Zobrazeno 1 - 10
of 79
pro vyhledávání: '"E. Hildner"'
Autor:
John M. Davis, Sandra Cauffman, Patricia L. Bornmann, C. C. Balch, K. Russell, K. S. Wallace, T. T. Saha, E. Hildner, Richard Grubb, D. A. Biesecker, S. M. Hill, E. G. Chipman, G. D. Berthiume, Victor J. Pizzo
Publikováno v:
Solar Physics. 226:283-315
The Solar X-ray Imager (SXI) was launched on 23 July 2001 on NOAA’s GOES-12 satellite and completed post-launch testing on 20 December 2001. It was brought into operations on 21 January 2003. This paper documents SXI performance and calibrations pr
Publikováno v:
International Astronomical Union Colloquium. 141:98-107
It has been recognized that the magnetic flux observed on the solar surface appears first in low latitudes, and then this flux is gradually dispersed by super granular convective motions and meridional circulation. Theoretically, the magnetic flux tr
Publikováno v:
Solar Physics. 137:317-328
An analysis is made of the Martens-Kuin filament eruption model in relation to observations of coronal mass ejections (CMEs). The field lines of this model are plotted in the vacuum or infinite resistivity approximation with two background fields. Th
Publikováno v:
Journal of Geophysical Research. 107
[i] Since measurements began in the late nineteenth century, there has been a secular increase (with superposed ripples due to solar cycles) of the aa geomagnetic index [Mayaud, 1972]. Starting from this observation, Lockwood et al. [1999a, 1999b] co
Autor:
E. Hildner, Rainer Schwenn, David F. Webb, Russell A. Howard, G. M. Simnett, M. J. Koomen, Philippe Lamy, Joseph B. Gurman, D. J. Michels, Barbara J. Thompson, O. C. St. Cyr, S. E. Paswaters, Simon Plunkett, N. R. Sheeley
Publikováno v:
Journal Geophysical Research
Scopus-Elsevier
Scopus-Elsevier
We report the properties of all the 841 coronal mass ejections (CMEs) observed by the Solar and Heliospheric Observatory (SOHO) Large Angle Spectroscopic Coronagraph (LASCO) C2 and C3 white-light coronagraphs from January 1996 through June 1998, and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::95cbd1d1eb60c6374536a02bb663790a
https://hdl.handle.net/11858/00-001M-0000-0014-D237-7
https://hdl.handle.net/11858/00-001M-0000-0014-D237-7
Autor:
Barry J. Labonte, Dennis G. Socker, Rainer Schwenn, Spiro K. Antiochos, Judith T. Karpen, P. C. Liewer, Andrew Buffington, Jon A. Linker, Shi Tsan Wu, E. Hildner, James A. Klimchuk, Clarence M. Korendyke, N. R. Sheely, J. W. Cook, Henry Harris, John M. Davis, Z. Mikic, D. K. Prinz, Philippe Lamy, Bernard V. Jackson, Barry Goldstein, Guenter E. Brueckner, N. E. Moulton, Victor J. Pizzo, J. Daniel Moses, Russell A. Howard, Joseph M. Davila, H. Rosenbauer, Kenneth P. Dere, L. F. Burlaga, D. J. Michels, Marcia Neugebauer
Publikováno v:
SPIE Proceedings.
A STEREO mission concept requiring only a single new spacecraft has been proposed. The mission would place the new spacecraft in a heliocentric orbit and well off the Sun- Earth line, where it can simultaneously view both the solar source of heliosph
Autor:
E. Hildner, H. Hudson
Publikováno v:
AIP Conference Proceedings.
Because of the healt hazards of solar activity, human traffic in deep space will require facilities for monitoring, predicting, and altering the astronauts to potential danger. This suggests a ‘‘solar watch’’ program consisting of a network o
Autor:
E. Hildner
Publikováno v:
International Astronomical Union Colloquium. 144:82
Over the last twenty years, orbiting coronagraphs have vastly increased the amount of observational material for the whitelight corona. Spanning almost two solar cycles, and augmented by ground-based K-coronameter, emission-line, and eclipse observat
Publikováno v:
Eos, Transactions American Geophysical Union. 75:353
Space storms—for our purposes, meaning all particle, electromagnetic, and ionospheric disturbances resulting from solar storms, coronal mass ejections, fast solar wind streams, and ionospheric instabilities—pose several costly hazards. They can i
Publikováno v:
Journal of Geophysical Research. 95:917
We describe a set of solar coronal mass ejection (CME) events where coincident data sets from both X ray and white light instruments have been made available through deliberate planning. Using these we have been able to put tight limits on possible d