The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) will answer important
questions posed by the mission’s main objectives. After Giotto, this will be the first time …

… The energy pass of the ESA is about 5-6 e V at 100 e V of pre-acceleration, assuming all
deflection voltages are optimised. This energy pass is very sensitive to the actual RPA …

On board the four Cluster spacecraft, the Cluster Ion Spectrometry (CIS) experiment measures
the full, three-dimensional ion distribution of the major magnetospheric ions (H + , He + , …

We report observations of “fast solitary waves” that are ubiquitous in downward current regions
of the mid‐altitude auroral zone. The single‐period structures have large amplitudes (up …

Background The process of implementation of clinical guidelines ie getting guidelines into
practice has been extensively reviewed and meta-reviewed from a generic perspective. …

… The mass resolution characteristics of the spectrometers are illustrated in Figure 3, where
some flight data from CXA I on the energy step E/q -- 1.0 kev are shown. The data were taken …

… (E/Q), mass per charge (M/Q) and velocity distributions. The HERS E/Q range is 10 to 4,500
eV/e, … The HIS range is 300 to 1,400 eV/e. Both instrument fields of view are fans which rotate …

… Two examples, o•e on the dayside at high latitudes and one … up the field lines from t•e
ionosphere. A preliminary estimate of the … sampled the energy range 0.37 • E • 1.28 keV. The deep …

Electric field and energetic particle observations by the Fast Auroral Snapshot (FAST)
satellite provide convincing evidence of particle acceleration by quasi‐static, magnetic‐field‐…

Objective To determine if polymorphisms of the macrophage migration inhibitory factor (MIF)
gene are associated with juvenile idiopathic arthritis (JIA). Methods Denaturing high‐…