key role
since 1900 for observations of the Earth rotation, and it also has a potential to be applied for several other ob-
servations by taking advantage of automatic observations with self compensation of tilt of the tube. In the pro-
posed telescope ILOM (In-situ Lunar Orientation Measurement) to study lunar rotational dynamics by direct
observations of the lunar rotation from the lunar surface by using a small telescope like PZT with an accuracy of
1 milli-seconds of arc in the post-SELENE mission. Another application is to obtain local gravity field on the
Earth by combining deflection of the vertical measured by PZT and the position measured by GNSS (Global
Navigation Satellite System). The accuracy required for this purpose is not as high as ILOM. A Bread Board
Model (BBM) of the telescope for ILOM has already been developed for some experiments. See Figure 6.
Table 2. A Summary of the underground disturbed body parameters.
LGFC Location (degree) Depth (k m) Mass (unit: Earth) (1 × 10 - 13)
LGFC(1) (1995.42 - 1995.67) 116.35 (E) 40.17 (N) 15.75 ± 1.47 2.93 ± 0.72
LGFC(2) (1995.92 - 1996.42) 116.33 (E) 40.17 (N) 18.37 ± 0.76 3.16 ± 0.80
LGFC(3) (1998.00 - 1998.33) 116.37 (E) 39.83 (N) 14.81 ± 0.76 3.50 ± 1.63
LGFC(4) (1998.33 - 1998.67) 116.37 (E) 39.83 (N) 17.85 ± 2.85 5.45 ± 1.44
Figure 5. Optical system of DZT. 1: objective, 2: plain parallel, 3: prism, 4:
CCD, 5: mercury surface (After Hanada et al., 2012).
Z. X. Li et al.
Figure 6. Structure of BBM of the PZT (after Hanada et al.).
In the future survey at BTTZ area, both of the independent PZT and gravity methods should be used together
by means of taking the advantages of them, and of validating each other. Additionally, as the relation between
earthquake and the timing of a detected LGFC, it is still too early to draw any conclusion. The facts reported in
the paper should be considered as some new evidence supplemented to those already reported in the past (Li et
al., 2009; Li et al., 2011).
Authors thank the support of the Key Laboratory of Lunar and Deep Space, Chinese Academy of Sciences. Th e
gravimetric data for this research is supported from BTTZ gravimetric network. A. G. Thanks to the
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