Solar pores are efficient magnetic conduits for propagating magnetohydrodynamic wave
energy into the outer regions of the solar atmosphere. Pore observations often contain …

We present the first simultaneous observations of so-called" hot explosions" in the cool
atmosphere of the Sun made by the New Solar Telescope (NST) of Big Bear Solar …

We explore the similarity and difference of the quasi-periodic pulsations (QPPs) observed in
the decay phase of solar and stellar flares at X-rays. We identified 42 solar flares with …

Even though it is well-known from observations of the Sun that three-minute period
chromospheric oscillations persist in the internetwork quiet regions and sunspot umbrae …

We carried out an extensive statistical study of the properties of pores and sunspots, and
investigated the relationship among their physical parameters such as size, intensity …

Oscillations in sunspot umbrae exhibit remarkable differences between the photosphere and
chromosphere. We evaluate two competing scenarios proposed for explaining those …

Umbral oscillations constitute the most noticeable chromospheric feature of sunspot umbrae—
large-amplitude oscillations of intensity (umbral flashes, if very strong) and line-of-sight …

Context. Numerous magnetohydrodynamic oscillations have been reported within solar
pores over the past few decades, including in line-of-sight (LOS) velocities, intensities, and …

Atmosphere above sunspots is abundant with different types of waves. Among these waves
are running penumbral waves in the chromosphere, quasi-periodic oscillations in the lower …

With the high tempo-spatial Interface Region Imaging Spectrograph 1330 Å images, we find
that many bright structures are rooted in the light bridge of NOAA 12192, forming a light wall …