Long-Term Cosmic-Ray Modulation in the Heliosphere
By S. Ferreira, M. Potgieter. 2004
137 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/704f0262ff8fbe5f4f9f90a7ef1dfbd429d04b61
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In Astronomy and Astrophysics
In Atmospheric Science
Citations in the corpus
- The Solar Cycle (2010, background): “This behavior is accounted for in the transport models for galactic cosmic rays in the heliosphere (e.g., Ferreira and Potgieter, 2004).”
- The Solar Cycle (2007, background): “This behavior is accounted for in the transport models for galactic cosmic rays in the heliosphere (cf. Ferreira and Potgieter, 2004).”
- Solar Modulation of Cosmic Rays (2013, background): “Ferreira and Potgieter (2004) confirmed that using the HCS tilt angles as the only timedependent modulation parameter resulted in compatibility only with solar minimum observations.”
- RECORD-SETTING COSMIC-RAY INTENSITIES IN 2009 AND 2010 (2010, background): “Diffusion perpendicular to the magnetic field is often assumed to scale as KII (Ferreira & Potgieter 2004).”