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Publications3d ago83% confidenceConfidence 83% — the share of independent, credible sources corroborating the core facts.

Study Reveals How Coronal Mass Ejections Evolve Across Solar System Using 1,600+ Events

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Researchers used superposed epoch analysis on over 1,600 coronal mass ejection (CME) events to examine how their properties change from 0.2 to 2.2 astronomical units from the Sun. The study, drawing from the HELIO4CAST catalog, found that CMEs during the solar cycle's active phase are faster and carry stronger magnetic fields than those in the quiet phase, while also revealing how magnetic field components decay with distance. These findings suggest that solar cycle phase influences not just CME speed but potentially the fundamental eruption mechanism itself, with implications for space weather forecasting.

A new preprint posted to arXiv investigates the in-situ properties of coronal mass ejections (CMEs) — large eruptions of magnetized plasma from the Sun — across a wide range of heliocentric distances spanning 0.2 to 2.2 astronomical units. Using superposed epoch analysis applied to more than 1,600 events from the HELIO4CAST catalog, the authors compared CME characteristics during the active phase (AP) and quiet phase (QP) of the solar cycle. CMEs in the active phase were found to be faster and to carry stronger magnetic fields, while quiet-phase CMEs were denser but magnetically weaker. Crucially, these differences in magnetic field strength and plasma density persisted even after controlling for propagation speed, suggesting the distinctions may reflect intrinsic differences in how CMEs are generated during different solar cycle phases rather than being purely a speed-related effect. The study also characterized how the toroidal and poloidal components of the CME magnetic ejecta decay with distance, finding both follow similar power-law relationships, indicating roughly symmetric expansion in those dimensions. Additionally, the researchers quantified magnetic field asymmetry — often linked to CME aging during propagation — and found that the front-to-rear ratio of the toroidal component increases with heliocentric distance, consistent with the CME structure evolving as it travels outward.

What's missing

The study relies on catalog-based in-situ measurements and does not directly validate whether the observed active-phase vs. quiet-phase differences stem from eruption mechanism differences or from selection effects (e.g., stronger events being more reliably detected and cataloged during the active phase). The analysis is statistical in nature and does not trace individual CME events from eruption to distant measurement, leaving open questions about how much propagation effects versus source-region properties drive the observed trends. The preprint has not yet undergone peer review.

What different sources said

  • Evolution of Coronal Mass Ejection Properties through Superposed Epoch Analysis from 0.2 to 2.2 au

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