Altmetric

Characterizing cometary electrons with kappa distributions

File Description SizeFormat 
Broiles_et_al-2016-Journal_of_Geophysical_Research-_Space_Physics.pdfPublished version2.93 MBAdobe PDFView/Open
Title: Characterizing cometary electrons with kappa distributions
Authors: Broiles, TW
Livadiotis, G
Burch, JL
Chae, K
Clark, G
Cravens, TE
Davidson, R
Eriksson, A
Frahm, RA
Fuselier, SA
Goldstein, J
Goldstein, R
Henri, P
Madanian, H
Mandt, K
Mokashi, P
Pollock, C
Rahmati, A
Samara, M
Schwartz, SJ
Item Type: Journal Article
Abstract: The Rosetta spacecraft has escorted comet 67P/Churyumov-Gerasimenko since 6 August 2014 and has offered an unprecedented opportunity to study plasma physics in the coma. We have used this opportunity to make the fi rst characterization of cometary electrons with kappa distributions. Two three-dimensional kappa functions were fi t to the observations, which we interpret as two populations of dense and warm (density=10cm 3 , temperature=2×10 5 K, invariant kappa index=10 > 1000), and rare fi ed and hot (density=0.005cm 3 , temperature=5×10 5 K, invariant kappa index=1 – 10) electrons. We fi t the observations on 30 October 2014 when Rosetta was 20km from 67P, and 3AU from the Sun. We repeated the analysis on 15 August 2015 when Rosetta was 300km from the comet and 1.3AU from the Sun. Comparing the measurements on both days gives the fi rst comparison of the cometary electron environment between a nearly inactive comet far from the Sun and an active comet near perihelion. We fi nd that the warm population density increased by a factor of 3, while the temperature cooled by a factor of 2, and the invariant kappa index was unaffected. We fi nd that the hot population density increased by a factor of 10, while the temperature and invariant kappa index were unchanged. We conclude that the hot population is likely the solar wind halo electrons in the coma. The warm population is likely of cometary origin, but its mechanism for production is not known.
Issue Date: 12-Aug-2016
Date of Acceptance: 21-Jul-2016
URI: http://hdl.handle.net/10044/1/42807
DOI: https://dx.doi.org/10.1002/2016JA022972
ISSN: 2169-9356
Publisher: American Geophysical Union (AGU)
Start Page: 7407
End Page: 7422
Journal / Book Title: Journal of Geophysical Research. Solid Earth
Volume: 121
Issue: 8
Copyright Statement: © 2016. American Geophysical Union. All Rights Reserved.
Sponsor/Funder: Science and Technology Facilities Council (STFC)
The Leverhulme Trust
Funder's Grant Number: ST/K001051/1
RF-2015-188
Keywords: Science & Technology
Physical Sciences
Astronomy & Astrophysics
GIACOBINI-ZINNER
SOLAR-WIND
SPACE PLASMAS
BOW SHOCK
ROSETTA
67P/CHURYUMOV-GERASIMENKO
COMA
ION
HALLEY
SENSOR
Publication Status: Published
Appears in Collections:Space and Atmospheric Physics
Physics
Faculty of Natural Sciences



Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

Creative Commons