Neutral interstellar He parameters in front of the heliosphere 1994--2007
arXiv:1405.0623 · doi:10.1051/0004-6361/201424127
Abstract
Analysis of IBEX measurements of neutral interstellar He flux brought the inflow velocity vector different from the results of earlier analysis of observations from GAS/Ulysses. Recapitulation of results on the helium inflow direction from the past ~40 years suggested that the inflow direction may be changing with time. We reanalyze the old Ulysses data and reprocess them to increase the accuracy of the instrument pointing to investigate if the GAS observations support the hypothesis that the interstellar helium inflow direction is changing. We employ a similar analysis method as in the analysis of the IBEX data. We seek a parameter set that minimizes reduced chi-squared, using the Warsaw Test Particle Model for the interstellar He flux at Ulysses with a state of the art model of neutral He ionization in the heliosphere, and precisely reproducing the observation conditions. We also propose a supplementary method of constraining the parameters based on cross-correlations of parameters obtained from analysis of carefully selected subsets of data. We find that the ecliptic longitude and speed of interstellar He are in a very good agreement with the values reported in the original GAS analysis. We find, however, that the temperature is markedly higher. The 3-seasons optimum parameter set is lambda = 255.3, beta = 6, v = 26.0 km/s, T = 7500 K. We find no evidence that it is varying with time, but the uncertainty range is larger than originally reported. The originally-derived parameters of interstellar He from GAS are in good agreement with presently derived, except for the temperature, which seems to be appreciably higher, in good agreement with interstellar absorption line results. While the results of the present analysis are in marginal agreement with the earlier reported results from IBEX, the most likely values from the two analyses differ for reasons that are still not understood.
submitted for publication in Astronomy & Astrophysics
References in corpus (5)
- The Structure of the Local Interstellar Medium V: Electron Densities
- Heliolatitude and time variations of solar wind structure from in situ measurements and interplanetary scintillation observations
- Solar parameters for modeling interplanetary background
- Modulation of neutral interstellar He, Ne, O in the heliosphere. Survival probabilities and abundances at IBEX
- Neutral interstellar hydrogen in the inner heliosphere under the influence of wavelength-dependent solar radiation pressure
Cited by in corpus (29)
- Three-dimensional kinetic-MHD model of the global heliosphere with the heliopause-surface fitting
- Interstellar neutral helium in the heliosphere from IBEX observations. III. Mach number of the flow, velocity vector, and temperature from the first six years of measurements
- Revisiting Ulysses Observations of Interstellar Helium
- Magnitude and direction of the local interstellar magnetic field inferred from Voyager 1 and 2 interstellar data and global heliospheric model
- Interstellar neutral helium in the heliosphere from IBEX observations. IV. Flow vector, Mach number, and abundance of the Warm Breeze
- Interstellar neutral helium in the heliosphere from IBEX observations. II. The Warsaw Test Particle Model (WTPM)
- Interstellar neutral helium in the heliosphere from IBEX observations. VI. The He density and the ionization state in the Very Local Interstellar Matter
- The helium Warm Breeze in IBEX observations as a result of charge exchange collisions in the outer heliosheath
- Interstellar Neutral Helium in the Heliosphere from IBEX Observations. I. Uncertainties and Backgrounds in the Data and Parameter Determination Method
- Interstellar neutral helium in the heliosphere from IBEX observations. V. Observations in IBEX-Lo ESA steps 1, 2, & 3
- Very Local Interstellar Medium Revealed by Complete Solar Cycle of Interstellar Neutral Helium Observations with IBEX
- Interstellar Neutral Gas Species And Their Pickup Ions Inside The Heliospheric Termination Shock. The Large-scale Structures
- The Interstellar Neutral He haze in the heliosphere: what can we learn?
- Interstellar hydrogen fluxes measured by IBEX-Lo in 2009: numerical modeling and comparison with the data
- Evolution of the solar Ly- line profile during the solar cycle. II. How accurate is the present radiation pressure paradigm for interstellar neutral H in the heliosphere?
- Mixing Interstellar Clouds Surrounding the Sun
- A new 3D solar wind speed and density model based on interplanetary scintillation
- Solar cycle variation of interstellar neutral He, Ne, O density and pick-up ions along the Earth's orbit
- Correcting the record on the analysis of IBEX and STEREO data regarding variations in the neutral interstellar wind
- Interstellar Conditions Deduced from Interstellar Neutral Helium Observed by IBEX and Global Heliosphere Modeling
- Angular Scattering in Charge Exchange: Issues and Implications for Secondary Interstellar Hydrogen
- Science Opportunities from Observations of the Interstellar Neutral Gas with Adjustable Boresight Direction
- A Ulysses Detection of Secondary Helium Neutrals
- On the sensitivity of heliosphere models to the uncertainty of the low-energy charge exchange cross section
- Synthesis of the distribution function of ISN He
- Heliospheric structure as revealed by the 3 -- 88 keV H ENA spectra
- The flow direction of interstellar neutral H from SOHO/SWAN
- An Improved Parametrized Representation of the Secondary He Neutral Flow in its Source Region
- Ulysses and IBEX Constraints on the Interstellar Neutral Helium Distribution