2009
DOI: 10.5194/angeo-27-4349-2009
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The radial width of a Coronal Mass Ejection between 0.1 and 0.4 AU estimated from the Heliospheric Imager on STEREO

Abstract: Abstract. On 15-17 February 2008, a CME with an approximately circular cross section was tracked through successive images obtained by the Heliospheric Imager (HI) instrument onboard the STEREO-A spacecraft. Reasoning that an idealised flux rope is cylindrical in shape with a circular cross-section, best fit circles are used to determine the radial width of the CME. As part of the process the radial velocity and longitude of propagation are determined by fits to elongation-time maps as 252±5 km/s and 70±5 • re… Show more

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Cited by 48 publications
(60 citation statements)
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“…By assuming our sample is normally distributed, the 95% confidence interval for our aspect ratio estimate is 2.8 ± 0.5. This strongly supports that fast ICMEs are elliptical, and have significantly evolved away from the circular cross section found in the high solar corona and estimated by remote observations from the HI instrument on board STEREO (Savani et al 2009). Figure 5 displays a histogram of the aspect ratio; this figure also displays a Gaussian distribution using the mean and standard deviation calculated earlier.…”
Section: Resultssupporting
confidence: 63%
See 1 more Smart Citation
“…By assuming our sample is normally distributed, the 95% confidence interval for our aspect ratio estimate is 2.8 ± 0.5. This strongly supports that fast ICMEs are elliptical, and have significantly evolved away from the circular cross section found in the high solar corona and estimated by remote observations from the HI instrument on board STEREO (Savani et al 2009). Figure 5 displays a histogram of the aspect ratio; this figure also displays a Gaussian distribution using the mean and standard deviation calculated earlier.…”
Section: Resultssupporting
confidence: 63%
“…This enables remote observations at distances further away from the Sun, where only in situ measurements had been previously available (e.g., Davis et al 2009;Liu et al 2010aLiu et al , 2010bMostl et al 2009;Rouillard et al 2009Rouillard et al , 2010aRouillard et al , 2010bRouillard et al , 2010c. Therefore, similar to the work by Savani et al (2009Savani et al ( , 2010, the evolving aspect ratio of a single ICME may be investigated over large distances. In the future, it is hoped that these types of detailed studies may substantially reduce this variability caused between events.…”
Section: Discussionmentioning
confidence: 69%
“…Indeed, the self-consistency tests of Lepping et al (1990) only check that the fit to the data provides coherent results with the hypothesis of the model. Evidences of compression in the direction of propagation are present in CME observations (e.g., Savani et al 2009Savani et al , 2010 and in magnetohydrodynamics (MHD) simulations (e.g., Cargill & Schmidt 2002;Odstrcil et al 2004;Manchester et al 2004;Lugaz et al 2005b;Xiong et al 2006). Such a compression flattens the cross section, and such a geometrical feature has been partly taken into account by .…”
Section: Introductionmentioning
confidence: 95%
“…This expression shows that magnetic energy is reduced in time primarily by the expansion of magnetic flux "rope" often seen at the beginning of a CME (Harrison 1986(Harrison , 1995Harrison et al 1990;Savani et al 2009). As the rope unwinds and rotates, the area increases rapidly with time.…”
Section: Magnetic Storage and Types Of Magnetic Configurationsmentioning
confidence: 99%