IBEX : THE FIRST FIVE YEARS (2009-2013)

The Interstellar Boundary Explorer (IBEX) returned its first five years of scientific observations from 2009 to 2013. In this study, we examine, validate, initially analyze, and provide to the broad scientific community this complete set of energetic neutral atom (ENA) observations for the first tim...

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Veröffentlicht in:The Astrophysical journal. Supplement series 2014-08, Vol.213 (2), p.1-28
Hauptverfasser: McComas, D J, Allegrini, F, BZOWSKI, M, Dayeh, M A, DEMAJISTRE, R, FEINSTEN, H O, Fuselier, S A, Gruntman, M, Janzen, P H, Kubiak, M A
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container_end_page 28
container_issue 2
container_start_page 1
container_title The Astrophysical journal. Supplement series
container_volume 213
creator McComas, D J
Allegrini, F
BZOWSKI, M
Dayeh, M A
DEMAJISTRE, R
FEINSTEN, H O
Fuselier, S A
Gruntman, M
Janzen, P H
Kubiak, M A
description The Interstellar Boundary Explorer (IBEX) returned its first five years of scientific observations from 2009 to 2013. In this study, we examine, validate, initially analyze, and provide to the broad scientific community this complete set of energetic neutral atom (ENA) observations for the first time. IBEX measures the fluxes of ENAs reaching 1 AU from sources in the outer heliosphere and most likely the very nearby interstellar space beyond the heliopause. The data, maps, and documentation provided in this study represent the fourth major release of the IBEX data, incorporate important improvements, and should be used for future studies and as the citable reference for the current version of the IBEX data. In this study, we also examine five years of time evolution in the outer heliosphere and the resulting ENA emissions. These observations show a complicated variation with a general decrease in ENA fluxes from 2009 to 2012 over most regions of the sky, consistent with a 2-4 year recycle time for the previously decreasing solar wind flux. In contrast, the heliotail fluxes continue to decrease, again consistent with a significantly more distant source in the downwind direction. Finally, the Ribbon shows the most complicated time variations, with a leveling off in the southern hemisphere and continued decline in the northern one; these may be consistent with the Ribbon source being significantly farther away in the north than in the south. Together, the observations and results shown in this study expose the intricacies of our heliosphere's interaction with the local interstellar medium.
doi_str_mv 10.1088/0067-0049/213/2/20
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subjects ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
ATOMS
Boundaries
EMISSION
Emission analysis
Fluxes
Heliopause
HELIOSPHERE
INTERSTELLAR SPACE
Local interstellar medium
Neutral atoms
Ribbons
SKY
SOLAR WIND
SOUTHERN HEMISPHERE
title IBEX : THE FIRST FIVE YEARS (2009-2013)
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