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Table 3 Estimated Dstmin based on formulae obtained from Wu and Lepping (2016) for a MC event that occurred on 17 March 2015

From: The first super geomagnetic storm of solar cycle 24: “The St. Patrick’s day event (17 March 2015)”

 

Event

Dstmin formulaa

Pred. Dst bmin

Source of \( B_{{z_{ \hbox{min} } }} \) c

Errors (%)

(a)

168 MCs

Dstmin = −3.30 + 6.82 × \( B_{{z_{ \hbox{min} } }} \)

−160.2

MC

29.8

(b)

168 MCs

Dstmin = 8.04 + 6.34 × \( B_{{z_{ \hbox{min} } }} \)

−137.8

Sheath or MC

39.6

(c)

94 MC SHOCK

Dstmin = −22.89 + 6.12 × \( B_{{z_{ \hbox{min} } }} \)

163.7

MC

28.2

(d)

94 MCSHOCK

Dstmin = 11.01 + 6.47 × \( B_{{z_{ \hbox{min} } }} \)

−137.8

Sheath or MC

39.6

(e)

94 MCSHOCK

Dstmin = 21.18 + 5.26 × \( B_{{z_{ \hbox{min} } }} \)

−142.2

Sheath

37.6

(f)

74 MCNOSHOCK

Dstmin = 4.18 + 5.83 × \( B_{{z_{ \hbox{min} } }} \)

−129.9

MC

43.0

(g)

83 MC1995–2003

Dstmin = 0.83 + 7.85 × \( B_{{z_{ \hbox{min} } }} \)

−179.7

MC

21.2

  1. aLinear-fitted function for Dstmin obtained from Wu and Lepping (2016)
  2. bPredicted Dstmin by using Dstmin formula listed in the left
  3. c \( B_{{z_{ \hbox{min} } }} \) = −23 nT within the MC event recorded from wind spacecraft
  4. Italics: the “best prediction” (with the lowest error) for Dstmin