Granulation, supergranulation and atmospheric waves

A short review of the last years investigations of the fine and large scale structure of the solar atmosphere and connected with this structure atmospheric waves is given. The intergranular network and the supergranulation are considered as general strong magnetic field and the measured faint magnetic field as a statistical mean of quasiopen fields of granulation. There is a tendency of systematical formation of large scale structures beginning from the mesogranulation to the configurations of 105 km scale size. (Auth.)