ANGEO - Topical Library
Volume 25, 2007 - Solar Corona & Heliospheric Physics| The prominent 1.6-year periodicity in solar motion due to the inner planets Page(s) 1227-1232 Abstract Full Article (PDF, 4031 KB) | ||
| Magnetically dominated structures as an important component of the solar wind turbulence Page(s) 1913-1927 Abstract Full Article (PDF, 818 KB) | ||
| Hysteresis loops of Cosmic Ray intensity decreases versus solar and interplanetary parameters Page(s) 2087-2097 Abstract Full Article (PDF, 8259 KB) | ||
| Long-duration magnetic clouds: a comparison of analyses using torus- and cylinder-shaped flux rope models Page(s) 2453-2477 Abstract Full Article (PDF, 9596 KB) | ||
| Comparison of magnetic field observations of an average magnetic cloud with a simple force free model: the importance of field compression and expansion Page(s) 2641-2648 Abstract Full Article (PDF, 363 KB) | ||
| Revisiting the theory of the evolution of pick-up ion distributions: magnetic or adiabatic cooling? Page(s) 2649-2659 Abstract Full Article (PDF, 360 KB) |
