Coronal Mass Ejections and Forbush Decreases

By H. Cane. 2000

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In Astronomy and Astrophysics

Citations in the corpus

Mars’ Surface Radiation Environment Measured with the Mars Science Laboratory’s Curiosity Rover (2014, neutral): “During this time, RAD observed a dose rate enhancement from one hard SEP event on sol 242 (12 to 13 April 2013) and several Forbush decreases (32), resulting from soft SEP eventrelated interplanetary coronal mass ejections (ICMEs) on sols 50, 97, 208, and 259.”
Applications and usage of the real-time Neutron Monitor Database (2011, background): “FEs have been extensively studied over the years (Lockwood, 1971; Iucci et al., 1979a,b; 1988; Cane, 2000; Belov et al., 2003; Storini, 1991; Storini et al., 1997; Usoskin et al., 2002, 2005; Kudela and Storini, 2006; Munakata et al., 2000; Belov, 2009; Papaioannou et al., 2009a; Kuwabara et al., 20”
Space weather: the solar perspective (2021, background): “At that time also galactic cosmic rays were studied and found that they are anti-correlated with solar activity (so-called Forbush decrease, measured as sudden drop in the cosmic ray flux due to interplanetary disturbances; see also Cane 2000).”
STEREO IMPACT Investigation Goals, Measurements, and Data Products Overview (2008, neutral): “Large decreases in energetic ion intensity are often observed during passage of ICMEs (e.g., Mazur et al. 1998; Cane 2000), probably indicating the inability of the shock-accelerated particles to penetrate significantly into the closed field regions of the ICMEs.”
Near-earth solar wind flows and related geomagnetic activity during more than four solar cycles (1963-2011) (2012, background): “…(i.e., ‘‘Forbush decreases’’; Forbush 1937) can help to identify the passage of shocks and ICMEs (e.g., Barnden 1973a, 1973b; Cane et al. 1993, 1996; Cane 2000; Richardson & Cane 2011b, and references therein) and also corotating streams (Simpson et al. 1955; Iucci et al. 1979; Richardson et…”
Energetic Particle Influence on the Earth’s Atmosphere (2015, background): “The exact shape of the Forbush decrease depends on the relative geometry of the interplanetary shock and Earth (Cane 2000).”
A survey of interplanetary coronal mass ejections in the near-Earth solar wind during 1996-2002 (2003, background): “When combined with the preceding decrease that often occurs at shock passage, this produces the classic ‘‘two step’’ cosmic ray Forbush decrease [Cane, 2000, and references therein].”
Cosmic ray decreases affect atmospheric aerosols and clouds (2009, background): “Such Forbush decreases (FDs) are now understood to be the result of magnetic plasma clouds from solar coronal mass ejections that pass near the Earth and provide a temporary shield against GCRs [ Hilary, 2000 ].”