Enhanced Spontaneous Emission Into The Mode Of A Cavity QED System

We study the light generated by spontaneous emission into a mode of a cavity QED system under weak excitation of the orthogonally polarized mode. Operating in the intermediate regime of cavity QED with comparable coherent and decoherent coupling constants, we find an enhancement of the emission into the undriven cavity mode by more than a factor of 18.5 over that expected by the solid angle subtended by the mode. A model that incorporates three atomic levels and two polarization modes quantitatively explains the observations.Comment: 9 pages, 2 figures, to appear in May 2007 Optics Letter

Idealized Antenna Patterns for Use in Communication-satellite Interference Studies

Idealized antenna patterns for communication satellite interference studie

Steady State Entanglement in Cavity QED

We investigate steady state entanglement in an open quantum system, specifically a single atom in a driven optical cavity with cavity loss and spontaneous emission. The system reaches a steady pure state when driven very weakly. Under these conditions, there is an optimal value for atom-field coupling to maximize entanglement, as larger coupling favors a loss port due to the cavity enhanced spontaneous emission. We address ways to implement measurements of entanglement witnesses and find that normalized cross-correlation functions are indicators of the entanglement in the system. The magnitude of the equal time intensity-field cross correlation between the transmitted field of the cavity and the fluorescence intensity is proportional to the concurrence for weak driving fields.Comment: enhanced discussion, corrected formulas, title change, 1 added figur

Studies of auroral X-ray imaging from high altitude spacecraft

Results of a study of techniques for imaging the aurora from a high altitude satellite at X-ray wavelengths are summarized. The X-ray observations allow the straightforward derivation of the primary auroral X-ray spectrum and can be made at all local times, day and night. Five candidate imaging systems are identified: X-ray telescope, multiple pinhole camera, coded aperture, rastered collimator, and imaging collimator. Examples of each are specified, subject to common weight and size limits which allow them to be intercompared. The imaging ability of each system is tested using a wide variety of sample spectra which are based on previous satellite observations. The study shows that the pinhole camera and coded aperture are both good auroral imaging systems. The two collimated detectors are significantly less sensitive. The X-ray telescope provides better image quality than the other systems in almost all cases, but a limitation to energies below about 4 keV prevents this system from providing the spectra data essential to deriving electron spectra, energy input to the atmosphere, and atmospheric densities and conductivities. The orbit selection requires a tradeoff between spatial resolution and duty cycle

An experimental study of the temporal statistics of radio signals scattered by rain

A fixed-beam bistatic CW experiment designed to measure the temporal statistics of the volume reflectivity produced by hydrometeors at several selected altitudes, scattering angles, and at two frequencies (3.6 and 7.8 GHz) is described. Surface rain gauge data, local meteorological data, surveillance S-band radar, and great-circle path propagation measurements were also made to describe the general weather and propagation conditions and to distinguish precipitation scatter signals from those caused by ducting and other nonhydrometeor scatter mechanisms. The data analysis procedures were designed to provide an assessment of a one-year sample of data with a time resolution of one minute. The cumulative distributions of the bistatic signals for all of the rainy minutes during this period are presented for the several path geometries

Ukraine At The Fulcrum: A Nuclear House Of Cards

The foundation of preserving and enhancing global nuclear security rests on three fundamental pillars: nuclear disarmament; preventing further proliferation of nuclear weapons; and international cooperation aimed at safeguarding nuclear materials. Today, experts argue that the recent decision of Russian president Vladimir Putin to cut cooperative efforts to secure nuclear materials are placing in peril the future of international efforts to promote global nuclear security. We argue that in addition to the clear erosion of the third pillar of nuclear security, there are more threatening ramifications resulting from the recent actions of Russia in Ukraine. The aggressive actions of Russia in Ukraine, together with the unwillingness of the international community to exert sufficient pressure on Russia to honor the promises made to Ukraine in exchange for giving up nuclear weapons in 1990s (the Budapest Memorandum) are detrimental to non-proliferation objectives and reach far beyond the geographic boundaries of the current conflict. In addition, they may disrupt both further nuclear disarmament and stimulate proliferation of nuclear weapons. To the government of any country who has resisted the push toward nuclearization based on trust placed in international agreements, the inactions and/or inability of the international community to resist or reverse Russia’s illegal actions must cause great concern. If binding diplomatic agreements are seen to only bind one party – the weaker party – that party will understandably be very hesitant to place full faith in any diplomatic document short of a binding treaty that has clear and required enforcement mechanisms. This is especially true when the stakes are a country’s national security and ultimately its sovereignty. If any one of these nations moved toward nuclear status, the atomic dominos would surely begin to tumble, and the delicate nuclear equilibrium that defines the global nuclear security landscape today would be lost

Stochastic modelling of intermittent scrape-off layer plasma fluctuations

Single-point measurements of fluctuations in the scrape-off layer of magnetized plasmas are generally found to be dominated by large-amplitude bursts which are associated with radial motion of blob-like structures. A stochastic model for these fluctuations is presented, with the plasma density given by a random sequence of bursts with a fixed wave form. Under very general conditions, this model predicts a parabolic relation between the skewness and kurtosis moments of the plasma fluctuations. In the case of exponentially distributed burst amplitudes and waiting times, the probability density function for the fluctuation amplitudes is shown to be a Gamma distribution with the scale parameter given by the average burst amplitude and the shape parameter given by the ratio of the burst duration and waiting times.Comment: 11 pages, 1 figur