title: Review: Erica Burman: Deconstructing Developmental Psychology, London and New York: Routledge, 2008, 356 pp. £21.50 ISBN 978—0—415—39562—5 (pbk) Erica Burman: Developments: Child, Image, Nation, London and New York: Routledge, 2008, 328 pp. £21.50 ISBN 978—0—415—37792—8 (pbk)

authors: Claiborne, Lise Bird

subjects: book review

abstract: The article reviews the book “Deconstructing Developmental Psychology”and “Developments: Child, Image, Nation”, By Erica Burman.

text: Review: Erica Burman: Deconstructing Developmental Psychology, London and New York: Routledge, 2008, 356 pp. £21.50 ISBN 978—0—415—39562—5 (pbk) Erica Burman: Developments: Child, Image, Nation, London and New York: Routledge, 2008, 328 pp. £21.50 ISBN 978—0—415—37792—8 (pbk) The article reviews the book “Deconstructing Developmental Psychology”and “Developments: Child, Image, Nation”, By Erica Burman.

year: 2010

title: A two-component transport model for solar wind fluctuations: Waves plus quasi-2D turbulence

authors: Oughton, Sean

subjects: solar wind

abstract: We present a model for the transport of solar wind fluctuations, based on the assumption that they can be well-represented using two distinct components: a quasi-2D turbulence piece and a wave-like piece. For each component, coupled transport equations for its energy, cross helicity, and characteristic lengthscale(s) are derived, along with an equation for the proton temperature. This energy-containing “two-component” model includes the effects of solar wind expansion and advection, driving by stream shear and pickup ions, and nonlinear cascades. Nonlinear effects are modeled using a recently developed one-point phenomenology for such a two-component model of homogeneous MHD turbulence [1]. Heating due to these nonlinear effects is included in the temperature equation. Numerical solutions are discussed and compared with observations

text: A two-component transport model for solar wind fluctuations: Waves plus quasi-2D turbulence We present a model for the transport of solar wind fluctuations, based on the assumption that they can be well-represented using two distinct components: a quasi-2D turbulence piece and a wave-like piece. For each component, coupled transport equations for its energy, cross helicity, and characteristic lengthscale(s) are derived, along with an equation for the proton temperature. This energy-containing “two-component” model includes the effects of solar wind expansion and advection, driving by stream shear and pickup ions, and nonlinear cascades. Nonlinear effects are modeled using a recently developed one-point phenomenology for such a two-component model of homogeneous MHD turbulence [1]. Heating due to these nonlinear effects is included in the temperature equation. Numerical solutions are discussed and compared with observations

year: 2010

title: Te Tiriti o Waitangi

authors: Maxwell, Te Kahautu

abstract: Whakawātea. Lyrics composed by Te Kahautu Maxwell. Performed by Ōpōtiki Mai Tawhiti (Kapa Haka group)

Waiata ā Tira: Aroha
Whakaeke: Pinepine Te Kura
Mōteatea: Tērā te haeata
Waiata ā Ringa: Tiaho Mai
Poi: E ia, e ia
Haka: Ranginui
Whakawātea: Te Tiriti o Waitangi

text: Te Tiriti o Waitangi Whakawātea. Lyrics composed by Te Kahautu Maxwell. Performed by Ōpōtiki Mai Tawhiti (Kapa Haka group)

Waiata ā Tira: Aroha
Whakaeke: Pinepine Te Kura
Mōteatea: Tērā te haeata
Waiata ā Ringa: Tiaho Mai
Poi: E ia, e ia
Haka: Ranginui
Whakawātea: Te Tiriti o Waitangi

year: 2024-02-23