Table 2

Magnitudes of largest GLEs in solar cycles 17–23 (in %) over the pre-event GCR level.

Rank Date IC/Station MT/Station NM/Station Estimate/Reference
1 – GLE05 23 Feb. 1956 300%, 2.05 GV, Moscow, 15-min 280%, 2.32 GV, London, 15-min 4554%, 1.70 GV, Leeds, 15-min 9000%, Duggal (1979)
2 – GLE69 20 Jan. 2005 N.O. 13%, 1.89 GV, GRAND- project, 1-min D’Andrea & Poirier (2005) 5500%, 0.02 GV, SOPO NM64, 1-min http://cosrays.izmiran.ru No Duggal’s estimate
3 – GLE04 19 Nov. 1949 40%, 2.19 GV, Cheltenham, 15-min 70%, 0.64 GV, Ottawa, 15-min 563%, 1.70 GV, Manchester, 60-min 2000%, Duggal (1979)
4 – GLE03 25 Jul. 1946 22%, 2.19 GV, Cheltenham, 15-min 13%, 1.70 GV, Manchester, 60-min N.O. 1100%, Duggal (1979)
5 – GLE02 07 Mar. 1942 15%, 2.19 GV, Cheltenham, 15-min 27%, Friedrichshafen, 60-min N.O. 750%, Duggal (1979)
6 – GLE01 28 Feb. 1942 15.5%, 0.03 GV, Godhavn, 15-min 00%, 4.06 GV – no increase, Friedrichshafen, 60-min N.O. 600%, Duggal (1979)
7 – GLE42 29 Sep. 1989 N.O. 41%, 0.07 GV, Inuvik, 5-min Smart & Shea (1991) >400%, 0.72 GV, Calgary, 5-min http://cosrays.izmiran.ru No Duggal’s estimate

Notes.

  1. For technical reasons, when registering the early GLEs, the averaging time intervals (given after the name of CR station) were different for different detectors and may be changed from 1 h (60 min) to 1 min.

  2. Maximum amplitudes of the first 4 GLEs have been reduced to a 15-minute averaging time interval (Dorman, 1957).

  3. Ionization chamber (IC) events have been normalized to correspond to the increase that a high-latitude neutron monitor (NM) would have observed at sea level (Duggal, 1979).

  4. Neutron component records for the GLE04 in Manchester were not obtained with the help of a “classical” NM, but with the help of the neutron detector that consisted of boron-trifluoride filled counters embedded in a “pile” built of high purity graphite (Adams, 1950).

  5. The effective vertical cutoff rigidities of the neutron monitors (in GV units) are indicated for the CR stations with maximal observed amplitude of the corresponding GLEs.

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