No CrossRef data available.
Article contents
Solar Activity Dependence of Interplanetary Disturbances
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Interplanetary scintillation measurements obtained inside 200 R⊙ using the Ooty Radio Telescope during August 1986 - April 1991 have been analysed to study the interplanetary disturbances (or events) and their occurrence rates at various phases of the solar cycle. The disturbances are identified by the increase in the level of scintillation compared with the expected value. In total, 735 events have been identified. The results show a rate of 0.49 events per day near solar maximum and a low rate of 0.16 events per day during minimum of activity. The results are compared with coronal mass ejection (CME) rates and transients rates obtained from the Doppler scintillation measurements.
- Type
- IPS and Other Remote Sensing Measurements
- Information
- International Astronomical Union Colloquium , Volume 154: Solar and Interplanetary Transients , 1996 , pp. 221 - 224
- Copyright
- Copyright © Kluwer 1997
References
Manohaian, P.K., Ananthakrishnan, S., Dryer, M., Detman, T.R., Leinbach, H., Kojima, M., Watanabe, T. and Kahn, J.: 1995, Solar Phys.
156, 377.CrossRefGoogle Scholar
Swarup, G., Sarma, N.V.G., Joshi, M.N., Kapahi, V.K., Bagri, D.S., Damle, S.H., Ananthakrishnan, S., Balasubramanian, V., Bhave, S.S., and Sinha, R.P.: 1971, Nature Phys. Sci.,
230, 185.CrossRefGoogle Scholar
You have
Access