School Evaluation, Teacher Appraisal and Feedback and the Impact on Schools and Teachers

2009 ◽  
pp. 137-188
Author(s):  
Keyword(s):  
Teacher Appraisal ◽  
School Evaluation ◽  
The Impact

La valutazione dei sistemi educativi: alcune linee di tendenza nei processi di riforma in corso in area OCSE

2012 ◽  
pp. 73-76
Author(s):  
Luca Dordit
Keyword(s):  
Student Assessment ◽  
Teacher Appraisal ◽  
System Evaluation ◽  
School Evaluation ◽  
Sulla Base

Il lavoro intende ricostruire alcune tra le principali linee di tendenza osservabili nei processi di riforma dei sistemi di valutazione dei sistemi educativi a livello nazionale, sulla base delle molteplici attivitŕ di ricerca compiute dall'OCSE negli anni recenti. Per tracciare il quadro dei principali elementi comuni ai processi riformatori, inizialmente si prendono in esame gli approcci ispirati alle logiche di accountability e di improvement, applicati alla valutazione nel settore dell'education. Si introducono successivamente le quattro dimensioni in cui l'OCSE articola il sistema valutativo: accertamento degli esiti di apprendimento degli studenti (student assessment), valutazione della performance degli insegnanti (teacher appraisal), valutazione delle istituzioni scolastiche (school evaluation) e valutazione complessiva del sistema educativo (system evaluation). Infine vengono riprese ed approfondite alcune tendenze comuni, riscontrabili sul piano internazionale per ciascuna delle dimensioni considerate.

scholarly journals Teachers’ views of the impact of school evaluation and external inspection processes

2016 ◽  
Vol 19 (1) ◽  
pp. 52-61 ◽  
Author(s):  
Elizabeth Hopkins ◽  
Helen Hendry ◽  
Frank Garrod ◽  
Siobhan McClare ◽  
Daniel Pettit ◽  
...  
Keyword(s):  
School Evaluation ◽  
The Impact ◽  
External Inspection

scholarly journals Changing medical students’ perception of the evaluation culture: Is it possible?

2016 ◽  
Vol 13 ◽  
pp. 8 ◽  
Author(s):  
Jorie M. Colbert-Getz ◽  
Steven Baumann
Keyword(s):  
Best Practices ◽  
Survey Design ◽  
Evaluation Process ◽  
Course Evaluations ◽  
Process Time ◽  
School Evaluation ◽  
University Of Utah ◽  
School Of Medicine ◽  
The Impact ◽  
Academic Year

Student feedback is a critical component of the teacher-learner cycle. However, there is not a gold standard course or clerkship evaluation form and limited research on the impact of changing the evaluation process. Results from a focus group and pre-implementation feedback survey coupled with best practices in survey design were used to improve all course/clerkship evaluation for academic year 2013-2014. In spring 2014 we asked all subjected students in University of Utah School of Medicine, United States of America to complete the same feedback survey (post-implementation survey). We assessed the evaluation climate with 3 measures on the feedback survey: overall satisfaction with the evaluation process; time students gave effort to the process; and time students used shortcuts. Scores from these measures were compared between 2013 and 2014 with Mann-Whitney U-tests. Response rates were 79% (254) for 2013 and 52% (179) for 2014. Students’ overall satisfaction score were significantly higher (more positive) post-implementation compared to pre-implementation (P<0.001). There was no change in the amount of time students gave effort to completing evaluations (P=0.981) and no change for the amount of time they used shortcuts to complete evaluations (P=0.956). We were able to change overall satisfaction with the medical school evaluation culture, but there was no change in the amount of time students gave effort to completing evaluations and times they used shortcuts to complete evaluations. To ensure accurate evaluation results we will need to focus our efforts on time needed to complete course evaluations across all four years.

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.

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