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ANGEO - Topical Library
Volume 25, 2007 - Solar Corona & Heliospheric Physics
- The prominent 1.6-year periodicity in solar motion due to the inner planets
I. Charvátová
Page(s) 1227-1232
Abstract Full Article in 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 in 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 in 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 in 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 in 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 in PDF (360 KB)
| | 02 Jan 2008 |
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