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Coronal heating has been a long-standing problem in solar physics. With advances in Extreme UV Imager during the last decade, it has been possible to probe the MHD wave heating mechanisms. The Omnipresence of Decayless oscillations in the coronal loops makes it an excellent candidate to explain coronal heating. These oscillations, characterized by their lack of decay, are commonly found in coronal loops within active regions. The coexistence of long and short-period decayless oscillations in these loops remains relatively unexplored, potentially restricting our complete understanding of decayless oscillations in small-scale loops within the active region. In this talk, I will discuss the properties of long-period oscillations in these small-scale coronal loops. |