487 research outputs found
A survey of users of earth resources remote sensing data
The results of a NASA supported Battelle survey to obtain user views on the nature and value of LANDSAT data use, on current LANDSAT capabilities, and on ways to improve data use were summarized. Questionnaire and interview responses from over 1000 private and public sector users were analyzed and discussed
Survey of users of earth resources remote sensing data
A user survey was conducted to determine current earth resources survey (ERS) data use/user status and recommendations for strengthening use. Only high-altitude aircraft and satellite (primarily LANDSAT) data were included. Emphasis was placed on the private sector/industrial user. Objectives of the survey included: who is using ERS data, how they are using the data, the relative value of current data use as well as obtaining user views as to possible ways of strengthening future ERS data use. The survey results are documented and should provide relevant decision making information for developing future programs of maximum benefit to all end users of satellite ERS data
Utilizing Skylab data in on-going resources management programs in the state of Ohio
The author has identified the following significant results. The use of Skylab imagery for total area woodland surveys was found to be more accurate and cheaper than conventional surveys using aerial photo-plot techniques. Machine-aided (primarily density slicing) analyses of Skylab 190A and 190B color and infrared color photography demonstrated the feasibility of using such data for differentiating major timber classes including pines, hardwoods, mixed, cut, and brushland providing such analyses are made at scales of 1:24,000 and larger. Manual and machine-assisted image analysis indicated that spectral and spatial capabilities of Skylab EREP photography are adequate to distinguish most parameters of current, coal surface mining concern associated with: (1) active mining, (2) orphan lands, (3) reclaimed lands, and (4) active reclamation. Excellent results were achieved when comparing Skylab and aerial photographic interpretations of detailed surface mining features. Skylab photographs when combined with other data bases (e.g., census, agricultural land productivity, and transportation networks), provide a comprehensive, meaningful, and integrated view of major elements involved in the urbanization/encroachment process
Prevalence of Color Blindness Among Students of Four Basic Schools in Koya City
Color blindness or color vision deficiency is X-linked recessive disorder that affects males more frequently than females. Abnormality in any one or all three cone photoreceptors caused Congenital disorders. Protanopia, deuteranopia results when long wavelength (L), photopigments (red), middle wavelength (M) and photopigments (green) are missing.
This cross-sectional study was done to find out the prevalence of color vision deficiency among basic school students in Koya city with different ages and genders. The study was conducted in four basic schools that were present in Koya city (Zheen, Zanst, Nawroz and Najibaxan).
All students screened by using Ishihara 24 plates. For the study (n=400, male=206, female=194, age=8-14) were selected & examined. The result revealed that the prevalence rate of the deficiency in four primary schools 3.39% (7) in males and 0% females. The study concluded that color blindness is different between students in each school, cannot find the prevalence of Color blindness in females in each school and affects males more than females because color blindness is an X-linked recessive disorder. The aim of the study was to determine the prevalence of color blindness in some basic schools in Koya city, Kurdistan Region/ Iraq
Globular Clusters in Dense Clusters of Galaxies
Deep imaging data from the Keck II telescope are employed to study the
globular cluster (GC) populations in the cores of six rich Abell clusters. The
sample includes A754, A1644, A2124, A2147, A2151, and A2152, and spans the
redshift range z = 0.035-0.066. The clusters also range in morphology from
spiral-rich, irregular systems to centrally concentrated cD clusters rich in
early-type galaxies. Globular cluster specific frequencies S_N and luminosity
function dispersions are measured for a total of 9 galaxies in six central
fields. The measured values of S_N for the six brightest cluster galaxies
(BCGs) are all higher than typical values for giant ellipticals, in accord with
the known S_N-density correlations. The three non-BCGs analyzed also have
elevated values of S_N, confirming that central location is a primary factor.
The number of GCs per unit mass for these fields are consistent with those
found in an earlier sample, giving further evidence that GC number scales with
mass and that the S_N variations are due to a deficit of halo light, i.e., S_N
reflects mass-to-light ratio.
The discussion builds on an earlier suggestion that the GCs (both metal rich
and metal poor) around the central cluster galaxies were assembled at early
times, and that star formation halted prematurely in the central galaxies at
the epoch of cluster collapse. This is consistent with recent simulations of
BCG/cluster formation. The subsequent addition of luminous material through
cluster dynamical evolution can cause S_N to decrease, and we may be seeing the
first evidence of this. Finally, the GC luminosity function measurements are
used to constrain the relative distances of the three clusters that make up the
Hercules supercluster.Comment: Uses emulateapj.sty (included); 17 pages with 9 included PostScript
figures. Figures 1-6 are separate GIF images (so 15 figures total) available
from http://astro.caltech.edu/~jpb/clusters -- the full PostScript version of
the paper (20 pages; 2.2 Mb compressed) incorporating Figures 1-6 can also be
grabbed from this URL. Accepted for publication in A
Environment of MAMBO galaxies in the COSMOS field
Submillimeter galaxies (SMG) represent a dust-obscured high-redshift
population undergoing massive star formation activity. Their properties and
space density have suggested that they may evolve into spheroidal galaxies
residing in galaxy clusters. In this paper, we report the discovery of compact
(~10"-20") galaxy overdensities centered at the position of three SMGs detected
with the Max-Planck Millimeter Bolometer camera (MAMBO) in the COSMOS field.
These associations are statistically significant. The photometric redshifts of
galaxies in these structures are consistent with their associated SMGs; all of
them are between z=1.4-2.5, implying projected physical sizes of ~170 kpc for
the overdensities. Our results suggest that about 30% of the radio-identified
bright SMGs in that redshift range form in galaxy density peaks in the crucial
epoch when most stars formed.Comment: Accepted for publication in ApJ Letter
Constraining beyond the Standard Model nucleon isovector charges
At the TeV scale, low-energy precision observations of neutron
characteristics provide unique probes of novel physics. Precision studies of
neutron decay observables are susceptible to beyond the Standard Model (BSM)
tensor and scalar interactions, while the neutron electric dipole moment,
, also has high sensitivity to new BSM CP-violating interactions. To fully
utilise the potential of future experimental neutron physics programs, matrix
elements of appropriate low-energy effective operators within neutron states
must be precisely calculated. We present results from the QCDSF/UKQCD/CSSM
collaboration for the isovector charges and using lattice QCD
methods and the Feynman-Hellmann theorem. We use a flavour symmetry breaking
method to systematically approach the physical quark mass using ensembles that
span five lattice spacings and multiple volumes. We extend this existing
flavour breaking expansion to also account for lattice spacing and finite
volume effects in order to quantify all systematic uncertainties. Our final
estimates of the isovector charges are
and renormalised, where
appropriate, at in the scheme.Comment: 16 pages, 11 figures, 6 table
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