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
This article has no abstract.
Key words: Sun: UV radiation / ISM: atoms / ultraviolet: ISM / errata, addenda
© ESO, 2014
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