Zobrazeno 1 - 10
of 29
pro vyhledávání: '"B. V. Jackson"'
Autor:
M. M. Bisi, B. V. Jackson, J. M. Clover, P. K. Manoharan, M. Tokumaru, P. P. Hick, A. Buffington
Publikováno v:
Annales Geophysicae, Vol 27, Pp 4479-4489 (2009)
Interplanetary scintillation (IPS) remote-sensing observations provide a view of the solar wind covering a wide range of heliographic latitudes and heliocentric distances from the Sun between ~0.1 AU and 3.0 AU. Such observations are used to study
Externí odkaz:
https://doaj.org/article/8b5bcbb3153c4517a0e2c7693521299a
Publikováno v:
Annales Geophysicae, Vol 27, Pp 4097-4104 (2009)
In this paper we present the results of the analysis of the late January 2007 Coronal Mass Ejection (CME) events recorded by the Solar Mass Ejection Imager (SMEI), the Solar TErrestrial RElations Observatory (STEREO), and the SOlar and Heliospheri
Externí odkaz:
https://doaj.org/article/7edbee14ee7c4905af4174601891a890
Autor:
B. V. Jackson, A. Buffington, P. P. Hick, R. C. Altrock, S. Figueroa, P. E. Holladay, J. C. Johnston, S. W. Kahler, J. B. Mozer, S. Price, R. R. Radick, R. Sagalyn, D. Sinclair, G. M. Simnett, C. J. Eyles, M. P. Cooke, S. J. Tappin, T. Kuchar, D. Mizuno, D. F. Webb, P. A. Anderson, S. L. Keil, R. E. Gold, N. R. Waltham
Publikováno v:
Solar Physics. 225:177-207
We have launched into near-Earth orbit a solar mass-ejection imager (SMEI) that is capable of measuring sunlight Thomson-scattered from heliospheric electrons from elongations to as close as 18∘ to greater than 90∘ from the Sun. SMEI is designed
Autor:
Patricia H. Reiff, B. V. Jackson, A. E. Potter, Rosemary M. Killen, Menelaos Sarantos, Barbara L. Giles, P. Hick
Publikováno v:
Journal of Geophysical Research: Planets. 106:20509-20525
Mercury's sodium atmosphere is known to be highly variable both temporally and spatially. During a week-long period from November 13 to 20, 1997, the total sodium content of the Hermean atmosphere increased by a factor of 3, and the distribution vari
Autor:
Oddbjørn Engvold, J. P. Rozelot, I. Kim, A. Hood, B. V. Jackson, Arnold O. Benz, Kazunari Shibata, A. J. Sanchez, K. P. Dere, Nat Gopalswamy, G. Ai, R. Hammer, L. van Driel-Geztelyi, G. Poletto, P. C. Marten
Publikováno v:
Transactions of the International Astronomical Union. 24:67-72
The Sun’s activity has been evolving in the ascending phase of Solar Cycle 23 since 1996. Similarly, the research on solar activity is also in the ascending phase of a new active period. Numerous new results have been obtained from a large amount o
Publikováno v:
Solar Physics. 145:403-406
Autor:
B. V. Jackson, P. P. Hick, A. Buffington, M. M. Bisi, J. M. Clover, M. S. Hamilton, M. Tokumaru, K. Fujiki, M. Maksimovic, K. Issautier, N. Meyer-Vernet, M. Moncuquet, F. Pantellini
Publikováno v:
AIP Conference Proceedings.
The Solar Mass Ejection Imager (SMEI) observes the increased brightness from the density enhancements behind interplanetary shocks that are also observed in situ near the Earth. We use the University of California, San Diego (UCSD) time‐dependent t
Autor:
M. M. Bisi, B. V. Jackson, P. P. Hick, J. M. Clover, S. Hamilton, M. Tokumaru, K. Fujiki, M. Maksimovic, K. Issautier, N. Meyer-Vernet, M. Moncuquet, F. Pantellini
Publikováno v:
AIP Conference Proceedings.
Interplanetary scintillation (IPS) observations provide information about a large portion of the inner heliosphere. We have used Solar‐Terrestrial Environment Laboratory (STELab) IPS velocity and g‐level observations with our three‐dimensional