Zobrazeno 1 - 10
of 843
pro vyhledávání: '"Funsten H"'
Autor:
Livadiotis, G., McComas, D. J., Funsten, H. O., Schwadron, N. A., Szalay, J. R., Zirnstein, E.
We derive annual skymaps of the proton temperature in the inner heliosheath (IHS), and track their temporal evolution over the years from 2009 to 2016 of Interstellar Boundary Explorer observations. Other associated thermodynamic parameters also dete
Externí odkaz:
http://arxiv.org/abs/2209.14897
Autor:
Frisch, P. C., Berdyugin, A. B., Piirola, V., Cole, A. A., Hill, K., Harlingten, C., Magalhaes, A. M., Seriacopi, D. B., Ferrari, T., Ribeiro, N. L., Santos, F. P., Cotton, D. V., Bailey, J., Kedziora-Chudczer, L., Marshall, J. P., Bott, K., Wiktorowicz, S. J., Heiles, C., McComas, D. J., Funsten, H. O., Schwadron, N. A., Livadiotis, G., Redfield, S.
Starlight that becomes linearly polarized by magnetically aligned dust grains provides a viable diagnostic of the interstellar magnetic field (ISMF). A survey is underway to map the local ISMF using data collected at eight observatories in both hemis
Externí odkaz:
http://arxiv.org/abs/1806.02806
Autor:
Galli, A., Wurz, P., Schwadron, N. A., Kucharek, H., Möbius, E., Bzowski, M., M., J., Sokół, Kubiak, M. A., Fuselier, S. A., Funsten, H. O., McComas, D. J.
We present a comprehensive study of energetic neutral atoms (ENAs) of 10 eV to 2.5 keV from the downwind hemisphere of the heliosphere. These ENAs are believed to originate mostly from pickup protons and solar wind protons in the inner heliosheath. T
Externí odkaz:
http://arxiv.org/abs/1712.01151
Autor:
McComas, D. J., Zirnstein, E. J., Bzowski, M., Dayeh, M. A., Funsten, H. O., Fuselier, S. A., Janzen, P. H., Kubiak, M. A., Kucharek, H., Möbius, E., Reisenfeld, D. B., Schwadron, N. A., Sokół, J. M., Szalay, J. R., Tokumaru, M.
Publikováno v:
The Astrophysical Journal Supplement Series, 229:41 (32pp), 2017 April
The Interstellar Boundary Explorer (IBEX) has now operated in space for 7 years and returned nearly continuous observations that have led to scientific discoveries and reshaped our entire understanding of the outer heliosphere and its interaction wit
Externí odkaz:
http://arxiv.org/abs/1704.06316
Autor:
Swaczyna, P., Bzowski, M., Christian, E. R., Funsten, H. O., McComas, D. J., Schwadron, N. A.
Publikováno v:
ApJ 823 (2016), 119
Maps of Energetic Neutral Atom (ENA) fluxes obtained from Interstellar Boundary Explorer (IBEX) observations revealed a bright structure extending over the sky, subsequently dubbed the IBEX ribbon. The ribbon had not been expected from the existing m
Externí odkaz:
http://arxiv.org/abs/1603.09134
Autor:
Frisch, P. C., Berdyugin, A., Piirola, V., Magalhaes, A. M., Seriacopi, D. B., Wiktorowicz, S. J., Andersson, B-G, Funsten, H. O., McComas, D. J., Schwadron, N. A., Slavin, J. D., Hanson, A. J., Fu, C. -W.
The interstellar magnetic field (ISMF) near the heliosphere is a basic part of the solar neighborhood that can only be studied using polarized starlight. Results of an ongoing survey of polarized starlight are analyzed with the goal of linking the in
Externí odkaz:
http://arxiv.org/abs/1510.04679
Autor:
Frisch, P. C., Andersson, B-G, Berdyugin, A., Funsten, H. O., Magalhaes, A. M., McComas, D. J., Piirola, V., Schwadron, N. A., Seriacopi, D. B., Slavin, J. D., Wiktorowicz, S. J.
A recently discovered filament of polarized starlight that traces a coherent magnetic field is shown to have several properties that are consistent with an origin in the outer heliosheath of the heliosphere: (1) The magnetic field that provides the b
Externí odkaz:
http://arxiv.org/abs/1503.00353
Akademický článek
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Autor:
Frisch, P. C., Berdyugin, A., Funsten, H. O., Magalhaes, A. M., McComas, D. J., Piirola, V., Schwadron, N. A., Seriacopi, D. B., Wiktorowicz, S. J.
The local interstellar magnetic field affects both the heliosphere and the surrounding cluster of interstellar clouds (CLIC). Measurements of linearly polarized starlight provide the only test of the magnetic field threading the CLIC. Polarization me
Externí odkaz:
http://arxiv.org/abs/1409.5428
Autor:
Frisch, P. C., Andersson, B-G, Berdyugin, A., Piirola, V., DeMajistre, R., Funsten, H. O., Magalhaes, A. M., Seriacopi, D. B., McComas, D. J., Schwadron, N. A., Slavin, J. D., Wiktorowicz, S. J.
A key indicator of the galactic environment of the Sun is provided by the magnetic field in the interstellar medium (ISM), which influences the shape of the heliosphere. The direction of the nearby interstellar magnetic field (ISMF) is determined fro
Externí odkaz:
http://arxiv.org/abs/1206.1273