Richard Delgado and Ice Cube: Brothers in Arms

Symposium: Examining Critical Race Theory: Honoring Professor Richard Delgad

Toward a Socially Just Peace in the War on Drugs?: The Illinois Cannabis Social-Equity Program

Laudably, when Illinois legalized the recreational use of cannabis, it also sought to repair the damage wrought by the War on Drugs (WOD)through its social-equity initiatives. That harm included excessive and disproportionate incarceration in communities of color, over-policing within those communities, and all of the social and economic harms implicit in those realities. This harm necessarily creates intergenerational harm, as parents and children lose necessary pillars of support. Moreover, compelling evidence suggests that the progenitors of the WOD in-tended this harm. Measured against this historic social injustice, the social equity efforts in Illinois fail to secure a material unwinding of the WOD harms. Illinois needs a broader approach to ending the War on Drugs beyond cannabis. Treatment should displace criminalization for narcotics. Expungements should become automatic and more widely available. The state should immediately issue more social-equity licenses in affected communities. Investment of revenues from cannabis and other decriminalized drugs in affected communities should continue

Boundary Conditions of the Heliosphere

Radiative transfer equilibrium models of nearby interstellar matter (ISM) yield the boundary conditions of the heliosphere when constrained with observations of ISM inside and outside of the heliosphere. Filtration factors for interstellar neutrals crossing the heliosheath region, from charge exchange with interstellar plasma, are given for H, He, N, O, Ar, and Ne. The best models predict n(HI)~0.2 /cc, n(e)~0.1 /cc, however if the isotropic 2 kHz emission observed by Voyager (Kurth & Gurnett 2003) is formed in the surrounding ISM, an alternate model with lower electron densities is indicated. Observations of nearby ISM, the radiative transfer models, and historical 10Be records provide information on past variations in the galactic environment of the Sun

Numerical and experimental investigations for insulation particle transport phenomena in water flow

The investigation of insulation debris generation, transport and sedimentation becomes more important with regard to reactor safety research for pressurized and boiling water reactors, when considering the long-term behaviour of emergency core coolant systems during all types of loss of coolant accidents (LOCA). The insulation debris released near the break during a LOCA incident consists of a mixture of a disparate particle population that varies with size, shape, consistency and other properties. Some fractions of the released insulation debris can be transported into the reactor sump, where it may perturb or impinge on the emergency core cooling systems. Open questions of generic interest are for example the particle load on strainers and corresponding pressure-drop, the sedimentation of the insulation debris in a water pool, its possible re-suspension and transport in the sump water flow. A joint research project on such questions is being performed in cooperation with the University of Applied Science Zittau/Görlitz and the Forschungszentrum Dresden-Rossendorf. The project deals with the experimental investigation and the development of computational fluid dynamic (CFD) models for the description of particle transport phenomena in coolant flow. While the experiments are performed at the University Zittau/Görlitz, the theoretical work is concentrated at Forschungszentrum Dresden-Rossendorf. In the present paper, the basic concepts for computational fluid dynamic (CFD) modelling are described and experimental results are presented. Further experiments are designed and feasibility studies were performed

The Iowa Homemaker vol.37, no.2

They Say it’s Love, Ann Baur, page 4 Marry in a College Chapel, Merna Borror, page 6 Learned by Heart, Beth Cummings Paschal, page 7 I’d Like to Know, Sandy Newman, page 8 Blueprint for Packing, Carolyn McIntyre, page 10 The Honeymoon, Reverie to Reality, Jackie Andre, page 11 Present Picker, Marilyn Jensen Nadler, page 12 An Electric Dinner, Ann Walters, page 14 Say Yes… To Entertaining, Rosemary McBride and Roma Walker, page 15 ABC’s of Money Management, Linda Nelson and Marie Budolfson, page 16 What’s in a Wedding Custom, Janice Furman, page 18 Plain Clothes Man? Ha!, Norma Scholes, page 22 Why All This Fuss Over Sex, Gail A. McClure, page 2

Why Study Interstellar Matter Very Close to the Sun?

Interstellar matter (ISM) sets the boundary conditions of the heliosphere and dominates the interplanetary medium. The heliosphere configuration has varied over recent history, as the Sun emerged from the Local Bubble and entered a turbulent outflow of cloudlets originating from the Scorpius-Centaurus Association direction. Several indicators suggest that the local interstellar magnetic field is weak and parallel to the galactic plane. Observations of the interaction products of the ISM with the heliosphere, such as pickup ions and anomalous cosmic rays, when combined with data on the ISM towards nearby stars, provide unique constraints on the composition and physical properties of nearby gas. These data suggest abundances in nearby ISM are subsolar, and that gas and dust are not well mixed at the solar location.Comment: 10 pages, 4 figures; Proceedings Houston 2002 COSPAR Outer Heliosphere meetin