Skip to main content
Log in

Measurement of the Abundance of Helium-3 in the Sun and in the Local Interstellar Cloud with SWICS on Ulysses

  • Published:
Space Science Reviews Aims and scope Submit manuscript

Abstract

The abundance of 3He in the present day local interstellar cloud (LIC) and in the sun has important implications for the study of galactic evolution and for estimating the production of light nuclei in the early universe. Data from the Solar Wind Ion Composition Spectrometer (SWICS) on Ulysses is used to measure the isotopic ratio of helium (3He/4He = Γ) both in the solar wind and the local interstellar cloud. For the solar wind, the unique high-latitude orbit of Ulysses allows us to study this ratio in the slow and highly dynamic wind in the ecliptic plane as well as the steady high-latitude wind of the polar coronal holes. The 3He+/4He+ ratio in the local cloud is derived from the isotopic ratio of pickup helium measured in the high-speed solar wind. In the LIC the ratio is found to be (2.48 +0.68-0.62 ) × 10-4 with the 1-σ uncertainty resulting almost entirely from statistical error. In the solar wind, Γ is determined with great statistical accuracy but shows systematic differences between fast and slow solar wind streams. The slow wind ratio is variable. Its weighted average value (4.08 ± 0.25) × 10-4 is, within uncertainties, in agreement with the Apollo SWC results. The high wind ratio is less variable but smaller. The average Γ in the fast wind is (3.3 ± 0.3) × 10-4.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Bochsler, P.: 1984, Helium and Oxygen in the solar wind: Dynamic properties and abundances of elements and Helium isotopes as observed with the ISEE-3 plasma composition experiment, Habilitationsschrift, Univ. of Bern.

  • Bodmer, R.: 1996, The Helium Isotopic Ratio as a Test for Mi nor Ion Fractionation in the Solar Wind Acceleration Process: SWICS/ULYSSES Data Compared with Results from a Multifluid Models, Ph.D. Thesis, Univ. of Bern.

  • Coplan, M. A., Ogilvie, K. W., Bochsler, P. and Geiss, J.: 1984,Solar Phys. 93, 415.

    Google Scholar 

  • Geiss, J., Eberhardt, P., Bühler, F., Meister, J. and Signer, P.: 1970, J Geophys. Res. 75, 5972.

    Google Scholar 

  • Geiss, J., Bühler, F., Cerutti, H., Eberhardt, P. and Filleux, C.: 1972, in Apollo 16 Preliminary Science Report, NASA SP-315, section 14.

  • Geiss, J. and Gloeckler, G.: 1998, Space Sci. Rev., this issue.

  • Geiss, J., Gloeckler, G., Mall, U., von Steiger, R., Galvin, A. B., and Ogilvie, K. W.: 1994, “Interstellar oxygen, nitrogen, and neon in the heliosphere”, Astr. Astrophys. 282, 924–933.

    Google Scholar 

  • Gloeckler, G., et al.: 1992, Geiss, J., Balsiger, H., Bedini, P., Cain, J. C., Fischer, J., Fisk, L. A., Galvin, A. B., Gliem, F., Hamilton, D. C., Hollweg, J. V., Ipavich, F. M., Joss, R., Livi, S., Lundgren, R., Mall, U., McKenzie, J. F., Ogilvie, K. W., Ottens, F., Rieck, W., Tums, E. O., von Steiger, R., Weiss, W., and Wilken, B.: 1992, “The solar wind ion composition spectrometer”, Astr. Astrophys. Suppl. Ser. 92, 267–289.

    Google Scholar 

  • Gloeckler, G., et al.: 1993, Geiss, J., Balsiger, H., Fisk, L. A., Galvin, A. B., Ipavich, F. M., Ogilvie, K. W., von Steiger, R., and Wilken, B.: 1993, Science 261, 70.

    Google Scholar 

  • Gloeckler, G. and Geiss, J.: 1996, “Abundance of 3He in the local interstellar cloud”, Nature 381, 210.

    Google Scholar 

  • Gloeckler, G. and Geiss, J.: 1998, “Interstellar and Inner Source Pickup Ions Observed with SWICS on Ulysses”, Space Sci. Rev., in press.

  • Gloeckler, G., Fisk, L. A. and Geiss, J: 1997a, “Anomalously small magnetic field in the local interstellar cloud”, Nature 386, 374–377.

    Google Scholar 

  • Gloeckler, G., Galvin, A. B., Hamilton, D. C., Ipavich, F. M., Fisk, L. A., Geiss, J., Bochsler, P., and Wilken, B.: 1997b, “The Unusual Solar Wind in the High-Density Pulse of the Magnetic Cloud Associated With the Halo CME of January, 1997”, Spring AGU meeting, Baltimore, MD, EOS Trans. American Geophys. Union 47.

  • Murphy, R. J.,. Share, G. H,. Grove, J. E, Johnson, W. N., Kinzer, R. L., Kurfess, J. D., Strickman, M. S. and Jung, G. V.: 1997, “Accelerated Particle Composition and Energetics and Ambient Abundances from Gamma-Ray Spectroscopy of the 1991 June 4 Solar Flare, Astrophys J., submitted.

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Gloeckler, G., Geiss, J. Measurement of the Abundance of Helium-3 in the Sun and in the Local Interstellar Cloud with SWICS on Ulysses. Space Science Reviews 84, 275–284 (1998). https://doi.org/10.1023/A:1005095907503

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1023/A:1005095907503

Keywords

Navigation