Molecular Divergence in the Galapagos Islands—Baja California Species Pair, Gossypium klotzschianum and G. davidsonii (Malvaceae)

Molecular divergence betweenGossypium klotzschianum andG. davidsonii was studied. The former is endemic to five of the larger islands of the Galapagos, whileG. davidsonii is restricted to the southern half of Baja California, approximately 2 500 km distant. A substantial body of genetic and taxonomic data suggests that these two species are related as progenitor and derivative. Interspecific hybrids are fully fertile, with no evidence of F2 breakdown and normal segregation of genetic markers. Allozyme analysis of 33 populations for 41 loci indicated that the allelic composition ofG. klotzschianum represents a subset ofG. davidsonii. Although genetic diversity is relatively restricted in both species, calculated measures demonstrate higher levels of genetic variability and greater population structuring inG. davidsonii than inG. klotzschianum. The interspecific genetic identity of 0.87 is typical for progenitor-derivative species pairs. Chloroplast DNAs were surveyed for variation with 25 restriction enzymes using hybridization probes that cover the entire chloroplast genome. No intraspecific and little interspecific variation was detected among 560 cpDNA restriction sites, representing sequence information for approximately 3200 nucleotides. Only 3 mutational differences distinguished the two species, resulting in a sequence divergence estimate of 0.09%. Divergence times were estimated from both the isozyme data and the cpDNA restriction site data. Although these estimates have several sources of error, both molecular data sets were congruent in suggesting that the two lineages diverged between 250000 and 700000 years ago. Accumulated evidence suggests that dispersal was from Baja California to the Galapagos Islands rather than the reverse, and most likely was mediated by trans-oceanic drift.G. klotzschianum may be the only species of the endemic Galapagos flora to have arisen from a northern Mexican progenitor

THE COMET MINE: AN ENGENDERED STUDY OF VICTORIAN CONSUMPTION PRACTICES AND MATERIAL CULTURE ON A SMALL MINING LANDSCAPE

The Comet mine is an early 20th-century, largely undocumented mining community that existed along the periphery of the Coloma Mining District in the Garnet Range of western Montana. During the summer of 2010, archaeological excavations occurred at multiple features at the site. Through an analysis of cultural material found in deposits at the Comet, this study interprets the way in which patterns of refuse can reveal information about consumption behavior and evolving gender roles in mining communities in Montana, during late Victorian era

Wind-tunnel free-flight investigation of a supersonic persistence fighter

Wind-tunnel free-flight tests have been conducted in the Langley 30- by 60-Foot Wind Tunnel to examine the high-angle-of-attack stability and control characteristics and control law design of a supersonic persistence fighter (SSPF) at 1 g flight conditions. In addition to conventional control surfaces, the SSPF incorporated deflectable wingtips (tiperons) and pitch and yaw thrust vectoring. A direct eigenstructure assignment technique was used to design control laws to provide good flying characteristics well into the poststall angle-of-attack region. Free-flight tests indicated that it was possible to blend effectively conventional and unconventional control surfaces to achieve good flying characteristics well into the poststall angle-of-attack region

Source of the Bursty Bulk Flow Diffuse Aurora: Electrostatic Cyclotron Harmonic and Whistler Waves in the Coupling of Bursty Bulk Flows to Auroral Precipitation

Electron cyclotron harmonic (ECH) and whistler chorus waves are recognized as the two mechanisms responsible for the resonant waveparticle interactions necessary to precipitate plasma sheet electrons into the ionosphere, producing the diffuse Aurora. Previous work has demonstrated ECH waves dominate electron scattering at L shells >8, while whistler chorus dominates scattering at L shells L 1, consistent with electron betatron acceleration. Here, however, we nd whistler chorus emissions throughout an interval of fast ows where Te,/Te,||< 1. Parallel electron beams account for the enhanced parallel electron temperature and serve as the instability mechanism for the whistler chorus. The parallel electron beams and associated cigarshaped distributions are consistent with Fermi acceleration at dipolarizations in fast ows. We demonstrate that the scattering efciency of the whistler chorus exceeds that of ECH waves, which THEMIS also detects during the fast ows. The obliquity of the whistler waves permits efcient scattering of lowerenergy electrons into the diffuse aurora. We conclude that Fermi acceleration of electrons provides one important freeenergy source for the waveparticle interactions responsible for coupling plasma sheet electrons into the diffuse aurora during substorm conditions

Bursty, Broadband Electromagnetic Waves Associated with Thin Current Layers and Turbulent Magnetosheath Reconnection

We investigate observations of intense bursts of electromagnetic wave energy in association with the thin current layers of turbulent magnetosheath reconnection. These observed emissions form two distinct types: (i) broadband emissions that extend continuously to lOs of Hertz; and (ii) structured bursts of emitted energy that occur above 80-Hz, often displaying features reminiscent of absorption bands and are observed at local minima in the magnetic field. We present detailed analyses of these intense bursts of electromagnetic energy and quantify their proximity to X- and O-nulls, as well as their correlation to the amount of magnetic energy converted by the process of magnetic reconnection

Examination of Bursty Electromagnetic Waves Observed During Intervals of Turbulent Magnetosheath Reconnection

We investigate observations of intense bursts of electromagnetic waves in association with magnetic reconnection in the turbulent magnetosheath. These structured, broadband bursts occur above 80-Hz, often displaying features reminiscent of absorption bands and are observed at local minima in the magnetic field. We present detailed analyses of these intense bursts of electromagnetic waves and quantify their proximity to X- and O-nulls

Academic Motherhood: Managing Complex Roles in Research Universities

This is the publisher's version, also available electronically from http://muse.jhu.edu/journals/review_of_higher_education/v027/27.2ward.html.No abstract is available for this item

Bursty, Broadband Electromagnetic Waves Associated with Three-Dimensional Nulls Observed in Turbulent Magnetosheath Reconnection

We investigate observations of intense bursts of electromagnetic wave energy in association with the thin current layers of turbulent magnetosheath reconnection. These observed emissions - typically detected in the layers immediately outside of the current layer proper - form two distinct types: (i) broadband emissions that extend continuously to lOs of Hertz; and (ii) structured bursts of emitted energy that occur above 80-Hz, often displaying features reminiscent of absorption bands and are observed near the local minima in the magnetic field. We present detailed analyses of these intense bursts of electromagnetic energy and quantify their proximity to X-IO-nulls and magnetic spine connected null pairs, as well as their correlation - if any - to the amount of magnetic energy converted by the process of magnetic reconnection

A Tangled Web of Terms: The Overlap and Unique Contribution of Involvement, Engagement, and Integration to Understanding College Student Success

This is the publisher's version, also available electronically from http://muse.jhu.edu/journals/journal_of_college_student_development/v050/50.4.wolf-wendel.html.Established theories and constructs long associated with student success, including involvement, engagement, and integration, provide common language and a body of knowledge to inform understanding of the challenges currently facing higher education. This paper examines how the theories and terms have evolved, explores how the terms are currently used, and considers their legacy for understanding contemporary concerns about student development and success