2,056 research outputs found
Analisis Pendapatan Usaha Industri Jamu di Kelompok Tani Prima Mandiri Desa Usapinonot
Penelitian ini dilakukan di Kecamatan Insana Barat Kabupaten Timor Tengah Utara, tujuan penelitian ini untuk mengetahui pendapatan USAha industri jamu di Kelompok Tani Prima Mandiri, dan untuk mengetahui keuntungan relatif USAha industri jamu di Kelompok Tani Mandiri. Metode pengambilan data dilakukan secara survei dengan jenis data berupa data primer dan data sekunder. Analisis data dilakukan dengan menggunakan analisis deskriptif, analisis pendapatan dan analisis R/C ratio. Hasil penelitian ini menunjukkan beberapa kesimpulan yakni, penerimaan untuk keseluruhan responden dalam empat kali produksi (1 bulan) adalah sebesar Rp. 44.000.000 dengan rata-rata per responden adalah sebesar Rp. 4.000.000. Total biaya produksi untuk keseluruhan responden dalam empat kali produksi (bulan) adalah sebesar Rp. 18.329.500 dengan rata-rata Rp. 1.666.318 per responden. Total pendapatan USAha industri jamu untuk keseluruhan responden dalam satu kali produksi adalah sebesar Rp. 4.776.500 dengan rata-rata Rp. 434.277, sedangkan total pendapatan untuk keseluruhan responden dalam empat kali produksi (bulan) adalah sebesar Rp. 19.248.000 dengan rata-rata per responden adalah sebesar Rp.1.749.818. hal ini menunjukkan bahwa penerimaan, biaya produksi dan pendapatan sangat bervariasi. Nilai rata-rata R/C ratio dari USAha industri jamu adalah sebesar 1,9 sehingga USAha industri jamu tersebut secara ekonomis menguntungkan dan dapat dilanjutkan.. ©2016 dipublikasikan oleh Agrimor
High-Resolution X-Ray Spectroscopy of the Accretion Disk Corona Source 4U 1822-37
We present a preliminary analysis of the X-ray spectrum of the accretion disk
corona source, 4U 1822-37, obtained with the High Energy Transmission Grating
Spectrometer onboard the Chandra X-ray Observatory. We detect discrete emission
lines from photoionized iron, silicon, magnesium, neon, and oxygen, as well as
a bright iron fluorescence line. Phase-resolved spectroscopy suggests that the
recombination emission comes from an X-ray illuminated bulge located at the
predicted point of impact between the disk and the accretion stream. The
fluorescence emission originates in an extended region on the disk that is
illuminated by light scattered from the corona.Comment: 12 pages, 6 figures; Accepted for publication in ApJ Letter
The flux of noncommutative U(1) instanton through the fuzzy spheres
From the ADHM construction on noncommutative we investigate
different U(1) instanton solutions tied by isometry trasformations. These
solutions present a form of vector fields in noncommutative
vector space which makes possible the calculus of their fluxes through fuzzy
spheres. We establish the noncommutative analog of Gauss theorem from which we
show that the flux of the U(1) instantons through fuzzy spheres does not depend
on the radius of these spheres and it is invariant under isometry
transformations.Comment: 18 pages, new version to appear in Int. Jour. of Mod. Phys.
Instanton Number of Noncommutative U(n) gauge theory
We show that the integral of the first Pontrjagin class is given by an
integer and it is identified with instanton number of the U(n) gauge theory on
noncommutative . Here the dimension of the vector space that
appear in the ADHM construction is called Instanton number. The calculation is
done in operator formalism and the first Pontrjagin class is defined by
converge series. The origin of the instanton number is investigated closely,
too.Comment: 6 color figures, 27 pages, some comments and references are
added,typos fixe
The Ionized Stellar Wind in Vela X-1 During Eclipse
We present a first analysis of a high resolution X-ray spectrum of the
ionized stellar wind of Vela X-1 during eclipse. The data were obtained with
the High Energy Transmission Grating Spectrometer onboard the Chandra X-ray
Observatory. The spectrum is resolved into emission lines with fluxes between
0.02 and 1.04x10^4 ph/cm^2/s. We identify lines from a variety of charge
states, including fluorescence lines from cold material, a warm photoionized
wind. We can exclude signatures from collisionally ionized plasmas. For the
first time we identify fluorescence lines from L-shell ions from lower Z
elements. We also detect radiative recombination continua from a kT = 10 eV
(1.2 x 10^5 K) photoionized optically thin gas. The fluorescence line fluxes
infer the existence of optically thick and clumped matter within or outside the
warm photoionized plasma.Comment: 4 pages, 2 figures, accepted by ApJ letter
Polar Field Reversal Observations with Hinode
We have been monitoring yearly variation in the Sun's polar magnetic fields
with the Solar Optical Telescope aboard {\it Hinode} to record their evolution
and expected reversal near the solar maximum. All magnetic patches in the
magnetic flux maps are automatically identified to obtain the number density
and magnetic flux density as a function of th total magnetic flux per patch.
The detected magnetic flux per patch ranges over four orders of magnitude
( -- Mx). The higher end of the magnetic flux in the polar
regions is about one order of magnitude larger than that of the quiet Sun, and
nearly that of pores. Almost all large patches ( Mx) have the
same polarity, while smaller patches have a fair balance of both polarities.
The polarity of the polar region as a whole is consequently determined only by
the large magnetic concentrations. A clear decrease in the net flux of the
polar region is detected in the slow rising phase of the current solar cycle.
The decrease is more rapid in the north polar region than in the south. The
decrease in the net flux is caused by a decrease in the number and size of the
large flux concentrations as well as the appearance of patches with opposite
polarity at lower latitudes. In contrast, we do not see temporal change in the
magnetic flux associated with the smaller patches ( Mx) and that of
the horizontal magnetic fields during the years 2008--2012.Comment: 21 pages, 7 figures. Accepted for publication in Ap
Instanton Number Calculus on Noncommutative R^4
In noncommutative spaces, it is unknown whether the Pontrjagin class gives
integer, as well as, the relation between the instanton number and Pontrjagin
class is not clear. Here we define ``Instanton number'' by the size of
in the ADHM construction. We show the analytical derivation of the
noncommuatative U(1) instanton number as an integral of Pontrjagin class
(instanton charge) with the Fock space representation. Our approach is for the
arbitrary converge noncommutative U(1) instanton solution, and is based on the
anti-self-dual (ASD) equation itself. We give the Stokes' theorem for the
number operator representation. The Stokes' theorem on the noncommutative space
shows that instanton charge is given by some boundary sum. Using the ASD
conditions, we conclude that the instanton charge is equivalent to the
instanton number.Comment: 29 pages, 7 figures, some statements in Sec.4.3 correcte
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