Zobrazeno 1 - 10
of 124
pro vyhledávání: '"A.H. Gabriel"'
Autor:
A.H. Gabriel, null the GOLF Team
Publikováno v:
Advances in Space Research. 11:103-112
The GOLF experiment on the SOHO mission aims to study the internal structure of the sun by measuring the spectrum of global oscillations in the frequency range 10-7 to 10-2 Hz. Both p and g mode oscillations will be investigated, with the emphasis on
Autor:
A.H. Gabriel
Publikováno v:
Advances in Space Research. 11:253-261
In this review we discuss in general terms the relationship between some current ideas on the heating of the corona, the onset of the solar wind, and the observational possibilities which exist for making significant measurements over the next few ye
Autor:
K. Wilhelm, W.I. Axford, W. Curdt, E. Marsch, A.K. Richter, M. Grewing, A.H. Gabriel, P. Lemaire, J.-C. Vial, M.C.E. Huber, M. Kühne, S.D. Jordan, A.I. Poland, R.J. Thomas, J.G. Timothy
The experiment Solar Ultraviolet Measurements of Emitted Radiation (SUMER) is designed for the investigations of plasma flow characteristics, turbulence and wave motions, plasma densities and temperatures, structures and events associated with solar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a59dfbb35fbd7e359565f66237a01f36
https://doi.org/10.1016/b978-0-08-042049-3.50027-2
https://doi.org/10.1016/b978-0-08-042049-3.50027-2
Autor:
P. Faucher, J. Dubau, S. Volonte, F. Bely Dubau, A.H. Gabriel, L. Steenman-Clark, M. Loulergue
Publikováno v:
Le Journal de Physique Colloques. 40:C1-98
Resonance lines of highly ionized H and He-like ions and their associated sa- tellite lines are used to determine the electron temperature and the transient state of the plasma in solar flares. The intensity ratio of the satellite lines l~~nll-ls2~nL
Publikováno v:
Le Journal de Physique Colloques. 49:C1-325
Analysis of solar flares using the data from the Bent Crystal Spectrometer on the SMM solar flare satellite, shows a thermal plasma which expands vertically at a velocity of up to 350 km s−1. This plasma, at a temperature of the order 25 106K is ob
Autor:
K. W. Hill, S. Volonté, A.H. Gabriel, S. von Goeler, N. R. Sauthoff, J. Dubau, F. Bely-Dubau, P. Faucher, Manfred Bitter
Publikováno v:
Physics Letters A. 93:189-192
The FeXXV dielectronic recombination rate coefficient associated with the 1s-2p core excitation has been measured as a function of the electron temperature in the range from 0.9–3 keV from the observations of the satellite lines emitted from the PL
Autor:
R.W. Nicholls, S. Sahal, A.H. Gabriel, T. Kato, F.J. Lovas, S.L. Mandel’shtam, H. Nussbaumer, W.H. Parkinson, Z.R. Rudzigas, W.L. Wiese
Publikováno v:
Transactions of the International Astronomical Union. 20:111-117
The Commission has, since its inception, been devoted to the continually increasing needs of astronomy and astrophysics for reliable atomic and molecular data a) for diagnostic interpretation of astronomical observations, and b) for support of theore
Publikováno v:
International Astronomical Union Colloquium. 102:235-238
We present a revised theory and atomic model for the line intensities emitted by O VII, taking into account all of the processes responsible for the emission. This is used to provide a revision of the density measurements made during solar flares, as
Publikováno v:
International Astronomical Union Colloquium. 86:13-16
The relative concentrations of different ionization stages of iron are measured using the spectral emission of plasmas formed during solar flares. This is an extension of a study on the ionization balance of heavy elements, initiated with the analysi
Autor:
L.A. Vainshtein, J. Dubau, A.H. Gabriel, F. Bely-Dubau, M. Cornille, Y.A. Mikhailov, A.V. Rode, P. Faucher, M. Loulergue, U I Safronova
Publikováno v:
Le Journal de Physique Colloques. 50:C1-589
Satellite lines of the Phosphorus H-like and He-like resonance lines have been observed in the DELPHiN plasma laser device at the Lebedev Institute in Moscow. Analysis of some wavelength ranges i s carried out by adjusting a theoretical spectrum to t