Yoshinori Hayashi

Intermittent magnetic reconnection in TS-3 merging experiment

Ejection of current sheet with plasma mass causes impulsive and intermittent magnetic reconnection in the TS-3 spherical tokamak (ST) merging experiment. Under high guide toroidal field, the sheet resistivity is almost classical due to the sheet thickness much longer than the ion gyroradius. Large inflow flux and low current-sheet resistivity result in flux and plasma pileup followed by rapid growth of the current sheet. When the pileup exceeds a critical limit, the sheet is ejected mechanically from the squeezed X-point area. The reconnection (outflow) speed is slow during the flux/plasma pileup and is fast during the ejection, suggesting that intermittent reconnection similar to the solar flare increases the averaged reconnection speed. These transient effects enable the merging tokamaks to have the fast reconnection as well as the high-power reconnection heating, even when their current-sheet resistivity is low under high guide field.

A LABORATORY EXPERIMENT OF MAGNETIC RECONNECTION: OUTFLOWS, HEATING, AND WAVES IN CHROMOSPHERIC JETS

Hinode observations have revealed intermittent recurrent plasma ejections/jets in the chromosphere. These are interpreted as a result of non-perfectly anti-parallel magnetic reconnection, i.e. component reconnection, between a twisted magnetic flux tube and the pre-existing coronal/chromospheric magnetic field, though the fundamental physics of component reconnection is unrevealed. In this paper, we experimentally reproduced the magnetic configuration and investigated the dynamics of plasma ejections, heating and wave generation triggered by component reconnection in the chromosphere. We set plasma parameters as in the chromosphere (density 10^14 cm^-3, temperature 5-10 eV, i.e. (5-10)x10^4 K, and reconnection magnetic field 200 G) using argon plasma. Our experiment shows bi-directional outflows with the speed of 5 km/s at maximum, ion heating in the downstream area over 30 eV and magnetic fluctuations mainly at 5-10 us period. We succeeded in qualitatively reproducing chromospheric jets, but quantitatively we still have some differences between observations and experiments such as jet velocity, total energy and wave frequency. Some of them can be explained by the scale gap between solar and laboratory plasma, while the others probably by the difference of microscopy and macroscopy, collisionality and the degree of ionization, which have not been achieved in our experiment.

Physician obligation to provide care during disasters: should physicians have been required to go to Fukushima?

On 11 March 2011, Japan experienced a major disaster brought about by a 9.0-magnitude earthquake and a massive tsunami that followed. This disaster caused extensive damage to the Fukushima Daiichi nuclear power plant with the release of a large amount of radiation, leading to a crisis level 7 on the International Atomic Energy Agency scale. In this report, we discuss the obligations of physicians to provide care during the initial weeks after the disaster. We appeal to the obligation of general beneficence and argue that physicians should go to disaster zones only if there is no significant risk, cost or burden associated with doing so. We conclude that physicians were not obligated to go to Fukushima given the high risk of radiation exposure and physical and psychological harm. However, we must acknowledge that there were serious epistemic difficulties in accurately assessing the risks or benefits of travelling to Fukushima at the time. The discussion that follows is highly pertinent to all countries that rely on nuclear energy.