Zobrazeno 1 - 10
of 108
pro vyhledávání: '"Steven T. Suess"'
Autor:
Robert J. Leamon, Barbara A. Emery, Peter Riley, Deborah A. Haber, David F. Webb, P. K. Manoharan, Bernard V. Jackson, Patrick S. McIntosh, Antoinette B. Galvin, Gordon Petrie, Charles N. Arge, Brian T. Welsch, Thomas N. Woods, Jiuhou Lei, Sarah Gibson, M. Leila Mays, Simon Plunkett, Elizabeth A. Jensen, P. Schroeder, Liying Qian, Munetoshi Tokumaru, Steven T. Suess, Giuliana de Toma, Mario M. Bisi, Barbara J. Thompson
Publikováno v:
Solar Physics. 274:29-56
We present an overview of the data and models collected for the Whole Heliosphere Interval, an international campaign to study the three-dimensional solar–heliospheric–planetary connected system near solar minimum. The data and models correspond
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b270abc175ff331c8b8690678c98d7b4
https://doi.org/10.1007/s11207-011-9891-6
https://doi.org/10.1007/s11207-011-9891-6
Publikováno v:
The Astrophysical Journal. 668:1221-1231
We show that the strength (B(sub F1are)) of the magnetic field in the area covered by the flare arcade following a CME-producing ejective solar eruption can be estimated from the final angular width (Final Theta(sub CME)) of the CME in the outer coro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1cfb38eb8de13ea12a84acdc8f8e89cb
https://doi.org/10.1086/521215
https://doi.org/10.1086/521215
Autor:
Steven T. Suess, Alessandro Bemporad, Nathan A. Schwadron, Giannina Poletto, Yuan-Kuen Ko, John C. Raymond, H. A. Elliott
Publikováno v:
The Astrophysical Journal. 638:1110-1128
We report on SOHO UVCS observations of the coronal restructuring following a coronal mass ejection (CME) on 2002 November 26, at the time of a SOHO-Ulysses quadrature campaign. Starting about 1.5 hr after a CME in the northwest quadrant, UVCS began t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bed5e7ee7b872dd0b5d24df12afcbbab
https://doi.org/10.1086/497529
https://doi.org/10.1086/497529
Autor:
Steven T. Suess, Steven Nerney
Publikováno v:
The Astrophysical Journal. 624:378-391
Slow solar wind is believed to arise in the legs or near the cusp of streamers, inside the brightness boundary. In an earlier study, we used an analytic model of flow in this layer to analyze the effect of the magnetic field on the geometry of the fl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2143446e868393d881f480cc80fed2be
https://doi.org/10.1086/428924
https://doi.org/10.1086/428924
Autor:
Giannina Poletto, Steven T. Suess
Publikováno v:
Highlights of Astronomy. 13:213-241
As knowledge of the Sun and the heliosphere grows, it is becoming not only possible but preferable to view the global structure, the interaction with the local interstellar medium, and changes over a solar cycle as the behavior of an integrated syste
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3d85e500669d97cabeef1b9330fa83f1
https://doi.org/10.1017/s153929960001577x
https://doi.org/10.1017/s153929960001577x
Autor:
Alessandro Bemporad, Nathan A. Schwadron, Giannina Poletto, Thomas H. Zurbuchen, H. A. Elliott, Yuan-Kuen Ko, Steven T. Suess
Publikováno v:
The Astrophysical Journal. 613:L173-L176
We present here evidence for highly ionized Fe observed both in the corona, in the aftermath of a coronal mass ejection, and, after propagation, in situ. The apparent source temperature is greater than 6 MK. To our knowledge, this is the first time t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::85bcf4b948fda407b5fd3a2df5ec94bd
https://doi.org/10.1086/425136
https://doi.org/10.1086/425136
Publikováno v:
The Astrophysical Journal. 605:511-520
Measurements by Ulysses in the high-speed polar solar wind have shown the wind to carry some fine-scale structures in which the magnetic field reverses direction by having a switchback fold in it. The lateral span of these magnetic switchbacks, trans
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::00c6cdccc20ab83cfc7cfa7d1d731a98
https://doi.org/10.1086/381240
https://doi.org/10.1086/381240
Autor:
Steven T. Suess, S. Nerney
Publikováno v:
Advances in Space Research. 33:668-675
Streamers can extend to many solar radii but the closed field regions, or helmets, reach no higher than 2-4 solar radii. The brightness boundary defining streamers is therefore a boundary between different flow regimes rather than between static plas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::17333aa505b562c2805f65d933f3e512
https://doi.org/10.1016/s0273-1177(03)00237-0
https://doi.org/10.1016/s0273-1177(03)00237-0
Autor:
Giannina Poletto, Pete Riley, Yuan-Kuen Ko, Alessandro Bemporad, Marco Romoli, T. Z. Zurbuchen, Susanna Parenti, Steven T. Suess
Publikováno v:
The Astrophysical Journal. 593:1146-1163
In this paper we report on observations acquired by the Ultra Violet Coronagraph Spectrometer (UVCS) aboard the Solar and Heliospheric Observatory (SOHO), from 10 to 17 June 2000, at the time of a SOHO-Sun-Ulysses quadrature. UVCS took data at 1.6 an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4cbe978018266bd6fcf49532c7bc7b20
https://doi.org/10.1086/376605
https://doi.org/10.1086/376605
Autor:
Steven Nerney, Steven T. Suess
Publikováno v:
The Astrophysical Journal. 565:1275-1288
It is possible for flow tubes adjacent to closed magnetic field lines on the boundaries of streamers to have spreading factors that change rapidly according to height. Mathematical models in this thin layer are prone to uncertainties. In this paper w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e59ba09d49ab78e75cace235333ae019
https://doi.org/10.1086/324697
https://doi.org/10.1086/324697