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Richard Strauss’s contacts with Vienna spanned more than six decades, from the time of his brief stint as a university student in 1882 through the Allied air campaigns of 1944. This chapter focuses on the city of Vienna during the period of Strauss’s tenure as codirector of the State Opera from 1919–24, years defined by the founding of the First Austrian Republic and policies instituted by the Municipal Council in response to ongoing economic turmoil. While the situation was less dire than in Berlin, Vienna was nonetheless a city in crisis when Strauss arrived in early December 1919. Examination of “Red Vienna,” named for initiatives of the ruling Social Democratic Party, serves as context for the cultural life in which he participated as a well-respected and well-paid musical celebrity. Attention then shifts to Strauss’s life and work in Vienna with an emphasis on the institutions and figures comprising his private and professional orbit.
Richard Strauss in Context offers a distinctive approach to the study of a composer in that it places the emphasis on contextualizing topics rather than on biography and artistic output. One might say that it inverts the relationship between composer and context. Rather than studies of Strauss's librettists that discuss the texts themselves and his musical settings, for instance, this book offers essays on the writers themselves: their biographical circumstances, styles, landmark works, and broader positions in literary history. Likewise, Strauss's contributions to the concert hall are positioned within the broader development of the orchestra and trends in programmatic music. In short, readers will benefit from an elaboration of material that is either absent from or treated only briefly in existing publications. Through this supplemental and broader contextual approach, this book serves as a valuable and unique resource for students, scholars, and a general readership.
Head impact exposure (HIE) in youth football is a public health concern. The objective of this study was to determine if one season of HIE in youth football was related to cognitive changes.
Method:
Over 200 participants (ages 9–13) wore instrumented helmets for practices and games to measure the amount of HIE sustained over one season. Pre- and post-season neuropsychological tests were completed. Test score changes were calculated adjusting for practice effects and regression to the mean and used as the dependent variables. Regression models were calculated with HIE variables predicting neuropsychological test score changes.
Results:
For the full sample, a small effect was found with season average rotational values predicting changes in list-learning such that HIE was related to negative score change: standardized beta (β) = -.147, t(205) = -2.12, and p = .035. When analyzed by age clusters (9–10, 11–13) and adding participant weight to models, the R2 values increased. Splitting groups by weight (median split), found heavier members of the 9–10 cohort with significantly greater change than lighter members. Additionaly, significantly more participants had clinically meaningful negative changes: X2 = 10.343, p = .001.
Conclusion:
These findings suggest that in the 9–10 age cluster, the average seasonal level of HIE had inverse, negative relationships with cognitive change over one season that was not found in the older group. The mediation effects of age and weight have not been explored previously and appear to contribute to the effects of HIE on cognition in youth football players.
The Murchison Widefield Array (MWA) is an open access telescope dedicated to studying the low-frequency (80–300 MHz) southern sky. Since beginning operations in mid-2013, the MWA has opened a new observational window in the southern hemisphere enabling many science areas. The driving science objectives of the original design were to observe 21 cm radiation from the Epoch of Reionisation (EoR), explore the radio time domain, perform Galactic and extragalactic surveys, and monitor solar, heliospheric, and ionospheric phenomena. All together
$60+$
programs recorded 20 000 h producing 146 papers to date. In 2016, the telescope underwent a major upgrade resulting in alternating compact and extended configurations. Other upgrades, including digital back-ends and a rapid-response triggering system, have been developed since the original array was commissioned. In this paper, we review the major results from the prior operation of the MWA and then discuss the new science paths enabled by the improved capabilities. We group these science opportunities by the four original science themes but also include ideas for directions outside these categories.