Visual Culture Project: Confederate War Etchings: Searching for Arms by Adalbert Johann Volck

Adalbert Johann Volck’s 1861 sketch of Union soldiers, “Searching for Arms,” represents a substantial contribution to the narrative about gender relations during the American Civil War. This simple, small sketch offers the observer a window into the past. It is a collision of symbols and meaning—from gender to war to the household—all wrapped up in one image. This is a portrait sketch of a woman being invaded in her domestic, private sphere, revealing so much about gender relations during the time. The mistress herself seemed to embody a vast range of sentiments such as anger, fear, frailty, and strength, proving the tension in her role as a wife, a mother, and guardian of the home. This inner conflict is something that all women faced during this time as they strove to remain loyal to the cause for which their husbands fought

Longitudinal Polarization at future e+e−e^+e^- Colliders and Virtual New Physics Effects

The theoretical merits of longitudinal polarization asymmetries of electron-positron annihilation into two final fermions at future colliders are examined, using a recently proposed theoretical description. A number of interesting features, valid for searches of virtual effects of new physics, is underlined, that is reminiscent of analogous properties valid on top of $Z$ resonance. As an application to a concrete example, we consider the case of a model with triple anomalous gauge couplings and show that the additional information provided by these asymmetries would lead to a drastic reduction of the allowed domain of the relevant parameters.Comment: 18 pages and 1 figure. e-mail: [email protected]

Underlying causes of commercial bank failures in the 1980s

An examination of the contributions of economic and managerial factors to commercial bank failures in the 1980s.Bank failures

To cope with California’s drought, policymakers must gobeyond water conservation and rationing

Two thirds of the state of California is experiencing extreme to exceptional drought conditions after four dry years. B. Lynn Ingram writes that to cope with the drought, those in the Golden State need to plan for the long-term to increase resilience to extended water scarcity. She argues that policymakers must now think more collaboratively about reducing the ‘water footprint’ of Californians and the products they produce

California needs to begin a serious and comprehensive plan to adapt to what may be a very long drought

California is currently in the midst of one of the worst droughts in the state’s history. Despite the crisis, the Golden State’s taps continue to run, with water use now far exceeding supply. B. Lynn Ingram writes that the current drought is just one of many very dry periods California has experienced regularly over the last 5,000 years or so. Taking the hardship of indigenous populations in previous droughts as a warning, she writes that the state’s rapid population growth is placing huge pressure on local water reserves. A comprehensive plan which takes advantage of new technologies such as wastewater recycling and ocean desalinization is now needed to adapt to the growing scarcity of water

Kinetic Theory and Fast Wind Observations of the Electron Strahl

We develop a model for the strahl population in the solar wind -- a narrow, low-density and high-energy electron beam centered on the magnetic field direction. Our model is based on the solution of the electron drift-kinetic equation at heliospheric distances where the plasma density, temperature, and the magnetic field strength decline as power-laws of the distance along a magnetic flux tube. Our solution for the strahl depends on a number of parameters that, in the absence of the analytic solution for the full electron velocity distribution function (eVDF), cannot be derived from the theory. We however demonstrate that these parameters can be efficiently found from matching our solution with observations of the eVDF made by the Wind satellite's SWE strahl detector. The model is successful at predicting the angular width (FWHM) of the strahl for the Wind data at 1 AU, in particular by predicting how this width scales with particle energy and background density. We find the strahl distribution is largely determined by the local temperature Knudsen number $\gamma \sim |T dT/dx|/n$, which parametrizes solar wind collisionality. We compute averaged strahl distributions for typical Knudsen numbers observed in the solar wind, and fit our model to these data. The model can be matched quite closely to the eVDFs at 1 AU, however, it then overestimates the strahl amplitude at larger heliocentric distances. This indicates that our model may be improved through the inclusion of additional physics, possibly through the introduction of "anomalous diffusion" of the strahl electrons

Characteristics of Electron Distributions Observed During Large Amplitude Whistler Wave Events in the Magnetosphere

We present a statistical study of the characteristics of electron distributions associated with large amplitude whistler waves inside the terrestrial magnetosphere using waveform capture data as an addition of the study by Kellogg et al., [2010b]. We identified three types of electron distributions observed simultaneously with the whistler waves including beam-like, beam/flattop, and anisotropic distributions. The whistlers exhibited different characteristics dependent upon the observed electron distributions. The majority of the waveforms observed in our study have f/fce or = 8 nT pk-pk) whistler wave measured in the radiation belts. The majority of the largest amplitude whistlers occur during magnetically active periods (AE > 200 nT)