Stability of the interstellar hydrogen inflow longitude from 20 years of SOHO/SWAN observations
2017
Aims. A recent debate on the decade-long stability of the interstellar He flow vector, and in particular the flow
longitude, has prompted us to check for any variability in the interstellar H flow vector as observed by the SWAN instrument on board SOHO. Methods. We used a simple model-independent method to determine the interstellar H flow
longitude, based on the
parallaxeffects induced on the Lyman- α intensity measured by SWAN following the satellite motion around the Sun. Results. Our results show that the interstellar H flow vector
longitudedoes not vary significantly from an average value of 252.9°± 1.4° throughout the 20-year span of the SWAN dataset, further strengthening the arguments for the stability of the interstellar gas flow.
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