Earth resources evaluation for New Mexico by LANDSAT-2

The author has identified the following significant results. The Middle Rio Grande project has not yet progressed to the point where mineral exploration sites can be chosen; however, there does appear to be some correlation between the known structure and mineral deposits and the LANDSAT lineament map. A circular feature identified in the southern Magdalena Mountains on LANDSAT-1 imagery agrees well with the location of a newly proposed caldron complex. Several recognized and unrecognized circular features were identified on imagery of the Mogollon-Datil volcanic field. A check of aeromagnetic maps for New Mexico found that the circular features on the LANDSAT imagery showed up as areas of generally high magnetic intensity

A mutant of Metarhizium anisopliae var. acridum with enhanced submerged conidiation.

Made available in DSpace on 2018-06-06T01:01:38Z (GMT). No. of bitstreams: 1 ID278831.pdf: 343982 bytes, checksum: 1b1ebb921fe53464e93c15e17e4d406c (MD5) Previous issue date: 2007-01-16bitstream/item/178116/1/ID-27883-1.pd

Geologic analysis of ERTS-1 imagery for the State of New Mexico

There are no author-identified significant results in this report

The lived experience of health sciences students’ participation in an interprofessional community-based stroke class

Background. Collaborative approaches in healthcare contexts may provide better care for patients. Interprofessional circuit-based group therapy could counter profession-specific tribalism. There is no evidence on interprofessional education (IPE) community-based interventions on student learning in the health professions. Objective. To explore undergraduate health sciences students’ experience of being involved in community-based interprofessional circuit-based group therapy. Methods. Semi-structured interviews were inductively analysed exploring undergraduate health sciences students’ experience of involvement in an IPE community-based stroke intervention. Results. A total of 12 final-year students participated, with representation from physiotherapy, occupational therapy and speech therapy. This IPE opportunity beneficially impacted students’ collaborative competencies in knowledge, attitudes, skills and behaviours. This community-based rotation immersed students in a service-delivery environment where patient management was co-ordinated by a multiprofessional rehabilitation team. The integrated stroke circuit group activity aimed to enhance further interconnectedness between student participants. Students who were exposed to this clinical activity reported an understanding of (i) patients’ unique contexts; (ii) role development and complementary overlap between health professions; and (iii) the value of joint interventions to both patients and rehabilitation teams in resource-constrained settings. Conclusion. These students have been primed in their practice-readiness as healthcare professionals for the 21st century who will promote quality care, and embrace collaborative professional practice and person-centredness

Multi-wavelength spatially resolved analysis of quasi-periodic pulsations in a solar flare

Aims. We aim to perform a spatially resolved analysis of a quasi-periodic pulsation event from 8th May 1998 using microwave data from the Nobeyama Radioheliograph and Radiopolarimeter, and X-ray data from the Yohkoh satellite. Methods. Time spectra of the signals integrated over the emission source are constructed with the use of the Lomb-Scargle periodogram method, revealing the presence of a pronounced 16 s periodicity. The Pixon image reconstruction algorithm and Hanaoka algorithm are used to reconstruct images from the hard X-ray data from Yohkoh/HXT and Nobeyama Radioheliograph respectively. The phase relationship of the microwave emission was analysed with the use of cross-correlation techniques. Results. The flaring loop was resolved in the microwave band. The hard X-ray sources are found to be located near the footpoint and at the loop apex determined by the soft X-ray image. The apex source is much fainter than footpoint one. In microwave, all parts of the loop are seen to oscillate with the same period and almost in phase. It was not possible to determine the spatial structure of the oscillation in the hard X-ray band. The period and the coherent spatial structure of the oscillation are indicative of the presence of either an MHD sausage mode or a periodic regime of magnetic reconnectio

ISO-SWS spectroscopy of NGC 1068

We present ISO-SWS spectroscopy of NGC 1068 for the wavelength range 2.4 to 45um, detecting a total of 36 emission lines. Most of the observed transitions are fine structure and recombination lines originating in the narrow line region. We compare the line profiles of optical lines and reddening-insensitive infrared lines to constrain the dynamical structure and extinction properties of the NLR. The considerable differences found are most likely explained by two effects. (1) The spatial structure of the NLR is a combination of a highly ionized outflow cone and lower excitation extended emission. (2) Parts of the NLR, mainly in the receding part at velocities above systemic, are subject to extinction that is significantly suppressing optical emission. Line asymmetries and net blueshifts remain, however, even for infrared fine structure lines suffering very little obscuration. This may be either due to an intrinsic asymmetry of the NLR, or due to a very high column density obscuring component which is hiding part of the NLR even from infrared view. Mid-infrared emission of molecular hydrogen in NGC 1068 arises in a dense molecular medium at temperatures of a few hundred Kelvin that is most likely closely related to the warm and dense components seen in the near-infrared H2 transitions, and in millimeter wave tracers of molecular gas. Any emission of the putative pc-scale molecular torus is likely overwhelmed by this larger scale emission.Comment: aastex (V4), 9 eps figures. Accepted by Ap

The Electron Scattering Region in Seyfert Nuclei

The electron scattering region (ESR) is one of important ingredients in Seyfert nuclei because it makes possible to observe the hidden broad line region (hereafter HBLR) in some type 2 Seyfert nuclei (hereafter S2s). However, little is known about its physical and geometrical properties. Using the number ratio of S2s with and without HBLR, we investigate statistically where the ESR is in Seyfert nuclei. Our analysis suggests that the ESR is located at radius between $\sim$ 0.01 pc and $\sim$ 0.1 pc from the central engine. We also discuss a possible origin of the ESR briefly.Comment: 5 pages and 1 figure. The Astrophysical Journal (Letters), in pres