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Waves propagation in network and inter-network bright points channels between the chromosphere and transition regions with IRIS observations

Zeighami, Sima; Tavabi, Ehsan; Amirkhanlou, Elnaz

The significance increase of the plasma temperature from the solar photosphere to the corona up to 1MK is still unresolved. One of the candidates for this issue is waves and instabilities in the solar plasma. It was suggested that the energy of these waves could heat the solar atmosphere to transition-region (TR) and corona. Despite many recent ki…