|
|
ANGEO - Topical LibraryVolume 25, 2007 - Solar Corona & Heliospheric PhysicsThe prominent 1.6-year periodicity in solar motion due to the inner planets I. Charvátová Page(s) 1227-1232 Abstract Full Article (PDF, 4031 KB)
| | 04 Jun 2007 | Magnetically dominated structures as an important component of the solar wind turbulence R. Bruno, R. D'Amicis, B. Bavassano, V. Carbone, and L. Sorriso-Valvo Page(s) 1913-1927 Abstract Full Article (PDF, 818 KB)
| | 29 Aug 2007 | Hysteresis loops of Cosmic Ray intensity decreases versus solar and interplanetary parameters R. P. Kane Page(s) 2087-2097 Abstract Full Article (PDF, 8259 KB)
| | 02 Oct 2007 | Long-duration magnetic clouds: a comparison of analyses using torus- and cylinder-shaped flux rope models K. Marubashi and R. P. Lepping Page(s) 2453-2477 Abstract Full Article (PDF, 9596 KB)
| | 29 Nov 2007 | Comparison of magnetic field observations of an average magnetic cloud with a simple force free model: the importance of field compression and expansion R. P. Lepping, T. W. Narock, and H. Chen Page(s) 2641-2648 Abstract Full Article (PDF, 363 KB)
| | 02 Jan 2008 | Revisiting the theory of the evolution of pick-up ion distributions: magnetic or adiabatic cooling? H. J. Fahr Page(s) 2649-2659 Abstract Full Article (PDF, 360 KB)
| | 02 Jan 2008 |
|
|