Cometary science. Birth of a comet magnetosphere: a spring of water ions.

The Rosetta mission shall accompany comet 67P/Churyumov-Gerasimenko from a heliocentric distance of >3.6 astronomical units through perihelion passage at 1.25 astronomical units, spanning low and maximum activity levels. Initially, the solar wind permeates the thin comet atmosphere formed from sublimation, until the size and plasma pressure of the ionized atmosphere define its boundaries: A magnetosphere is born. Using the Rosetta Plasma Consortium ion composition analyzer, we trace the evolution from the first detection of water ions to when the atmosphere begins repelling the solar wind (~3.3 astronomical units), and we report the spatial structure of this early interaction. The near-comet water population comprises accelerated ions (<800 electron volts), produced upstream of Rosetta, and lower energy locally produced ions; we estimate the fluxes of both ion species and energetic neutral atoms.

Climate change and mitigation.

Planet Earth has experienced repeated changes of its climate throughout time. Periods warmer than today as well as much colder, during glacial episodes, have alternated. In our time, rapid population growth with increased demand for natural resources and energy, has made society increasingly vulnerable to environmental changes, both natural and those caused by man; human activity is clearly affecting the radiation balance of the Earth. In the session "Climate Change and Mitigation" the speakers offered four different views on coal and CO2: the basis for life, but also a major hazard with impact on Earth's climate. A common denominator in the presentations was that more than ever science and technology is required. We need not only understand the mechanisms for climate change and climate variability, we also need to identify means to remedy the anthropogenic influence on Earth's climate.

Attitudes of nursing staff working with older people towards nutritional nursing care.

AIM: The aim of this study was to examine attitudes of the nursing staff in geriatric care towards factors of importance for nutritional nursing care. BACKGROUND: Studies show that nutritional risk assessment is seldom performed on older patients as routine and very few patients have a nutritional care plan. Patients in long-term care who are easy to feed are also found to be looked upon more positively than those with high feeding needs. METHODS: A total of 252 registered nurses and nurse aids working at geriatric rehabilitation and medical care clinics and resident homes participated in the study. Attitudes were examined using the Staff Attitudes to Nutritional Nursing Care Geriatric scale. The scale includes 18 items and was designed as a one to five-point Lickert-type scale. It gives a total score and five subscales representing the dimensions 'Norms', 'Habits', 'Assessment', 'Intervention' and 'Individualization'. A higher score indicates a more positive attitude. RESULTS: Of all nursing staff, 53% displayed a positive attitude towards factors of importance for nutritional nursing care and the rest displayed a neutral or negative attitude. The 'Intervention' dimension, dealing with nutritional problems and how to manage them, reflected the highest level of positive attitudes, which represents 71% of the nursing staff. The 'Norms' dimension had the lowest relative frequency of positive attitudes, 27%. The registered nurses held significantly more positive attitudes than the nurse aids did. CONCLUSIONS: Nutritional issues comprise an important and time-consuming responsibility in geriatric care; however, nursing staff do not show an unequivocal positive attitude regarding this responsibility. The consequences this entails for the older patient need to be examined further. Relevance to clinical practice. Nursing staff play an important role in caring for patients who are malnourished or at risk for malnutrition. Positive attitudes might hinder the development of undernourishment or the further worsening of an already undernourished patient's condition.

Martian atmospheric erosion rates.

Mars was once wet but is now dry, and the fate of its ancient carbon dioxide atmosphere is one of the biggest puzzles in martian planetology. We have measured the current loss rate due to the solar wind interaction for different species: Q(O+) = 1.6.10(23) per second = 4 grams per second (g s(-1)), Q(O+2) = 1.5.10(23) s(-1) = 8 g s(-1), and Q(CO+2) = 8.10(22) s(-1) = 6 g s(-1) in the energy range of 30 to 30,000 electron volts per charge. These rates can be propagated backward over a period of 3.5 billion years, resulting in the total removal of 0.2 to 4 millibar of carbon dioxide and a few centimeters of water. The escape rate is low, and thus one has to continue searching for water reservoirs and carbon dioxide stores on or beneath the planetary surface and investigate other escape channels.