New approach to construction of the earth upper atmosphere model with the use of satellite local data on the atmosphere

Present-day models of the Earth's upper atmosphere allow to build a spatio-temporal picture of variations in atmosphere parameters on a planetary scale, per se, in an averaged view. To build-up these standard models one uses data set on satellite braking in the atmosphere, probe measurings aboard geophysical rockets, measurings of non-coherent radio scattering in the Earth's atmosphere. The current level of space research allows to apply a new method to study the Earth's upper atmosphere: to research the upper atmosphere by measuring the absorption of solar XUV-radiation by the Earth's atmosphere when observing the solar disk.