Volume 566, June 2014
|Number of page(s)||1|
|Section||Interstellar and circumstellar matter|
|Published online||26 June 2014|
Diagnostics of interstellar hydrogen in the heliosphere
UV optical measurements of the Nozomi spacecraft interpreted with a two-component LIC-flow model (Corrigendum)
1 Department of Geophysics, University of Tohoku, 980-8577 Miyagi, Sendai, Japan
2 Space Research Centre PAS, Bartycka 18A, 00-716 Warsaw, Poland
3 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 229-8510 Kanagawa, Sagamihara, Japan
4 Japan Society for the Promotion of Science, 100084 Beijing, PR China
5 Department of Earth and Planetary Science, University of Hokkaido, 001-0021 Hokkaido, Japan
6 Department of Physics, College of Science, Rikkyo University, 171-8501 Tokyo, Japan
7 Department of Earth and Planetary Science, University of Tokyo, 113-0033 Tokyo, Japan
8 Earth Observation Research Center, Japan Aerospace Exploration Agency, 305-8505 Ibaraki, Tsukuba, Japan
Key words: Sun: UV radiation / ISM: atoms / ultraviolet: ISM / errata, addenda
We found a typographical error regarding the uncertainty of the helium flow direction in our published paper Nakagawa et al. (2008). The helium flow direction should be (258.7 ± 8.0°,3.4 ± 8.0°) instead of (258.7 ± 3.4°). As a consequence, the description for the helium flow direction in page 39 has to be replaced by “Residuals of simulated intensities with respect to observations attained minimum values for a downwind direction of (78.78 ± 8.0°,−3.48 ± 8.0°), corresponding to an upwind direction of (258.78 ± 8.0°,3.48 ± 8.0°).” All conclusions of the original paper remain unaffected. H. Nakagawa is grateful to Priscilla Frisch for pointing out this error.
© ESO, 2014
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