Short-term periodicities in the downward longwave radiation and their associations with cosmic ray and solar interplanetary data

Abstract

Abstract In this study downward longwave (LW) atmospheric radiation data for the period of 2014–2020 were used to search for short-term periodicities using fast Fourier transform (FFT). Several local peaks in the power spectrum density were found and established. The time series exhibits a series of significant peaks (exceeding the 95% confidence limit), such as at 273\xa0days, 227\xa0days, 200\xa0days, 178\xa0days, 157\xa0days, 110\xa0days, 120\xa0days, 87\xa0days, 73\xa0days, 53–56\xa0days, 35–30\xa0days, 25–27\xa0days, 21\xa0days, 13\xa0days, and 9–10\xa0days. Moreover, cosmic ray data from KACST muon detector and the Oulu neutron monitor, as well as the data for the solar radio flux at 10.7\xa0cm (F10.7\xa0cm), Dst index, and solar wind speed for the same period as the LW data, were used to look for common cyclic variations and periodicities matching those found in the LW radiation. This was done to investigate the possible effect of the solar activity parameters on LW radiation. Several common periodicities were observed in the spectra of all the variables considered, such as 227\xa0days, 154–157\xa0days, 25–27\xa0days, and 21\xa0days. Some of the periodicities found in the LW radiation spectrum can be attributed to the modulation of the cosmic ray intensity by solar activity. Others are attributed to the disturbances in the interplanetary magnetic field. Based on the spectral results, we suggest that the solar signals may directly or indirectly affect the variations of the downward longwave radiation, which in turn may affect climate change.