Interplanetary Lymanαline profiles: variations with solar activity cycle

2006/08/04 by Éric Quémerais, Eric Quémerais, R. Lallement +10 · 24 citations
Earth and Planetary Sciences · Physics and Astronomy · #Astronomy #Atmospheric sciences #Environmental science #Geophysics and Gravity Measurements #Interplanetary medium #Interplanetary spaceflight #Line (geometry) #Physics #Plasma #Solar and Space Plasma Dynamics #Solar cycle #Solar cycle 22 #Solar cycle 23 #Solar maximum #Solar wind #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065169

published in Astronomy and Astrophysics 455(3), 1135-1142 (EDP Sciences) · 9 pages, 9 figures

openalex publication_date 2006/08/04 · arxiv created 2006/09/11 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims.Interplanetary Lyman α line profiles are derived from the SWAN H cell data measurements. The measurements cover a 6-year period from solar minimum (1996) to after the solar maximum of 2001. This allows us to study the variations of the line profiles with solar activity.

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