The Insider Threat

The Insider threat is defined similarly by experts in the information technology world for businesses, but addressing the threat has not been of great focus for most organizations. Technology and the Internet have grown exponentially over the past decade leading to changes in how business is conducted. Some basic business practices remain the same; protect the organization and its customers from breach of privacy. How data is gathered, stored, and retrieved has changed. Protecting the perimeter is still important, but these changes in technology now open the doors to a new threat; one that is known but not commonly protected against; the insider. Whether intentionally, or accidentally, the insider threat needs to be incorporated into the currently used security architectures and best practices. How should an organization include the insider threat to the current architecture is the question. Changes need to be made by organizations to the current security architecture. Currently, using technology is not enough, but is still necessary. In order to make it better, considering the employee as a whole and the daily activities necessary to complete a job, as well as working with other business units as a whole needs to be included in the architecture. Behavioral traits can be considered but there are issues in privacy that also need to be considered. Monitoring can be done, but that should not be the only thing considered. Employees lack knowledge as to why actions can have a negative effect on an organization and the way to address this is education. Educating end users is necessary and should be performed regularly to keep not just the technologically inclined up to date. Without education, the current technology used will continue to keep out the intruders, but will not be effective enough to protect against intentional and accidental misuse of the organization and its networks

Noncontact modulation calorimetry of metallic liquids in low Earth orbit

Noncontact modulation calorimetry using electromagnetic heating and radiative heat loss under ultrahigh-vacuum conditions has been applied to levitated solid, liquid, and metastable liquid samples. This experiment requires a reduced gravity environment over an extended period of time and allows the measurement of several thermophysical properties, such as the enthalpy of fusion and crystallization, specific heat, total hemispherical emissivity, and effective thermal conductivity with high precision as a function of temperature. From the results on eutectic glass forming Zr-based alloys thermodynamic functions are obtained which describe the glass-forming ability of these alloys

New Insights into Cosmic Ray induced Biosignature Chemistry in Earth-like Atmospheres

With the recent discoveries of terrestrial planets around active M-dwarfs, destruction processes masking the possible presence of life are receiving increased attention in the exoplanet community. We investigate potential biosignatures of planets having Earth-like (N$_2$-O$_2$) atmospheres orbiting in the habitable zone of the M-dwarf star AD Leo. These are bombarded by high energetic particles which can create showers of secondary particles at the surface. We apply our cloud-free 1D climate-chemistry model to study the influence of key particle shower parameters and chemical efficiencies of NOx and HOx production from cosmic rays. We determine the effect of stellar radiation and cosmic rays upon atmospheric composition, temperature, and spectral appearance. Despite strong stratospheric O$_3$ destruction by cosmic rays, smog O$_3$ can significantly build up in the lower atmosphere of our modeled planet around AD Leo related to low stellar UVB. N$_2$O abundances decrease with increasing flaring energies but a sink reaction for N$_2$O with excited oxygen becomes weaker, stabilizing its abundance. CH$_4$ is removed mainly by Cl in the upper atmosphere for strong flaring cases and not via hydroxyl as is otherwise usually the case. Cosmic rays weaken the role of CH$_4$ in heating the middle atmosphere so that H$_2$O absorption becomes more important. We additionally underline the importance of HNO$_3$ as a possible marker for strong stellar particle showers. In a nutshell, uncertainty in NOx and HOx production from cosmic rays significantly influences biosignature abundances and spectral appearance.Comment: Manuscript version after addressing all referee comments. Published in Ap

FlexRiLoG -- A SageMath Package for Motions of Graphs

In this paper we present the SageMath package FlexRiLoG (short for flexible and rigid labelings of graphs). Based on recent results the software generates motions of graphs using special edge colorings. The package computes and illustrates the colorings and the motions. We present the structure and usage of the package

Franck-Condon Physics in A Single Trapped Ion

We propose how to explore the Franck-Condon (FC) physics via a single ion confined in a spin-dependent potential, formed by the combination of a Paul trap and a magnetic field gradient. The correlation between electronic and vibrational degrees of freedom, called as electron-vibron coupling, is induced by a nonzero gradient. For a sufficiently strong electron-vibron coupling, the FC blockade of low-lying vibronic transitions takes place. We analyze the feasibility of observing the FC physics in a single trapped ion, and demonstrate various potential applications of the ionic FC physics in quantum state engineering and quantum information processing.Comment: 7 pages, 5 figure