Zobrazeno 1 - 10
of 1 718
pro vyhledávání: '"Sumner, M"'
Autor:
Graham, G., Chimenti, M.S., Knudtson, K.L., Grenard, D.N., Co, L., Sumner, M., Tchou, T., Bieszczad, K.M.
Publikováno v:
In Hearing Research October 2023 438
Autor:
Saleh, Kamel1 (AUTHOR) kamel.saleh@najah.edu, Sumner, M.2 (AUTHOR)
Publikováno v:
Electrical Engineering. Oct2022, Vol. 104 Issue 5, p3073-3090. 18p.
Autor:
Biver, N., Bockelée-Morvan, D., Boissier, J., Crovisier, J., Colom, P., Lecacheux, A., Moreno, R., Paubert, G., Lis, D., Sumner, M., Frisk, U., Hjalmarson, A., Olberg, M., Winnberg, A., Florén, H. -G., Sandqvist, Aa., Kwok, Sun
Publikováno v:
Icarus 187: 253-271,2007
Comet 9P/Tempel 1 was the target of a multi-wavelength worldwide investigation in 2005. The NASA Deep Impact mission reached the comet on 4.24 July 2005, delivering a 370 kg impactor which hit the comet at 10.3 km/s. Following this impact, a cloud of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610717
Autor:
Sumner, M.
This thesis describes the design and construction of a high performance induction motor drive, controlled by a network of parallel (INMOS) Transputer processors. The flexibility and high computational ability of the controller is demonstrated by the
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.335288
Publikováno v:
Astrophys.J. 512 (1999) 683-692
The variability observed in many complex gamma-ray bursts (GRBs) is inconsistent with causally connected variations in a single, symmetric, relativistic shell interacting with the ambient material ("external shocks"). Rather, the symmetry of the shel
Externí odkaz:
http://arxiv.org/abs/astro-ph/9802200
Publikováno v:
In Energy & Buildings 15 January 2017 135:350-366
Autor:
Sumner, M. C., Fenimore, E. E.
Many cosmological models of gamma-ray bursts (GRBs) assume that a single relativistic shell carries kinetic energy away from the source and later converts it into gamma rays, perhaps by interactions with the interstellar medium or by shocks within th
Externí odkaz:
http://arxiv.org/abs/astro-ph/9712302
Two main types of models have been suggested to explain the long durations and multiple peaks of Gamma-Ray Bursts (GRBs). In one, there is a very quick release of energy at a central site resulting in a single relativistic shell that produces peaks i
Externí odkaz:
http://arxiv.org/abs/astro-ph/9712303
Autor:
Fenimore, E. E., Sumner, M. C.
In many models of Gamma-Ray Bursts (GRBs) relativistic shells are responsible for the overall envelope of emission. We use kinematics and symmetry to calculate the time history and spectral evolution expected from a relativistic shell including effec
Externí odkaz:
http://arxiv.org/abs/astro-ph/9705052