bluuebunny/crossref_metadata_2025_split huggingface dataset:
JARINGAN SOSIAL DAN STRATEGI ADAPTASI TENAGA KERJA MIGRAN ASAL LAMPUNG DI DESA JAYAMUKTI, KECAMATAN CIKARANG PUSAT, KABUPATEN BEKASI, PROVINSI JAWA BARAT
Authors: Marga Safitri Yessi , Wahyuni Ekawati S 
Published: December 2016

Tingkat pertumbuhan penduduk meningkat secara cepat pada beberapa tahun terakhir menimbulkan permasalahan pada ketenagakerjaan. Pertumbuhan penduduk yang tidak didukung dengan peningkatan sumberdaya dan lapangan pekerjaan menambah jumlah pengangguran. Kondisi tersebut memacu penduduk untuk melakukan migrasi. Perpindahan penduduk dipengaruhi oleh faktor pendorong dari daerah asal, diantaranya yakni terbatasnya pekerjaan dan juga faktor penarik dari daerah tujuan, salah satunya lapangan pekerjaan yang lebih banyak. Fenomena perpindahan penduduk di Indonesia umumnya membentuk siklus dimana migran yang kaya secara ekonomi dan sosial akan memengaruhi keluarga mereka, saudara atau teman untuk ikut bermigrasi. Situasi yang berbeda dan kondisi pada daerah tujuan mendorong mereka untuk beradaptasi sebagai strategi bertahan hidup. Jaringan sosial sangat penting bagi para migran di daerah tujuan. <br />
PENGARUH TAMAN WISATA ALAM PANGANDARAN TERHADAP KONDISI SOSIAL EKONOMI MASYARAKAT (Studi: Desa Pangandaran, Kecamatan Pangandaran, Kabupaten Ciamis, Provinsi Jawa Barat)
Authors: Dhalyana Dini , Adiwibowo Soeryo 
Published: December 2016

Penelitian ini dilakukan selama bulan April 2012 di Desa Pangandaran, Kecamatan Pangandaran, <br />Kabupaten Ciamis, Jawa Barat. Tujuan penelitian ini, pertama mengidentifikasi jenis-jenis pekerjaan yang tumbuh di TWA Pangandaran akibat adanya kegiatan pariwisata. Kedua, menganalisis kontribusi pekerjaan di sektor pariwisata dalam menyumbang pendapatan rumah tangga pelaku usahanya. Ketiga, menganalisis pengaruh kegiatan pariwisata terhadap kehidupan sosial penduduk lokal. Metode penelitiannya menggunakan pendekatan kualitatif dan kuantitatif. Sekitar 63 responden rumahtangga yang diwawancarai berasal dari jenis pekerjaan yang berbeda. Selama pengambilan data dilakukan wawancara mendalam yang didukung dengan studi literatur. Hasil penelitian ini menunjukkan bahwa keberadaan sektor pariwisata di Pangandaran telah menciptakan lapangan pekerjaan terutama terhadap total pendapatan rumah tangga penduduk lokal. Sementara pada pola kerjasama antar sesama pelaku usaha, keberadaan industri pariwisata mempererat hubungan diantara pelaku usaha. Namun disisi lain, aktivitas wisata di Pangandaran memberikan pengaruh lain kehidupan masyarakat, seperti perubahan gaya hidup dan perilaku menyimpang. Kata kunci : kehidupan sosial, masyarakat lokal, pendapatan rumah tangga, pekerjaan pada sektor wisata, wisata <br />
IDEOLOGI AKTOR DAN PERSEPSI MASYARAKAT TERHADAP DAMPAK PERTAMBANGAN PASIR DI PEDESAAN GUNUNG GALUNGGUNG
Authors: Rahmadian Faris , Dharmawan Arya Hadi 
Published: December 2016

Pasca erupsi, kawasan Gunung Galunggung merupakan salah satu kawasan yang menjadi arena besar pertarungan kepentingan antara pemerintah, masyarakat dan swasta. Objek pasir yang berlimpah menjadikan pertambangan skala besar hadir dan berimplikasi secara esensial terhadap kehidupan masyarakat lokal yang tidak hanya berada dekat dengan kawasan pertambangan, namun juga berada jauh dengan lokasi pertambangan. Terlebih diketahui bahwa ideologi masyarakat yang menekankan pada kesejahteraan dan populisme, berbanding terbalik dengan ideologi swasta dan pemerintah yang menekankan pada profit dan pembangunan. Dampak negatif dan positif aktivitas pertambangan mulai secara nyata dirasakan oleh masyarakat, diantaranya seperti degradasi kualitas air, tingkat pendapatan atau konflik yang secara krusial merepresentasikan respons masyarakat terhadap keberadaan perusahaan pertambangan pasir yang telah hampir tiga puluh tahun mengeruk kawasan ini. <br />Kata kunci: Analisis aktor, analisis dampak, pemanfaatan sumber daya alam, persepsi masyarakat, pertambangan pasir <br />
PENGARUH IKLIM KOMUNIKASI ORGANISASI TERHADAP KINERJA APARATUR DI PEMERINTAHAN DESA
Authors: Fauzi Ahmad , Sarwoprasodjo Sarwititi 
Published: December 2016

Permintaan terhadap pelayanan umum guna memenuhi kebutuhan masyarakat saat ini semakin menjadi isu <br />yang semakin berkembang. Penelitian ini bertujuan untuk menganalisis iklim komunikasi organisasi, menganalisis praktik penerapan tata kelola pemerintahan yang baik, kinerja aparatur, dan menganalisis <br />pengaruh iklim komunikasi terhadap kinerja aparatur di lingkungan Pemerintahan Desa Situ Udik. Penelitian ini menggunakan pendekatan kuantitatif dan didukung oleh pendekatan kualitatif untuk 69 responden melalui metode penelitian sensus. Hasil penelitian menunjukkan bahwa Iklim <br />komunikasi organisasi berpengaruh signifikan terhadap kinerja aparatur, terutama pada variabel kepercayaan, pembuatan keputusan bersama, keterbukaan dalam komunikasi ke bawah, mendengarkan dalam komunikasi ke atas. Aspek penerapan tata kelola pemerintahan yang baik berpengaruh signifikan terhadap kinerja aparatur pada seluruh variabel (keterbukaan, tanggung jawab, dan hukum). Berdasarkan hasil uji analisis regresi statisti, nilai alpha &lt; 0.05 yang menunjukkan bahwa iklim komunikasi organisasi berpengaruh 33.8 persen terhadap kinerja aparatur dan praktik peneraan tata kelola yang baik berpengaruh 16.9 persen terhadap kinerja aparatur <br />Kata kunci : iklim komunikasi, tata kelola yang baik, kinerja aparatur <br />
HUBUNGAN GAYA KEPEMIMPINAN LURAH DENGAN KUALITAS PELAYANAN KELURAHAN (Studi di Kelurahan Lenteng Agung, Jakarta Selatan)
Authors: Olivianti Bebby , M. Kolopaking Lala 
Published: December 2016

Gaya kepemimpinan direktif dan konsultatif diterapkan oleh kepala desa dan disesuaikan untuk <br />permasalahan. Tipe direktif digunakan ketika melimpahkan tugas kepada petugas desa. Tipe konsultatif digunakan dalam mengarahkan pekerja ketika memberikan pelayanan publik. Tujuan penelitianini adalah menganalisis hubungan antara tipe kepemimpinan kepada desa dengan kualitas pelayanan publik. Metode penelitian yang digunakan adalah accidental sampling dengan total responden sebanyak 60 orang. Pengolahan data menggunakan uji korelasi rank-spearman. Hasil penelitian menunjukkan bahwa gaya kepemimpinan konsultatif dapat meningkatkan kualitas pelayanan masyarakat. Hal ini dibuktikan sebesar 80 persen responden menyatakan bahwa terdapat hubungan yang signifikan antara gaya kepemimpinan konsultatif dengan kualitas pelayanan publik. <br />Kata kunci : gaya kepemimpinan, kualitas pelayanan publik
INDUSTRIALISASI PERTAMBANGAN DAN DEAGRARIANISASI MASYARAKAT DESA (Studi Kasus Masyarakat Desa Embalut dan Desa Bangunrejo, Kecamatan Tenggarong Seberang, Kabupaten Kutai Kartanegara, Kalimantan Timur)
Authors: Gandi Rajib , Sunito Satyawan 
Published: December 2016

East Kalimantan province has issued a mining license (IUP) reached 1,192 pieces, until August 2014. Kutai Kartanegara is a county that issued the largest IUP is 407 companies, which 218 companies have been involved in the production, while the remaining 189 are still in the exploratory stage. Embalut village and village Bangunrejo which become part of the administration Tenggarong Seberang Sub-District, Kutai Kartanegara, is a village that has more than 30 years was associated with the mining industry, PT. Kitadin. The results showed that: (1) the mining industrialization has changed the structure of land in the village Embalut and village Bangunrejo where land holdings in both villages have concentrated on coal mining companies. (2) mining Industrialization increasingly encourage people to work or livelihood in outside agriculture (deagrarianization). This study used qualitative methods, with in-depth interview techniques, group discussions, observation, and study of literature / documents. <br />Keywords: Industrialization Mining, deagrarianization, land tenure
DAMPAK REMITAN EKONOMI TERHADAP POSISI SOSIAL BURUH MIGRAN PEREMPUAN DALAM RUMAH TANGGA
Authors: Asih Sulistiyo Putri , Sri Wahyuni Ekawati 
Published: December 2016

The objectives of this study are to analyse the push-pull factor of international migration and the <br />impact of economic re mittance s t o migrant women’ s soc i al posit i on i n t he house hol d. Background of i ts research is feminization of international migrant into line with the phenomenon of economic globalization. The magnitude economic remittances generate by the women migrants pre sumabl y wi ll aff ect women’ s social position in the houshold. <br />Culturally, women in this areas do not have a strong decision making power relative to the men in the household. The women migrant working abroad was mainly driven bThe women migrant working abroad was mainly driven b proverty. The return women migrant are likely to have stroger decision making power in the household be case of their major contribution in the household economy. <br /> Keywords: woman migrant, social position, household.
DAMPAK REFORMA AGRARIA DARI BAWAH TERHADAP KESEJAHTERAAN MASYARAKAT DI DESA GARONGAN DAERAH ISTIMEWA YOGYAKARTA
Authors: Sokoastri Valentina , Soetarto Endriatmo 
Published: December 2016

Agrarian reform by leverage or commonly known as landreform by leverage is a peasant movements which <br />is organized by peasant initiative to defend their land. This movement could be associated with social welfare and negative excess like criminalization that frequently take place in Garongan village. There, most people involved in conflict because of their persistence to keep their land. There is a strong relationship between agrarian reform by leverage and peasant welfare. Land which is frequently referred as crucial donation of life has a vital value for human survival. The function of land is not only considered as human nee ds but al so as i dent it y t hat al ways t ri ggers any c onfl i ct nowadays . So, it ’s not st range if thi s condi ti on causes any negative impacts of criminalization including psychological, physical or both psychological and physical effects for those who involved. At the end of this description, farmers who have been sovereign from agriculture will be interferred by iron sand mining company which is supported by feudal forces and private corporations. This research examine more deeply about the relationship between agrarian reform by leverage and social welfare, the impact of agrarian reform by leverage to the criminalization and the differences of level of social welfare before and after agrarian reform in Garongan village. <br />Keywords: agrarian reform by leverage, criminalization, social welfare.
NEAR-INFRARED IMAGING POLARIMETRY OF INNER REGION OF GG TAU A DISK
Authors: Yang Yi , Hashimoto Jun , Hayashi Saeko S. , Tamura Motohide , Mayama Satoshi , Rafikov Roman , Akiyama Eiji , Carson Joseph C. , Janson Markus , Kwon Jungmi , de Leon Jerome , Oh Daehyeon , Takami Michihiro , Tang Ya-wen , Kudo Tomoyuki , Kusakabe Nobuhiko , Abe Lyu , Brandner Wolfgang , Brandt Timothy D. , Egner Sebastian , Feldt Markus , Goto Miwa , Grady Carol A. , Guyon Olivier , Hayano Yutaka , Hayashi Masahiko , Henning Thomas , Hodapp Klaus W. , Ishii Miki , Iye Masanori , Kandori Ryo , Knapp Gillian R. , Kuzuhara Masayuki , Matsuo Taro , Mcelwain Michael W. , Miyama Shoken , Morino Jun-Ichi , Moro-martin Amaya , Nishimura Tetsuo , Pyo Tae-Soo , Serabyn Eugene , Suenaga Takuya , Suto Hiroshi , Suzuki Ryuji , Takahashi Yasuhiro H. , Takato Naruhisa , Terada Hiroshi , Thalmann Christian , Turner Edwin L. , Watanabe Makoto , Wisniewski John , Yamada Toru , Takami Hideki , Usuda Tomonori 
Published: December 2016

ABSTRACT
By performing non-masked polarization imaging with Subaru/HiCIAO, polarized scattered light from the inner region of the disk around the GG Tau A system was successfully detected in the H band, with a spatial resolution of approximately 0.″07, revealing the complicated inner disk structures around this young binary. This paper reports the observation of an arc-like structure to the north of GG Tau Ab, and part of a circumstellar structure that is noticeable around GG Tau Aa, extending to a distance of approximately 28 au from the primary star. The speckle noise around GG Tau Ab constrains its disk radius to

au. Based on the size of the circumbinary ring and the circumstellar disk around GG Tau Aa, the semimajor axis of the binary’s orbit is likely to be 62 au. A comparison of the present observations with previous Atacama Large Millimeter Array and near-infrared H2 emission observations suggests that the north arc could be part of a large streamer flowing from the circumbinary ring to sustain the circumstellar disks. According to the previous studies, the circumstellar disk around GG Tau Aa has enough mass and can sustain itself for a duration sufficient for planet formation; thus, our study indicates that planets can form within close (separation ≲ 100 au) young binary systems.
MODELING THE GAMMA-RAY EMISSION IN THE GALACTIC CENTER WITH A FADING COSMIC-RAY ACCELERATOR
Authors: Liu Ruo-Yu , Wang Xiang-Yu , Prosekin Anton , Chang Xiao-Chuan 
Published: December 2016

ABSTRACT
Recent HESS observations of the ∼200 pc scale diffuse gamma-ray emission from the central molecular zone (CMZ) suggest the presence of a PeV cosmic-ray accelerator (PeVatron) located in the inner 10 pc region of the Galactic center. Interestingly, the gamma-ray spectrum of the point-like source (HESS J1745-290) in the Galactic center shows a cutoff at ∼10 TeV, implying a cutoff around 100 TeV in the cosmic-ray proton spectrum. Here we propose that the gamma-ray emission from the inner and the outer regions may be explained self-consistently by run-away protons from a single yet fading accelerator. In this model, gamma-rays from the CMZ region are produced by protons injected in the past, while gamma-rays from the inner region are produced by protons injected more recently. We suggest that the blast wave formed in a tidal disruption event (TDE) caused by the supermassive black hole (Sgr A*) could serve as such a fading accelerator. With typical parameters of the TDE blast wave, gamma-ray spectra of both the CMZ region and HESS J1745-290 can be reproduced simultaneously. Meanwhile, we find that the cosmic-ray energy density profile in the CMZ region may also be reproduced in the fading accelerator model when appropriate combinations of the particle injection history and the diffusion coefficient of cosmic rays are adopted.
A HIGH-RESOLUTION VACUUM ULTRAVIOLET LASER PHOTOIONIZATION AND PHOTOELECTRON STUDY OF THE CO ATOM
Authors: Huang Huang , Wang Hailing , Luo Zhihong , Shi Xiaoyu , Chang Yih-Chung , Ng C. Y. 
Published: December 2016

ABSTRACT
We have measured the vacuum ultraviolet–photoionization efficiency (VUV–PIE) spectrum of Co in the energy range of 63,500–67,000 cm−1, which covers the photoionization transitions of Co(3d74s2 4F9/2)

Co+(3d8 3F4), Co(3d74s2 4F7/2)

Co+(3d8 3F3), Co(3d74s2 4F9/2)

Co+(3d8 3F3), Co(3d74s2 4F9/2)

Co+(3d8 3F2), and Co(3d74s2 4F9/2)

Co+(3d74s1 5F5). We have also recorded the pulsed field ionization photoelectron spectrum of Co in the same energy range, allowing accurate determinations of ionization energies (IEs) for the photoionization transitions from the Co(3d74s2 4F9/2) ground neutral state to the Co+(3F
J
) (J = 4 and 3) and Co+(5F5) ionic states, as well as from the Co(3d74s2 4F7/2) excited neural state to the Co+(3d8 3F3) ionic state. The high-resolution nature of the VUV laser used has allowed the observation of many well-resolved autoionizing resonances in the VUV–PIE spectrum, among which an autoionizing Rydberg series, 3d74s1(5F5)np (n = 19–38), converging to the Co+(3d74s1 5F5) ionic state from the Co(3d74s2 4F9/2) ground neutral state is identified. The fact that no discernible step-like structures are present at these ionization thresholds in the VUV–PIE spectrum indicates that direct photoionization of Co is minor compared to autoionization in this energy range. The IE values, the autoionizing Rydberg series, and the photoionization cross sections obtained in this experiment are valuable for understanding the VUV opacity and abundance measurement of the Co atom in stars and solar atmospheres, as well as for benchmarking the theoretical results calculated in the Opacity Project and the IRON Project, and thus are of relevance to astrophysics.
LARGE-SCALE FILAMENTARY STRUCTURES AROUND THE VIRGO CLUSTER REVISITED
Authors: Kim Suk , Rey Soo-Chang , Bureau Martin , Yoon Hyein , Chung Aeree , Jerjen Helmut , Lisker Thorsten , Jeong Hyunjin , Sung Eon-Chang , Lee Youngdae , Lee Woong , Chung Jiwon 
Published: December 2016

ABSTRACT
We revisit the filamentary structures of galaxies around the Virgo cluster, exploiting a larger data set, based on the HyperLeda database, than previous studies. In particular, this includes a large number of low-luminosity galaxies, resulting in better sampled individual structures. We confirm seven known structures in the distance range 4 h
−1 Mpc < SGY < 16 h
−1 Mpc, now identified as filaments, where SGY is the axis of the supergalactic coordinate system roughly along the line of sight. The Hubble diagram of the filament galaxies suggests they are infalling toward the main body of the Virgo cluster. We propose that the collinear distribution of giant elliptical galaxies along the fundamental axis of the Virgo cluster is smoothly connected to two of these filaments (Leo II A and B). Behind the Virgo cluster (16 h
−1 Mpc < SGY < 27 h
−1 Mpc), we also identify a new filament elongated toward the NGC 5353/4 group (“NGC 5353/4 filament”) and confirm a sheet that includes galaxies from the W and M clouds of the Virgo cluster (“W–M sheet”). In the Hubble diagram, the NGC 5353/4 filament galaxies show infall toward the NGC 5353/4 group, whereas the W–M sheet galaxies do not show hints of gravitational influence from the Virgo cluster. The filamentary structures identified can now be used to better understand the generic role of filaments in the build-up of galaxy clusters at z ≈ 0.
THE EFFECT OF ELECTRON THERMAL PRESSURE ON THE OBSERVED MAGNETIC HELICITY IN THE SOLAR WIND
Authors: Markovskii S. A. , Vasquez Bernard J. , Smith Charles W. 
Published: December 2016

ABSTRACT
Statistical analysis of magnetic helicity spectra in the solar wind at 1 au is carried out. A large database of the solar wind intervals assembled from Wind spacecraft magnetic and plasma data is used. The effect of the electron thermal pressure on the wavenumber position of the helicity signature, i.e., the peak of the spectrum, is studied. The position shows a statistically significant dependence on both the electron and proton pressures. However, the strongest dependence is seen when the two pressures are summed. These findings confirm that the generation of the magnetic helicity is associated with an increasing compressibility of the turbulent fluctuations at smaller kinetic scales. It is argued that instrumental artifacts do not contribute to the helicity signature.
TURBULENT DYNAMO IN A CONDUCTING FLUID AND A PARTIALLY IONIZED GAS
Authors: Xu Siyao , Lazarian A. 
Published: December 2016

ABSTRACT
By following the Kazantsev theory and taking into account both microscopic and turbulent diffusion of magnetic fields, we develop a unified treatment of the kinematic and nonlinear stages of a turbulent dynamo process, and we study the dynamo process for a full range of magnetic Prandtl number P

m
and ionization fractions. We find a striking similarity between the dependence of dynamo behavior on P

m
in a conducting fluid and

(a function of ionization fraction) in a partially ionized gas. In a weakly ionized medium, the kinematic stage is largely extended, including not only exponential growth but a new regime of dynamo characterized by a linear-in-time growth of magnetic field strength, and the resulting magnetic energy is much higher than the kinetic energy carried by viscous-scale eddies. Unlike the kinematic stage, the subsequent nonlinear stage is unaffected by microscopic diffusion processes and has a universal linear-in-time growth of magnetic energy with the growth rate as a constant fraction 3/38 of the turbulent energy transfer rate, showing good agreement with earlier numerical results. Applying the analysis to the first stars and galaxies, we find that the kinematic stage is able to generate a field strength only an order of magnitude smaller than the final saturation value. But the generation of large-scale magnetic fields can only be accounted for by the relatively inefficient nonlinear stage and requires longer time than the free-fall time. It suggests that magnetic fields may not have played a dynamically important role during the formation of the first stars.
THE 2012 JULY 23 BACKSIDE ERUPTION: AN EXTREME ENERGETIC PARTICLE EVENT?
Authors: Gopalswamy N. , Yashiro S. , Thakur N. , Mäkelä P. , Xie H. , Akiyama S. 
Published: December 2016

ABSTRACT
The backside coronal mass ejection (CME) of 2012 July 23 had a short Sun-to-Earth shock transit time (18.5 hr). The associated solar energetic particle (SEP) event had a >10 MeV proton flux peaking at ∼5000 pfu, and the energetic storm particle event was an order of magnitude larger, making it the most intense event in the space era at these energies. By a detailed analysis of the CME, shock, and SEP characteristics, we find that the July 23 event is consistent with a high-energy SEP event (accelerating particles to gigaelectronvolt energies). The times of maximum and fluence spectra in the range 10–100 MeV were very hard, similar to those of ground-level enhancement (GLE) events. We found a hierarchical relationship between the CME initial speeds and the fluence spectral indices: CMEs with low initial speeds had SEP events with the softest spectra, while those with the highest initial speeds had SEP events with the hardest spectra. CMEs attaining intermediate speeds result in moderately hard spectra. The July 23 event was in the group of hard-spectrum events. During the July 23 event, the shock speed (>2000 km s−1), the initial acceleration (∼1.70 km s−2), and the shock-formation height (∼1.5 solar radii) were all typical of GLE events. The associated type II burst had emission components from meter to kilometer wavelengths, suggesting a strong shock. These observations confirm that the 2012 July 23 event is likely to be an extreme event in terms of the energetic particles it accelerated.
ALMA OBSERVATIONS OF ORION SOURCE I AT 350 AND 660 GHz
Authors: Plambeck R. L. , Wright M. C. H. 
Published: December 2016

ABSTRACT
Orion Source I (“SrcI”) is the protostar at the center of the Kleinmann-Low Nebula. ALMA observations of SrcI with 0.″2 angular resolution were made at 350 and 660 GHz to search for the H26α and H21α hydrogen recombination lines and to measure the continuum flux densities. The recombination lines were not detected, ruling out the possibility that SrcI is a hypercompact H ii region. The deconvolved size of the continuum source is approximately 0.″23 × 0.″07 (∼100 × 30 au); it is interpreted as a disk viewed almost edge-on. Optically thick thermal emission from ∼500 K dust is the most plausible source of the continuum, even at frequencies as low as 43 GHz; the disk mass is most likely in the range 0.02–0.2

. A rich spectrum of molecular lines is detected, mostly from sulfur- and silicon-rich molecules like SO, SO2, and SiS, but also including vibrationally excited CO and several unidentified transitions. Lines with upper energy levels

K appear in emission and are symmetric about the source’s LSR velocity of 5

, while lines with

K appear as blueshifted absorption features against the continuum, indicating that they originate in outflowing gas. The emission lines exhibit a velocity gradient along the major axis of the disk that is consistent with rotation around a 5–7

central object. The relatively low mass of SrcI and the existence of a 100 au disk around it are difficult to reconcile with the model in which SrcI and the nearby Becklin–Neugebauer Object were ejected from a multiple system 500 years ago.