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  • Hatti, Neelambar, et al. (författare)
  • Disappearing Daughters and Intensification of Gender Bias : Evidence from Two Villages studies in South India
  • 2010
  • Ingår i: Sociological Bulletin. - 0038-0229. ; 59:1, s. 111-133
  • Tidskriftsartikel (refereegranskat)abstract
    • Why are female children still at risk in India despite progress in education, increasing participation of women in economic and political activities, and an overall improvement in the status of women? Is there any significant shift from 'son preference' to 'daughter discrimination'? Based on a study of two villages from low-fertility regions of Karnataka and Tamil Nadu, this paper attempts to understand the factors responsible for the increasing discrimination against girls, even before they are born. The widespread use of sex-determination tests and abortion facilities has given an opportunity for parents to acheive the desired family size and the desired gender composition of children. There is an intesification of gender bias particularly among the peasant communities. The rapid fertility decline, not accompanied by changes in the cultural values and gender inequality, has resulted in a deliberate attempt to 'get rid of girls'.
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  • Wedemeyer, S., et al. (författare)
  • Solar Science with the Atacama Large Millimeter/Submillimeter Array-A New View of Our Sun
  • 2016
  • Ingår i: Space Science Reviews. - : Springer Science and Business Media LLC. - 0038-6308 .- 1572-9672. ; 200:1-4, s. 1-73
  • Forskningsöversikt (refereegranskat)abstract
    • The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can address a broad range of fundamental scientific questions in solar physics. The radiation observed by ALMA originates mostly from the chromosphere-a complex and dynamic region between the photosphere and corona, which plays a crucial role in the transport of energy and matter and, ultimately, the heating of the outer layers of the solar atmosphere. Based on first solar test observations, strategies for regular solar campaigns are currently being developed. State-of-the-art numerical simulations of the solar atmosphere and modeling of instrumental effects can help constrain and optimize future observing modes for ALMA. Here we present a short technical description of ALMA and an overview of past efforts and future possibilities for solar observations at submillimeter and millimeter wavelengths. In addition, selected numerical simulations and observations at other wavelengths demonstrate ALMA's scientific potential for studying the Sun for a large range of science cases.
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  • Resultat 1-7 av 7

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