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We observed the aftershocks along the same seismic line as that of the 2006 and 2007 active source experiments.
Seismic investigation of the lithosphere by means of active source experiments is mostly confined to the crust and the Moho.
Laboratory recorded data in the linear source experiments were used to estimate the wetted area-time function.
Silver et al. (2007) find both increase and decrease of velocity changes during an increase of atmospheric pressure loading from active source experiments.
In our particular case, we calculated an error of less than ±3% in the calculation of mix of sources in the two-source experiments, based on the distances from the single source experiments.
For both of the single source experiments, isotope ratios of crickets were strongly positively correlated, forming regression lines on dual isotope plots (Table 2; Figure 2; Figure 3).
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During the year the Burst and Transient Source Experiment (BATSE) aboard the Earth-orbiting Compton Gamma Ray Observatory (GRO) steadily detected such events, with more than 700 bursts reported by late 1993.
A high-brilliance (∼1022 photon s−1 mrad−2/0.1%/0.1%) gamma-ray source experiment is currently being planned at Fermilab (Eγ≃1.1 MeV).
Related sites A copy of the paper in press Peter Mészáros's site The Burst and Transient Source Experiment that spotted the bursts examined in the report Gamma Ray Burst FAQ.
The results are compared with the information provided by endogenous pulsed neutron source experiment and a good agreement is seen within the statistical uncertainties of the results.
An instrument called the Burst and Transient Source Experiment on board the orbiting Compton Gamma Ray Observatory caught the first sight of the burst on 23 January (ScienceNOW, 25 January).
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