Time series of SXT (Soft X-ray Telescope) images have revealed many jet-like features in the
solar corona. Typical size of the “jet” is 5 × 103 – 4 × 105 km, the typical projected velocity …

We propose a comprehensive model which explains the activities in the region of star formation
recently found in optical, X-ray, and radio observations. The large-scale cold bipolar flow …

Moreton's wave phenomenon, observed to propagate across the solar disk during certain
solar flares, may be explained as the intersection line between an expanding coronal …

Collapsin response mediating protein‐2 (CRMP2) has been identified as an intracellular
protein mediating Semaphorin3A (Sema3A), a repulsive guidance molecule. In this study, we …

A number of astronomical systems have been discovered that generate collimated flows of
plasma with velocities close to the speed of light. In all cases, the central object is probably a …

Semaphorin-3A (Sema3A), a member of class 3 semaphorins, regulates axon and dendrite
guidance in the nervous system. How Sema3A and its receptors plexin-As and neuropilins …

The exciters of transient solar radio emissions-the type II and type III bursts in the nomenclature
by WILD and his collaborstors1-are from the view point of the velocity with which their …

… Yutaka UCHIDA … be due to the fast-mode shockfront in the corona (UcHIDA 1960), and
further … UCHIDA 1969) is required to explain the overall velocity …

Both in the Faraday Rotation Measure and the intrinsic polarization angle, new features are
revealed to indicate a helical magnetic field operating along the jet of the bright active …

The paper presents a nonsteady magnetodynamic mechanism for the formation of astrophysical
jets in a magnetized accretion disk system. The dynamical processes in the contraction …