Specification for X-ray lead-rubber protective aprons for personal use

2015 ◽  
Keyword(s):  
X Ray ◽  
Personal Use

Hukum Kepabeanan dalam Kegiatan Pelaku Usaha Jasa Titip Online

2021 ◽  
Vol 2 (4) ◽  
Author(s):  
Rafli Wiratama ◽  
Fahmi Muhammad Ahmadi ◽  
M. Nuzul Wibawa
Keyword(s):  
United States ◽  
Import Duty ◽  
Modus Operandi ◽  
Business Services ◽  
X Ray ◽  
United States Dollar ◽  
Service Business ◽  
Personal Use ◽  
Type C

ABSTRACTThe role of Customs and Excise Type C Soekarno-Hatta in carrying out supervision of onlne deposit service business operators who do not pay import duty and tax in the framework of import as well as the modus operandi carried out by online deposit service business actors to avoid payment of import duty and deeds of perpetrators online courier services business perspective criminal law because, the number of online entourage business operators who use passenger luggage facilities contained in Article 7 and Article 12 of the Minister of Finance Regulation Number 203 / PMK.04 / 2017 concerning the provisions on the export and import of goods carried by passengers and the crew of the means of conveyance, namely exemption of imported imported goods up to a maximum value of Free On Boad USD 500.00 (Five Hundred United States Dollars) per person for each arrival is exempted from import duty. However, this exemption from import duty is utilized by business people who entrust online services to carry out trading activities, because basically this regulation is for personal goods of passengers or personal use and not for goods. This research uses qualitative research by combining an empirical approach is legal research on law in fact and applied by humans who live in the community itself and to determine the implementation of legal norms that have been applied. The results of this study aimed that the role of Customs and Excise Soekarno-Hatta in carrying out complaints against business operators entrusting services online, using the category of passenger luggage control by conducting preliminary supervision by looking at, baggage x-ray analysis and looking at passenger profiles using the Passanger Name Record system For Government (PNR-GOV), then the modus operandi of online business services is to use deminimis threshold by recognizing that service goods are left as personal goods and not giving actual customs notification. Acts carried out by online deposit service business operators who do not pay taxes by physically smuggling by placing their merchandise in improper places have violated the rules of Article 102 letter (e) of Law Number 17 Year 2006 concerning Customs of the act of entrusted business services online by not notifying the type and / or quantity of imported goods in customs notification wrongly violating Article 102 letter (h) of Law Number 17 Year 2006 concerning Customs. The threat of criminal imprisonment is 1 (one) year and a maximum of 10 (ten) years and a fine of at least Rp.50,000,000.00 (fifty million rupiah) and a maximum of Rp.5,000,000,000.00 (five billion rupiah).Keywords: Business Executives Services Online, Customs Type C Soekarno Hatta, Exemption from Import Duties.ABSTRAKPeran Bea dan Cukai Tipe C Soekarno-Hatta dalam melakukan pengawasan terhadap pelaku usaha jasa titip onlne yang tidak melakukan pembayaran pajak bea masuk dan pajak dalam rangka impor serta modus operandi yang dilakukan oleh pelaku usaha jasa titip online untuk melakukan penghindaran pembayaran bea masuk serta perbuatan pelaku usaha jasa titip online perspektif hukum pidana karena, banyaknya pelaku usaha jasa titip online yang menggunakan fasilitas barang bawaan penumpang yang terdapat dalam Pasal 7 dan Pasal 12 Peraturan Menteri Keuangan  Nomor 203/PMK.04/2017 tentang ketentuan ekspor dan impor barang yang dibawa oleh penumpang dan awak sarana pengangkut yaitu pembebasan barang impor bawaan sampai dengan nilai paling banyak Free On Boad USD 500.00 (Lima Ratus United States Dollar) perorang untuk setiap kedatangan diberikan pembebasan bea masuk. Namun pembebasan bea masuk ini dimanfaatkan oleh pelaku usaha jasa titip online untuk melakukan kegiatan perdagangan, karena pada dasarnya peraturan ini untuk barang pribadi penumpang atau personal use dan bukan untuk barang daganangan. Penelitian ini menggunakan jenis penelitian kualitatif dengan menggabungkan pendekatan empiris adalah penelitian hukum tentang hukum pada kenyataanya dan diterapkan oleh manusia yang hidup dalam masyarakat itu sendiri dan untuk mengetahui implementasi norma hukum yang telah berlaku.Hasil penelitian ini menujukan bahwa peran Bea dan Cukai Soekarno-Hatta dalam melakukan pengawsaan terhadap pelaku usaha jasa titip online, menggunakan katagori pengawasan barang bawaan penumpang dengan melakukan pengawasan pendahuluan dengan melihat, analisis x-ray bagasi dan melihat profil penumpang dengan menggunakan sistem Passanger Name Record For Government (PNR-GOV), kemudian modus operandi yang di lakukan pelaku usaha jasa titip online adalah menggunakan deminimis threshold dengan mengakui bahwa barang jasa titip sebagai barang pribadinya dan tidak memberikan pemberitahuan pabean dengan sebenarnya. Perbuatan yang dilakukan oleh pelaku usaha jasa titip online yang tidak membayar pajak dengan melakukan penyeludupan secara fisik dengan meletakan barang daganganya di tempat yang tidak sewajarnya telah melanggar peraturan Pasal 102 huruf (e) Undang-Undang Nomor 17 Tahun 2006 tentang Kepabeanan perbuatan pelaku usaha jasa titip online dengan tidak memberitahukan jenis dan/atau jumlah barang impor dalam  pemberitahuan  pabean  secara salah melanggar Pasal 102 huruf (h) Undang-Undang Nomor 17 Tahun 2006 tentang Kepabeanan. Ancaman pidananya pidana penjara  1 (satu) tahun dan paling lama 10 (sepuluh) tahun dan pidana  denda paling sedikit Rp.50.000.000.00 (lima puluh juta rupiah) dan paling banyak Rp.5.000.000.000.00 (lima milyar rupiah).

Space and Time Distribution of Hard X-Ray Emission in a Loop at the Beginning of a Flare

1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux
Keyword(s):  
Time Distribution ◽  
Electron Bombardment ◽  
Spatial Evolution ◽  
Superthermal Electrons ◽  
Flare Loop ◽  
X Ray ◽  
Superthermal Electron ◽  
Flare Loops ◽  
Chromospheric Evaporation ◽  
Temporal And Spatial

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.

Some Problems in Understanding the Solar Corona

1994 ◽  
Vol 144 ◽  
pp. 1-9
Author(s):  
A. H. Gabriel
Keyword(s):  
Solar Corona ◽  
Solar Atmosphere ◽  
Theoretical Modelling ◽  
Total System ◽  
Major Advance ◽  
X Ray ◽  
Proper Perspective ◽  
Space Observations

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.

White-Light Coronal Structures: Streamers and CMEs

1994 ◽  
Vol 144 ◽  
pp. 82
Author(s):  
E. Hildner
Keyword(s):  
Emission Line ◽  
Electron Density ◽  
White Light ◽  
Coronal Mass Ejections ◽  
X Rays ◽  
Solar Cycles ◽  
Temperature Function ◽  
X Ray ◽  
Eclipse Observations ◽  
Coronal Structures

AbstractOver the last twenty years, orbiting coronagraphs have vastly increased the amount of observational material for the whitelight corona. Spanning almost two solar cycles, and augmented by ground-based K-coronameter, emission-line, and eclipse observations, these data allow us to assess,inter alia: the typical and atypical behavior of the corona; how the corona evolves on time scales from minutes to a decade; and (in some respects) the relation between photospheric, coronal, and interplanetary features. This talk will review recent results on these three topics. A remark or two will attempt to relate the whitelight corona between 1.5 and 6 R⊙to the corona seen at lower altitudes in soft X-rays (e.g., with Yohkoh). The whitelight emission depends only on integrated electron density independent of temperature, whereas the soft X-ray emission depends upon the integral of electron density squared times a temperature function. The properties of coronal mass ejections (CMEs) will be reviewed briefly and their relationships to other solar and interplanetary phenomena will be noted.

Iron K-Line Emission from X-Ray Binaries

1988 ◽  
Vol 102 ◽  
pp. 47-50
Author(s):  
K. Masai ◽  
S. Hayakawa ◽  
F. Nagase
Keyword(s):  
Accretion Disk ◽  
Radiative Recombination ◽  
Characteristic Temperature ◽  
Line Emission ◽  
Ionization Front ◽  
Continuum Radiation ◽  
X Ray ◽  
Low Mass ◽  
X Ray Binaries

AbstractEmission mechanisms of the iron Kα-lines in X-ray binaries are discussed in relation with the characteristic temperature Txof continuum radiation thereof. The 6.7 keV line is ascribed to radiative recombination followed by cascades in a corona of ∼ 100 eV formed above the accretion disk. This mechanism is attained for Tx≲ 10 keV as observed for low mass X-ray binaries. The 6.4 keV line observed for binary X-ray pulsars with Tx> 10 keV is likely due to fluorescence outside the He II ionization front.

Diagnostics of Gold Laser Plasmas

1988 ◽  
Vol 102 ◽  
pp. 357-360
Author(s):  
J.C. Gauthier ◽  
J.P. Geindre ◽  
P. Monier ◽  
C. Chenais-Popovics ◽  
N. Tragin ◽  
...  
Keyword(s):  
Experimental Results ◽  
Pure Gold ◽  
Electronic Temperature ◽  
X Ray ◽  
Laser Plasmas ◽  
Collisional Radiative Model ◽  
Radiative Model

AbstractIn order to achieve a nickel-like X ray laser scheme we need a tool to determine the parameters which characterise the high-Z plasma. The aim of this work is to study gold laser plasmas and to compare experimental results to a collisional-radiative model which describes nickel-like ions. The electronic temperature and density are measured by the emission of an aluminium tracer. They are compared to the predictions of the nickel-like model for pure gold. The results show that the density and temperature can be estimated in a pure gold plasma.

Axial Observation of X-Ray Spectra from a Beam-Foil Source

1988 ◽  
Vol 102 ◽  
pp. 339-342
Author(s):  
J.M. Laming ◽  
J.D. Silver ◽  
R. Barnsley ◽  
J. Dunn ◽  
K.D. Evans ◽  
...  
Keyword(s):  
Spectral Resolution ◽  
Heavy Ion ◽  
Ion Beams ◽  
Beam Axis ◽  
Doppler Broadening ◽  
X Ray ◽  
Beam Foil

AbstractNew observations of x-ray spectra from foil-excited heavy ion beams are reported. By observing the target in a direction along the beam axis, an improvement in spectral resolution, δλ/λ, by about a factor of two is achieved, due to the reduced Doppler broadening in this geometry.

Observed and Theoretical Spectra in the 10–100Å Interval

1988 ◽  
Vol 102 ◽  
pp. 259-261
Author(s):  
W.A. Brown ◽  
M.E. Bruner ◽  
L.W. Acton
Keyword(s):  
Sounding Rocket ◽  
Full Spectrum ◽  
X Ray

AbstractThe soft x-ray spectra recorded in two sounding rocket flights in 1982 and 1985 are compared with with predicted spectra. The poster presents the processed densitometer trace of the full spectrum together with the new spectrum from the 1985 experiment. This note compares the intensities of the lines with predictions.

Quaternary structure of Limulus polyphemus hemocyanin

1978 ◽  
Vol 36 (2) ◽  
pp. 176-177
Author(s):  
T. Wichertjes ◽  
E.J. Kwak ◽  
E.F.J. Van Bruggen
Keyword(s):  
Electron Microscopy ◽  
Functional Properties ◽  
Horseshoe Crab ◽  
Temperature Jump ◽  
Quaternary Structure ◽  
Crystallographic Analysis ◽  
Limulus Polyphemus ◽  
Oxygen Binding ◽  
X Ray ◽  
Intact Molecule

Hemocyanin of the horseshoe crab (Limulus polyphemus) has been studied in nany ways. Recently the structure, dissociation and reassembly was studied using electron microscopy of negatively stained specimens as the method of investigation. Crystallization of the protein proved to be possible and X-ray crystallographic analysis was started. Also fluorescence properties of the hemocyanin after dialysis against Tris-glycine buffer + 0.01 M EDTA pH 8.9 (so called “stripped” hemocyanin) and its fractions II and V were studied, as well as functional properties of the fractions by NMR. Finally the temperature-jump method was used for assaying the oxygen binding of the dissociating molecule and of preparations of isolated subunits. Nevertheless very little is known about the structure of the intact molecule. Schutter et al. suggested that the molecule possibly consists of two halves, combined in a staggered way, the halves themselves consisting of four subunits arranged in a square.

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