Direct support and general support maintenance manual : truck, container handler, rough terrain, 50,000 lb capacity, DED, PT, NSN 3930-01-082-3758, with tophandler(s).

"October 1981"--Vol. 2.

Operator and organizational maintenance manual : tank, fabric, collapsible, POL, 3,000 gallon (11,355 liter), NSN 5430-00-268-8187, 10,000 gallon (37,850 liter), NSN 5430-00-052-3412, 10,000 gallons (37,850 liter), NSN 5430-00-641-8552), 50,000 gallon (189,250 liter), NSN 5430-00-182-8181.

"30 November 1978."

The large- and small-scale Ca IIK structure of the Milky Way from observations of Galactic and Magellanic sightlines

Aims. The large and small-scale (pc) structure of the Galactic interstellar medium can be investigated by utilising spectra of early-type stellar probes of known distances in the same region of the sky. This paper determines the variation in line strength of Ca ii at 3933.661 Å as a function of probe separation for a large sample of stars, including a number of sightlines in the Magellanic Clouds. 

Methods. FLAMES-GIRAFFE data taken with the Very Large Telescope towards early-type stars in 3 Galactic and 4 Magellanic open clusters in Ca ii are used to obtain the velocity, equivalent width, column density, and line width of interstellar Galactic calcium for a total of 657 stars, of which 443 are Magellanic Cloud sightlines. In each cluster there are between 43 and 111 stars observed. Additionally, FEROS and UVES Ca ii K and Na i D spectra of 21 Galactic and 154 Magellanic early-type stars are presented and combined with data from the literature to study the calcium column density - parallax relationship. 

Results. For the four Magellanic clusters studied with FLAMES, the strength of the Galactic interstellar Ca ii K equivalent width on transverse scales from ∼0.05-9 pc is found to vary by factors of ∼1.8-3.0, corresponding to column density variations of ∼0.3-0.5 dex in the optically-thin approximation. Using FLAMES, FEROS, and UVES archive spectra, the minimum and maximum reduced equivalent widths for Milky Way gas are found to lie in the range ∼35-125 mÅ and ∼30-160 mÅ for Ca ii K and Na i D, respectively. The range is consistent with a previously published simple model of the interstellar medium consisting of spherical cloudlets of filling factor ∼0.3, although other geometries are not ruled out. Finally, the derived functional form for parallax (π) and Ca ii column density (N_CaII) is found to be π(mas) = 1 / (2.39 × 10^-13 × N_CaII (cm^-2) + 0.11). Our derived parallax is ∼25 per cent lower than predicted by Megier et al. (2009, A&A, 507, 833) at a distance of ∼100 pc and ∼15 percent lower at a distance of ∼200 pc, reflecting inhomogeneity in the Ca ii distribution in the different sightlines studied.

New York 1:25,000. West Point and vicinity /

Scale 1:25,000.

Constrained Linear Spectral Unmixing Technique for Regional Land Cover Mapping Using MODIS Data

Over the last few decades, there has been a significant land cover (LC) change across the globe due to the increasing demand of the burgeoning population and urban sprawl. In order to take account of the change, there is a need for accurate and up-to-date LC maps. Mapping and monitoring of LC in India is being carried out at national level using multi-temporal IRS AWiFS data. Multispectral data such as IKONOS, Landsat-TM/ETM+, IRS-ICID LISS-III/IV, AWiFS and SPOT-5, etc. have adequate spatial resolution (similar to 1m to 56m) for LC mapping to generate 1:50,000 maps. However, for developing countries and those with large geographical extent, seasonal LC mapping is prohibitive with data from commercial sensors of limited spatial coverage. Superspectral data from the MODIS sensor are freely available, have better temporal (8 day composites) and spectral information. MODIS pixels typically contain a mixture of various LC types (due to coarse spatial resolution of 250, 500 and 1000 in), especially in more fragmented landscapes. In this context, linear spectral unmixing would be useful for mapping patchy land covers, such as those that characterise much of the Indian subcontinent. This work evaluates the existing unmixing technique for LC mapping using MODIS data, using end-members that are extracted through Pixel Purity Index (PPI), Scatter plot and N-dimensional visualisation. The abundance maps were generated for agriculture, built up, forest, plantations, waste land/others and water bodies. The assessment of the results using ground truth and a LISS-III classified map shows 86% overall accuracy, suggesting the potential for broad-scale applicability of the technique with superspectral data for natural resource planning and inventory applications. Index Terms-Remote sensing, digital

Contrained linear spectral unmixing technique for regional land cover mapping using MODIS data

Over the last few decades, there has been a significant land cover (LC) change across the globe due to the increasing demand of the burgeoning population and urban sprawl. In order to take account of the change, there is a need for accurate and up- to-date LC maps. Mapping and monitoring of LC in India is being carried out at national level using multi-temporal IRS AWiFS data. Multispectral data such as IKONOS, Landsat- TM/ETM+, IRS-1C/D LISS-III/IV, AWiFS and SPOT-5, etc. have adequate spatial resolution (~ 1m to 56m) for LC mapping to generate 1:50,000 maps. However, for developing countries and those with large geographical extent, seasonal LC mapping is prohibitive with data from commercial sensors of limited spatial coverage. Superspectral data from the MODIS sensor are freely available, have better temporal (8 day composites) and spectral information. MODIS pixels typically contain a mixture of various LC types (due to coarse spatial resolution of 250, 500 and 1000 m), especially in more fragmented landscapes. In this context, linear spectral unmixing would be useful for mapping patchy land covers, such as those that characterise much of the Indian subcontinent. This work evaluates the existing unmixing technique for LC mapping using MODIS data, using end- members that are extracted through Pixel Purity Index (PPI), Scatter plot and N-dimensional visualisation. The abundance maps were generated for agriculture, built up, forest, plantations, waste land/others and water bodies. The assessment of the results using ground truth and a LISS-III classified map shows 86% overall accuracy, suggesting the potential for broad-scale applicability of the technique with superspectral data for natural resource planning and inventory applications.

A gestão de pessoas nas Câmaras de Vereadores de municípios de até 50.000 habitantes

A expectativa de contribuir para o aprimoramento e o equilíbrio da democracia brasileira tem estimulado a Câmara dos Deputados a criar programas e projetos para promover a modernização dos órgãos legislativos estaduais e municipais. A fim de melhor direcionar as ações previstas e de identificar novas oportunidades de atuação, é necessário conhecer a situação administrativa atual das câmaras municipais, em especial no que diz respeito à gestão de pessoas. A observação cotidiana nos leva a supor que a infraestrutura administrativa existente nas câmaras de vereadores de municípios com população de até 50.0000 habitantes é inadequada e insuficiente para o pleno desempenho das atribuições institucionais dos parlamentares. O estudo propõe um projeto de pesquisa à Câmara dos Deputados para levantar dados que comprovem ou rejeitem a hipótese. São abordados princípios gerais da gestão de pessoas, segundo os critérios da Administração Pública e a nova visão gerencial apresentada pelo Plano Diretor de Reforma do Estado.

Evolución geodinámica poliorogénica de los dominios septentrionales de la zona de Ossa Morena

377 p.

《广东省的植被和植被区划》含1:50万植被图

本项目成果以图文结合，系统的论述了广东省现状植被的基本特征、地理分布规律与生境的关系。并根据植被的特征及生产利用进行植被区划及分区评述。还从植被的角度提出开发利用和改造的意见。该成果是一项科学性较强的基础性调查研究报告，正确的评述广东植被的特点和植被分区，具有较高的学术水平，进一步开发利用和改造的方向措施，切合实际，对国土整治、保护环境提供了科学依据。