UV optical measurements of the Nozomi spacecraft interpreted with a two-component LIC-flow model (Corrigendum)

1 Department of Geophysics, University of Tohoku, 980-8577 Miyagi, Sendai, Japan e-mail: rom@pat.gp.tohoku.ac.jp 2 Space Research Centre PAS, Bartycka 18A, 00-716 Warsaw, Poland e-mail: bzowski@cbk.waw.pl 3 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 229-8510 Kanagawa, Sagamihara, Japan 4 Japan Society for the Promotion of Science, 100084 Beijing, PR China 5 Department of Earth and Planetary Science, University of Hokkaido, 001-0021 Hokkaido, Japan 6 Department of Physics, College of Science, Rikkyo University, 171-8501 Tokyo, Japan 7 Department of Earth and Planetary Science, University of Tokyo, 113-0033 Tokyo, Japan 8 Earth Observation Research Center, Japan Aerospace Exploration Agency, 305-8505 Ibaraki, Tsukuba, Japan

[1]  G. Gloeckler,et al.  Density of neutral interstellar hydrogen at the termination shock from Ulysses pickup ion observations , 2007, 0710.1480.

[2]  M. Ruderman,et al.  Modeling of the outer heliosphere with the realistic solar cycle , 2008 .

[3]  D. C. Hamilton,et al.  Voyager 1 in the Foreshock, Termination Shock, and Heliosheath , 2005, Science.

[4]  E. C. Stone,et al.  Voyager 1 Explores the Termination Shock Region and the Heliosheath Beyond , 2005, Science.

[5]  V. Jansen,et al.  Making Sense of Evolution in an Uncertain World , 2005, Science.

[6]  V. Izmodenov,et al.  Direction of the interstellar H atom inflow in the heliosphere : Role of the interstellar magnetic field , 2005 .

[7]  J. Bertaux,et al.  Deflection of the Interstellar Neutral Hydrogen Flow Across the Heliospheric Interface , 2005, Science.

[8]  M. Witte.  Kinetic parameters of interstellar neutral helium - Review of results obtained during one solar cycle with the Ulysses/GAS-instrument , 2004 .

[9]  J. Vallerga,et al.  EUVE observations of the helium glow: Interstellar and solar parameters , 2004 .

[10]  E. Möbius,et al.  Observations of the helium focusing cone with pickup ions , 2004 .

[11]  R. Kallenbach,et al.  Synopsis of the interstellar He parameters from combined neutral gas, pickup ion and UV scattering observations and related consequences , 2004 .

[12]  J. Geiss,et al.  Filtration of interstellar H, O, N atoms through the heliospheric interface: Inferences on local interstellar abundances of the elements , 2004 .

[13]  B. Tsurutani,et al.  An unexplained 10–40° shift in the location of some diverse neutral atom data at 1 AU , 2003, astro-ph/0304368.

[14]  J. Geiss,et al.  Effects of Interstellar and Solar Wind Ionized Helium on the Interaction of the Solar Wind with the Local Interstellar Medium , 2003, astro-ph/0308210.

[15]  E. Kyrölä,et al.  Latitudinal structure and north-south asymmetry of the solar wind from Lyman-alpha remote sensing by SWAN , 2003 .

[16]  E. Quémerais,et al.  Effects of the heliospheric interface on the interplanetary Lyman $\alpha$ glow seen at 1 AU from the Sun , 2002 .

[17]  J. Bertaux,et al.  14‐day forecast of solar indices using interplanetary Lyman α background data , 2002 .

[18]  V. Izmodenov.  Velocity Distribution of Interstellar H Atoms in the Heliospheric Interface , 2001 .

[19]  M. Bzowski.  Time dependent radiation pressure and time dependent, 2D ionisation rate for heliospheric modelling , 2001 .

[20]  Gary J. Rottman,et al.  The SOLAR2000 empirical solar irradiance model and forecast tool , 2000 .

[21]  J. Bertaux,et al.  Monitoring solar activity on the far side of the sun from sky reflected Lyman α radiation , 2000 .

[22]  Takuya D. Kawahara,et al.  Ultraviolet imaging spectrometer (UVS) experiment on board the NOZOMI spacecraft: Instrumentation and initial results , 2000 .

[23]  Eric Quémerais,et al.  Interplanetary Lyman α line profiles derived from SWAN/SOHO hydrogen cell measurements: Full‐sky Velocity Field , 1999 .

[24]  M. Taguchi,et al.  MARS ULTRAVIOLET IMAGING SPECTROMETER EXPERIMENT ON THE PLANET-B MISSION , 1999 .

[25]  I. Yoshikawa,et al.  Helium observation in the Martian ionosphere by an X-ray ultraviolet scanner on Mars orbiter NOZOMI , 1999 .

[26]  G. Gloeckler.  The abundance of atomic 1H, 4He and 3He in the local interstellar cloud from pickup ion observations with SWICS on Ulysses , 1996 .

[27]  R. Lallement,et al.  SWAN: A study of Solar Wind Anisotropies on SOHO with Lyman alpha sky mapping , 1995 .

[28]  G. Zank.  Interaction of the solar wind with the local interstellar medium: a theoretical perspective , 1995 .

[29]  D. Rucinski,et al.  Solar cycle dependence of the production of H+ pick-up ions in the inner heliosphere , 1995 .

[30]  V. Baranov,et al.  Model of the solar wind interaction with the local interstellar medium: Numerical solution of self‐consistent problem , 1993 .

[31]  D. Judge,et al.  Temperature and flow velocity of the interplanetary gases along solar radii , 1979 .

[32]  S. Bowyer,et al.  On the opacity of the interstellar medium to ultrasoft X-rays and extreme-ultraviolet radiation. , 1974 .