Board 117: Work in Progress: Impact of Teaching Engineering Summer Academy on Teacher Efficacy and Teaching Beliefs

Mapping Intimacies ◽

10.18260/1-2--32202 ◽

2020 ◽

Author(s):

Joni Lakin ◽

Mary Lou Ewald ◽

Nancy Blanco ◽

Jessica Gilpin

Keyword(s):

Teacher Efficacy ◽

Teaching Beliefs ◽

Work In Progress ◽

Summer Academy

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Work in Progress: The Impact of Faculty Development Workshops on Shifting Faculty Teaching Beliefs and Classroom Practice toward Student Centeredness

10.18260/1-2--29184 ◽

2018 ◽

Author(s):

Elizabeth Lopez ◽

Yong Seok Park ◽

Bethany Smith ◽

James Middleton ◽

Keith Hjelmstad ◽

...

Keyword(s):

Faculty Development ◽

Classroom Practice ◽

Teaching Beliefs ◽

Work In Progress ◽

Faculty Teaching ◽

Student Centeredness ◽

The Impact

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The Effect of Early Childhood Teachers' Teacher Efficacy, Teaching Beliefs and Self-directed Learning Ability on Teaching Professionalism

Journal of Parent Education ◽

10.36431/jpe.11.4.10 ◽

2019 ◽

Vol 11 (4) ◽

pp. 187-209

Author(s):

Jin Hwa Lee ◽

Eun-Jung Kim

Keyword(s):

Early Childhood ◽

Teacher Efficacy ◽

Early Childhood Teachers ◽

Learning Ability ◽

Teaching Beliefs ◽

Self Directed Learning ◽

Directed Learning

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Meridional Circulation, Turbulence, and Diffusion Processes in Stars

International Astronomical Union Colloquium ◽

10.1017/s0252921100080477 ◽

1976 ◽

Vol 32 ◽

pp. 109-116 ◽

Cited By ~ 1

Author(s):

S. Vauclair

Keyword(s):

Convection Zone ◽

Diffusion Processes ◽

Meridional Circulation ◽

Diffusion Time ◽

Work In Progress ◽

First Results ◽

Stellar Envelopes ◽

And Diffusion ◽

Turbulence And Diffusion ◽

Hr Diagram

This paper gives the first results of a work in progress, in collaboration with G. Michaud and G. Vauclair. It is a first attempt to compute the effects of meridional circulation and turbulence on diffusion processes in stellar envelopes. Computations have been made for a 2 Mʘstar, which lies in the Am - δ Scuti region of the HR diagram.Let us recall that in Am stars diffusion cannot occur between the two outer convection zones, contrary to what was assumed by Watson (1970, 1971) and Smith (1971), since they are linked by overshooting (Latour, 1972; Toomre et al., 1975). But diffusion may occur at the bottom of the second convection zone. According to Vauclair et al. (1974), the second convection zone, due to He II ionization, disappears after a time equal to the helium diffusion time, and then diffusion may happen at the bottom of the first convection zone, so that the arguments by Watson and Smith are preserved.

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