Coronal jets represent important manifestations of ubiquitous solar transients, which may be the source of significant mass and energy input to the upper solar atmosphere and the solar …
THE solar corona (the outermost portion of the Sun's atmosphere) is far hotter than the'surface'(the photosphere). Recent observations of X-ray jets1á€-4 (collimated flows of …
Context. Recent observations by the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter have characterized prevalent small-scale transient brightenings in the corona above the …
T Yokoyama, K Shibata - … of the Astronomical Society of Japan, 1996 - ieeexplore.ieee.org
We performed two-dimensional numerical simulations of solar coronal X-ray jets by solving the resistive magnetohydrodynamic (MHD) equations. The simulations were based on the …
E Pariat, SK Antiochos, CR DeVore - The Astrophysical Journal, 2009 - iopscience.iop.org
We propose a model for the jetting activity that is commonly observed in the Sun's corona, especially in the open-field regions of polar coronal holes. Magnetic reconnection is the …
K Shibata, T Nakamura, T Matsumoto, K Otsuji… - Science, 2007 - science.org
The heating of the solar chromosphere and corona is a long-standing puzzle in solar physics. Hinode observations show the ubiquitous presence of chromospheric anemone jets …
Since their discovery over 100 years ago, there have been many suggestions for the origin and development of solar spicules. Because the velocities of spicules are comparable to the …
K Shibata - Astrophysics and Space Science, 1998 - Springer
The solar X-ray observing satellite Yohkoh has discovered various new dynamic features in solar flares and corona, eg, cusp-shaped flare loops, above-the-loop-top hard X-ray …
The twentieth century has witnessed the transformation of astronomy from celestial mechanics to astrophysics. While optical telescopes may have presented a peek into the …