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1. Dietary phosphorus requirement of juvenile Chinese sucker, Myxocyprinus asiaticus

Author

S.Y. Gong, Hui-jun Yang, Zhi Luo, Yongchao Yuan, Deng-hang Yu, J.L. Yan, and X.F. Yang

Subjects
medicine.medical_specialty, Protein efficiency ratio, Phosphorus, chemistry.chemical_element, Aquatic Science, Biology, Mineralization (biology), chemistry.chemical_compound, Animal science, Endocrinology, chemistry, Blood chemistry, Internal medicine, medicine, Sucker, Phosphorus deficiency, medicine.symptom, Weight gain, Monocalcium phosphate
Abstract

A growth trial was conducted to estimate the optimum requirement of dietary available phosphorus (P) for Chinese sucker juveniles. Triplicate groups of juveniles Chinese sucker (initial mean weight: 1.77 ± 0.02 g, mean ± SD) were fed diets containing graded levels (3.1, 5.3, 7.5, 9.6 and 11.8 g kg⁻¹) of available phosphorus. The basal diet (diet 1), containing 3.1 g kg⁻¹ available P, was supplemented with graded levels of monocalcium phosphate to formulate four experimental diets. The fish were fed twice daily (08:00 and 17:00 h) to satiation for 8 weeks. During the experimental period, the water temperature fluctuated from 27.5 to 30.5 °C and dissolved oxygen was more than 6 mg L⁻¹. The specific growth rate, protein efficiency ratio were all significantly increased by dietary available phosphorus up to 7.5 g kg⁻¹ (P 0.05). Efficiency of phosphorus (P) utilization significantly decreased with dietary available phosphorus level (P 0.05). Dietary phosphorus levels also significantly affected the mineralization of vertebrae and scale (P < 0.05), and Ca/P ratios in scale were not influenced by dietary P supplementation, while vertebrae Ca/P ratio decreased with dietary available P levels (P < 0.05) (quadratic effect, P < 0.001). Signs of phosphorus deficiency were characterized by poor growth, slightly reduced mineralization and an increase in body lipid content. The blood chemistry analysis showed that dietary available P had distinct effects on enzyme activities of alkaline phosphatase, as well as contents of triacyglycerol and total cholesterol (P < 0.05). Broken-line analysis based on weight gain indicated the minimum available phosphorus requirement for the optimal growth of juvenile Chinese sucker was 7.4 g kg⁻¹. Based on the phosphorus content in whole body, vertebrae or scale indicated that the requirements were 8.3, 8.8 and 8.6 g kg⁻¹ respectively.

Published
2011
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2. Isothermal section of the Nd–Co–Ti ternary system at 500°C

Author

Xiangzhong Wei, C. Gao, J.L. Yan, S.L. Hu, Yinghong Zhuang, and Junqin Li

Subjects
Ternary numeral system, Materials science, Rietveld refinement, Mechanical Engineering, Metals and Alloys, Analytical chemistry, Crystal structure, Isothermal process, Tetragonal crystal system, chemistry.chemical_compound, chemistry, Mechanics of Materials, Ternary compound, X-ray crystallography, Materials Chemistry, Orthorhombic crystal system
Abstract

The isothermal section of the Nd–Co–Ti system at 500 °C has been investigated by means of XRD and SEM/EDS techniques. Compound Nd2Co3 was observed to exist at 500 °C with the orthorhombic La2Ni3-type structure, space group Cmca and unit cell parameters a = 0.4986(2) nm, b = 1.0000(2) nm, c = 0.7546(2) nm. One ternary compound NdTixCo12−x with the tetragonal ThMn12-type structure (space group I4/mmm) was found with a homogeneity range of 1.43 ≤ x ≤ 1.82, i.e. 11–14 at.% Ti. The structure of NdTi1.7Co10.3 was determined by Rietveld refinement method with the unit cell parameters a = 0.84616 (1) nm, c = 0.47447 (1) nm. The maximum solid solubilities of Ti in Nd2Co17, Nd2Co7, NdCo3, NdCo2, and Nd3Co are 6, 1.5, 2, 4 and 2 at.%, respectively.

Published
2010
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3. The isothermal section of the Nd–Fe–Ga ternary system at 773K

Author

Junqin Li, J.L. Yan, Wei Zhang, Weiqin Ao, Fuyuan Liu, and Y.J. Yu

Subjects
Ternary numeral system, Mechanical Engineering, Metals and Alloys, Space group, Crystal structure, Isothermal process, chemistry.chemical_compound, Crystallography, chemistry, Mechanics of Materials, Ternary compound, X-ray crystallography, Materials Chemistry, Ternary operation, Solid solution
Abstract

The isothermal section of the Nd–Fe–Ga ternary system at 773 K was constructed using X-ray diffraction analysis. Ten binary compounds, Nd2Fe17, Nd5Fe17, Nd9Ga4, Nd5Ga3, NdGa, NdGa2, FeGa3, Fe3Ga4, α-Fe6Ga5 and α-Fe3Ga, and three ternary compounds, NdFe2Ga8, NdFe5Ga7 and Nd6Fe13Ga were existed in this isothermal section. The solid solutions Nd2Fe17.00–15.57Ga0–1.43 (Th2Zn17-type structure, space group R 3 ¯ m ), NdFe5.46–4.65Ga6.54–7.35 (ThMn12-type structure, space group I4/mmm) and Nd6Fe13.0–12.0Ga1.0–2.0 (La6Co11Ga3-type structure, space group I4/mcm) were formed by substitution of Ga for Fe in the compounds Nd2Fe17, NdFe5Ga7 and Nd6Fe13Ga at 773 K, respectively. The ternary compound NdFe2Ga8 is CaCo2Al8-type (space group Pbam) with a = 1.43742 (4), b = 1.24601 (4), c = 0.40479 (1)). The homogeneity range of NdGa2 is from 66.7 to 74.7 at.% Ga in Nd–Ga side but the solid solubility of Fe in this compound is very small. The homogeneity ranges of Nd6Fe13Ga and NdFe5Ga7 are from 5.0 to 10.0 and from 50.3 to 56.5 at.% Ga, respectively. The maximum solid solubilities of Ga in Nd2Fe17 is 7.5. The homogeneity ranges for the other compounds are small.

Published
2009
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4. Isothermal section of the Dy–Co–Ti ternary system at 500°C

Author

Q. X. Long, J.L. Yan, D. X. Liu, J. Q. Li, Jinli Huang, and Yinghong Zhuang

Subjects
Ternary numeral system, Chemistry, Mechanical Engineering, Metals and Alloys, Analytical chemistry, Space group, chemistry.chemical_element, Isothermal process, Crystallography, Mechanics of Materials, Phase (matter), X-ray crystallography, Materials Chemistry, Dysprosium, Thermal analysis, Phase diagram
Abstract

The isothermal section of the Dy–Co–Ti system at 500 °C has been investigated in the whole composition range by means of X-ray diffraction, thermal analysis, scanning electron microscopy and energy dispersive X-ray spectroscopy. The only ternary phase DyTi x Co 12− x is of ThMn 12 -type structure, space group I 4/ mmm , and shows a small homogeneity range of 1 ≤ x ≤ 1.6. The lattice parameters for DyTi x Co 12− x with 1 ≤ x ≤ 1.56 are a = 0.8336(4)–0.8402(1) nm and c = 0.4691(3)–0.4727(1) nm. Along a constant Dy concentration, the solid solubilities of Ti in the compounds Dy 2 Co 17 , DyCo 3 , DyCo 2 and Dy 3 Co are about 2.0, 2.0, 3.0 and 4.0 at.%, respectively. The TiCo phase has a homogeneity range of 50–54 at.% Co at 500 °C and dissolves up to 2.0 at.% Dy.

Published
2009
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5. The isothermal section of Tb–Dy–Co ternary system at 773K and magnetic property of (Tb1−xDyx)Co2 alloys

Author

Yinghong Zhuang, J.L. Yan, F. Fei, and X. Chen

Subjects
Ternary numeral system, Mechanical Engineering, Metals and Alloys, Intermetallic, chemistry.chemical_compound, Crystallography, chemistry, Mechanics of Materials, Ternary compound, Differential thermal analysis, Materials Chemistry, Curie temperature, Powder diffraction, Phase diagram, Solid solution
Abstract

The isothermal section of the phase diagram of the Tb–Dy–Co ternary system at 773 K was investigated by X-ray powder diffraction (XRD), differential thermal analysis (DTA) and scanning electron microscope (SEM). The result shows that this section consists of 9 single-phase regions and 8 two-phase regions, and no three-phase region. The compounds Tb 2 Co 17 and Dy 2 Co 17 , Tb 2 Co 7 and Dy 2 Co 7 , TbCo 3 and DyCo 3 , TbCo 2 and DyCo 2 , Tb 4 Co 3 and Dy 4 Co 3 , Tb 12 Co 7 and Dy 12 Co 7 , Tb 3 Co and Dy 3 Co form a continuous series of solid solutions. The single phases Tb and Dy also form a continuous solid solution. The binary compounds TbCo 5 and DyCo 5 were not observed at 773 K. No ternary compound was found. In addition, we experimentally determined the vertical section of pseudobinary system and magnetic property of Tb 1− x Dy x Co 2 ( x from 0 to 1) series alloys, T c decreases and the maximum magnetic entropy change |Δ S M ,max | increases with the increase of Dy content. The Arrott plots and the change of |Δ S M ,max | show that magnetic phase transition from second-order to first-order occurs with the increase of Dy content between x = 0.6 and 0.8.

Published
2009
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6. The isothermal section phase diagram of the La–Fe–Ge ternary system at 773K

Author

Yinghong Zhuang, K.F. Li, X. Chen, C.H. Ma, and J.L. Yan

Subjects
Ternary numeral system, Chemistry, Mechanical Engineering, Metals and Alloys, Isothermal process, Crystallography, Mechanics of Materials, Differential thermal analysis, X-ray crystallography, Materials Chemistry, Ternary operation, Powder diffraction, Phase diagram, Solid solution
Abstract

The isothermal section of the phase diagram of the La–Fe–Ge ternary system at 773 K was investigated by X-ray powder diffraction (XRD), differential thermal analysis (DTA) and optical microscopy. The existences of 12 binary compounds, La 3 Ge, La 5 Ge 3 , La 4 Ge 3 , La 5 Ge 4 , LaGe, La 2 Ge 3 , LaGe 2− x , Fe 3 Ge, Fe 5 Ge 3 , Fe 6 Ge 5 , FeGe, FeGe 2 , were confirmed. Three ternary compounds LaFe 2 Ge 2 , LaFe 0.6 Ge 2 and LaFeGe 3 were confirmed too. Ge in Fe, LaGe, LaGe 2− x and Fe 5 Ge 3 and Fe in LaFe 0.6 Ge 2 have solid solution phenomenon. This section consists of 18 single-phase regions, 37 two-phase regions, and 20 three-phase regions.

Published
2008
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7. Intermetallics and phase transformations of the Zr-1.0Sn-0.3Nb-0.3Fe-0.1Cr alloy

Author

Jianlie Liang, Yinghong Zhuang, Yiyuan Tang, J.L. Yan, and Liangqin Nong

Subjects
Diffraction, Zirconium, Materials science, Metallurgy, Alloy, Metals and Alloys, Analytical chemistry, Intermetallic, chemistry.chemical_element, engineering.material, Condensed Matter Physics, Differential scanning calorimetry, chemistry, Phase (matter), Martensite, X-ray crystallography, Materials Chemistry, engineering, Physical and Theoretical Chemistry
Abstract

Intermetallics and phase transformations of the zirconium-based alloy, Zr-1.0Sn-0.3Nb-0.3Fe-0.1Cr, were investigated by conventional X-ray diffraction (XRD), differential scanning calorimetry (DSC), and dilation measurement. Three types of precipitates, namely, (ZrNb)2Fe, Zr(CrFe)2, and Zr3Fe, were detected by XRD. The cubic Ti2Ni-type (ZrNb)2Fe was found to be the main precipitate in the alloy, and it was proposed to dissolve at 861°C, whereas Zr3Fe dissolved at 780°C and Zr(CrFe)2 at 814°C. No precipitates were observed at a temperature higher than 900°C. The transformation-start temperature of α-Zr → β-Zr was reconfirmed to be 780°C, and the end temperature of α-Zr → β-Zr was determined to be 955°C. The dilation result also revealed that the martensitic transformation-start temperature, Ms, and the finish temperature, Mf, of this alloy were 741°C and 645°C, respectively.

Published
2008
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8. A model for precipitation kinetics and strengthening in Al–Cu–Mg alloys

Author

I.N. Khan, J.L. Yan, and Marco J. Starink

Subjects
Materials science, Precipitation (chemistry), Mechanical Engineering, Metallurgy, chemistry.chemical_element, Modulus, Condensed Matter Physics, Microstructure, Isothermal process, Precipitation hardening, chemistry, Mechanics of Materials, Aluminium, Phase (matter), General Materials Science, Dislocation
Abstract

A physically based numerical model is developed to predict the microstructural evolution and strengthening in Al–Cu–Mg alloys during isothermal treatments. The modelling of the formation kinetics of the precipitates is based on the Kampmann and Wagner model. The strengthening by the shearable Cu:Mg co-clusters is modelled on the basis of modulus strengthening mechanism and the strengthening by the non-shearable S phase precipitates is based on the Orowan looping mechanism. The model predictions are verified by comparing with the strength and differential isothermal calorimetery data on 2024-T351 aluminium alloys. The microstructural development and strength predictions of the model are generally in good agreement with the experimental data.

Published
2008
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9. ChemInform Abstract: Structural and Magnetic Properties of DyCo5-xGaxCompounds

Author

Jianqiang Li, Wenjing Zhang, F.S. Liu, Weiqin Ao, and J.L. Yan

Subjects
Diffraction, Magnetization, Hexagonal crystal system, Chemistry, Lattice (order), Cell volume, Analytical chemistry, Curie temperature, General Medicine, Anisotropy, Spin (physics)
Abstract

The structural and magnetic properties of DyCo 5− x Ga x compounds with x = 0.55, 0.85, 1.15, 1.45 and 1.75, have been investigated by X-ray diffraction and magnetic measurements. Powder X-ray diffraction analysis revealed that the DyCo 5− x Ga x samples are stabilized in single phase with a hexagonal CaCu 5 -type structure (space group P 6/ mmm ) for 0.55 ≤ x ≤ 1.45. The substitution of Co by Ga in this compound increases its lattice parameters a , c and cell volume V but decreases the 3d-sublattice moment and the 3d uniaxial anisotropy. As result, the compensation temperature T comp increases from 199 K (for the sample with x = 0.55) to 260 K (for the sample with x = 1.45). Two spin reorientation transitions, at T SR1 = 460 and T SR2 = 725 K, respectively, for the sample with x = 0.55, only one at T SR3 = 466 K for the sample with x = 0.85 while none for the samples with x = 1.15 or less were found. The Curie temperature decreases with increasing Ga content. The total magnetization for the compound increases at low temperature (e.g. 100 K) but decreases at high temperature with increasing Ga content (e.g. 300 K).

Published
2010
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10. ChemInform Abstract: Isothermal Section of the Dy-Co-Ti Ternary System at 500 °C

Author

Jinli Huang, Q. X. Long, J. Q. Li, J.L. Yan, D. X. Liu, and Yinghong Zhuang

Subjects
Diffraction, Ternary numeral system, Scanning electron microscope, Chemistry, Phase (matter), Homogeneity (physics), Analytical chemistry, General Medicine, Thermal analysis, Spectroscopy, Isothermal process
Abstract

The isothermal section of the Dy–Co–Ti system at 500 °C has been investigated in the whole composition range by means of X-ray diffraction, thermal analysis, scanning electron microscopy and energy dispersive X-ray spectroscopy. The only ternary phase DyTi x Co 12− x is of ThMn 12 -type structure, space group I 4/ mmm , and shows a small homogeneity range of 1 ≤ x ≤ 1.6. The lattice parameters for DyTi x Co 12− x with 1 ≤ x ≤ 1.56 are a = 0.8336(4)–0.8402(1) nm and c = 0.4691(3)–0.4727(1) nm. Along a constant Dy concentration, the solid solubilities of Ti in the compounds Dy 2 Co 17 , DyCo 3 , DyCo 2 and Dy 3 Co are about 2.0, 2.0, 3.0 and 4.0 at.%, respectively. The TiCo phase has a homogeneity range of 50–54 at.% Co at 500 °C and dissolves up to 2.0 at.% Dy.

Published
2009
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11. The Alpha Magnetic Spectrometer (AMS) on the International Space Station: Part I – results from the test flight on the space shuttle

Author

P. Extermann, H. Hofer, J.P. Richeux, Jose Maria Kenny, M. Jongmanns, H. Anderhub, P. Giusti, A. Hasan, Mauro Menichelli, G. Scolieri, Y.S. Lu, I. Lopes, S. Ro, G. Schwering, Eun-Suk Seo, L. Baldini, E. Lanciotti, F. Vezzu, Maria Ionica, S.W. Ye, V. Koutsenko, Eino Valtonen, M.Y. Kim, G. Sartorelli, D. Rapin, V. Plyaskin, Werner Lustermann, Behcet Alpat, W.Q. Gu, W.Z. Zhu, C. Delgado, E. Fiandrini, Yu. Galaktionov, D.H. Kim, J. Alcaraz, S. X. Wu, W.H. Park, Felicitas Pauss, B. Verlaat, P. Berges, K. Karlamaa, S.C.C. Ting, F. Palmonari, Zhenghao Xu, Zhuoxiang Ren, F. Velcea, Tzihong Chiueh, G. Barbier, H.B. Park, R. Kossakowski, A. Klimentov, S. Urpo, Ari Mujunen, A. Lebedev, Dong-Chul Son, G. Laurenti, K. Luebelsmeyer, E. Shoumilov, W. Hungerford, H. S. Chen, N. Produit, M. Buenerd, S. Waldmeier Wicki, M. Basile, E. Riihonen, A. Mihul, Timo Laitinen, J. Yang, V. Postolache, V. Pojidaev, M. Steuer, P.C. Xia, G.S. Sun, Jian Wang, M. Ribordy, K. Hangarter, H. L. Zhuang, M. Pauluzzi, Stefan Schael, H. Suter, Guohuai Zhu, G. Boella, X.W. Tang, M. Kraber, A. Pevsner, M. A. Huang, Mao-Zhi Yang, Tao Song, J.L. Yan, N.A. Chernoplekov, J. Vandenhirtz, Z.G. Chen, C. Camps, Ciaran Williams, D. Ren, D. Luckey, I. Vetlitsky, Samuel C.C. Ting, N. Dinu, Zhidong Zhang, Anselmo Margotti, E. Cortina-Gil, M. Bourquin, A. Papi, Adrian Biland, R. Ionica, L. Djambazov, Paolo Zuccon, A. Contin, I. D'Antone, M.W. Lee, Jungwook Shin, F. Barao, G. Castellini, J. P. Da Cunha, Gui Nyun Kim, N. Fouque, P. Levtchenko, Massimo Gervasi, Kyung-Suk Cho, J. D. Burger, F. Mayet, M. Pohl, P. Yeh, G. Lu, C. Maña, C. Lechanoine-Leluc, A. Schultz von Dratzig, C. Rossin, Hengchang Liu, A. Mourao, S. Blasko, G. Laborie, C. Sbarra, Peter H. Fisher, L.G. Yan, V. Hermel, J.D. Deus, X. D. Cai, M.J. Choi, O. Grimm, J. Casaus, M. Capell, Philipp Azzarello, R. Siedling, J. Berdugo, Yun Wang, A. Arefiev, Roald Z. Sagdeev, J. Engelberg, H. von Gunten, C.L. Liu, L. Bellagamba, Changgen Yang, D. Casadei, U. Roser, R. R. McNeil, B. Meillon, Giuseppe Levi, Y.L. Chuang, K. Wiik, P. Bene, Federico Cindolo, J. J. Torsti, Antonino Zichichi, L. Brocco, J. Ritakari, Y. H. Chang, G. Kenney, P. Cannarsa, Y.Y. Choi, D. Barancourt, J. Favier, Waclaw Karpinski, E. Babucci, U. Becker, Dawei Zhao, R. Becker, Z.R. Dong, E. Perrin, K.S. Kim, Claudia Cecchi, F. J. Eppling, M. Aguilar, V. Shoutko, S. Bizzaglia, G. Esposito, M. Pimenta, G. Fluegge, D. Grandi, B. Bertucci, D. Santos, G. Ambrosi, T. S. Dai, A. Pesci, B.C. Wang, D. Vité, G. Lamanna, G. Viertel, J. P. Vialle, H.F. Chen, G.P. Barreira, W. J. Burger, Frank Raupach, Roberto Battiston, L. Ao, J. Ulbricht, Hao Zhang, S.C. Lee, J. Trümper, P. Emonet, M. J. Boschini, V. Commichau, E. P. Velikhov, B. Zimmermann, Merja Tornikoski, Markus Cristinziani, T. Eronen, P. G. Rancoita, W. Wallraff, G. Bruni, Aguilar, M, Alcaraz, J, Allaby, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Boschini, M, Bourquin, M, Brocco, L, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cecchi, C, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Cho, K, Choi, M, Choi, Y, Chuang, Y, Cindolo, F, Commichau, V, Contin, A, Cortina-Gil, E, Cristinziani, M, da Cunha, J, Dai, T, Delgado, C, Deus, J, Dinu, N, Djambazov, L, D'Antone, I, Dong, Z, Emonet, P, Engelberg, J, Eppling, F, Eronen, T, Esposito, G, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Grandi, D, Grimms, O, Gu, W, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, M, Hungerford, W, Ionica, M, Ionica, R, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kenny, J, Kim, D, Kim, G, Kim, K, Kim, M, Klimentov, A, Kossakowski, R, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Lanciotti, E, Laurenti, G, Lebedev, A, Lechanoine-Leluc, C, Lee, M, Lee, S, Levi, G, Levtchenko, P, Liu, C, Liu, H, Lopes, I, Lu, G, Lu, Y, Lubelsmeyer, K, Luckey, D, Lustermann, W, Mana, C, Margotti, A, Mayet, F, Mcneil, R, Meillon, B, Menichelli, M, Mihul, A, Mourao, A, Mujunen, A, Palmonari, F, Papi, A, Park, H, Park, W, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pimenta, M, Plyaskin, V, Pojidaev, V, Pohl, M, Postolache, V, Produit, N, Rancoita, P, Rapin, D, Raupach, F, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Ro, S, Roeser, U, Rossin, C, Sagdeev, R, Santos, D, Sartorelli, G, Sbarra, C, Schael, S, von Dratzig, A, Schwering, G, Scolieri, G, Seo, E, Shin, J, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, G, Suter, H, Tang, X, Ting, S, Tornikoski, M, Torsti, J, Trumper, J, Ulbricht, J, Urpo, S, Valtonen, E, Vandenhirtz, J, Velcea, F, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, V, Jp, Viertel, G, Vite, D, Von Gunten, H, Wicki, S, Wallraff, W, Wang, B, Wang, J, Wang, Y, Wiik, K, Williams, C, Wu, S, Xia, P, Yan, J, Yan, L, Yang, C, Yang, J, Yang, M, Ye, S, Yeh, P, Xu, Z, Zhang, H, Zhang, Z, Zhao, D, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Zimmermann, B, Zuccon, P, Ambrosi, Giovanni, Azzarello, Philipp, Bene, Pierre, Bourquin, Maurice, Cortina Gil, Eduardo, Cristinziani, Markus, Emonet, Pascal Philippe, Extermann, Pierre, Leluc, Catherine, Perrin, Eric, Pohl, Martin, Produit, Nicolas, Rapin, Divic Jean, Ribordy, Mathieu, Richeux, Jean-Pierre, Vite, Davide, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), AMS, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, CIEMAT, E-28040, Madrid, Spain, and UCL - SST/IRMP - Institut de recherche en mathématique et physique

Subjects
Physics, 010308 nuclear & particles physics, FIS/06 - FISICA PER IL SISTEMA TERRA E PER IL MEZZO CIRCUMTERRESTRE, General Physics and Astronomy, chemistry.chemical_element, Electron, ddc:500.2, 01 natural sciences, Spectral line, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Nuclear physics, FIS/05 - ASTRONOMIA E ASTROFISICA, Positron, Earth's magnetic field, FIS/01 - FISICA SPERIMENTALE, chemistry, 13. Climate action, Antiproton, 0103 physical sciences, Alpha Magnetic Spectrometer, Nucleon, 010303 astronomy & astrophysics, AMS, Cosmic Rays, Antimatter, Helium, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
Abstract

The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7 deg orbit at altitudes between 320 and 390 km. A search for antihelium nuclei in the rigidity range 1–140 GV was performed. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1×10^−6 was obtained. The high energy proton, electron, positron, helium, antiproton and deuterium spectra were accurately measured. For each particle and nuclei two distinct spectra were observed: a higher energy spectrum and a substantial second spectrum. Positrons in the second spectrum were found to be much more abundant than electrons. Tracing particles from the second spectra shows that most of them travel for an extended period of time in the geomagnetic field, and that the positive particles (p and e+) and negative ones (e−) originate from two complementary geographic regions. The second helium spectrum flux over the energy range 0.1–1.2 GeV/nucleon was measured to be (6.3 ± 0.9) × 10^−3(m^2 s sr)^−1. Over 90 percent of the helium flux was determined to be 3He at the 90% confidence level

Published
2002
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12. Search for antihelium in cosmic rays

Author

Z.R. Dong, S. Bizzaglia, G. Ambrosi, J. Casaus, M. Pimenta, T. S. Dai, Samuel C.C. Ting, L. Djambazov, B.C. Wang, G. Molinari, A. Klimentov, B. Bertucci, S. X. Wu, R. Pilastrini, G. Lamanna, L.G. Yan, R. Siedling, J. Favier, Philipp Azzarello, J. J. Torsti, Antonino Zichichi, A. Hasan, Mauro Menichelli, L. Ao, Inkyu Park, J.P. Vialle, M. Steuer, P.C. Xia, Peter H. Fisher, Ilya Usoskin, P. G. Rancoita, Jing Wang, F. Palmonari, J. Isbert, M. Ribordy, G. Boella, H. von Gunten, P. Crespo, W. J. Burger, N. Fouque, R. Ionica, Federico Cindolo, J.P. Richeux, R. Cavalletti, D.X. Zhao, U. Roeser, N.A. Chernoplekov, C. G. Yang, Nicolas Produit, M. Buenerd, A. Cotta-Ramusino, R. Flaminio, J. P. Da Cunha, Anselmo Margotti, D. Rapin, V. Plyaskin, W. Kim, Roberto Battiston, G.Y. Zhu, W.Z. Zhu, G. Fluegge, G. Bruni, G. Viertel, P. Levtchenko, E. Fiandrini, G. Laurenti, K. Luebelsmeyer, S. Waldmeier Wicki, S.C. Lee, Yu. Galaktionov, F. Massera, D. Vité, J. Ulbricht, A. Chiarini, Hao Zhang, H. S. Chen, C. Rossin, G. Pancaldi, Felicitas Pauss, S. Recupero, Ciaran Williams, R. Kossakowski, W. Karpinski, J. Alcaraz, F. Barao, P. Yeh, E. Emonet, L.K. Ding, H.T. Liu, E. P. Velikhov, G. Torromeo, M. Basile, G.S. Sun, A. Pevsner, J.L. Yan, X. D. Cai, L. Baldini, F. Mezzanotte, C.L. Liu, L. Bellagamba, S. Blasko, K. Hangarter, J. Berdugo, Adrian Biland, G. Barbier, J. Vandenhirtz, V. Hermel, A. Arefiev, E. Prati, Jose Maria Kenny, R. R. McNeil, T.G. Guzik, B. Meillon, W.K. Gu, G. Kenney, I. D'Antone, J.P. Wefel, Markus Cristinziani, T. Eronen, R. Becker, Y.L. Chuang, P. Bene, B. Alpat, D. Luckey, E. Riihonen, A. Mihul, M. Jongmanns, C.C. Feng, D. Casadei, W. Wallraff, J. Krieger, H.L. Zhuang, G. Castellini, Massimo Gervasi, Zhuoxiang Ren, G. Schwering, W. Hungerford, A. Papi, Timo Laitinen, D. Santos, F. Tenbusch, B. Verlaat, P. Berges, Raffaele Mezzenga, S. Urpo, Ari Mujunen, G. Laborie, V. Shoutko, M. Pauluzzi, Y. S. Lu, G.P. Barreira, Yun Wang, V. Commichau, J. Truemper, A. Pesci, D. Ren, M. Capell, V. Koutsenko, Eino Valtonen, F. Vezzu, P. Cannarsa, C. Camps, T.P. Li, M. Ionica, H. Postema, A. Contin, M. Yang, E. Babucci, U. Becker, A. Lebedev, Dong-Chul Son, P. Giusti, I. Lopes, E. Perrin, F. J. Eppling, D. Alvisi, G. Lu, F. Raupach, C. Maña, P. Extermann, S. M. Ting, H. Hofer, G. Esposito, I. Vetlitsky, G. Sartorelli, M. Lolli, G. Maehlum, E.A. Werner, Fabio Finelli, Z.G. Chen, Werner Lustermann, Giuseppe Levi, X. W. Tang, Tao Song, M. Bourquin, V. Pojidaev, E. Shoumilov, H. Suter, J. D. Burger, Roald Z. Sagdeev, A. Mourao, J. Ritakari, Y. H. Chang, D. Barancourt, N. Dinu, H. Anderhub, Tzihong Chiueh, M. A. Huang, Jorge Dias de Deus, F. Mayet, A. Schultz von Dratzig, Alcaraz, J, Alvisi, D, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Barancourt, D, Barao, F, Barbier, G, Barreira, G, Battiston, R, Becker, R, Becker, U, Bellagamba, L, Béné, P, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Bourquin, M, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Cavalletti, R, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiarini, A, Chiueh, T, Chuang, Y, Cindolo, F, Commichau, V, Contin, A, Cotta Ramusino, A, Crespo, P, Cristinziani, M, Dacunha, J, Dai, T, Deus, J, Ding, L, Dinu, N, Djambazov, L, D'Antone, I, Dong, Z, Emonet, P, Eppling, F, Eronen, T, Esposito, G, Extermann, P, Favier, J, Feng, C, Fiandrini, E, Finelli, F, Fisher, P, Flaminio, R, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Gu, W, Guzik, T, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, M, Hungerford, W, Ionica, M, Ionica, R, Isbert, J, Jongmanns, M, Karpinski, W, Kenney, G, Kenny, J, Kim, W, Klimentov, A, Krieger, J, Kossakowski, R, Koutsenko, V, Laborie, G, Laitinen, T, Lamanna, G, Laurenti, G, Lebedev, A, Lee, S, Levi, G, Levtchenko, P, Li, T, Liu, C, Liu, H, Lolli, M, Lopes, I, Lu, G, Lu, Y, Lübelsmeyer, K, Luckey, D, Lustermann, W, Maehlum, G, Maña, C, Margotti, A, Massera, F, Mayet, F, Mcneil, R, Meillon, B, Menichelli, M, Mezzanotte, F, Mezzenga, R, Mihul, A, Molinari, G, Mourao, A, Mujunen, A, Palmonari, F, Pancaldi, G, Papi, A, Park, I, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pilastrini, R, Pimenta, M, Plyaskin, V, Pojidaev, V, Postema, H, Prati, E, Produit, N, Rancoita, P, Rapin, D, Raupach, F, Recupero, S, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Roeser, U, Roissin, C, Sagdeev, R, Santos, D, Sartorelli, G, Schultzvondratzig, A, Schwering, G, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, G, Suter, H, Tang, X, Ting, S, Tenbusch, F, Torromeo, G, Torsti, J, Trümper, J, Ulbricht, J, Urpo, S, Usoskin, I, Valtonen, E, Vandenhirtz, J, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, Vialle, J, Viertel, G, Vité, D, Vongunten, H, Waldmeierwicki, S, Wallraff, W, Wang, B, Wang, J, Wang, Y, Wefel, J, Werner, E, Williams, C, Wu, S, Xia, P, Yan, J, Yan, L, Yang, C, Yang, M, Yeh, P, Zhang, H, Zhao, D, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), and AMS

Subjects
Astrophysics and Astronomy, Nuclear and High Energy Physics, FOS: Physical sciences, chemistry.chemical_element, Space Shuttle, Cosmic ray, Astrophysics, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], High Energy Physics - Experiment (hep-ex), FIS/05 - ASTRONOMIA E ASTROFISICA, Rigidity (electromagnetism), 0103 physical sciences, Alpha Magnetic Spectrometer, 010306 general physics, Helium, Physics, 010308 nuclear & particles physics, Astrophysics (astro-ph), Astronomy, Flux ratio, FIS/01 - FISICA SPERIMENTALE, chemistry, Cosmic rays: anti-helium, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
Abstract

The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 in a 51.7 degree orbit at altitudes between 320 and 390 km. A total of 2.86 * 10^6 helium nuclei were observed in the rigidity range 1 to 140 GV. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1 * 10^-6 is obtained., 18 pages, Latex, 9 .eps figures

Published
2000

13. Helium in near earth orbit

Author

D. Vité, Peter H. Fisher, Yu. Galaktionov, J. Alcaraz, Roald Z. Sagdeev, D.X. Zhao, K. Karlamaa, A. Arefiev, S.W. Ye, E. Riihonen, W. Hungerford, M. A. Huang, R. R. McNeil, B. Meillon, V. Shoutko, G. Kenney, J. Ritakari, Y. H. Chang, J. Engelberg, C. Camps, G. Sartorelli, D. Barancourt, A. Mihul, Timo Laitinen, R. Ionica, Jorge Dias de Deus, W. Kim, H. von Gunten, P. G. Rancoita, V. Postolache, M. Pauluzzi, G. Lu, C. Maña, Werner Lustermann, Federico Cindolo, F. Mayet, G. Fluegge, Mao-Zhi Yang, D. Ren, A. Schultz von Dratzig, G. Barbier, W.Z. Zhu, W. J. Burger, A. Papi, J. Casaus, U. Roeser, M. Ribordy, G. Ambrosi, Y.L. Chuang, A. Contin, P. Levtchenko, M. Buenerd, X.W. Tang, M. Pimenta, W. Wallraff, T. S. Dai, F. Vezzu, B. Verlaat, Maria Ionica, G.S. Sun, Samuel C.C. Ting, Frank Raupach, E. Shoumilov, P. Berges, B.C. Wang, S. Urpo, Ari Mujunen, G. Bruni, H. Suter, P. Bene, Hengchang Liu, D. Rapin, C. Roissin, V. Plyaskin, G. Laurenti, S. Waldmeier Wicki, D. Grandi, A. Pevsner, Z. L. Ren, F. Velcea, Tao Song, G. Lamanna, M. J. Boschini, B. Bertucci, J. J. Torsti, Antonino Zichichi, Waclaw Karpinski, J. Berdugo, H. Anderhub, V. Commichau, R. Becker, Roberto Battiston, B. Alpat, N. Fouque, J.P. Richeux, Zhenghao Xu, M. Bourquin, A. Lebedev, Dong-Chul Son, E. Fiandrini, F. Palmonari, Yun Wang, G. Boella, P. Yeh, J.L. Yan, H.F. Chen, L. Brocco, Felicitas Pauss, L. Baldini, A. Pesci, H. S. Chen, J. Ulbricht, K. Wiik, R. Kossakowski, N.A. Chernoplekov, Nicolas Produit, K. Lübelsmeyer, S. X. Wu, M. Basile, P. Cannarsa, Hao Zhang, S. Blasko, M. Jongmanns, G. Castellini, E. P. Velikhov, B. Zimmermann, G.P. Barreira, K. Hangarter, H. L. Zhuang, Anselmo Margotti, Tzihong Chiueh, J. P. Da Cunha, Y.S. Lu, Inkyu Park, J.P. Vialle, Ciaran Williams, A. Klimentov, G. Laborie, L. Ao, M. Pohl, N. Dinu, Merja Tornikoski, Markus Cristinziani, M. Steuer, P.C. Xia, G. Viertel, D. Luckey, Jose Maria Kenny, J. Trümper, L. Djambazov, Paolo Zuccon, O. Grimm, T. Eronen, E. Babucci, U. Becker, I. Vetlitsky, S.C. Lee, Eun-Suk Seo, E. Perrin, M. Kraeber, F. J. Eppling, S. M. Ting, Changgen Yang, V. Koutsenko, Eino Valtonen, P. Giusti, Adrian Biland, G. Scolieri, G. Esposito, Z.R. Dong, Claudia Cecchi, Philipp Azzarello, I. Lopes, Massimo Gervasi, P. Emonet, S. Bizzaglia, Z.G. Chen, J. Favier, M. Capell, R. Siedling, X. D. Cai, C.L. Liu, L. Bellagamba, L.G. Yan, Ilya Usoskin, Jing Wang, J. Vandenhirtz, A. Hasan, Mauro Menichelli, G. Schwering, P. Extermann, W.Q. Gu, H. Hofer, F. Barao, V. Hermel, Zhidong Zhang, D. Casadei, I. D'Antone, Guohuai Zhu, J. D. Burger, A. Mourao, V. Pojidaev, Giuseppe Levi, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), AMS, Alcaraz, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Barancourt, D, Barao, F, Barbier, G, Barreira, G, Battiston, R, Becker, R, Becker, U, Bellagamba, L, Béné, P, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Boschini, M, Bourquin, M, Brocco, L, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cecchi, C, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Chuang, Y, Cindolo, F, Commichau, V, Contin, A, Cristinziani, M, Cunha, J, Dai, T, Deus, J, Dinu, N, Djambazov, L, D'Antone, I, Dong, Z, Emonet, P, Engelberg, J, Eppling, F, Eronen, T, Esposito, G, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Grandi, D, Grimm, O, Gu, W, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, M, Hungerford, W, Ionica, M, Ionica, R, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kenny, J, Kim, W, Klimentov, A, Kossakowski, R, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Laurenti, G, Lebedev, A, Lee, S, Levi, G, Levtchenko, P, Liu, C, Liu, H, Lopes, I, Lu, G, Lu, Y, Lübelsmeyer, K, Luckey, D, Lustermann, W, Maña, C, Margotti, A, Mayet, F, Mcneil, R, Meillon, B, Menichelli, M, Mihul, A, Mourao, A, Mujunen, A, Palmonari, F, Papi, A, Park, I, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pimenta, M, Plyaskin, V, Pojidaev, V, Pohl, M, Postolache, V, Produit, N, Rancoita, P, Rapin, D, Raupach, F, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Roeser, U, Roissin, C, Sagdeev, R, Sartorelli, G, Schultz&nbsp, von&nbsp, Dratzig, A, Schwering, G, Scolieri, G, Seo, E, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, G, Suter, H, Tang, X, Ting, S, Tornikoski, M, Torsti, J, Trümper, J, Ulbricht, J, Urpo, S, Usoskin, I, Valtonen, E, Vandenhirtz, J, Velcea, F, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, Vialle, J, Viertel, G, Vité, D, Gunten, H, Wicki, S, Wallraff, W, Wang, B, Wang, J, Wang, Y, Wiik, K, Williams, C, Wu, S, Xia, P, Yan, J, Yan, L, Yang, C, Yang, M, Ye, S, Yeh, P, Xu, Z, Zhang, H, Zhang, Z, Zhao, D, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Zimmermann, B, Zuccon, P, Ambrosi, Giovanni, Azzarello, Philipp, Bene, Pierre, Bourquin, Maurice, Cristinziani, Markus, Emonet, Pascal Philippe, Extermann, Pierre, Perrin, Eric, Pohl, Martin, Produit, Nicolas, Rapin, Divic Jean, Ribordy, Mathieu, Richeux, Jean-Pierre, and Vite, Davide

Subjects
Physics, Nuclear and High Energy Physics, Earth's orbit, Range (particle radiation), 010308 nuclear & particles physics, chemistry.chemical_element, Flux, ddc:500.2, 01 natural sciences, Spectral line, Nuclear physics, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], FIS/05 - ASTRONOMIA E ASTROFISICA, FIS/01 - FISICA SPERIMENTALE, Earth's magnetic field, chemistry, 0103 physical sciences, Alpha Magnetic Spectrometer, Atomic physics, Cosmic rays: helium, Nuclear Experiment, Nucleon, 010303 astronomy & astrophysics, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE, Helium
Abstract

The helium spectrum from 0.1 to 100 GeV/nucleon was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-91 at altitudes near 380 km. Above the geomagnetic cutoff the spectrum is parameterized by a power law. Below the geomagnetic cutoff a second helium spectrum was observed. In the second helium spectra over the energy range 0.1 to 1.2 GeV/nucleon the flux was measured to be (6.3±0.9)×10 −3 ( m 2 sec sr ) −1 and more than ninety percent of the helium was determined to be 3He (at the 90% CL). Tracing helium from the second spectrum shows that about half of the 3He travel for an extended period of time in the geomagnetic field and that they originate from restricted geographic regions similar to protons and positrons.

Published
2000

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