... ultraviolet region P. Beiersdorfer Lawrence Livermore National Laboratory, Livermore, California 94550 G. V. Browna ) University of Maryland, College Park, Maryland 20742 R. Goddard and B. J. Wargelin Harvard-Smithsonian Center for Astrophysics, Cambridge ...
... PROJECT TITLE: Testing Solar Wind Models with data from the SOHO Ultraviolet Coronagraph Spectrometer . Abstract: . ... One of the major discoveries from the SOHO Ultraviolet Coronagraph Spectrometer is that ions in the solar corona are heated to ...
... PROJECT TITLE: Testing Solar Wind Models with data from the SOHO Ultraviolet Coronagraph Spectrometer . Abstract: . ... One of the major discoveries from the SOHO Ultraviolet Coronagraph Spectrometer is that ions in the solar corona are heated to ...
... for the 10--60 Ъ A Extreme Ultraviolet Region,'' P. Beiersdorfer, G.V. Brown, R ... B.J. Wargelin, in XнRay and Extreme Ultraviolet Optics, ed. R.B. Hoover and A.B.C ...
... Ultraviolet Mg II emission is found that signifies a stellar chromosphere -- and ... of these chromospheres can be detected in ultraviolet spectra of the same or similar ...
... 2008 Ultraviolet Observations of the X-ray Photoionized Wind of Cygnus X-1 during X ... 1997 Hopkins Ultraviolet Telescope Observations of Her X-1 (B. Boroson, W.P. Blair ...
... 2008 Ultraviolet Observations of the Xray Photoionized Wind of Cygnus X1 during X ... 1997 Hopkins Ultraviolet Telescope Observations of Her X1 (B. Boroson, W.P. Blair ...
... Comparisons among farultraviolet (FUV), extremeultraviolet (EUV), Xray lines xviii particularly useful, since strong 2 EUV lines essentially entirely produced by direct collisional excitation and should easier interpret than FUV Xray lines, which ...
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