Jovian electrons in the inner heliosphere - Proposing a new source spectrum based on 30 years of measurements

Free Access

Fig. 3

Open with DEXTER Download original image

Proposed new Jovian spectrum according to Eq. (11) together with the Pioneer 10 CPI and Ulysses COSPIN-KET data. The ± σ uncertainty has been derived by the same method as detailed in Fig. 2.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.