THE ACCURACY OF USING THE ULYSSES RESULT OF THE SPATIAL INVARIANCE OF THE RADIAL HELIOSPHERIC FIELD TO COMPUTE THE OPEN SOLAR FLUX (2009)

First Author: Lockwood M

Attributed to: THE APPLICATION OF 3-D MHD MODELS OF THE HELIOSPHERE TO UNDERSTANDING OF CENTURY-SCALE VARIATIONS IN GALACTIC COSMIC RAYS funded by STFC

No abstract provided

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2