The impact of school emotional climate on student psychopathology

1990 ◽  
Vol 18 (2) ◽  
pp. 165-177 ◽  
Author(s):  
Stephanie Kasen ◽  
Jim Johnson ◽  
Patricia Cohen
Keyword(s):  
Emotional Climate ◽  
The Impact

scholarly journals How and when customer feedback influences organizational health

2016 ◽  
Vol 31 (2) ◽  
pp. 624-640 ◽  
Author(s):  
Petra Kipfelsberger ◽  
Dennis Herhausen ◽  
Heike Bruch
Keyword(s):  
Organizational Climate ◽  
Organizational Health ◽  
Organizational Level ◽  
Equation Modeling ◽  
Emotional Climate ◽  
Content Type ◽  
Customer Feedback ◽  
Affective Climate ◽  
Empowerment Climate ◽  
The Impact

Purpose – The purpose of this paper is to explore how and when customers influence organizational climate and organizational health through their feedback. Based on affective events theory, the authors classify both positive and negative customer feedback (PCF and NCF) as affective work events. The authors expect that these events influence the positive affective climate of an organization and ultimately organizational health, and that the relationships are moderated by empowerment climate. Design/methodology/approach – Structural equation modeling was utilized to analyze survey data obtained from a sample of 178 board members, 80 HR representatives, and 10,953 employees from 80 independent organizations. Findings – The findings support the expected indirect effects. Furthermore, empowerment climate strengthened the impact of PCF on organizational health but does not affect the relationship between NCF and organizational health. Research limitations/implications – The cross-sectional design is a potential limitation of the study. Practical implications – Managers should be aware that customer feedback influences an organization’s emotional climate and organizational health. Based on the results organizations might actively disseminate PCF and establish an empowerment climate. With regard to NCF, managers might consider the potential affective and health-related consequences for employees and organizations. Social implications – Customers are able to contribute to an organization’s positive affective climate and to organizational health if they provide positive feedback to organizations. Originality/value – By providing first insights into the consequences of both PCF and NCF on organizational health, this study opens a new avenue for scientific inquiry of customer influences on employees at the organizational level.

Reflections on Motherhood and Leadership During the COVID-19 Pandemic

2021 ◽  
pp. 206-218
Author(s):  
Sapna V. Thwaite
Keyword(s):  
Young Child ◽  
Professional Identities ◽  
Female Leaders ◽  
Emotional Climate ◽  
Female Leader ◽  
The Impact

This chapter explores the impact of motherhood on the professional identities of female leaders during the COVID-19 pandemic. It focuses on five principles related to parenting a young child that one might apply to one's experiences as a female leader during the COVID-19 pandemic: 1) listen with your eyes, 2) recognize that not knowing is part of growing, 3) release the need for perfection, 4) engage in restorative rituals, and 5) focus on those things that are within your control. It also expands upon the notion that creating an emotional climate where faculty, staff, and administrators can bring their “whole selves” to work would be beneficial, both during a pandemic and beyond.

scholarly journals RELATIONSHIP BETWEEN SOCIO-EMOTIONAL CLIMATE IN THE CLASSROOM AND STUDENTS’ SCHOOL SUCCESS

2020 ◽  
pp. 145-166
Author(s):  
Belma Alić-Ramić
Keyword(s):  
Elementary School Students ◽  
School Success ◽  
Emotional Climate ◽  
School Students ◽  
Factors Influencing ◽  
Pearson Coefficient ◽  
Teachers Beliefs ◽  
Main Factors ◽  
The Impact ◽  
The Relationship

The paper deals with the issue of socio-emotional climate and students' school success, it attempts to point out their importance, as well as to explicate particular aspects and dimensions of these two concepts, with a special emphasis on the investigation of their interconnection. The aim of the research is to determine the relationship between socio-emotional climate and students' school success in elementary schools in the municipality of Ilijaš. This research, based on the survey conducted among both students and teachers, will provide us with the interpretation of students' and teachers' beliefs about socio-emotional climate and school success among ninth grade elementary school students in the municipality of Ilijaš. Moreover, the main factors influencing socio-emotional climate and students' school success will be identified. The findings indicate that there is a correlation (Pearson coefficient .643) between school success and socio-emotional climate in the classroom. This correlation coefficient shows that the impact of school success on socio-emotional climate in the classroom becomes stronger as the students' numerical success increases.

Merry Christmas and Happy New Year! The impact of Christmas rituals on subjective well-being and family's emotional climate

2011 ◽  
Vol 26 (3) ◽  
pp. 373-386 ◽  
Author(s):  
Darío Páez ◽  
M. Ángeles Bilbao ◽  
Magdalena Bobowik ◽  
Miryam Campos ◽  
Nekane Basabe
Keyword(s):  
Well Being ◽  
Subjective Well Being ◽  
Emotional Climate ◽  
The Impact

The Impact of the Madrid Bombing on Personal Emotions, Emotional Atmosphere and Emotional Climate

2007 ◽  
Vol 63 (2) ◽  
pp. 273-287 ◽  
Author(s):  
Susana Conejero ◽  
Itziar Etxebarria
Keyword(s):  
Emotional Climate ◽  
The Impact

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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