House at Bogwest, Wexford, Ireland: Steve Larkin Architect

Critical review of House at Bogwest by Steve Larkin Architects. Text by editorial team, drawings by Steve Larkin and photographs by Alice Clancy.

Lost and Found? A Parable of the Architect (Male) and the Academic (Female)

The following text captures an interview, conducted over three evenings, between a practicing architect (male) and an architecture academic (female and feminist). This is a conversation between two long-standing friends who did their Part 3 professional exam together more than twenty-five years ago. Since then, they have taken different career paths and lived lives at different paces and in different places. Every so often they meet over coffee to laugh and argue about architecture, bemoan failures, and share successes.

The academic initiated the interview in order to hear an honest and open account of the career experience of a male architect. She hoped that their longstanding friendship would lead to less guarded responses. The answers to the questions were always going to be personally challenging to the interviewer and possibly to their friendship. The interview is a form of ethnographic study: a structured, qualitative process within a long term, immersed context. But when ‘the immersed context’ is a much-valued friendship, it is a precarious action. Nevertheless, for the future of gendered relationships both protagonists accepted the risks.

Extreme ultraviolet emission lines of Ca XV in solar and laboratory spectra

New R-matrix calculations of electron impact excitation rates in Ca XV are used to derive theoretical electron density diagnostic emission line intensity ratios involving 2s(2)2p(2)- 2s2p(3) transitions, specifically R-1 = I(208.70 Angstrom)/I(200.98 Angstrom), R-2 = I(181.91 Angstrom)/I(200.98 Angstrom), and R-3 = I(215.38 Angstrom)/I(200.98 Angstrom), for a range of electron temperatures (T-e = 10(6.4)-10(6.8) K) and densities (Ne = 10(9)-10(13) cm(-3)) appropriate to solar coronal plasmas. Electron densities deduced from the observed values of R-1, R-2, and R-3 for several solar flares, measured from spectra obtained with the Naval Research Laboratory's S082A spectrograph on board Skylab, are found to be consistent. In addition, the derived electron densities are in excellent agreement with those determined from line ratios in Ca XVI, which is formed at a similar electron temperature to Ca XV. These results provide some experimental verification for the accuracy of the line ratio calculations, and hence the atomic data on which they are based. A set of eight theoretical Ca XV line ratios involving 2s(2)2p(2)-2s2p(3) transitions in the wavelength range similar to140-216 Angstrom are also found to be in good agreement with those measured from spectra of the TEXT tokamak plasma, for which the electron temperature and density have been independently determined. This provides additional support for the accuracy of the theoretical line ratios and atomic data.