Zobrazeno 1 - 10
of 17
pro vyhledávání: '"M M, Bisi"'
Autor:
R. A. Fallows, B. Forte, M. Mevius, M. A. Brentjens, C. G. Bassa, M. M. Bisi, A. Offringa, G. Shaifullah, C. Tiburzi, H. Vedantham, P. Zucca
Context. The occultation of a radio source by the plasma tail of a comet can be used to probe structure and dynamics in the tail. Such occultations are rare, and the occurrence of scintillation, due to small-scale density variations in the tail, rema
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c003eb09a7f2b02774ab8b7c8e168262
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:
M. M. Bisi1,2 Mario.Bisi@aber.ac.uk, A. R. Breen2 azb@aber.ac.uk, B. V. Jackson1 bvjackson@ucsd.edu, R. A. Fallows2 raf@aber.ac.uk, A. P. Walsh3 apw@mssl.ucl.ac.uk, Z. Mikić4 mikicz@predsci.com, P. Riley4 pete@predsci.com, C. J. Owen3 cjo@mssl.ucl.ac.uk, A. Gonzalez-Esparza5 americo@geofisica.unam.mx, E. Aguilar-Rodriguez5 ernesto@geofisica.unam.mx, H. Morgan6 hmorgan@IfA.Hawaii.Edu, E. A. Jensen7,8 eaj@acs-consulting.com, A. G. Wood2 aow@aber.ac.uk, M. J. Owens2,9 m.j.owens@reading.ac.uk, M. Tokumaru10 tokumaru@stelab.nagoya-u.ac.jp, P. K. Manoharan11 mano@ncra.tifr.res.in, I. V. Chashei12 chashey@prao.ru, A. S. Giunta13,14 alessandra.giunta@stfc.ac.uk, J. A. Linker4 linkerj@predsci.com, V. I. Shishov12 shishov@prao.ru
Publikováno v:
Solar Physics. Aug2010, Vol. 265 Issue 1/2, p49-127. 79p. 3 Color Photographs, 4 Black and White Photographs, 7 Diagrams, 10 Charts, 29 Graphs.
Autor:
J P, Eastwood, E, Biffis, M A, Hapgood, L, Green, M M, Bisi, R D, Bentley, R, Wicks, L-A, McKinnell, M, Gibbs, C, Burnett
Publikováno v:
Risk analysis : an official publication of the Society for Risk Analysis. 37(2)
Space weather describes the way in which the Sun, and conditions in space more generally, impact human activity and technology both in space and on the ground. It is now well understood that space weather represents a significant threat to infrastruc
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
Publikováno v:
Jensen, E. A.; Hick, P. P.; Bisi, M. M.; Jackson, B. V.; Clover, J.; & Mulligan, T.(2010). Faraday Rotation Response to Coronal Mass Ejection Structure. Solar Physics: A Journal for Solar and Solar-Stellar Research and the Study of Solar Terrestrial Physics, 265(1), pp 31-48. doi: 10.1007/s11207-010-9543-2. Retrieved from: http://www.escholarship.org/uc/item/2q46j8vx
We present the results from modeling the coronal mass ejection (CME) properties that have an effect on the Faraday rotation (FR) signatures that may be measured with an imaging radio antenna array such as the Murchison Widefield Array (MWA). These in
Publikováno v:
Astrophysical Journal Letters; 9/1/2016, Vol. 828 Issue 1, p1-1, 1p
Publikováno v:
Astrophysical Journal Letters; 4/10/2015, Vol. 803 Issue 1, p1-1, 1p