Zobrazeno 1 - 10
of 26
pro vyhledávání: '"L. D. de Feiter"'
Publikováno v:
Solar Physics. 47:117-126
Examination of X-ray images obtained by the S-054 X-ray spectrographic telescope on Skylab shows the presence of some atypical X-ray emitting coronal structures in active regions which are not consistent with potential extrapolations of photospheric
Autor:
L. D. De Feiter
Publikováno v:
Space Science Reviews. 17:181-193
This paper discusses some of the well-documented flare phenomena and possible analogies with magnetospheric substorm phenomena. Such analogies do exist, but also important differences. The combination of forces from magnetospheric and solar physicist
Autor:
L. D. De Feiter
Publikováno v:
Symposium - International Astronomical Union. 68:283-297
This review discusses the available observational material of solar hard X-ray bursts, their interpretation in terms of a model of the source region and their relation with other flash-phase phenomena, in particular the impulsive microwave bursts.
Autor:
K. O. Kiepenheuer, G. Newkirk, V. Bumba, A. Bruzek, L. W. Acton, L. D. de Feiter, J. T. Jefferies, V. A. Krat, F. Moriyama, P. Simon
Publikováno v:
Transactions of the International Astronomical Union. 16:13-54
Autor:
L. D. de Feiter, Z. Švestka
Publikováno v:
Solar Physics. 41:415-424
The Lyman spectrum of hydrogen has been computed for a number of flare models, characterized by the column density of hydrogen atoms in the ground state (N1), the electron density (ne) and the electron temperature (Te). Broadening by the thermal Dopp
Publikováno v:
Planetary and Space Science. 2:223-227
On the basis of a 24-hr patrol of solar radio noise established since the beginning of the International Geophysical Year, an identification is attempted of those solar flares which, on account of their associated radio responses, most probably were
Autor:
L. D. De Feiter
Publikováno v:
International Astronomical Union Colloquium. 14:827-842
Recent observations of the energetic particles produced in solar flares indicate that the production of electrons, with energies up to about 100 keV, is a fairly common feature of small flares. In those flares the acceleration of protons and other nu
Autor:
C. de Jager, L. D. de Feiter
Publikováno v:
Solar Physics. 28:183-186
We define superthermal plasma nodules as bright points (diameter ≲ 20″), visible on high resolution X-ray heliograms. Flares appear to show a strong tendency to occur at the places of these nodules. There are indications that (part of) the hot pl
Autor:
C. de Jager, D. G. King-Hele, John Heise, P. L´ena, R. Somoza, Per Olof Lindblad, H. W. Ritchey, L. D. de Feiter
Publikováno v:
Space Science Reviews. 10:737-740
Publikováno v:
Solar Physics. 17:277-283