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Table 1 \(T-A\), \(\sqrt{\sigma _T \sigma _A}\), T / A separation, and success rate

From: Erratum to: The spatial density gradient of galactic cosmic rays and its solar cycle variation observed with the Global Muon Detector Network

 

Nagoya GG

GMDN

NMs

\(T - A\) (%)

 Daily

0.1504

0.1398

0.1090

 Hourly

0.1324

0.1258

\(\sqrt{\sigma _{T}\sigma _{A}}\) (%)

 Daily

0.0033

0.0044

0.0062

 Hourly

0.0016

0.0013

T / A separation

 Daily

46.2

31.5

17.8

 Hourly

81.2

96.6

Success rate (%)

 Daily

73.5

68.7

59.6

 Hourly

58.2

62.0

  1. Difference (\(T - A\)) between average \(\xi ^\mathrm{GEO}_z\)s in toward (T) and away (A) IMF sectors, geometric mean (\(\sqrt{\sigma _{T}\sigma _{A}}\)) of the standard errors of \(\xi ^\mathrm{GEO}_z\)s in T and A sectors, “T / A separation” (\(= (T - A)/\sqrt{\sigma _{T}\sigma _{A}}\)) and “success rate” (see text) derived from Nagoya GG-component, GMDN, and NM (Thule–McMurdo) data in 2006–2013 on daily and hourly bases