New observations of the out-of-the ecliptic trajectories of type III solar radio bursts have been obtained from simultaneous direction finding measurements on two independent satellite experiments, IMP-6 with spin plane in the ecliptic, and RAE-2 with spin plane normal to the ecliptic. Burst exciter
Modeling the out-of-ecliptic interplanetary magnetic field in the declining phase of sunspot Cycle 22
β Scribed by Xuepu Zhao; J. Todd Hoeksema
- Publisher
- Springer Netherlands
- Year
- 1995
- Tongue
- English
- Weight
- 240 KB
- Volume
- 72
- Category
- Article
- ISSN
- 0038-6308
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π SIMILAR VOLUMES
The method proposed by Hathaway et al. [SoPh 151 (1994) 177] was employed to predict the magnitude of sunspot activities in the declining phase of solar Cycle 23, based on the monthly averages of sunspot number and the smoothed monthly averages of sunspot number, respectively. Our results show that:
The Return Flux (RF) sunspot model (Osherovich, 1982) imposes a restriction on the value of the vertical gradient of the magnetic field, dB/dz, analogous to a restriction implied by the self-similar sunspot model of Schliiter and Temesvary (ST). The maximum value of the gradient, (dB/dz),~ax, is sho