title: Transformative pedagogy and language learning in Maori and Irish contexts

authors: Glynn, Ted

subjects: transformative pedagogy

abstract: Establishing positive learning communities in classrooms where pedagogies are socially and culturally responsive and centred on shared life experiences is critical for the revitalisation of minoritised languages such as Irish and Māori, which lack the dominance and power of the wider languages of government and communication. Transformative pedagogy and pedagogical re-positioning of teachers are essential to legitimising and affirming minoritised languages in the classroom. Three small-scale New Zealand studies of emerging literacy in Māori are introduced, exemplifying a responsive and transformative pedagogy that enables teachers to position themselves as socially and culturally responsive participants within classroom contexts. These studies offer strategies that might facilitate the development of similar transformative pedagogy in Irish contexts also.

text: Transformative pedagogy and language learning in Maori and Irish contexts Establishing positive learning communities in classrooms where pedagogies are socially and culturally responsive and centred on shared life experiences is critical for the revitalisation of minoritised languages such as Irish and Māori, which lack the dominance and power of the wider languages of government and communication. Transformative pedagogy and pedagogical re-positioning of teachers are essential to legitimising and affirming minoritised languages in the classroom. Three small-scale New Zealand studies of emerging literacy in Māori are introduced, exemplifying a responsive and transformative pedagogy that enables teachers to position themselves as socially and culturally responsive participants within classroom contexts. These studies offer strategies that might facilitate the development of similar transformative pedagogy in Irish contexts also.

year: 2009

title: Te Kahautu Maxwell on Te Kooti and Ringatu (Interviewed by Tama Muru)

authors: Maxwell, Te Kahautu

abstract: In October 1869 musket fire erupted at Te Porere about sixty kilometres north of here, in the shadow of Mount Tongariro in the last major battle of the New Zealand wars. 

Armed constabulary and Maori fighters, clashed with the forces of the prophet Te Kooti Arikinui Te Turiki who had built an earth redoubt at Te Porere.  It was overwhelmed during the battle, but Te Kooti and his surviving followers escaped. 

Today the site is a tourist attraction but what also endured is the Ringatu Church, founded by Te Kooti. In 2018 it celebrated its 150th anniversary. 

Ringatu mixes the Bible with Maori custom and, like Matariki, follows annual cycles such as Te Huamata in June for planting and Te Pure, the harvest, each November. 

We spoke to Professor Te Kahautu Maxwell , a minister in the Ringatu Church and a senior academic in Maori and Indigenous Studies at the University of Waikato.

text: Te Kahautu Maxwell on Te Kooti and Ringatu (Interviewed by Tama Muru) In October 1869 musket fire erupted at Te Porere about sixty kilometres north of here, in the shadow of Mount Tongariro in the last major battle of the New Zealand wars. 

Armed constabulary and Maori fighters, clashed with the forces of the prophet Te Kooti Arikinui Te Turiki who had built an earth redoubt at Te Porere.  It was overwhelmed during the battle, but Te Kooti and his surviving followers escaped. 

Today the site is a tourist attraction but what also endured is the Ringatu Church, founded by Te Kooti. In 2018 it celebrated its 150th anniversary. 

Ringatu mixes the Bible with Maori custom and, like Matariki, follows annual cycles such as Te Huamata in June for planting and Te Pure, the harvest, each November. 

We spoke to Professor Te Kahautu Maxwell , a minister in the Ringatu Church and a senior academic in Maori and Indigenous Studies at the University of Waikato.

year: 2025

title: Rates of photospheric magnetic flux cancellation measured with Hinode

authors: Park, Soyoung

subjects: magnetic fields

abstract: Photospheric magnetic flux cancellation on the Sun is generally believed to be caused by magnetic reconnection occurring in the low solar atmosphere. Individual canceling magnetic features are observationally characterized by the rate of flux cancellation. The specific cancellation rate, defined as the rate of flux cancellation divided by the interface length, gives an accurate estimate of the electric field in the reconnecting current sheet. We have determined the specific cancellation rate using the magnetograms taken by the Solar Optical Telescope (SOT) aboard the Hinode satellite. The specific rates determined with SOT turned out to be systematically higher than those based on the data taken by the Michelson Doppler Imager (MDI) aboard the Solar and Heliospheric Observatory. The median value of the specific cancellation rate was found to be 8 × 106 G cm s-1—a value four times that obtained from the MDI data. This big difference is mainly due to a higher angular resolution and better sensitivity of the SOT, resulting in magnetic fluxes up to five times larger than those obtained from the MDI. The higher rates of flux cancellation correspond to either faster inflows or stronger magnetic fields of the reconnection inflow region, which may have important consequences for the physics of photospheric magnetic reconnection.

text: Rates of photospheric magnetic flux cancellation measured with Hinode Photospheric magnetic flux cancellation on the Sun is generally believed to be caused by magnetic reconnection occurring in the low solar atmosphere. Individual canceling magnetic features are observationally characterized by the rate of flux cancellation. The specific cancellation rate, defined as the rate of flux cancellation divided by the interface length, gives an accurate estimate of the electric field in the reconnecting current sheet. We have determined the specific cancellation rate using the magnetograms taken by the Solar Optical Telescope (SOT) aboard the Hinode satellite. The specific rates determined with SOT turned out to be systematically higher than those based on the data taken by the Michelson Doppler Imager (MDI) aboard the Solar and Heliospheric Observatory. The median value of the specific cancellation rate was found to be 8 × 106 G cm s-1—a value four times that obtained from the MDI data. This big difference is mainly due to a higher angular resolution and better sensitivity of the SOT, resulting in magnetic fluxes up to five times larger than those obtained from the MDI. The higher rates of flux cancellation correspond to either faster inflows or stronger magnetic fields of the reconnection inflow region, which may have important consequences for the physics of photospheric magnetic reconnection.

year: 2009