The temporal variations of solar rotation in the photosphere, chromosphere, and corona
have been widely investigated, whereas the rotation of the solar transition region is rarely …

The temporal variation of solar coronal rotation appears to be very complex and its
relevance to the 11-year solar activity cycle is still unclear. Using the modified coronal index …

Context. The strength and morphology of the Sun's magnetic field evolve significantly during
the solar cycle, with the overall polarity of the Sun's magnetic field reversing during the …

In this article, we present the differential rotational profile of extreme ultraviolet (EUV)
corona. For this purpose, we used observations with high resolution obtained from SDO/AIA …

To date, the rotational characteristics of the solar transition region remain unclear. In this
work, by applying the flux modulation method to the images derived from the Solar …

Two relatively modern analysis techniques, including the empirical mode decomposition
and Morlet wavelet transform, are combined to investigate the short-and mid-term …

ABSTRACT A full-disk solar magnetogram has been measured each day since 1970
January 19, and the daily Magnetic Plage Strength Index (MPSI) and the daily Mount Wilson …

In this paper, by applying the wavelet transformation analysis to the data of the daily 10.7 cm
radio flux covering the period from 1947 February 14 to 2014 August 31, a significant period …

Coronal heating is a big question for modern astronomy. Daily measurement of 985 solar
spectral irradiances (SSIs) at the spectral intervals 1–39 and 116–2416 nm during 2003 …

Daily solar spectral irradiances (SSIs) at the spectral intervals 1–40, 116–264 and 950–
1600 nm and four categories of solar small-scale magnetic elements (MF no, MF anti, MF …