ERRATUM: "SPECTRAL PROPERTIES OF LARGE GRADUAL SOLAR ENERGETIC PARTICLE EVENTS. I. FE, O, AND SEED MATERIAL" (vol 816, pg 68, 2016)

作者：Desai M I^*; Mason G M; Dayeh M A; Ebert R W; Mccomas D J; Li G; Cohen C M S; Mewaldt R A; Schwadron N A; Smith C W

来源：Astrophysical Journal, 2016, 831(2): 209.

DOI：10.3847/0004-637X/831/2/209

Due to an error at the publisher, in the published article multiple values were incorrect in Table 1 and in the text. Accordingly, Table 1 has been reproduced below, and the values in the text should be cited as follows.
In the final paragraph of Section 3.2, the final sentence should read, "correlation coefficient r similar to 0.103 for N = 36 has a > 55% probability of being exceeded by two uncorrelated quantities."
In the first paragraph of Section 3.5, the third sentence should read, "We used the technique described in Desai et al. ( 2003, 2006) to subtract the background and contributions to spill-over from the more abundant He-4 peak to the He-3 mass range between 2.8 and 3.2 AMU."
In the first paragraph of Section 3.7, the second sentence should read, "We identify a new set of variables by eliminating those that do not contribute significantly to the overall variability in the data set through a multivariate, principal component analysis (PCA) that uses the Karhunen-Loeve Transform method (see Murtagh & Heck 1987) for 25 SEP events using the following 8 variables: O low-energy and high-energy SEP Band-parameters, Theta, gamma(a) and gamma(b); O break energy E-B; CME speed V-CME; flare longitude; peak proton flux P-P; the Fe/O ratios at similar to 15-21 and similar to 0.16-0.23 MeV nucleon(-1) Fe/O18 and Fe/O-0.2."
IOP Publishing sincerely regrets these errors.

• 出版日期2016-11-10