Zobrazeno 1 - 10
of 188
pro vyhledávání: '"W. W. White"'
Autor:
N. C. Maynard, W. J. Burke, J. D. Scudder, D. M. Ober, G. L. Siscoe, W. W. White, K. D. Siebert, D. R. Weimer, G. M. Erickson, J. Schoendorf, M. A. Heinemann
Publikováno v:
Annales Geophysicae, Vol 22, Pp 2151-2169 (2004)
We present observations from the Polar satellite that confirm the existence of two types of depletion layers predicted under southward interplanetary magnetic field (IMF) conditions in magnetohydrodynamic simulations. The first depletion type occu
Externí odkaz:
https://doaj.org/article/8518f7e23e704661a4c7612c6db0eb16
Autor:
W. W. White
Publikováno v:
Journal of the American Society for Naval Engineers. 10:1-87
Autor:
W. W. White
Publikováno v:
Journal of the American Society for Naval Engineers. 22:701-830
Autor:
W. W. White, H. Jung
Publikováno v:
Journal of Polymer Science: Polymer Symposia. 45:197-207
A series of ten oligomeric surfactants of general formula RS (CH2CHCN)a(CH2COOK)bH were prepared and tested for surface activity. The R groups (corresponding to the lipophile of a conventional surfactant) studied were n-butyl, n-octyl, and n-dodecyl.
Autor:
G. M. Erickson, Daniel R. Weimer, N. C. Maynard, K. D. Siebert, George Siscoe, M. A. Heinemann, Bengt U. Ö. Sonnerup, W. W. White
Publikováno v:
Planetary and Space Science. 50:627-632
Results of global MHD simulations are used to examine the susceptibility of magnetosheath plasma to anisotropy-driven instabilities, specifically the mirror mode, electromagnetic ion cyclotron (EMIC), and firehose instabilities. Advection of magnetos
Autor:
Bengt U. Ö. Sonnerup, Daniel R. Weimer, K. D. Siebert, N. C. Maynard, George Siscoe, W. W. White, J. A. Schoendorf, Gordon R. Wilson, G. M. Erickson, N. U. Crooker
Publikováno v:
Planetary and Space Science. 50:461-471
We discuss four aspects of magnetosheath flow that require MHD for their calculation and understanding. We illustrate these aspects with computations using a numerical MHD code that simulates the global magnetosphere and its magnetosheath. The four i
Autor:
G. M. Erickson, Daniel R. Weimer, W. W. White, K. D. Siebert, George L. Siscoe, Bengt U. Ö. Sonnerup, Nelson C. Maynard, J. A. Schoendorf, Gordon R. Wilson
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:29419-29434
A global MHD simulation code, the Integrated Space Weather Prediction Model, is used to examine the steady state properties of the magnetosphere for zero interplanetary magnetic field. In this “ground state” of the system, reconnection at the mag
Autor:
Daniel R. Weimer, George Siscoe, W. W. White, K. D. Siebert, N. C. Maynard, Bengt U. Ö. Sonnerup, G. M. Erickson
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:13015-13022
We use a global MHD simulation to compute the distribution of E‖ on the face of the magnetopause as represented by the last closed field line surface. In MHD codes, E‖ is a proxy for magnetic reconnection. Integrating E‖ along the topological s
Autor:
N. C. Maynard, George Siscoe, G. M. Erickson, Daniel R. Weimer, W. W. White, Bengt U. Ö. Sonnerup, K. D. Siebert
Publikováno v:
Geophysical Research Letters. 28:1921-1924
The magnetospheric sash is a ribbon of weak field shaped like a horseshoe with its open ends adjacent to the north and south dayside, magnetopause cusps and its closed end forming the cross-tail current sheet. The clock angle of the sash in the dawn-
Autor:
W. W. White, Gordon R. Wilson, Hideaki Kawano, Bengt U. Ö. Sonnerup, J. D. Scudder, S. Savin, J. Šafránoková, George Siscoe, I. Sandahl, Zdeněk Němeček, W. K. Peterson, G. M. Erickson, N. C. Maynard, Daniel R. Weimer
Publikováno v:
Scopus-Elsevier
Using a unique data set from the Wind, Polar, Interball 1, Magion 4, and Defense Meteorological Satellite Program (DMSP) F11 satellites, comparisons with the Integrated Space Weather Model (ISM) have provided validation of the global structure predic