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  1. Article

    Open Access

    Inner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission

    Mercury’s southern inner magnetosphere is an unexplored region as it was not observed by earlier space missions. In October 2021, BepiColombo mission has passed through this region during its first Mercury fly...

    S. Orsini, A. Milillo, H. Lichtenegger, A. Varsani, S. Barabash in Nature Communications (2022)

  2. Article

    Author Correction: The loss of ions from Venus through the plasma wake

    S. Barabash, A. Fedorov, J. J. Sauvaud, R. Lundin, C. T. Russell, Y. Futaana in Nature (2022)

  3. Article

    Correction to: SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo

    A Correction to this paper has been published: https://doi.org/10.1007/s11214-021-00809-8

    S. Orsini, S. A. Livi, H. Lichtenegger, S. Barabash, A. Milillo in Space Science Reviews (2021)

  4. Article

    Open Access

    SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo

    The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at M...

    S. Orsini, S. A. Livi, H. Lichtenegger, S. Barabash, A. Milillo in Space Science Reviews (2021)

  5. No Access

    Article

    A 2.488–11.2 Gb/s SerDes in 40 nm low-leakage CMOS with multi-protocol compatibility for FPGA applications

    This paper presents the design and Silicon verification of a 2.488–11.2 Gbps multi-standard SerDes transceiver in a 40 nm low-leakage CMOS process. The paper explores the architectural and circuit techniques u...

    Socrates D. Vamvakos, Claude R. Gauthier in Analog Integrated Circuits and Signal Proc… (2014)

  6. No Access

    Article

    Experimental Determination of the Ti-Nb-Al Phase Diagram At 1200°C.

    Studies consisting of both bulk sample and diffusion couple experiments have been conducted in order to establish an isothermal section of the Ti-Nb-Al system. Bulk samples were prepared by arc-melting and the...

    T. J. Jewett, J. C. Lin, N. R. Bonda, L. E. Seitzman in MRS Online Proceedings Library (2011)

  7. No Access

    Article

    Synthesis of Nitrogen-Rich GaNAs Semiconductor Alloys and Arsenic-Doped GaN by Metalorganic Chemical Vapor Deposition

    Arsenic-doped GaN films and GaNAs films have been synthesized by MOCVD. Samples were grown on sapphire, GaN-coated sapphire, and GaAs substrates. Composition, structure, and phase distribution were characteriz...

    M. Gherasimova, B. Gaffey, P. Mitev, L. J. Guido in MRS Online Proceedings Library (2011)

  8. No Access

    Article

    The loss of ions from Venus through the plasma wake

    ESA's Venus Express probe has been in orbit since April 2006. Eight research papers in this issue present new results from the mission, covering the atmosphere, polar features, interactions with the solar wind...

    S. Barabash, A. Fedorov, J. J. Sauvaud, R. Lundin, C. T. Russell, Y. Futaana in Nature (2007)

  9. No Access

    Article

    Poster abstracts

    J. Ferrie, M. Shipley, F. Cappuccio, E. Brunner, M. Miller in Sleep and Biological Rhythms (2007)

  10. No Access

    Article

    Phase Equilibria of the Sn-Ag-Cu-Ni Quaternary System at 210°C

    Sn-Ag-Cu alloys are the most promising Pb-free solders, and Ni is a common barrier layer material for the under-bump metallurgy. Although the Sn-Ag-Cu-Ni quaternary system is important for industry, no solid-p...

    S.-W. Chen, C.-N. Chiu, K.-C. Hsieh in Journal of Electronic Materials (2007)

  11. No Access

    Chapter

    The Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) for the Mars Express Mission

    The general scientific objective of the ASPERA-3 experiment is to study the solar wind — atmosphere interaction and to characterize the plasma and neutral gas environment within the space near Mars through the...

    S. Barabash, R. Lundin, H. Andersson, K. Brinkfeldt in The Mars Plasma Environment (2007)

  12. No Access

    Chapter

    Auroral Plasma Acceleration above Martian Magnetic Anomalies

    Aurora is caused by the precipitation of energetic particles into a planetary atmosphere, the light intensity being roughly proportional to the precipitating particle energy flux. From auroral research in the ...

    R. Lundin, D. Winningham, S. Barabash, R. Frahm, D. Brain in The Mars Plasma Environment (2007)

  13. No Access

    Chapter

    IMF Direction Derived from Cycloid-Like Ion Distributions Observed by Mars Express

    Although the Mars Express (MEX) does not carry a magnetometer, it is in principle possible to derive the interplanetary magnetic field (IMF) orientation from the three dimensional velocity distribution of pick...

    M. Yamauchi, Y. Futaana, A. Fedorov, E. Dubinin, R. Lundin in The Mars Plasma Environment (2007)

  14. No Access

    Article

    IMF Direction Derived from Cycloid-Like Ion Distributions Observed by Mars Express

    Although the Mars Express (MEX) does not carry a magnetometer, it is in principle possible to derive the interplanetary magnetic field (IMF) orientation from the three dimensional velocity distribution of pick...

    M. Yamauchi, Y. Futaana, A. Fedorov, E. Dubinin, R. Lundin in Space Science Reviews (2006)

  15. No Access

    Article

    Auroral Plasma Acceleration Above Martian Magnetic Anomalies

    Aurora is caused by the precipitation of energetic particles into a planetary atmosphere, the light intensity being roughly proportional to the precipitating particle energy flux. From auroral research in the ...

    R. Lundin, D. Winningham, S. Barabash, R. Frahm, D. Brain in Space Science Reviews (2006)

  16. No Access

    Article

    The Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) for the Mars Express Mission

    The general scientific objective of the ASPERA-3 experiment is to study the solar wind – atmosphere interaction and to characterize the plasma and neutral gas environment with within the space near Mars throug...

    S. Barabash, R. Lundin, H. Andersson, K. Brinkfeldt, A. Grigoriev in Space Science Reviews (2006)

  17. No Access

    Article

    An empirical comparison of GARCH option pricing models

    Recent empirical studies have shown that GARCH models can be successfully used to describe option prices. Pricing such contracts requires knowledge of the risk neutral cumulative return distribution. Since the...

    K. C. Hsieh, P. Ritchken in Review of Derivatives Research (2005)

  18. No Access

    Article

    The joint strength and microstructure of fluxless Au/Sn solders in InP-based laser diode packages

    The joint strength and microstructure of fluxless Au/Sn solders in InP-based laser-diode packages after thermal-aging testing were studied experimentally and numerically. Specimens were aged at 150°C for up to...

    M. T. Sheen, Y. H. Ho, C. L. Wang, K. C. Hsieh in Journal of Electronic Materials (2005)

  19. No Access

    Article

    Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

    The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the o...

    S. M. Krimigis, D. G. Mitchell, D. C. Hamilton, S. Livi in Space Science Reviews (2004)

  20. No Access

    Chapter

    Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

    The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the o...

    S. M. Krimigis, D. G. Mitchell, D. C. Hamilton, S. Livi in The Cassini-Huygens Mission (2004)

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