The ScalarAtmosphericDensity type exposes the following members.
Gets or sets the central body of the atmosphere described by the density model. This is set to the Earth by default.
Gets a value indicating whether this object is frozen. A frozen object cannot be modified and an ObjectFrozenException will be thrown if an attempt is made to do so.(Inherited from DefinitionalObject.)
Gets the lower bound of the height (in meters above the ellipsoid) for which the density model is valid.
Gets or sets the solar and magnetic flux information.
Gets or sets the target point describing the time-varying position at which density is to be calculated.
Gets or sets the upper bound of the height (in meters above the ellipsoid) above which the density model will return a value of zero.
Gets or sets the vector to the sun to use for modeling the effects of solar radiation on the atmosphere. By default, this is set to represent the apparent displacement from the Earth to the Sun based on light time delay and aberration from the relative motion of the celestial bodies. Setting this to use the true displacement will be slightly less accurate but take less time to compute. However, not all density models will use the Sun's position.