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X flares and geomagnetic storms The Earth responds two to three days later

Correspondences

What is linked, what is not

Each arc joins two phenomena tested on this site. Green and animated: clear link (correlation significant at 5 % after correcting for autocorrelation, or a response outside chance in an event study). Grey: inconclusive test. A statistical link alone does not establish causation.

  • Clear link
  • Inconclusive
Hypotheses tested
16
Clear links
11
correlation p < 0.05 or epochs outside chance
Causation demonstrated
0
a correlation demonstrates none

Arc width from |r| of the stored result; several tests between the same phenomena are drawn as stacked arcs.

Hypothesis tested: The strongest flares are often accompanied by coronal mass ejections that reach the Earth in one to three days and compress the magnetosphere: Dst should drop in the following days (Gopalswamy, 2009).
Events used
484
minimum composite anomaly -13.30 nT
Days outside chance
6
out of 7 days tested after the event
Verdict
Clear effect
clear effect: two consecutive days outside the 5–95 % band
Period analysed
1976-01-01 → 2026-10-16
computed on Oct 23, 2026 · engine v1.0
Superposed epochs
Show the data as a table

Aligned series (CSV)

Method and sources

For each day with at least one X flare in the GOES catalogue, the daily minimum Dst (OMNI2) is expressed as the departure from the mean of the five previous days, then averaged over all events. The 5–95 % band comes from 1,000 draws of random dates. The link is called clear if the composite leaves the band on two consecutive days.

Computation parameters
{
    "draws": 1000,
    "events": "days with an X-class flare (GOES)",
    "response": "daily minimum Dst (OMNI2), nT",
    "after_days": 6,
    "before_days": 5,
    "significance": "at least two consecutive days outside the Monte-Carlo 5–95 % band"
}

Inputs : goes.flares.x.yearly (51 pts, run #111) · omni.dst.hourly (559,191 pts, run #133)

Reading this result
Not every X flare launches an Earth-directed ejection: the mean composite (about −13 nT) is much weaker than individual storms, which can exceed −300 nT. The result illustrates the Sun–Earth chain; it does not forecast a given storm. X flares often come in series from the same active region: Dst already drops slightly before day 0, under the effect of the previous flares. Correlation is not causation: common factors (seasons, cycles, trends) or coincidence can produce it. The p-values account for autocorrelation (effective n) but not for preprocessing choices; the confidence interval comes from a block bootstrap. The limits of the source data apply.
SOURCES OF THIS PAGE
GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC)
NOAA SWPC/NGDC GOES X-ray flare event lists (1975–), yearly compilations by K. Tolbert, NASA GSFC Hesperia. Flare classes as reported by NOAA at the time: until December 2019 the XRS-B flux carried a 0.7 scaling factor (Janssens et al., 2025). · source page ↗
Licence : U.S. Government work, public domain (NOAA/NASA) · retrieved on Oct 23, 2026 · SHA-256 9c4ca1a2c018…
OMNI2 hourly near-Earth solar wind and geomagnetic indices
King, J. H., & Papitashvili, N. E. (2005). Solar wind spatial scales in and comparisons of hourly Wind and ACE plasma and magnetic field data. J. Geophys. Res., 110, A02104. OMNI2 data from NASA/GSFC SPDF OMNIWeb; Kp/ap from GFZ Potsdam, Dst from WDC Kyoto, F10.7 from NRC Canada (Penticton). · doi:10.1029/2004JA010649 · source page ↗
Licence : NASA data, public domain; acknowledge SPDF/OMNIWeb and the index providers · retrieved on Oct 23, 2026 · SHA-256 6de9b217bd4b…
Gopalswamy (2009)
Gopalswamy, N. (2009). Coronal mass ejections and space weather. In Climate and Weather of the Sun-Earth System (CAWSES), Terrapub, 77–120.
Licence : Published literature; cited
Gonzalez (1994)
Gonzalez, W. D., et al. (1994). What is a geomagnetic storm? Journal of Geophysical Research, 99(A4), 5771–5792. · doi:10.1029/93JA02867
Licence : Published literature; cited