Comment on "Interplanetary coronal mass ejections that are undetected by solar coronagraphs" by T. A. Howard and G. M. Simnett
Marta Skirgiello

TL;DR
This paper critiques Howard and Simnett's new CME association method, highlighting errors in trajectory parameters and speed estimations that compromise their conclusions on undetected interplanetary CMEs.
Contribution
It identifies critical errors in the trajectory and speed calculations of Howard and Simnett's method, emphasizing the need for reanalysis before conclusions are drawn.
Findings
Incorrect use of free parameters in trajectory determination
Multiple trajectories can match SMEI data, leading to incomplete associations
Speed estimates in the original study are significantly overestimated
Abstract
Howard and Simnett (HS) employed a new technique for associating LASCO CMEs to SMEI ICMEs. In order to extrapolate the SMEI data back to the LASCO field of view they used nonlinear trajectories, dependent on a speed and direction, what is more realistic than the linear extrapolation with only one parameter (a speed). However, there are two errors and one mistake in their procedure: (1) HS used two free parameters of the direction, whereas only one can be freely selected, because the second is provided by SMEI data. As a result, the directions determined by HS are incorrect. (2) HS overlooked that, since the trajectory depends on more than one parameter, there is a broad set of trajectories, for various speeds and directions, matching the event, and thus a broad range of the onset times. HS select only one trajectory for each SMEI event. Therefore the associations made by them are…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · Ionosphere and magnetosphere dynamics
