Empirical Solar Radiation Pressure Models for GLONASS Satellites


These models had been investigated for the IGS processing, but they were discarded because the use of the ROCK model in combination with the sine and cosine empirical accelerations proved to be equivalent. IGEX gave a second chance for the use of this implementation.

The parametrization of the model describes the forces on each of the reference frame axes as a function of the selected argument A as:

where K is a factor that can be 1 or a scaling including the variation in solar radiation pressure with satellite-sun distance and an estimable global scale factor.

Several arguments and reference frames have been tested.

The most interesting arguments are:

Tested reference frames are:

After several tests the selected argument is the solar anomaly, and the frame the solar one. Sine and cosine terms are only estimated in the z axis. Terms in 2A are not estimated.

Resulting in a 5 estimated coefficients model: constant terms in x, y and z directions and sine and cosine terms in the z direction. The x, y, z directions are defined as:

The selection of the model was based on the residuals of the orbit determination and the observability of the selected parameters.

The coefficients of the solar radiation pressure model are plotted for several days of the campaign.

If this model is used for the GPS satellites it produces a fit similar to the ROCK model plus four estimated parameters (scale, y-bias, two radial cyclical accelerations).

Solar radiation pressure reference systems and arguments


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Contact info.Last Update: August 2002