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Chris J. Scott

Researcher at University of Reading

Publications -  75
Citations -  1589

Chris J. Scott is an academic researcher from University of Reading. The author has contributed to research in topics: Solar wind & Space weather. The author has an hindex of 21, co-authored 67 publications receiving 1189 citations.

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Using Ghost Fronts Within STEREO Heliospheric Imager Data to Infer the Evolution in Longitudinal Structure of a Coronal Mass Ejection

TL;DR: In this article, the authors present an analysis of the Earth-directed CME launched on 12 December 2008 in which they intepret the revealed structure as projections of separate discrete sections of the physical boundary of the CME.
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Using the "Ghost Front" to Predict the Arrival Time and Speed of CMEs at Venus and Earth

TL;DR: In this article, the ghost front model was proposed to estimate the kinematics and propagation directions of two Coronal mass ejections (CMEs) that left the Sun on 13-14 June 2012 and impacted both Venus and Earth while the planets were in close radial alignment.
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Near-earth cosmic ray decreases associated with remote coronal mass ejections

TL;DR: In this article, the authors report on four Forbush decreases observed at ground-based neutron monitors which cannot be immediately associated with significant structures in the local solar wind, while there are significant near-Earth structures which do not produce any corresponding GCR variation.
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The Development of a Space Climatology: 2. The Distribution of Power Input Into the Magnetosphere on a 3-Hourly Timescale

TL;DR: In this article, it was shown that the form of the distribution of Pα at all averaging timescales is set by the IMF orientation factor via the nature of solar wind-magnetosphere coupling (due to magnetic reconnection in the dayside magnetopause).
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Extracting Inner‐Heliosphere Solar Wind Speed Information From Heliospheric Imager Observations

TL;DR: In this article, the authors present evidence that variability in the STEREO-A Heliospheric Imager (HI) data is correlated with in situ solar wind speed estimates from WIND, WIND and WIND-A. The authors compute the variability in HI differenced images in a plane-of-sky shell between 20 to 22.5 solar radii.