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Dandapat Sumit Chakraborty Arun Kuttippurath Jayanarayanan Bhagawati Chirantan Sen Radharani 《Ocean Dynamics》2021,71(10):963-979
Ocean Dynamics - This study investigates the role of driving atmospheric forces [winds, net heat flux, and evaporation–precipitation (E–P)] and the possible mechanisms on the mixed... 相似文献
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Jatin Rathod Girija Rajaram Radharani Alyana A. Chandrasekhar Reddy D. S. Misra C. G. Patil M. Y. S. Prasad A. G. Ananth 《Journal of Astrophysics and Astronomy》2008,29(1-2):293-302
In the present study, we investigate the possible relationship of IP parameters of solar wind and interplanetary magnetic field with ground-based geomagnetic indices. To carry out the study, we take all the IP shock events listed by Proton Monitor onboard Solar and Heliospheric Observatory (SOHO) during 2005, and plot the time variations of all the IP parameters and geomagnetic parameters (±5 days), centered at the shock arrival time. Next, we obtain scatter plots of absolute values of solar wind parameters such as Vsw, Nsw and Interplanetary Magnetic Field (IMF) components Bx, By, Bz and total B with the values of geomagnetic parameters such as Dst, Kp indices, dayside Magnetopause (MP) distance and Cosmic-Ray Neutron Monitor count (CRNM). The scatter plots show that before the IP shock, the pattern is random with no clear relationship. Following the shock, a clear pattern emerges with a type of relationship being seen — clear for SHARP shocks and less clear for DIFFUSE shocks. A total of 10 shock events for 2005 have been studied. Typical examples of this behaviour are the shock events of January 21, 2005 and May 15, 2005. Our study suggests a definite correlation between changes in the solar wind and interplanetary magnetic field parameters and ground-based geomagnetic response. We are trying to obtain quantitative relationships between these for shock events of 2005. 相似文献
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A. Chandrasekhar Reddy Jatin Rathod Girija Rajaram Radharani Alyana D. S. Misra C. G. Patil M. Y. S. Prasad A. G. Ananth 《Journal of Astrophysics and Astronomy》2008,29(1-2):313-317
In view of the renewed interest in the study of energetic particles in the outer radiation belt of the earth, we feel it will be helpful in looking for the energy dependence of the electron energy spectrum at geostationary orbit. This may give us some insight into how we can safeguard geostationary satellites from functional anomalies of the deep dielectric charging type, which are caused by charge accumulation and subsequent discharge of relativistic electrons. In this study we examine whether there is any energy dependence in relativistic electron enhancements at geosynchronous altitudes during solar energetic proton events of 2005. 相似文献
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Sen Radharani Francis Pavanathara Augustine Chakraborty Arun Effy John B. 《Ocean Dynamics》2021,71(5):527-543
Ocean Dynamics - This study addresses the air–sea interaction processes and mixed layer variability, which cause the intraseasonal oscillations in the sea surface temperature (SST) during... 相似文献
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