Interplanetary coronal mass ejection observed at STEREO-A, Mars, comet 67P/Churyumov-Gerasimenko, Saturn, and New Horizons en-route to Pluto. Comparison of its Forbush decreases at 1.4, 3.1 and 9.9 AU

O. Witasse; B. Sánchez-Cano; M. Mays; P. Kajdič; H. Opgenoorth; H. Elliott; G. Richardson; I. Zouganelis; J. Zender; R. Wimmer-Schweingruber; L. Turc; M. Taylor; E. Roussos; A. Rouillard; I. Richter; J. Richardson; R. Ramstad; G. Provan; A. Posner; J. Plaut; D. Odstrcil; H. Nilsson; P. Niemenen; S. Milan; K. Mandt; H. Lohf; M. Lester; Jean-Pierre Lebreton; E. Kuulkers; N. Krupp; C. Koenders; M. James; D. Intzekara; M. Holmstrom; M. Hassler; S. Hall; J. Guo; R. Goldstein; C. Goetz; H. Glassmeier; V. Génot; H. Evans; J. Espley; N. Edberg; M. Dougherty; S. Cowley; J. Burch; E. Behar; S. Barabash; D. J. Andrews; N. Altobelli

doi:10.1002/2017JA023884

Interplanetary coronal mass ejection observed at STEREO-A, Mars, comet 67P/Churyumov-Gerasimenko, Saturn, and New Horizons en-route to Pluto. Comparison of its Forbush decreases at 1.4, 3.1 and 9.9 AU

O. Witasse ¹ B. Sánchez-Cano ² M. Mays ³ P. Kajdič H. Opgenoorth H. Elliott ⁴ G. Richardson ⁵ I. Zouganelis ⁶ J. Zender ¹ R. Wimmer-Schweingruber L. Turc ¹ M. Taylor ¹ E. Roussos ⁷ A. Rouillard ⁸ I. Richter ⁹ J. Richardson R. Ramstad ⁹ G. Provan ² A. Posner ¹⁰ J. Plaut ¹¹ D. Odstrcil H. Nilsson ¹² P. Niemenen ¹ S. Milan ² K. Mandt ¹³ H. Lohf M. Lester ² Jean-Pierre Lebreton ¹⁴ E. Kuulkers ¹ N. Krupp C. Koenders ⁹ M. James ² D. Intzekara ¹ M. Holmstrom ¹⁵ M. Hassler ¹⁶ S. Hall ² J. Guo ¹⁷ R. Goldstein ¹³ C. Goetz ¹⁸ H. Glassmeier V. Génot H. Evans ¹ J. Espley ¹⁹ N. Edberg ¹² M. Dougherty S. Cowley ² J. Burch E. Behar S. Barabash D. J. Andrews N. Altobelli ²⁰

1 ESTEC - European Space Research and Technology Centre

2 RSPP - Radio and Space Plasma Physics Group [Leicester]

University of Leicester

3 GSFC Heliophysics Science Division

GSFC - NASA Goddard Space Flight Center

4 SPRL - Space Physics Research Laboratory [Ann Arbor]

5 School of Life Sciences

6 LPP - Laboratoire de Physique des Plasmas

7 MPS - Max-Planck-Institut für Sonnensystemforschung

8 IRAP - Institut de recherche en astrophysique et planétologie

9 IGEP - Institut für Geophysik und Extraterrestrische Physik [Braunschweig]

10 NASA Headquarters

11 JPL - Jet Propulsion Laboratory

12 IRF - Swedish Institute of Space Physics [Uppsala]

13 SwRI - Southwest Research Institute [San Antonio]

14 LPC2E - Laboratoire de Physique et Chimie de l'Environnement et de l'Espace

15 IRF - Swedish Institute of Space Physics [Kiruna]

16 Universität Klangenfurt

17 Institute of Experimental and Applied Physics

18 Technische Universität Braunschweig [Braunschweig]

19 GSFC - NASA Goddard Space Flight Center

20 ESAC - European Space Astronomy Centre

Abstract : We discuss observations of the journey throughout the Solar System of a large interplanetary coronal mass ejection (ICME) that was ejected at the Sun on 14 October 2014. The ICME hit Mars on 17 October, as observed by the Mars Express, MAVEN, Mars Odyssey and MSL missions, 44 hours before the encounter of the planet with the Siding-Spring comet, for which the space weather context is provided. It reached comet 67P/Churyumov-Gerasimenko, which was perfectly aligned with the Sun and Mars at 3.1 AU, as observed by Rosetta on 22 October. The ICME was also detected by STEREO-A on 16 October at 1 AU, and by Cassini in the solar wind around Saturn on the 12 November at 9.9 AU. Fortuitously, the New Horizons spacecraft was also aligned with the direction of the ICME at 31.6 AU. We investigate whether this ICME has a non-ambiguous signature at New Horizons. A potential detection of this ICME by Voyager-2 at 110-111 AU is also discussed. The multi-spacecraft observations allow the derivation of certain properties of the ICME, such as its large angular extension of at least 116°, its speed as a function of distance, and its magnetic field structure at four locations from 1 to 10 AU. Observations of the speed data allow two different solar wind propagation models to be validated. Finally, we compare the Forbush decreases (transient decreases followed by gradual recoveries in the galactic cosmic ray intensity) due to the passage of this ICME at Mars, comet 67P and Saturn.

Document type :

Journal articles

Domain :

Sciences of the Universe [physics]

Sciences of the Universe [physics] / Astrophysics [astro-ph]

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Interplanetary coronal mass ejection observed at STEREO-A, Mars, comet 67P/Churyumov-Gerasimenko, Saturn, and New Horizons en-route to Pluto. Comparison of its Forbush decreases at 1.4, 3.1 and 9.9 AU

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Interplanetary coronal mass ejection observed at STEREO-A, Mars, comet 67P/Churyumov-Gerasimenko, Saturn, and New Horizons en-route to Pluto. Comparison of its Forbush decreases at 1.4, 3.1 and 9.9 AU

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