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ISWAT S3 Cluster Paper

A proposed draft outline

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Tentative Title(s)

Tentative subtitle

  • Prediction of Solar Flares and Eruptive Manifestations
  • Prediction of Solar Weather Events Impacting Space Weather Conditions
  • … (open to suggestions)

State-of-the-art, Challenges and Outlook

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Top-level ToC

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Introduction

  • Solar Active Regions: distinguishing between flaring / eruptive regions and quiescent ones

  • Quiet-Sun eruptions

Note: discussion to make a case that we will be focusing on active regions

  • Rationale for predicting solar weather events

  • Recap from Schrijver et al., ASR, 2015

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The preflare / pre-eruption situation

  • Flares and CMEs
    • Connection to: S3-05: Understanding the onset of CMEs / Eruptive Flares
    • Connection to: Tier II paper on CME onset: “Recent Progress on Understanding Coronal Mass Ejection / Flare Onset”

  • Precursors (morphological, topological, spectroscopic, radio)

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Prediction of solar weather events

  • Solar Flares: setting the current state of the art
    • Statistical methods
    • Machine / Deep Learning Methods
    • Ensemble Methods

  • Onset of coronal mass ejections

Note: not to confuse with prediction of CME arrival times and geoeffectiveness

    • Statistical Methods
    • Machine / Deep learning methods
    • Ensemble methods

  • Predicted features of coronal mass ejections

  • Solar Energetic Particle Events

Note: this will need to keep short and focused on solar diagnostics, given a connection to: H2: SEP and GCR in Heliosphere

    • SEP event occurrence and profiles by properties of source eruptions and host active regions

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Envisioned framework of solar weather prediction methods

  • Data, model and performance verification

    • Data Verification in terms of benchmark datasets

    • Model verification - suggested practices

    • Performance verification
      • Binary and probabilistic forecasts and metrics
      • The scoreboard practice

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Challenges and short-term objectives

  • Predicting All Clear in terms of flares, CMEs, and SEPs

  • Missing data
    • Magnetic configurations beyond 70o EW
    • Farside events
      • Active regions rotating toward the eastern limb
      • Acting regions rotating beyond the western limb

  • Customizing forecasts for different stakeholder communities

  • Objectives given current observational, modeling and forecasting capabilities
    • Physical and statistical understanding
    • Interpretable machine (and physics-informed deep) learning
    • Technological infrastructure (portability, searchability)

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Future needs and outlook

  • Data beyond the Sun-Earth line and expectations
    • Mission to L5
    • Mission to L4

  • 24/7 full-Sun observations: when and how?

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Conclusions

  • Current status of solar weather events prediction

  • Challenges / drawbacks and caveats

  • Recommendations: suggested forecast framework

  • Short-term future expectations

  • Long-term needs and expectations

  • … [Other?]

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Tentative co-authors

  • S3 team leaders
    • Murray, Thompson, West, Guerra, Zucca, Antiochos, Linton

  • Names included in the draft (alphabetically)
    • Angryk, Arge, Aydin, Bain, Barnes, Bingham, Bisi, Bloomfield, Bobra, Camporeale, Chen, Chintzoglou, Collado-Vega, Crosby, De Pontieu, Falconer, Green, Guerra, Harra, Harrison, Hoeksema, Hurlburt, Ishii, Kitiashvili, Kleint, Kliem, Kusano, Leka, Malandraki, Mays, Nishizuka, Panos, Papaioannou, Park, Patsourakos, Piana, Posner, Richardson, Sadykov, Semones, StCyr, Trichas, Toriumi, Torok, Vourlidas, Wang, Yardley

  • A shorter list will need to be made, very likely

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QUESTIONS / COMMENTS / SUGGESTIONS ?