Can the direction of interstellar magnetic field be determined from the heliotail ENA flux?
- 1 June 1998
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 25 (11) , 1855-1858
- https://doi.org/10.1029/98gl51504
Abstract
No abstract availableThis publication has 12 references indexed in Scilit:
- Detection of 55–80 keV Hydrogen Atoms of Heliospheric Origin by CELIAS/HSTOF onSOHOThe Astrophysical Journal, 1998
- Heliosphere in the magnetized local interstellar medium: Results of a three‐dimensional MHD simulationJournal of Geophysical Research, 1998
- Distribution of ACR ions in the heliosheath and the related ENA fluxAdvances In Space Research, 1997
- Possible shock wave in the local interstellar plasma, very close to the heliosphereSpace Science Reviews, 1996
- A transport model for the diffusive shock acceleration and modulation of anomalous cosmic rays in the heliosphereJournal of Geophysical Research, 1996
- Characteristics of nearby interstellar matterSpace Science Reviews, 1995
- Radio Emission from the Heliopause Triggered by an Interplanetary ShockScience, 1993
- Probing the heliosphere with energetic hydrogen atomsThe Astrophysical Journal, 1992
- An open magnetopause model of the Earth's distant tail based on ISEE 3 evidenceJournal of Geophysical Research, 1988
- Expected immersion of Saturn's magnetosphere in the jovian magnetic tailNature, 1981