Selection and Crossbreeding in Relation to Plumage Color Inheritance in Three Chinese Egg Type Duck Breeds (Anas Platyrhynchos)

Lin, R.L.,Chen, H.P.,Rouvier, R.,Poivey, J.P. Asian Australasian Association of Animal Productio 2014 Animal Bioscience Vol.27 No.8

In China and South East Asia, the duck (common duck) is important in egg production for human consumption. Plumage color is a breed characteristic and of economic importance, together with egg production. Our aim in this study was to investigate the inheritance of plumage color in three Chinese indigenous egg-type duck breeds, Shan Ma (S), Putian White (F) and Putian black (P), and some of their crossbreds. These three breeds have different plumage color and are used in crossbreeding. The crossbred laying ducks $F{\times}(P{\times}S)$ and $F{\times}(S{\times}P)$ showed highly improved laying ability but heterogeneous plumage color. Genotypes at four relevant loci were investigated by studying down color and pattern in ducklings after crossbreeding. $F_1$ ducklings from the matings $F{\times}S$ and $S{\times}F$, $P{\times}S$, and $S{\times}P$ were classified into four classes of plumage color (the Shan Ma plumage color, black, white, or multicolored) over three generations. Parents were selected for the Shan Ma plumage color of their progeny. In the fourth generation, P male and P female ducks were selected according to the frequency of the desired class of plumage color (Shan Ma) of their $F_1$ progeny to obtain the so-called "Brown Putian Ma duck". The Shan Ma duck genotype was identified as having the restricted mallard color pattern ($M^RM^R$), full expression of any of the patterns or colors (CC), no extended black (ee) and no brown dilution D (D). The Putian White genotype was recessive white (cc), no extended black (ee) and no brown dilution D (D). The Putian Black genotype exhibited full expression of extended black (E gene) and no brown dilution (CCEE D [D]). It was shown that $F{\times}S$ and $S{\times}F$ tests should be implemented to eliminate the recessive white c allele in the S line and the dominant extended black E allele in the F line. It was also shown that the Brown Putian Ma obtained from Putian Black, with no extended black genotype (ee), could be used to get rid of the black plumage (E gene) in the crossbred ducks. This could provide a solution for producing 3-way crossbred ducks Putian $White{\times}$(Putian-$Ma{\times}Shan$ Ma) and Putian $White{\times}$(Shan $Ma{\times}Putian$-Ma), with the desired Shan Ma feather color.

Studies on Filariasis in Kinmen (Quemoy) Islands, Republic of China

Fan,P.C.,Wang,Y.C.,Liu,J.C.,Lo,H.S.,Hsu,Y.P.,Yen,C.H.,Lin,C.C.,Hsu,S.T. INSTITUTE OF TROPICAL MEDICINE YONSEI UNIVERSITY 1974 YONSEI REPORTS ON TROPICAL MEDICINE Vol.5 No.1

1972年 7月 1日부터 1973年 6月 30日까지 1年間 中華民國 臺?省 金門鳥에서 絲狀 症에 關한 調査硏究를 實施한 바 다음과 같은 結果를 얻었다. 1. 金門鳥 55村落에 居住하는 20,018 住民을 對象으로 調査한 바 血中 microfilariae (mf.) 兩性率은 8.8%였고 血液 20立方mm當 mf농도는 16.2였으며 絲狀 感染으로 因 臨床例 는 19.2%였다. 金門鳥 駐屯 軍人 2,428名에서 mf.양성율은 0.1%, mf. 감염농도는 20立方mm當 26.3이었으며 臨床例는 없었다. mf.感染濃度 및 臨床例에 있어 확실히 女性보다는 男性에서 高率을 보였으나 mf.陽性率은 兩性間에 差異가 없었다. mf.陽性率과 臨床例는 年齡의 增加와 一致하였으나 mf. 감렴농도는 年齡의 증가와 無關하였다. 2. 金文鳥 駐屯 軍人에 있어 주둔 其間과 絲狀 感染과는 關係가 없었으며 駐屯基地와 村落과의 距離와도 無關하였다. 軍人들은 모기에 물리지 않도록 잘 保護되어 있었고 주둔지역은 完全히 住民들과 격리되어 있었다. 3. 51村落으로부터의 血液檢査를 받은 1,470名의 絲狀 感染陽性者 中에서 臨床病勢르 보인 例는 19.2%였으며 女性보다는 男性에서 約 5倍가 많았다. 男性에 있어서의 大部分의 臨床例는 生殖器에 症狀을 보였는데 其中 10%는 象皮症을 가진 例는 2名뿐이었다. 4. 43村落의 家屋內에서 잡힌 모기는 4屬 14種(Culex 10種, Aedes 2種, Anopheles 1種, Armigeres 1種)이었으며 이들中 Cules P. fatigans와 Armigeres subalbatus가 大部分이었으나 其他 12種은 매우 적었다. Culcx mimesticus, C. (L) vorax, C. fuscocephala 및 Acdes nocturnus등 의 4新種은 처음으로 發見되었다. Culex p.fatigans는 現存「반크롭트」 絲狀 만을 옮기는 媒介昆 으로 알려져 있다. 治療前 8個 村落으로부터 잡은 438마리의 Culex p. fatigans에서 幼 을 內包하고 있는 모기는 1마리 平均 5.9마리의 絲狀 幼 을 갖고 있는 셈이었으며 全體 感染率은 11.9%, 感染期 幼 을 가진 모기는 10.5%이었다. 上記 8個 村落 住民을 治癒한 後의 樣狀은 治療前과 아주 달라서 모기 1마리當 平均 2.1마리의 幼 을 갖고 있었고 全體感染率은 2.2%, 感染期幼 內包率은 0.09%였다. 平均 pH가 7.4(6.4∼8.0)인 8個處의 모기 産卵場所에서 잡힌 모기 幼 은 모두 11種이었다. 有機燐劑의 一種인 Sumithion을 1平方m當 0.2gm의 농도로 모기 産卵場所 水面에 撒布하였던바 모든 모기 幼 에 對한 殺 果가 좋았다. 5. 總 1.590名의 絲狀 感染者에게 成人當 總量 5gm의 diethylcarbamazine을 10∼12日 間 服用시켜 보았다. 治療率은 80.6%, mf. 減少率은 96.9%였고 反應率는 67.2%였다. 여러 가지 副作用은 있었으나 一般的으로 輕微하였으며 患者가 참을 수 있었으므로 最高用量으로 投藥했을 경우에도 大部分 거절 하지 않았다. 8個 部落에서 捕獲된 Culex P. fatigans의 絲狀 幼 全體感染率, 感染期幼 內包率 및 感染濃度는 患者治療前에 各各 11.9%, 10.5%, 5.9였는데 治療後에는 2.2%, 0.09%, 2.1로 떨어져서 diethylcarbamazine은 microfilariae에 對한 殺충효果가 높을 뿐 아니라 絲狀충 만延을 組止시키는데 좋은 藥劑라고 思料된다 The present investigation is a serial study on “Filariasis in Kinmen (Quemoy) Islands”, which was performed from July 1, 1972 to June 30, 1973. The results are summarized as follows; 1. Parasitological investigation: Of 20,018 Kinmen Chinese in 55 villages examined, the microfilariae (mf.) rate of 8.8%, mf. density of 16.2 per 20cmm blood and clinical rate 19.2% were found: the corresponding figures for a total of 2,428 military personnel were 0.1%, 29.3 and 0.0% respectively. The mf. density and clinical rate were obviously higher in the males than in the females, but no difference was found for the microfilarial rate. The mf. rate and clinical rate were correspondingly increased with age, but there was no difference in mf. density. 2. Transmission of filariasis: It seems no any relation to the length of stationing of the Chinese troops on Kinmen Islands, and also no relation to the distance between the villages and camps; because the servicemen are well protected from the mosquito bites and bites and the camps are completely isolated, to and off limit to the villagers, though they have common places of entertainment. 3. Clinical investigation: Of 1,470 filarial carriers in 51 villages examined physically, the clinical rate of 19.2% was detected. It was about 5 times higher in males than in females. In the males, most of the cases the trouble in their reproductive organs, and 10% had elephantiasis; but in the females, the lymph nodes enlargement and chyluria were more common, only 2 cases had elephantiasis. The clinical rates increased corresponding with age. 4. Entomological investigation: Fourteen(14) species of 4 genera (10 Culex, 2 Aedes, 1 Anopheles and 1 Armigeres) of household mosquitoes were collected from indoor resting sites of 43 villages on kinmen Islands, in which, Cules P. fatigans and Armigeres subalbatus were the most common species, but the remaining 12 species are faily rare. Four (4) new species: Culex mimeticus, C. (L) vorax, C, fucocephala and Aedes noturnvs were found for the first time. Culex p.fatigans is still the only vector. in transmission of bancroftian filariasis. The infection rate of 11.9%, infective rate of 10.5% and 5.9 filarial larvae per infected mosquito were detected in 438 Culex p. fatigans from 8 villages before treatment. The corresponding figures were much lower in the above same villages after treatment (2.2%, 0.09% and 2.1). Eleven (11) species of moswquito larvae were collected from 8 kinds of breeding sites; where, the pH value of 7.4(ranged 6.4∼8.0) was measured. “Sumithion”is one of the organophosphorous compounds, which was first used on the water surface with the dosage of 0.2gm per square meter.A high insecticidal effect against different species of mosquito larvae was observed. 5. Chemotherapy of filariasis: Of 1.590 filarial carriers scheme, with a total does of 5 gm of diethylcarbamazine per adult case for a period of 10∼12 days schedule was performed. The cure rate of 80.6%, mf. reduction tate of 96.9% and reaction rate of 67.2% were found. Although many kinds of side effects were encountered, they were usually mild or transient and could be tolerated by the patients, thus there was almost no refused to the administration of the drug even if the drug was increased to the maximum dosage. The natural infection rate, infective rate and filarial larval density of Culex P. fatigans in 8 villages were found much higher before control measure (11.9%, 10.5% and 5.9%) than after control (2.2%, 0.09% and 2.1). It showed that diethylcarbamazine is a powerful microfilaricidal drug in eliminating the filarial infection and reducing this transmission.

TRANSPORT OF SOLAR WIND H ⁺ AND He ⁺⁺ IONS ACROSS EARTH’S BOW SHOCK

Parks, G. K.,Lee, E.,Fu, S. Y.,Kim, H. E.,Ma, Y. Q.,Yang, Z. W.,Liu, Y.,Lin, N.,Hong, J.,Canu, P.,Dandouras, I.,Rè,me, H.,Goldstein, M. L. American Astronomical Society 2016 ASTROPHYSICAL JOURNAL LETTERS - Vol.825 No.2

<P>We have investigated the dependence of mass, energy, and charge of solar wind ( SW) transport across Earth's bow shock. An examination of 111 crossings during quiet SW in both quasi-perpendicular and quasi-parallel shock regions shows that 64 crossings had various degrees of heating and thermalization of SW. We found 22 crossings where the SW speed was <400 km s(-1). The shock potential of a typical supercritical quasi-perpendicular shock estimated from deceleration of the SW and cutoff energy of electron flat top distribution is similar to 50 Volts. We find that the temperatures of H+ and He++ beams that penetrate the shock can sometimes be nearly the same in the upstream and downstream regions, indicating little or no heating had occurred crossing the bow shock. None of the models predict that the SW can cross the bow shock without heating. Our observations are important constraints for new models of collisionless shocks.</P>

Electron-Electron Interactions in a Two-Dimensional Electron Systemin an Al0.15Ga0.85N/GaN Heterostructure Grown on p-Type Si

Jian-Zhe Huang,Li-Hung Lin,Chin-An Chang,Chi-Te Liang,Kuang Yao Chen,Kui-Ming Chen,N. C. Chen,P. H. Chang,Shiou-Shian Han,Zhi-Hao Sun 한국물리학회 2007 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol.50 No.3

We report on experimental studies of an Al$_{0.15}$Ga$_{0.85}$N/GaN high-electron-mobility transistor structure grown on a $p$-type Si (111) substrate. This structure is compatible with complementary metal-oxide-semiconductor (CMOS) technology and, thus, has great potential device applications. The low-temperature magnetoresistivity shows a parabolic dependence on the applied perpendicular magnetic field. This effect is ascribed to electron-electron interaction (EEI) effects in a weakly-disordered two-dimensional system. Our experimental results agree with the EEI theory when the correction term in the ballistic region has been subtracted.

Electrical Measurements of an AlGaN/GaN High-electron-mobility Transistor Structure Grown on Si

Zhi-Yao Zhang,Shun-Tsung Lo,Li-Hung Lin,Kuang Yao Chen,J. Z. Huang,Zhi-Hao Sun,C.-T. Liang,N. C. Chen,Chin-An Chang,P. H. Chang 한국물리학회 2012 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol.61 No.9

We report on magnetotransport results for an Al_0.15Ga_0.85N/GaN high-electron-mobility-transistor structure grown on a p-type Si (111) substrate. Our results show that there exists an approximately temperature (<i>T</i>)-independent point, which could be ascribed to a direct transition from a weak insulator to a high Landau level filling factor quantum Hall state, exists in the longitudinal resistivity ρ_xx. The Hall resistivity decreases with increasing <i>T</i>, compelling experimental evidence for electron-electron interaction effects in a weakly-disordered two-dimensional (2D) system. We find that electron-electron interaction effects can be estimated and eliminated, giving rise to a corrected nominally temperature-independent Hall slope. By fitting the low-field magnetotransport data to conventional 2D weak localization theory, we find that the dephasing rate 1/τ_φ is proportional to <i>T</i>. Moreover, 1/τ_φ is finite as <i>T</i> → 0, evidence for zero-temperature dephasing in our system.

MEASUREMENTS OF THE CORONAL ACCELERATION REGION OF A SOLAR FLARE

Krucker, Sä,m,Hudson, H. S.,Glesener, L.,White, S. M.,Masuda, S.,Wuelser, J.-P.,Lin, R. P. IOP Publishing 2010 The Astrophysical journal Vol.714 No.2

<P>The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) and the Nobeyama Radioheliograph (NoRH) are used to investigate coronal hard X-ray and microwave emissions in the partially disk-occulted solar flare of 2007 December 31. The STEREO mission provides EUV images of the flare site at different viewing angles, establishing a two-ribbon flare geometry and occultation heights of the RHESSI and NoRH observations of similar to 16 Mm and similar to 25 Mm, respectively. Despite the occultation, intense hard X-ray emission up to similar to 80 keV occurs during the impulsive phase from a coronal source that is also seen in microwaves. The hard X-ray and microwave source during the impulsive phase is located similar to 6 Mm above thermal flare loops seen later at the soft X-ray peak time, similar in location to the above-the-loop-top source in the Masuda flare. A single non-thermal electron population with a power-law distribution (with spectral index of similar to 3.7 from similar to 16 keV up to the MeV range) radiating in both bremsstrahlung and gyrosynchrotron emission can explain the observed hard X-ray and microwave spectrum, respectively. This clearly establishes the non-thermal nature of the above-the-loop-top source. The large hard X-ray intensity requires a very large number (>5 x 10(35) above 16 keV for the derived upper limit of the ambient density of similar to 8 x 10(9) cm(-3)) of suprathermal electrons to be present in this above-the-loop-top source. This is of the same order of magnitude as the number of ambient thermal electrons. We show that collisional losses of these accelerated electrons would heat all ambient electrons to superhot temperatures (tens of keV) within seconds. Hence, the standard scenario, with hard X-rays produced by a beam comprising the tail of a dominant thermal core plasma, does not work. Instead, all electrons in the above-the-loop-top source seem to be accelerated, suggesting that the above-the-loop-top source is itself the electron acceleration region.</P>

ESTIMATES OF DENSITIES AND FILLING FACTORS FROM A COOLING TIME ANALYSIS OF SOLAR MICROFLARES OBSERVED WITH<i>RHESSI</i>

Baylor, R. N.,Cassak, P. A.,Christe, S.,Hannah, I. G.,Krucker, Sä,m,Mullan, D. J.,Shay, M. A.,Hudson, H. S.,Lin, R. P. IOP Publishing 2011 The Astrophysical journal Vol.736 No.1

<P>We usemore than 4500 microflares from the RHESSI microflare data set to estimate electron densities and volumetric filling factors of microflare loops using a cooling time analysis. We show that if the filling factor is assumed to be unity, the calculated conductive cooling times are much shorter than the observed flare decay times, which in turn are much shorter than the calculated radiative cooling times. This is likely unphysical, but the contradiction can be resolved by assuming that the radiative and conductive cooling times are comparable, which is valid when the flare loop temperature is a maximum and when external heating can be ignored. We find that resultant radiative and conductive cooling times are comparable to observed decay times, which has been used as an assumption in some previous studies. The inferred electron densities have a mean value of 10(11.6) cm(-3) and filling factors have a mean of 10(-3.7). The filling factors are lower and densities are higher than previous estimates for large flares, but are similar to those found for two microflares by Moore et al.</P>

X-Ray Study of Variable Gamma-Ray Pulsar PSR J2021+4026

Wang, H. H.,Takata, J.,Hu, C.-P.,Lin, L. C. C.,Zhao, J. American Astronomical Society 2018 The Astrophysical journal Vol.856 No.2

<P>PSR J2021+4026 showed a sudden decrease in the gamma-ray emission at the glitch that occurred around 2011 October 16, and a relaxation of the flux to the pre-glitch state at around 2014 December. We report X-ray analysis results of the data observed by XMM-Newton on 2015 December 20 in the post-relaxation state. To examine any change in the X-ray emission, we compare the properties of the pulse profiles and spectra at the low gamma-ray flux state and at the post-relaxation state. The phase-averaged spectra for both states can be well described by a power-law component plus a blackbody component. The former is dominated by unpulsed emission and probably originated from the pulsar wind nebula as reported by Hui et al. The emission property of the blackbody component is consistent with the emission from the polar cap heated by the back-flow bombardment of the high-energy electrons or positrons that were accelerated in the magnetosphere. We found no significant change in the X-ray emission properties between two states. We suggest that the change of the X-ray luminosity is at an order of similar to 4%, which is difficult to measure with the current observations. We model the observed X-ray light curve with the heated polar cap emission, and we speculate that the observed large pulsed fraction is owing to asymmetric magnetospheric structure.</P>

UPPER LIMITS ON THE NUMBER OF SMALL BODIES IN SEDNA-LIKE ORBITS BY THE TAOS PROJECT

Wang, J.-H.,Lehner, M. J.,Zhang, Z.-W.,Bianco, F. B.,Alcock, C.,Chen, W.-P.,Axelrod, T.,Byun, Y.-I.,Coehlo, N. ,K.,Cook, K. H.,Dave, R.,de Pater, I.,Porrata, R.,Kim, D.-W.,King, S.-K.,Lee, T.,Lin, American Institute of Physics 2009 The Astronomical journal Vol.138 No.6

<P>We present the results of a search for occultation events by objects at distances between 100 and 1000 AU in light curves from the Taiwanese-American Occultation Survey. We searched for consecutive, shallow flux reductions in the stellar light curves obtained by our survey between 2005 February 7 and 2006 December 31 with a total of ~4.5 × 10<SUP>9</SUP> three-telescope simultaneous photometric measurements. No events were detected, allowing us to set upper limits on the number density as a function of size and distance of objects in Sedna-like orbits, using simple models.</P>

DISCOVERY OF X-RAY PULSATIONS FROM THE NEXT GEMINGA, PSR J1836+5925

Lin, L. C. C.,Hui, C. Y.,Li, K. T.,Takata, J.,Hu, C. P.,Kong, A. K. H.,Yen, D. C. C.,Chou, Y. IOP Publishing 2014 ASTROPHYSICAL JOURNAL LETTERS - Vol.793 No.1

<P>We report recent XMM-Newton investigations of PSR J1836+5925, the 'next Geminga,' which determined an X-ray pulsation of similar to 173.3 ms. Its X-ray periodicity is consistent with the gamma-ray ephemeris at the same epoch. The X-ray folded light curve has a sinusoidal structure that is different from the double-peaked gamma-ray pulse profile. We have also analyzed the X-ray phase-averaged spectra which shows that the X-ray emission from PSR J1836+5925 is thermal dominant. This suggests that the X-ray pulsation mainly originates from the modulated hot spot on the stellar surface.</P>