Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Neil F. Cramer"'
Autor:
Neil F. Cramer
Publikováno v:
The Physics of Alfvén Waves
Autor:
Neil F. Cramer
Publikováno v:
The Physics of Alfvén Waves
Autor:
Neil F. Cramer
Publikováno v:
The Physics of Alfvén Waves
Autor:
Neil F. Cramer
Publikováno v:
The Physics of Alfvén Waves
Autor:
Neil F. Cramer
Publikováno v:
The Physics of Alfvén Waves
Autor:
Neil F. Cramer
Publikováno v:
The Physics of Alfvén Waves
Publikováno v:
The Astrophysical Journal. 550:1075-1092
Recent high-resolution observations from photospheric magnetograms made with the SOHO/Michelson Doppler Imager instrument and the Swedish Vacuum Solar Telescope on La Palma showed that magnetic flux tubes in the quiet photospheric network of the sola
Publikováno v:
The Astrophysical Journal. 537:1063-1072
To explain the observed dynamics of the small-scale magnetic flux tubes in the quiet photospheric network, Furusawa & Sakai presented simulation results on the collision of two flux tubes. They found that shock waves appear during the collision of tw
Publikováno v:
New Aspects of Plasma Physics.
The occurrence of amplitude-modulated electrostatic and electromagnetic wavepackets in pair plasmas is investigated. A static additional charged background species is considered, accounting for dust defects or for heavy ion presence in the background
Autor:
David F. Webb, Jean-Louis Bougeret, Hilary V. Cane, Neil F. Cramer, Stephen W. Kahler, Masayoshi Kojima, Blai Sanahuja, Marek Vandas, Frank Verheest, Rudolf von Steiger
Publikováno v:
Transactions of the International Astronomical Union, Series A
XXVIth IAU General Assembly
XXVIth IAU General Assembly, Aug 2006, Prague, Czech Republic. pp.103-120, ⟨10.1017/S1743921306004406⟩
XXVIth IAU General Assembly
XXVIth IAU General Assembly, Aug 2006, Prague, Czech Republic. pp.103-120, ⟨10.1017/S1743921306004406⟩
Commission 49 covers research on the solar wind, shocks and particle acceleration, both transient and steady-state, e.g., corotating, structures within the heliosphere, and the termination shock and boundary of the heliosphere. During the last three
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3766f20768d59eaf31bb06339ddf0974
https://hal.science/hal-03802210
https://hal.science/hal-03802210