The Impact of the Transition From In-Person to Remote Courses on MSW Students Due to COVID-19

2021 ◽  
Vol 41 (5) ◽  
pp. 550-562
Author(s):  
Kathleen Ray ◽  
Liat Shklarski
Keyword(s):  
Msw Students ◽  
The Impact

Recreational Drumming: A Creative Arts Intervention Strategy for Social Work Teaching and Practice

2010 ◽  
Vol 15 (1) ◽  
pp. 53-66 ◽  
Author(s):  
Tina Maschi ◽  
Carolyn Bradley
Keyword(s):  
Social Work ◽  
Intervention Strategy ◽  
Social Work Students ◽  
Well Being ◽  
Creative Arts ◽  
Stress Energy ◽  
Msw Students ◽  
Interpersonal Connectedness ◽  
Diverse Groups ◽  
The Impact

Recreational music-making has been shown to decrease stress and increase feelings of well-being and empowerment among diverse groups. This study examined the impact of recreational drumming among social work students on measures of well-being, empowerment, and connectedness. It used a pretest-posttest design to evaluate outcomes among a sample of 31 participants in the 2-hour I–We Rhythm Program for recreational drumming. Results of paired t-test analyses revealed significant differences in levels of stress, energy, and feelings of empowerment and community. Using this creative-arts intervention can be an effective self-care strategy for BSW and MSW students, practitioners, and/or clients in educational or agency-based settings to increase feelings of well-being and interpersonal connectedness, which, in turn, may help to increase effectiveness in practice.

scholarly journals The Impact of a Title IV-E Program on Perceived Practice Skills for Child Welfare Students: A Review of Five MSW Cohorts

2017 ◽  
Vol 18 (2) ◽  
pp. 474-489
Author(s):  
Elizabeth Jane Greeno ◽  
Lisa Fedina ◽  
Berenice Rushovich ◽  
Caroline Burry ◽  
Debra Linsenmeyer ◽  
...  
Keyword(s):  
Child Welfare ◽  
Child Welfare Workers ◽  
Field Instructors ◽  
Content Areas ◽  
Public Child Welfare ◽  
Title Iv ◽  
Msw Students ◽  
Specific Practice ◽  
The Impact ◽  
Practice Skills

Title IV-E Education for Public Child Welfare training programs are designed to build knowledge and practice skills among students and current child welfare workers in efforts to build a competent and highly trained workforce. A mixed methods study was conducted to: 1) measure changes in MSW Title IV-E students' perceived confidence to perform skills across 13 practice content areas for public child welfare practice, and 2) to explore students’ perceptions of their competency for child welfare practice. This study also focused on the impact of prior child welfare experiences on perceived child welfare knowledge and skills among Title IV-E students. A total of 224 Title IV-E MSW students over the course of five academic cohorts participated in this study. Surveys were conducted at three time points: pretest, posttest, and retrospective pretest. Twenty focus groups were conducted during the study time period. Findings indicate gains across all practice content areas with the largest gains in areas of working with the courts and conducting assessments. Qualitative findings assessing student's perception of competency to practice in child welfare include themes of students’ preparation to practice post-graduation and differences between the students’ experiences in the IV-E program and what they witness in the field. Specific practice area recommendations include addressing workers’ age and prior experience in Title IV-E seminars and trainings as well the importance of Title IV-E field instructors in helping to prepare students for child welfare practice.

Disclosure of Student Status in Agencies: Do We Still Have a Secret?

1997 ◽  
Vol 78 (1) ◽  
pp. 72-83 ◽  
Author(s):  
Jaclyn Miller ◽  
Mary K. Rodwell
Keyword(s):  
Social Work ◽  
Qualitative Analysis ◽  
Quantitative Data ◽  
Current Practice ◽  
Field Instruction ◽  
Field Instructors ◽  
Advantages And Disadvantages ◽  
Msw Students ◽  
The Impact ◽  
Schools Of Social Work

This study is about current practice regarding identification of student status in agencies where BSW and MSW students are placed for their field instruction experience. Agency administrators and field instructors responded to questions regarding student title designation during the practicum, the degree to which students are identified as students to clients and other community professionals, and their perceptions of current practice of identifying students and of what the practice ought to be. The impact of the disclosure of student status on clients and its implications for agencies, field instructors, and schools of social work are drawn from quantitative data and a qualitative analysis of data on the advantages and disadvantages of disclosure.

Formation of Lunar Craters and Bright Rays as a Result of Meteorite Impacts

1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten
Keyword(s):  
Explosive Charge ◽  
The Moon ◽  
Meteorite Impacts ◽  
The Earth ◽  
Lunar Craters ◽  
The Impact

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.

The Geosciences Applied to Lunar Exploration

1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green
Keyword(s):  
Lunar Surface ◽  
Probable Mechanism ◽  
Point Of View ◽  
Lunar Exploration ◽  
Geological Model ◽  
Apply Geophysics ◽  
Surface Features ◽  
The Impact

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.

Asteroid and Comet Impact Speeds upon Mars: Significance for Panspermia and the Supply of Organics

1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel
Keyword(s):  
Probability Distributions ◽  
Regions Of Interest ◽  
Significant Fraction ◽  
Organic Chemicals ◽  
Impact Speed ◽  
The Mean ◽  
The Impact

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.

Organic Syntheses During the Impact of a Comet with a Gaseous Planet

1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini
Keyword(s):  
Polymeric Material ◽  
Molecular Form ◽  
Parent Compound ◽  
Blue Filter ◽  
Organic Syntheses ◽  
The Impact

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.

Hydrogen Cyanide Polymers from the Impact of Comet P/Shoemaker-Levy 9 on Jupiter

1997 ◽  
Vol 161 ◽  
pp. 179-187
Author(s):  
Clifford N. Matthews ◽  
Rose A. Pesce-Rodriguez ◽  
Shirley A. Liebman
Keyword(s):  
Amino Acids ◽  
Solar System ◽  
Hydrogen Cyanide ◽  
Nitrogen Heterocycles ◽  
Laboratory Studies ◽  
Heterogeneous Solids ◽  
The Many ◽  
Comet Halley ◽  
The Impact ◽  
By Products

AbstractHydrogen cyanide polymers – heterogeneous solids ranging in color from yellow to orange to brown to black – may be among the organic macromolecules most readily formed within the Solar System. The non-volatile black crust of comet Halley, for example, as well as the extensive orangebrown streaks in the atmosphere of Jupiter, might consist largely of such polymers synthesized from HCN formed by photolysis of methane and ammonia, the color observed depending on the concentration of HCN involved. Laboratory studies of these ubiquitous compounds point to the presence of polyamidine structures synthesized directly from hydrogen cyanide. These would be converted by water to polypeptides which can be further hydrolyzed to α-amino acids. Black polymers and multimers with conjugated ladder structures derived from HCN could also be formed and might well be the source of the many nitrogen heterocycles, adenine included, observed after pyrolysis. The dark brown color arising from the impacts of comet P/Shoemaker-Levy 9 on Jupiter might therefore be mainly caused by the presence of HCN polymers, whether originally present, deposited by the impactor or synthesized directly from HCN. Spectroscopic detection of these predicted macromolecules and their hydrolytic and pyrolytic by-products would strengthen significantly the hypothesis that cyanide polymerization is a preferred pathway for prebiotic and extraterrestrial chemistry.

Unusual Microstructure in Shock-Compacted Graphite

1970 ◽  
Vol 28 ◽  
pp. 474-475
Author(s):  
Lucien F. Trueb
Keyword(s):  
Mechanical Characteristic ◽  
Compression Wave ◽  
Gray Zone ◽  
Flyer Plate ◽  
Compacted Graphite ◽  
The Impact

Crushed and statically compressed Madagascar graphite that was explosively shocked at 425 kb by means of a planar flyer-plate is characterized by a black zone extending for 2 to 3 nun below the impact plane of the driver. Beyond this point, the material assumes the normal gray color of graphite. The thickness of the black zone is identical with the distance taken by the relaxation wave to overtake the compression wave.The main mechanical characteristic of the black material is its great hardness; steel scalpels and razor blades are readily blunted during attempts to cut it. An average microhardness value of 95-3 DPHN was obtained with a 10 kg load. This figure is a minimum because the indentations were usually cracked; 14.8 DPHN was measured in the gray zone.

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