Nanoscale focused ion beams (FIBs) represent one of the most useful tools in nanotechnology, enabling nanofabrication via milling and gas-assisted deposition, microscopy and microanalysis, and selective, spatially resolved doping of materials. Recently, a new type of FIB source has emerged, which uses ionization of laser cooled neutral atoms to produce the ion beam. The extremely cold temperatures attainable with laser cooling (in the range of 100 μK or below) result in a beam of ions with a very small transverse velocity distribution. This corresponds to a source with extremely high brightness that rivals or may even exceed the brightness of the industry standard Ga+ liquid metal ion source. In this review we discuss the context of ion beam technology in which these new ion sources can play a role, their principles of operation, and some examples of recent demonstrations. The field is relatively new, so only a few applications have been demonstrated, most notably low energy ion microscopy with Li ions. Nevertheless, a number of promising new approaches have been proposed and/or demonstrated, suggesting that a rapid evolution of this type of source is likely in the near future.
Abstract:The photovoltaic bands on the long-wave infrared focal plane assembly of Terra MODIS, bands 27-30, have suffered from steadily increasing contamination from electronic crosstalk as the mission has progressed. This contamination has a great impact on MODIS data products, including image striping and radiometric bias in the Level-1B calibrated radiance product, and incorrect retrieval in atmospheric products that rely on data from bands 27-30, such as the cloud mask and cloud particle phase products. In this work, we describe the development of an electronic crosstalk correction for bands 27-30 of Terra MODIS using observations of the Moon. In this approach, the derived correction coefficients account for both the "in-band" and "out-of-band" contribution to the signal contamination, which is not considered in previous implementations of the lunar-based correction. The correction coefficients are applied to both the on-board calibrator data and the Earth-view data, resulting in a significant reduction in the image striping and radiometric bias in the Level-1B data, as well as a better performance in the Level-2 cloud mask and cloud particle phase products. This approach will be implemented for Terra MODIS Collection 6 in 2017.
A magneto-optic trap (MOT) can provide a well-polarized, backing-free, localized source of radioactive atoms for b-decay experiments. We have trapped approximately 6000 atoms of 38 K m (t 1͞2 0.925 s) and 2000 atoms of 37 K (1.226 s) produced at the TRIUMF on-line separator TISOL in a vapor-cell MOT. We have measured optical isotope shifts and deduced the nuclear charge radii, which show an unusual lack of change at the neutron number N 20 shell closure. Plans include a search for scalar contributions to the b 1 -n correlation in the 0 1 ! 0 1 decay of 38 K m . [S0031-9007(97)03637-5] PACS numbers: 23.40. Bw, 29.25.Rm, 32.80.Pj, 32.80.Ys The novel use of magneto-optically trapped radioactive atoms promises improvements in performing symmetry tests of the standard model. Optically trapped atoms are confined in a small volume in space (a few mm 3 ), have negligible source thickness, and can be optically pumped to achieve close to 100% atomic and nuclear polarization. These conditions are favorable for carrying out experiments to study weak interaction symmetries in b decay [1-3], and to measure isotopic dependence of parity nonconservation (PNC) in heavy atoms [2,[4][5][6]. Here we measure nuclear properties of ground and isomeric states of the trapped atoms.Among alkali atoms, which have simple electronic structure convenient for laser trapping, potassium isotopes offer rich opportunities for b-decay experiments. 37 K and 38 K m each decay predominantly by a single superallowed transition. The b-n correlation in a I p 0 1 ! 0 1 Fermi decay is sensitive to the exchange of hypothetical scalar bosons. Limits on the scalar interaction are poor, both from b decay and from high-energy experiments, and a 1% measurement of the b-n correlation coefficient a would be competitive [7]. Among alkali atoms, isomeric 38 K m has the only such pure Fermi decay. The mixed Fermi-Gamow-Teller (I p 3͞2 1 ! 3͞2 1 ) decay of 37 K is suitable for b-asymmetry experiments and positron longitudinal polarization measurements [8], which are sensitive to the presence of right-handed currents in the weak interaction.The half-lives of 38 K m (0.925 s) and 37 K (1.226 s) are an order of magnitude shorter than isotopes trapped in related work elsewhere [1,4,9]. This creates an experimental challenge in the production and trapping of these isotopes; however, the shorter lifetimes make it easier to achieve trap lifetimes long enough that nearly all trapped atoms undergo radioactive decay while in the trap (collisions with residual gas at 10 29 Torr produce a trap lifetime of 10 s).Here we report the successful coupling of a magnetooptic trap (MOT) to the copious production of an online isotope separator (TISOL). With this arrangement we have trapped approximately 6000 atoms of 38 K m or 2000 atoms of 37 K, sufficient to begin b-decay experiments. We have measured the isotope shifts of 37 K, 38 K m in the trapping transition: the deduced nuclear charge radii show an unusual lack of change at the major neutron number N 20 shell closure. We also wil...
The Moderate Resolution Imaging Spectroradiometer (MODIS) is one of the key sensors among the suite of remote sensing instruments on board the Earth Observing System Terra and Aqua spacecrafts. For each MODIS spectral band, the sensor degradation has been measured using a set of on-board calibrators. MODIS also uses lunar observations from nearly monthly spacecraft maneuvers, which bring the Moon into view through the spaceview port, helping to characterize the scan mirror degradation at a different angles of incidence. Throughout the Terra mission, contamination of the long-wave infrared photovoltaic band (LWIR PV, bands 27 − 30) signals has been observed in the form of electronic crosstalk, where signal from each of the detectors among the LWIR PV bands can leak to the other detectors, producing a false signal contribution. This contamination has had a noticeable effect on the MODIS science products since 2010 for band 27, and since 2012 for bands 28 and 29. Images of the Moon have been used effectively for determining the contaminating bands, and have also been used to derive correction coefficients for the crosstalk contamination. In this paper, we introduce an updated technique for characterizing the crosstalk contamination among the LWIR PV bands using data from lunar calibration events. This approach takes into account both the "in-band" and "out-of-band" contribution to the signal contamination for each detector in bands 27 − 30, which is not considered in previous works. The crosstalk coefficients can be derived for each lunar calibration event, providing the time dependence of the crosstalk contamination. Application of these coefficients to Earth-view image data results in a significant reduction in image contamination and a correction of the scene radiance for bands 27 − 30. Also, this correction shows a significant improvement to certain threshold tests in the MODIS Level-2 Cloud Mask. In this paper, we will detail the methodology used to identify and correct the crosstalk contamination for the LWIR PV bands in Terra MODIS. The derived time-dependent crosstalk coefficients will also be discussed. Finally, the impact of the correction on the downstream data products will be analyzed.
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