A New Method to Model Magnetic Cloud-driven Forbush Decreases: The 2016 August 2 Event
暂无分享,去创建一个
C. Grimani | G. Consolini | Q. Hu | R. Vainio | M. Laurenza | A. Afanasiev | S. Benella
[1] B. Heber,et al. A Catalogue of Forbush Decreases Recorded on the Surface of Mars from 2012 Until 2016: Comparison with Terrestrial FDs , 2019, Solar Physics.
[2] A. Petiteau,et al. Forbush Decreases and <2 Day GCR Flux Non-recurrent Variations Studied with LISA Pathfinder , 2019, The Astrophysical Journal.
[3] Q. Hu,et al. Automated Detection of Small-scale Magnetic Flux Ropes in the Solar Wind: First Results from the Wind Spacecraft Measurements , 2018, The Astrophysical Journal Supplement Series.
[4] M. L. Mays,et al. Opening a Window on ICME-driven GCR Modulation in the Inner Solar System , 2018 .
[5] A. Petiteau,et al. Characteristics and Energy Dependence of Recurrent Galactic Cosmic-Ray Flux Depressions and of a Forbush Decrease with LISA Pathfinder , 2018, 1802.09374.
[6] S. Krimigis,et al. Solar Energetic Particles (SEP) and Galactic Cosmic Rays (GCR) as tracers of solar wind conditions near Saturn:event lists and applications , 2018 .
[7] D. Ruffolo,et al. Galactic Cosmic-Ray Anistropy During the Forbush Decrease Starting 2013 April 13 , 2018 .
[8] D. Hassler,et al. Measurements of Forbush decreases at Mars: both by MSL on ground and by MAVEN in orbit , 2017, 1712.06885.
[9] B. Heber,et al. An Analytical Diffusion–Expansion Model for Forbush Decreases Caused by Flux Ropes , 2017, The Astrophysical Journal.
[10] Q. Hu. The Grad-Shafranov reconstruction in twenty years: 1996–2016 , 2017, Science China Earth Sciences.
[11] C. Grimani,et al. LISA Pathfinder test-mass charging during galactic cosmic-ray flux short-term variations , 2015 .
[12] G. Vichare,et al. Quantitative understanding of Forbush decrease drivers based on shock-only and CME-only models using global signature of February 14, 1978 event , 2014, 1406.4608.
[13] N. Gopalswamy,et al. Coronal Mass Ejections and Non-recurrent Forbush Decreases , 2014 .
[14] I. Usoskin,et al. Neutron monitor yield function: New improved computations , 2013, 1612.01498.
[15] H. M. Antia,et al. High-rigidity Forbush decreases: due to CMEs or shocks? , 2013, 1304.5343.
[16] M. Kravtsova,et al. Rigidity spectrum of cosmic ray variations over the periods of large forbush decreases during solar cycles 22 and 23 , 2013 .
[17] M. Alania,et al. Energy dependence of the rigidity spectrum of Forbush decrease of galactic cosmic ray intensity , 2012 .
[18] B. Vršnak,et al. Cosmic ray modulation by different types of solar wind disturbances , 2012 .
[19] I. Richardson,et al. Galactic Cosmic Ray Intensity Response to Interplanetary Coronal Mass Ejections/Magnetic Clouds in 1995 – 2009 , 2011 .
[20] H. Shimazu,et al. EFFECT OF FINITE LARMOR RADIUS ON COSMIC-RAY PENETRATION INTO AN INTERPLANETARY MAGNETIC FLUX ROPE , 2010, 1007.2714.
[21] D. Ruffolo,et al. DRIFT ORBITS OF ENERGETIC PARTICLES IN AN INTERPLANETARY MAGNETIC FLUX ROPE , 2009 .
[22] A. Belov. Forbush effects and their connection with solar, interplanetary and geomagnetic phenomena , 2008, Proceedings of the International Astronomical Union.
[23] T. Kuwabara,et al. ON THE CROSS-FIELD DIFFUSION OF GALACTIC COSMIC RAYS INTO AN ICME , 2006 .
[24] M. Forman. Solar modulation of galactic cosmic rays. , 1988 .