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  • Forbush decreases and turbulence levels at coronal mass ejection fronts 
    SUBRAMANIAN, PRASAD; Antia, H.M.; Dugad, S. R.; Goswami, U.D.; Gupta, S. K.; Hayashi, Y.; Ito, N.; Kawakami, S.; Kojima, H.; Mohanty, P.K.; Nayak, P.K.; Nonaka, T.; Oshima, A.; Sivaprasad, K.; Tanaka, H.; Tonwar, S.C. (EDP Sciences, 2009-02)
    Aims. We seek to estimate the average level of MHD turbulence near coronal mass ejection (CME) fronts as they propagate from the Sun to the Earth. Methods. We examined the cosmic ray data from the GRAPES-3 tracking muon ...
  • High-rigidity Forbush decreases: due to CMEs or shocks? 
    Arunbabu, K. P.; Antia, H.M.; Dugad, S. R.; Gupta, S. K.; Hayashi, Y.; Kawakami, S.; Mohanty, P.K.; Nonaka, T.; Oshima, A.; SUBRAMANIAN, PRASAD (EDP Sciences, 2013-07)
    Aims. We seek to identify the primary agents causing Forbush decreases (FDs) in high-rigidity cosmic rays observed from the Earth. In particular, we ask if these FDs are caused mainly by coronal mass ejections (CMEs) from ...

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