学びにはいろいろな方法があるけれども、体験 はとりわけ実りある教育をする教師である。現 在、原子力がいかに危険でありうるのかを学ん でいる日本人を例に考えてみよう。

日本にいる人びとが、核兵器による破滅的な体 験もしていることは言うまでもない。これ は、1945年に米国政府が原爆で広島と長崎を破 壊したときだけではない。1954年の米国の水爆 実験が、第五福竜丸という日本漁船に人の命に かかわるような放射性降下物を浴びせた時もそ うだ、この事件で死者が出て、広範な核兵器廃 絶運動が始まったのである。

This paper highlights the role that the World Wide Web (WWW) has to play as an aid to psychiatry. A basic history of the WWW is provided as is an introduction to some search techniques involved with the WWW. The literature on applications potentially relevant to psychiatry is reviewed using computer search facilities (BIDS, PsychLit and Medline). The WWW is one of the aspects of the Internet that possesses a huge potential for exploitation, both the clinical and research psychiatrist are able to benefit from its use.

Between 2012 and 2014 we posted a number of articles on contemporary affairs without giving them volume and issue numbers or dates. Often the date can be determined from internal evidence in the article, but sometimes not. We have decided retrospectively to list all of them as Volume 10, Issue 54 with a date of 2012 with the understanding that all were published between 2012 and 2014.

スティーブン・ローチ（Stephen Roach）は、日本で起きた3月11日の地震が世界経済に与える影響について、のんびり構えていてはいけないと警告する。彼が批判する視点、つまり世界経済における近年の日本経済の地位低下――世界における輸出とGDPで日本がシェアを落としていることや中国の台頭、そして成長が見込まれる重要な工業製品のなかで日本でしか生産できないものが少ない――にもとづく「狭い視点」の概要を説明したのち、ローチはこの観点から導かれる次のような「表面的な」結論を受け入れるべきでないとする。彼が批判する結論とは、日本は「すでに重要な役割を果たさなくなっており」、東日本大震災とその余波が世界経済にもたらす混乱は「一時的なもの」で「小さい」というものだ。

The 2011 tsunami and nuclear disaster at Fukushima has encouraged comparisons in many quarters with the tragic experience of Minamata more than 55 years earlier, when mercury-poisoned industrial runoff caused widespread illness and death in the human and animal populations. Rather than viewing these disasters as the unfortunate side effects of modern industrial capitalism (to be addressed, in the capitalist view, with financial compensation) Yoneyama Shoko draws on Minamata victim's advocate Ogata Masato to imagine a more humane and life-affirming vision of our obligations to one another. In crafting his response to the Chisso Corporation and the Japanese government, Ogata (who eschewed financial compensation) drew on elements of the popular Japanese religious heritage to affirm an ethos of interdependence and the responsibility that follows. This can be seen, for example, in Ogata's use of the term tsumi, an indigenous Japanese category of ritual impurity that encompasses both physical pollution and moral transgression. Combining notions of “defilement” and of “sin,” tsumi is a principle that (as Brian Victoria notes) has justified some in shunning the victims of chemical or radioactive contamination. Ogata, however, employs the traditional imagery of tsumi to describe, not the victims of pollution but its perpetrators, thereby presenting ecological damage as a profoundly moral matter, one that cannot be reduced to economic impacts or financial compensation.

Fourier coefficients are a valuable tool in the study of a wide variety of pulsating stars. They can be used to derive various physical parameters, including mass, luminosity, metallicity and effective temperature and are frequently used to discriminate between different pulsation modes. With the increase in large-scale surveys and the availability of data on the Internet, the number of Fourier coefficients available for study has expanded greatly and it is difficult to find all current data for individual stars or a subset of stars. To assist others in obtaining and making use of Fourier coefficients, an archive of published values of Fourier coefficients has been set up. Users can search for data on individual stars or for a range of parameters. Several Java programs are used to display the data in a variety of ways. The archive is located at the Web site http://www.earth.uni.edu/fourier/.

We have used the Automated Plate Scanner (APS) at the University of Minnesota to digitize glass copies of the blue and red plates of the original Palomar Observatory Sky Survey (POSS I) with |b| > 20°. The APS Image Database is a database of all digitized images larger than the photographic noise threshold. It includes all of the matched images in the object catalog, as well as those unmatched images above the noise threshold. The matched image data of the catalog has the advantage of confirming the reality of the image. This is especially important for small images near the plate limit. But these are not all of the detected real images; very blue or very red faint objects may be excluded by this matching requirement. The image database allows information on them to be retrieved, and is therefore a valuable complement to the object catalog. The operation of the APS and the scanning procedures are described in detail in Pennington et al. (1993). We are now processing plate data into the image database. A set of query forms, a tutorial and documentation can be found at http://isis.spa.umn.edu/IDB/homepage.idb.html.

The observation of an area of 120° × 56° centered on RA=8h DEC=20° at 408 MHz was the first astronomical use of the MPIfR 100-m telescope (1970) and was designed to compile a complete sky survey using also data from Jodrell Bank and Parkes (Haslam et al., 1982). The observation of the northern sky at 1420 MHz started in 1972 using the Stockert 25-m telescope and was finished in 1976 (Reich and Reich 1986). This survey has been completed to an all sky survey using data from Villa Elisa (Argentina). The two surveys are absolutely calibrated. The angular resolutions are 0.8° and 0.59°, respectively. A number of surveys of the Galactic plane have been made with the 100-m telescope at arc minute angular resolution. Surveys at 2695 MHz (|b| ≤ 5°) (Reich et al. 1990, Fürst et al. 1990) and at 1410 MHz (|b| < 4°) (Reich et al. 1990) are public.

At medium Galactic latitudes (up to |b| = 20°) the emission consists mainly of faint extended ridges or arcs superimposed on the still dominating, about 10 times stronger, diffuse Galactic emission. They have never been investigated in a systematic way although they provide important clues for the understanding of the “disk-halo connection”. This region is covered by new observations at 1400 MHz with the 100-m telescope.

On the fifth anniversary of the establishment of the Kyoko Selden Memorial Translation Prize through the generosity of her colleagues, students, and friends, the Department of Asian Studies at Cornell University is pleased to announce the winners of the 2018 Prize.

The status of the WWW-based Fourier Coefficient web site is presented. Currently the database has coefficients for not only galactic field variables, but also those found in globular clusters and other galaxies, including the Magellanic Clouds. The database can be used to show various correlations between physical characteristics of the stars and the coefficients, as well as inter-relationships between the coefficients themselves. The database is accessible at http://nitro9.earth.uni.edu/fourier/.