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We present measurement results demonstrating that a conducting lead sphere exposed to electromagnetic (e/m) waves in the infrared (IR) regime, is attracted by e/m waves. The result may seem surprising and against conventional wisdom that electromagnetic wave forcing should lead to a repulsive force. Nonetheless, all our experiments show that the attractive force can be determined quantitatively, and that they are reproducible. Our experiment setup is a Cavendish torsion-balance experiment with lead spheres, one of the spheres intermittently irradiated by IR light. Because the Cavendish experiment is well known, simple, and readily available, the results can be easily verified or falsified. However, to avoid Bernoulli and other external forcing effects, the entire experimental setup should be placed in a vacuum chamber. In our case the experiments were performed at \approx 4 \cdot 10^-7 mbar. One of the 20 g lead spheres was intermittently irradiated by infrared radiation from a lamp covered by an aluminium foil. Two independent experiments (V1 and V2) are described. Besides showing that wave energy and momentum transfer leads to attraction, we also describe some experimental requirements and constraints. The lamp was powered on during 10 or 12 s, the power changing between 8, 16, and 26 W. All measurements, including those affected by lamp out-gassing, shows that the attracting force on the lead sphere increases with increasing irradiative energy. From the V2 experiment, preceded by lamp "baking" to eliminate repulsive out-gassing forces, the irradiative energy 8.7 Ws on the sphere resulted in a total force 2.9+/-0.5\cdot 10^-9 (N). From the V2 experiment we also derive a power law relation between incident radiation energy (W) and the attractive force, corresponding to F=2.8\cdot 10^-10 W^1.1, with R^2=0.95., Comment: 17 pages, 6 figures

Wave induced attraction of matter is a unique aspect of ponderomotive forcing by electromagnetic (e/m) waves in plasmas. The Miller force, sometimes denoted the gradient force, is of particular interest, because the direction as well as magnitude of the Miller force on a plasma depends on the wave frequency. While plasma is usually considered in its gaseous form, solid bodies can also be treated as plasma, denoted solid-state plasma. The first experimental proof of wave effects in magnetized solid-state plasmas (Lundqvist, 1949, Herlofson, 1950) came after the suggestion by Alfv\'en (1942) on the possible existence of magneto-hydrodynamic (MHD) waves. However, most of our knowledge basis on MHD/Alfv\'en waves have since then emerged from space- and laboratory (gaseous) plasmas. It is therefore timely to investigate further the applicability of e/m wave ponderomotive forcing on solid-state plasma. In this report we discuss the applicability of the ponderomotive Miller force on solid-state plasmas. At this stage the treatise will be rather qualitative, based on theories developed for space plasma. We assume that e/m wave energy and momentum is transferred in a thin surface layer constituting solid-state plasma. A Miller force results from the wave pressure gradient set up in the surface layer. Since the solid body constitute a coupled system (lattice), the Miller force will act on all atoms in the body, the total force limited by the wave input power. A quantitative comparison with experimental results obtained from a Cavendish vacuum experiment (Lidgren and Lundin, 2010) gives a surprisingly good agreement between theory and experiments. As further proof for e/m wave attraction of matter, we show a simulation, taking into account the measured pendulum offsets., Comment: 13 pages, 2 figures

Observations of energetic neutral atoms (ENA) in the energy range 26- 52 keV are reported from four occasions during geomagnetically disturbed periods. The data were acquired by the ENA imager flown on the Swedish microsatellite Astrid in a 1000 km circular orbit with 83 deg inclination. The ENA imager separates charged particles from neutrals through an electrostatic deflection system in the energy range between 0.1 and 114 keV. ENA images obtained from vantage points in the polar cap and in the afternoon magnetic local time (MLT) hours looking into the antisunward hemisphere show intense ENA fluxes (approx. 10(exp 4)/sq cm sr s over 26-37 keV) coming from the dusk region and low altitudes (approx. 300 km). The morphology shows no relation to local magnetic field excluding the possibility of charged particle detection. It is concluded that the source of these ENAs are precipitating/mirroring ions from the ring current/trapped radiation interacting with the exobase on auroral L-shells and in the dusk region. The observed ENA fluxes show a relation with Kp and Dst geomagnetic indices. The observed ENA spectrum from a geomagnetic storm on February 8, 1995, is investigated in more detail and compared to the parent ion spectrum obtained by the Defense Meteorological Satellite Project (DMSP) satellite, Fl2, during the same period on L = 6 +/- 2 around dusk. The observed ENA spectral slope is used to derive the parent ion spectral temperature. The derived ion temperatures range is 3.0 - 6.0 keV for H and 4.5 - 8.5 keV for O. The higher of these ion temperatures comes closest in agreement to the extrapolated DMSP spectrum leading us to favor O over H as the species of the detected ENAS. It is shown that the detected ENAs must have been produced at L greater than or equal to 6 to reach the detector without atmospheric attenuation and that the main energy dependence of the ENA spectrum, apart from the parent ion spectrum, is governed by the energy dependence of the charge exchange cross section between ions and exospheric oxygen.