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First Direct Observation of the Interaction between a Comet and a Coronal Mass Ejection Leading to a Complete Plasma Tail Disconnection

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Angelos Vourlidas1, Chris J. Davis2, Chris J. Eyles2,3,4, Steve R. Crothers2, Richard A. Harrison2, Russell A. Howard1, J. Daniel Moses1 and Dennis G. Socker1

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[1]

Processes involving clusters and small particles in a buffer gas

Boris M Smirnov  Physics-Uspekhi 2011  54 691
IOPscience 
[2]

Reconstructing the Morphology of an Evolving Coronal Mass Ejection

B. E. Wood et al.  The Astrophysical Journal 2010  715 1524
IOPscience 
[3]

Solar Wind Speed Inferred from Cometary Plasma Tails using Observations from STEREO HI-1

John M. Clover et al.  The Astrophysical Journal 2010  713 394
IOPscience 
[4]

Demonstrations that the Solar Wind is Not Accelerated By Waves or Turbulence

D. Aaron Roberts  The Astrophysical Journal 2010  711 1044
IOPscience 
[5]

Study of the 2007 April 20 CME-Comet Interaction Event with an MHD Model

Y. D. Jia et al  The Astrophysical Journal Letters 2009  696 L56
IOPscience 
[6]

Analysis of Plasma-Tail Motions for Comets C/2001 Q4 (NEAT) and C/2002 T7 (LINEAR) Using Observations from SMEI

A. Buffington et al.  The Astrophysical Journal 2008  677 798
IOPscience 
crossref member

  1. First Direct Observation of the Interaction between a Comet and a Coronal Mass Ejection Leading to a Complete Plasma Tail Disconnection

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  5. Chandra X-Ray Observation of the Orion Nebula Cluster. II. Relationship between X-Ray Activity Indicators and Stellar Parameters

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  6. Near-Infrared Properties of Moderate-Redshift Galaxy Clusters. II. Halo Occupation Number, Mass-to-Light Ratios, and Ωm

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  7. Molasses for ethanol: the economic and environmental impacts of a new pathway for the lifecycle greenhouse gas analysis of sugarcane ethanol

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  8. The B-Band Luminosity Function of Red and Blue Galaxies up to z = 3.5

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