Zobrazeno 1 - 10
of 628
pro vyhledávání: '"Moebius E"'
Autor:
Islam, H., Schwadron, N., Moebius, E., Rahmanifard, F., Sokol, J. M., Galli, A., McComas, D. J., Wurz, P., Fuselier, S. A., Fairchild, K., Heirtzler, D.
The IBEX-Lo instrument on the Interstellar Boundary Explorer (IBEX) mission observes primary and secondary interstellar helium in its 4 lowest energy steps. Observations of these helium populations have been systematically analyzed and compared to si
Externí odkaz:
http://arxiv.org/abs/2409.11784
Direct-sampling observations of interstellar neutral (ISN) species and their secondary populations give information about the physical state of the local interstellar medium and processes occuring in the outer heliosheath. Such observations are perfo
Externí odkaz:
http://arxiv.org/abs/2309.06931
Autor:
Swaczyna, P., Bzowski, M., Heerikhuisen, J., Kubiak, M. A., Rahmanifard, F., Zirnstein, E. J., Fuselier, S. A., Galli, A., McComas, D. J., Möbius, E., Schwadron, N. A.
In situ observations of interstellar neutral (ISN) helium atoms by the IBEX-Lo instrument onboard the Interstellar Boundary Explorer (IBEX) mission are used to determine the velocity and temperature of the pristine very local interstellar medium (VLI
Externí odkaz:
http://arxiv.org/abs/2307.06694
Autor:
Rahmanifard, F., Swaczyna, P., Zirnstein, E. J., Heerikhuisen, J., Galli, A., Sokół, J. M., Schwadron, N. A., Möbius, E., McComas, D. J., Fuselier, S. A.
Angular scattering in charge exchange and elastic collisions between interstellar ions and neutral (ISN) atoms has been assumed to be negligible in previous studies. Here, we investigated the momentum transfer associated with the angular scattering o
Externí odkaz:
http://arxiv.org/abs/2306.04598
Autor:
Swaczyna, P., Bzowski, M., Fuselier, S. A., Galli, A., Heerikhuisen, J., Kubiak, M. A., McComas, D. J., Möbius, E., Rahmanifard, F., Schwadron, N. A.
The IBEX-Lo instrument on the Interstellar Boundary Explorer (IBEX) mission measures interstellar neutral (ISN) helium atoms. The detection of helium atoms is made through negative hydrogen (H$^-$) ions sputtered by the helium atoms from the IBEX-Lo
Externí odkaz:
http://arxiv.org/abs/2303.08195
A good understanding of the ionization rates of neutral species in the heliosphere is important for studies of the heliosphere and planetary atmospheres. So far, the intensities of the ionization reactions have been studied based on observations of t
Externí odkaz:
http://arxiv.org/abs/2301.10793
We analyze the reasons for the correlation between the temperature, direction, and speed of the interstellar neutral gas inflow into the heliosphere, obtained in analyzes of observations performed by the IBEX-Lo instrument onboard Interstellar Bounda
Externí odkaz:
http://arxiv.org/abs/2208.14101
Autor:
Swaczyna, P., Kubiak, M. A., Bzowski, M., Bower, J., Fuselier, S. A., Galli, A., Heirtzler, D., McComas, D. J., Möbius, E., Rahmanifard, F., Schwadron, N. A.
The IBEX-Lo instrument on board the Interstellar Boundary Explorer (IBEX) mission samples interstellar neutral (ISN) helium atoms penetrating the heliosphere from the very local interstellar medium (VLISM). In this study, we analyze the IBEX-Lo ISN h
Externí odkaz:
http://arxiv.org/abs/2201.05463
Autor:
Bzowski, M., Czechowski, A., Frisch, P. C., Fuselier, S. A., Galli, A., Grygorczuk, J., Heerikhuisen, J., Kubiak, M. A., Kucharek, H., McComas, D. J., Moebius, E., Schwadron, N. A., Slavin, J., Sokol, J. M., Swaczyna, P., Wurz, P., Zirnstein, E. J.
Interstellar neutral gas atoms penetrate the heliopause and reach 1~au, where they are detected by IBEX. The flow of neutral interstellar helium through the perturbed interstellar plasma in the outer heliosheath (OHS) results in creation of the secon
Externí odkaz:
http://arxiv.org/abs/1907.09645
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