Nature Communications (Jul 2018)
On the origin of molecular oxygen in cometary comae
- K. L. Heritier,
- K. Altwegg,
- J.-J. Berthelier,
- A. Beth,
- C. M. Carr,
- J. De Keyser,
- A. I. Eriksson,
- S. A. Fuselier,
- M. Galand,
- T. I. Gombosi,
- P. Henri,
- F. L. Johansson,
- H. Nilsson,
- M. Rubin,
- C. Simon Wedlund,
- M. G. G. T. Taylor,
- E Vigren
Affiliations
- K. L. Heritier
- Department of Physics, Imperial College London
- K. Altwegg
- Physikalisches Institut, University of Bern
- J.-J. Berthelier
- LATMOS/IPSL-CNRS-UPMC-UVSQ
- A. Beth
- Department of Physics, Imperial College London
- C. M. Carr
- Department of Physics, Imperial College London
- J. De Keyser
- BIRA-IASB, Royal Belgian Institute for Space Aeronomy
- A. I. Eriksson
- Swedish Institute of Space Physics, Ångström Laboratory
- S. A. Fuselier
- Southwest Research Institute
- M. Galand
- Department of Physics, Imperial College London
- T. I. Gombosi
- Department of Atmospheric, Oceanic and Space Sciences, University of Michigan
- P. Henri
- LPC2E, CNRS
- F. L. Johansson
- Swedish Institute of Space Physics, Ångström Laboratory
- H. Nilsson
- Swedish Institute of Space Physics
- M. Rubin
- Physikalisches Institut, University of Bern
- C. Simon Wedlund
- Department of Physics, University of Oslo
- M. G. G. T. Taylor
- European Space Agency
- E Vigren
- LATMOS/IPSL-CNRS-UPMC-UVSQ
- DOI
- https://doi.org/10.1038/s41467-018-04972-5
- Journal volume & issue
-
Vol. 9,
no. 1
pp. 1 – 4
Abstract
No abstracts available.