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THE INSIGHT AND FACTORS THAT PROMOTE JOB LONGEVITY FOR CHILD WELFARE SOCIAL WORKERS
The high turnover rate of child welfare social workers has been a chronic issue that society has yet to mitigate. To understand this problem, the researchers looked at contributing factors in comparison to the factors that promote job longevity. The researchers reviewed the multidimensional theory of burnout, to explore the ongoing issue of high turnover rates. Also, organizational support theory was examined to determine if support from organizations contributed to job longevity. The post-positivist approach was used to gather qualitative data from this study as to the potential factors promoting job longevity through individual interviews with seasoned child welfare social workers. The study participants identified potential barriers in the workplace, the skills needed for professional development, and the benefit of having a support system to effectively do their job. In addition, the study participants demonstrated a strong sense of self-awareness and utilization of internal traits that promoted job longevity. It was discovered that child welfare social workers who possess emotional intelligence had the ability to cope with stress better, had less health issues, and were more likely to promote to higher level positions. By understanding the factors that contribute to job longevity, child welfare agencies can implement measures to promote job retention. Furthermore, when agencies invest in child welfare social workers by providing them support, it is reflected in the quality of their work and client engagement
Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case Studies
Flare frequency distributions represent a key approach to addressing one of
the largest problems in solar and stellar physics: determining the mechanism
that counter-intuitively heats coronae to temperatures that are orders of
magnitude hotter than the corresponding photospheres. It is widely accepted
that the magnetic field is responsible for the heating, but there are two
competing mechanisms that could explain it: nanoflares or Alfv\'en waves. To
date, neither can be directly observed. Nanoflares are, by definition,
extremely small, but their aggregate energy release could represent a
substantial heating mechanism, presuming they are sufficiently abundant. One
way to test this presumption is via the flare frequency distribution, which
describes how often flares of various energies occur. If the slope of the power
law fitting the flare frequency distribution is above a critical threshold,
as established in prior literature, then there should be a
sufficient abundance of nanoflares to explain coronal heating. We performed
600 case studies of solar flares, made possible by an unprecedented number
of data analysts via three semesters of an undergraduate physics laboratory
course. This allowed us to include two crucial, but nontrivial, analysis
methods: pre-flare baseline subtraction and computation of the flare energy,
which requires determining flare start and stop times. We aggregated the
results of these analyses into a statistical study to determine that . This is below the critical threshold, suggesting that Alfv\'en
waves are an important driver of coronal heating.Comment: 1,002 authors, 14 pages, 4 figures, 3 tables, published by The
Astrophysical Journal on 2023-05-09, volume 948, page 7