Peranan Kantor Imigrasi Kelas I Malang dalam Pencegahan Tenaga Kerja Indonesia Ilegal Berdasarkan Undang –Undang Nomer 6 Tahun 2011

Di dalam penulisan skripsi ini, penulis membahas mengenai Peranan Kantor Imigrasi Kelas I Malang dalam pencegahan Tenaga Kerja Indonesia Ilegal berdasarkan Undang–undang nomer 6 tahun 2011. Hal ini dilatar belakangi oleh banyaknya pengangguran membuat para tenaga kerja bersedia bekerja apa saja untuk dapat melanjutkan kehidupan.Salah satu pemecahannya diantaranya adalah menjadi Tenaga Kerja Indonesia. Adanya peluang menjadi Tenaga Kerja Indonesia merupakan suatu angin segar ditengah kondisi kehidupan mereka yang serba kekurangan. Karena banyaknya permintaan tenaga kerja dari luar negeri dan juga banyaknya masyarakat yang ingin menjadi tenaga kerja dengan prosedur dari imigrasi yang berbelit – belit dan mahal membuat para calon Tenaga Kerja Indonesia ini lebih memilih untuk menjadi Tenaga Kerja Indonesia Ilegal. Rumusan Masalah : 1. Bagaimana peranan Kantor Imigrasi kelas I malang untuk mencegah ada nya Tenaga KerjaIndonesia ilegal berdasarkan Undang-undang Nomer 6 tahun 2011 ? 2.Apa saja hambatan yang dihadapi Kantor Imigrasi kelas I Malang dalam dalam peranannya untuk mencegah adanya Tenaga Kerja Indonesia illegal berdasarkan Undang-undang Nomor 6 tahun 2011 dan bagaimana upaya kantor Imigrasi kelas I Malang untuk mengatasi hambatan tersebut ? Penelitian ini menggunakan metode pendekatan yuridis Sosiologis. Prosedur pengumpulan data dan pengolahan data menggunakan tehnik wawancara, observasi lapanganserta studi dokumen dan kepustakaan yaitu mengumpulkan data dengan cara melakukan pengamatan dan pencatatan secara sistematis, langsung di lokasi penelitian. Data dianalisa dengan mempergunakan tehnik pengolahan data secara deskriptif analisis. Berdasarkan hasil penelitian diperoleh jawaban bahwa untuk melakukan pencegahan terhadap Tenaga Kerja Indonesia Ilegal tidak cukup hanya dengan Pasal 1 ayat 13, 14, 15, dan 16 Undang – undang nomer 6 tahun 2011 yang berisi tentang Dokumen Perjalanan Republik Indonesia saja namun di dalam Dokumen Perjalanan Indonesia tersebut harus disertai dengan Sistem Terpadu Berbasis Biometrik (SPTBB) yang diatur di Peraturan Menteri Hukum dan HAM RI No.M 02-IZ.03.10 Tahun 2006 tentang Penerapan SistemPhoto Terpadu Berbasis Biometrik pada Surat Perjalanan Republik Indonesia agar Dokumen Perjalanan Republik Indonesia tidak dapat dipalsukan, Salah satu USAha yang dilakukan untuk mengantisipasi penyalahgunaan maksud dan tujuan dalam proses pembuatan Dokumen Perjalanan Republik Indonesia (DPRI) adalah menyeleksi dan menghindari terjadinya penerbitan Dokumen Perjalanan Republik Indonesia (DPRI) dengan maksud dan dalih untuk kunjungan keluarga, kunjungan wisata ke Negara-negara penerima Tenaga Kerja Indonesia (TKI) dimana penerbitan Dokumen Perjalanan Republik Indonesia (DPRI) hanya dapat dibenarkan setelah semua persyaratan formal dan kebenaran materialnya misalnya kebenaran jati diri, nama, alamat, usia, kondisi fisik dan lain sebagainya telah diyakini dan tidak diragukan serta dalam hal tersebut tidak memberikan suatu dispensasi atau keringanan apapun kepada siapapun juga Dalam hal ini pemberian Dokumen Perjalanan Republik Indonesia (DPRI) bagi calon tenaga kerja hendaknya sesuai dengan ketentuan peraturan Perundang-undangan yang berlaku. Yang dimaksud disini yaitu mengenai persyaratan-persyaratan dalam mengajukan permohonan Dokumen Perjalanan Republik Indonesia (DPRI) hendaknya diperhatikan secara lebih teliti, karena banyak sekali pemalsuan-pemalsuan data yang dilakukan oleh para calon Tenaga Kerja. Selain itu, hendaknya Kantor Imigrasi Kelas I Malang dapat bertindak tegas apabila terdapat hal-hal yang mencurigakan dalam pengajuan permohonan paspor seperti misalnya penolakan permohonan paspor. Untuk lebih meningkatkan koordinasi antar Kantor Imigrasi Kelas I Malang dengan Penyalur Jasa Tenaga Kerja Indonesia (PJTKI) yang terkait dengan Tenaga Kerja Indonsia, maka hendaknya dilakukan pertemuan rutin yang dapat dilakukan setiap bulannya untuk membahas permasalahan- permasalahan yang muncul ataupun untuk mencari solusi dalam pemecahan masalah Tenaga Kerja Ilegal

Quasiparticles in the superconducting state of Bi2Sr2CaCu2O8

Recent improvements in momentum resolution by a factor of 32 lead to qualitatively new ARPES results on the spectra of Bi2Sr2CaCu2O8 (Bi2212) along the (pi,pi) direction, where there is a node in the superconducting gap. With improved resolution, we now see the intrinsic lineshape, which indicates the presence of true quasiparticles at the Fermi momentum in the superconducting state, and lack thereof in the normal state. The region of momentum space probed here is relevant for charge transport, motivating a comparison of our results to conductivity measurements by infrared reflectivity.Comment: revised paper with new figure

Measuring Omega_0 with higher-order Quasar-Galaxy Correlations induced by Weak Lensing

Via the magnification bias, gravitational lensing by large-scale structures causes angular cross-correlations between distant quasars and foreground galaxies on angular scales of arc minutes and above. We investigate the three-point cross-correlation between quasars and galaxy pairs measurable via the second moment of the galaxy counts around quasars and show that it reaches the level of a few per cent on angular scales near one arc minute. Combining two- and three-point correlations, a skewness parameter can be defined which is shown to be virtually independent on the shape and normalisation of the dark-matter power spectrum. If the galaxy bias is linear and deterministic, the skewness depends on the cosmic matter density parameter Omega_0 only; otherwise, it can be used to probe the linearity and stochasticity of the bias. We finally estimate the signal-to-noise ratio of a skewness determination and find that around twenty thousand distant quasars e.g. from the Sloan Digital Sky Survey should suffice for a direct measurement of Omega_0.Comment: 11 pages, 6 figures, submitted to Astronomy and Astrophysic

Fermi arc in doped high-Tc cuprates

We propose a $d$-density wave induced by the spin-orbit coupling in the CuO plane. The spectral function of high-temperature superconductors in the under doped and lightly doped regions is calculated in order to explain the Fermi arc spectra observed recently by angle-resolved photoemission spectroscopy. We take into account the tilting of CuO octahedra as well as the on-site Coulombrepulsive interaction; the tilted octahedra induce the staggered transfer integral between $p_{x,y}$ orbitals and Cu $t_{2g}$ orbitals, and bring about nontrivial effects of spin-orbit coupling for the $d$ electrons in the CuO plane. The spectral weight shows a peak at around ($\pi/2$,$\pi/2$) for light doping and extends around this point forming an arc as the carrier density increases, where the spectra for light doping grow continuously to be the spectra in the optimally doped region. This behavior significantly agrees with that of the angle-resolved photoemissionspectroscopy spectra. Furthermore, the spin-orbit term and staggered transfer effectively induce a flux state, a pseudo-gap with time-reversal symmetry breaking. We have a nodal metallic state in the light-doping case since the pseudogap has a $d_{x^2-y^2}$ symmetry.Comment: 5 pages, 7 figure

Analysis of Probabilistic Basic Parallel Processes

Basic Parallel Processes (BPPs) are a well-known subclass of Petri Nets. They are the simplest common model of concurrent programs that allows unbounded spawning of processes. In the probabilistic version of BPPs, every process generates other processes according to a probability distribution. We study the decidability and complexity of fundamental qualitative problems over probabilistic BPPs -- in particular reachability with probability 1 of different classes of target sets (e.g. upward-closed sets). Our results concern both the Markov-chain model, where processes are scheduled randomly, and the MDP model, where processes are picked by a scheduler.Comment: This is the technical report for a FoSSaCS'14 pape

Quasiparticle Interactions for f2^2-Impurity Anderson Model with Crystalline-Electric-Field: Numerical Renormalization Group Study

The aspect of the quasiparticle interaction of a local Fermi liquid, the impurity version of f$^2$-based heavy fermions, is studied by the Wilson numerical renormalization group method. In particular, the case of the f$^2$-singlet crystalline-electric-field ground state is investigated assuming the case of UPt$_3$ with the hexagonal symmetry. It is found that the interorbital interaction becomes larger than the intraorbital one in contrast to the case of the bare Coulomb interaction for the parameters relevant to UPt$_3$. This result offers us a basis to construct a microscopic theory of the superconductivity of UPt$_3$ where the interorbital interactions are expected to play important roles.Comment: 9 pages, 5 figure

The Statistics of Supersonic Isothermal Turbulence

We present results of large-scale three-dimensional simulations of supersonic Euler turbulence with the piecewise parabolic method and multiple grid resolutions up to 2048^3 points. Our numerical experiments describe non-magnetized driven turbulent flows with an isothermal equation of state and an rms Mach number of 6. We discuss numerical resolution issues and demonstrate convergence, in a statistical sense, of the inertial range dynamics in simulations on grids larger than 512^3 points. The simulations allowed us to measure the absolute velocity scaling exponents for the first time. The inertial range velocity scaling in this strongly compressible regime deviates substantially from the incompressible Kolmogorov laws. The slope of the velocity power spectrum, for instance, is -1.95 compared to -5/3 in the incompressible case. The exponent of the third-order velocity structure function is 1.28, while in incompressible turbulence it is known to be unity. We propose a natural extension of Kolmogorov's phenomenology that takes into account compressibility by mixing the velocity and density statistics and preserves the Kolmogorov scaling of the power spectrum and structure functions of the density-weighted velocity v=\rho^{1/3}u. The low-order statistics of v appear to be invariant with respect to changes in the Mach number. For instance, at Mach 6 the slope of the power spectrum of v is -1.69, and the exponent of the third-order structure function of v is unity. We also directly measure the mass dimension of the "fractal" density distribution in the inertial subrange, D_m = 2.4, which is similar to the observed fractal dimension of molecular clouds and agrees well with the cascade phenomenology.Comment: 15 pages, 19 figures, ApJ v665, n2, 200

Hubble Space Telescope Imaging in the Chandra Deep Field South: III. Quantitative Morphology of the 1Ms Chandra Counterparts and Comparison with the Field Population

We present quantitative morphological analyses of 37 HST/WFPC2 counterparts of X-ray sources in the 1 Ms Chandra Deep Field-South (CDFS). We investigate: 1) 1-D surface brightness profiles via isophotal ellipse fitting; 2) 2-D, PSF- convolved, bulge+disk+nucleus profile-fitting; 3) asymmetry and concentration indices compared with all ~3000 sources in our three WFPC2 fields; and 4) near- neighbor analyses comparing local environments of X-ray sources versus the field control sample. Significant nuclear point-source optical components appear in roughly half of the resolved HST/WFPC2 counterparts, showing a narrow range of F_X/F_{opt,nuc} consistent with the several HST-unresolved X-ray sources (putative type-1 AGN) in our fields. We infer roughly half of the HST/WFPC2 counterparts host unobscured AGN, which suggests no steep decline in the type-1/type-2 ratio out to the redshifts z~0.5-1 typical of our sources. The concentration indices of the CDFS counterparts are clearly larger on average than those of the field distribution, at 5-sigma, suggesting that the strong correlation between central black hole mass and host galaxy properties (including concentration index) observed in nearby galaxies is already evident by z~0.5-1. By contrast, the asymmetry index distribution of the 21 resolved CDFS sources at I<23 is indistinguishable from the I<23 field. Moreover, the frequency of I<23 near neighbors around the CDFS counterparts is not significantly different from the field sample. These results, combined with previous similar findings for local samples, suggest that recent merger/ interaction history is not a good indicator of AGN activity over a substantial range of look-back time.Comment: 30 pages, incl. 8 figures; accepted for publication in the Astrophysical Journa