Zobrazeno 1 - 10
of 18
pro vyhledávání: '"P. L. Bornmann"'
Autor:
P. L. Bornmann
Publikováno v:
Solar System Plasma Physics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::97208703457d7ca7bc117c1ede851185
https://doi.org/10.1029/gm054p0209
https://doi.org/10.1029/gm054p0209
Autor:
P. L. Bornmann, Donald L. Shaw
Publikováno v:
Solar Physics. 150:127-146
Multiple linear regression analysis was used to derive the effective solar flare contributions of each of the McIntosh classification parameters. The best fits to the combined average number of M- and X-class X-ray flares per day were found when the
Autor:
P. L. Bornmann
Publikováno v:
Reviews of Geophysics. 29:915-924
Research on solar X-ray phenomena performed by American scientists during 1987-1990 is reviewed. Major topics discussed include solar images observed during quiescent times, the processes observed during solar flares, and the coronal, interplanetary,
Autor:
Donald L. Shaw, P. L. Bornmann
Publikováno v:
Lecture Notes in Physics ISBN: 9783540552468
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::41c12faeae36f5223dc6aa388339e0a9
https://doi.org/10.1007/3-540-55246-4_120
https://doi.org/10.1007/3-540-55246-4_120
Autor:
P. L. Bornmann, J. R. Lemen
Publikováno v:
Lecture Notes in Physics ISBN: 9783540552468
The present study considers two types of fluid models as methods for reproducing the blueshifts and line broadening observed in soft X-ray lines during the rise of solar flares. The fluid models representing the laminar flow of material in a jet and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fdeaf3215635335f40d21438ac5c2b57
https://doi.org/10.1007/3-540-55246-4_83
https://doi.org/10.1007/3-540-55246-4_83
Autor:
P. L. Bornmann
Publikováno v:
The Many Faces of the Sun ISBN: 9781461271451
Chromospheric evaporation is currently the most popular theory for explaining the source of the coronal flare material and the upward motions of X-ray emitting material observed as soft X-ray line broadenings and line shifts at the start of solar fla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::61d93b506b7b9ad74d6e3116167a7def
https://doi.org/10.1007/978-1-4612-1442-7_9
https://doi.org/10.1007/978-1-4612-1442-7_9
Autor:
T. P. Hartsell, P. L. Bornmann
Publikováno v:
The Sun as a Variable Star: Solar and Stellar Irradiance Variations ISBN: 9789401044103
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::838d85cacc14b49064efb944c6fb61d4
https://doi.org/10.1007/978-94-011-0950-5_29
https://doi.org/10.1007/978-94-011-0950-5_29
Autor:
P. L. Bornmann, J. R. Lemen
Publikováno v:
The Astrophysical Journal. 385:363
Publikováno v:
The Astrophysical Journal. 375:382
Two-dimensional electrostatic particle simulations are presented which incorporate the effect of quasi-static electric fields on particle dynamics as well as effects associated with wave-particle interactions induced by the accelerated particles. The
Autor:
P. L. Bornmann
Publikováno v:
The Astrophysical Journal. 356:733
A method has been presented for restricting the random derived flare temperatures and emission measures. The method is based on three tests and is applicable not only to disk-integrated observations, but also for any high-resolution observations that