Zobrazeno 1 - 10
of 29
pro vyhledávání: '"H. E. Jorgensen"'
Publikováno v:
IEEE Transactions on Instrumentation and Measurement. 48:346-350
The Large Hadron Collider is CERN's next particle accelerator project, scheduled for commissioning in 2005. The project requires accurate current measurements above 10 kA. Calibration heads have been developed in collaboration with industry to work u
Publikováno v:
The Astrophysical Journal. 486:110-116
The prospects of detecting extragalactic supernovae (SNs) down to visual magnitudes 23-25 give us hope for observing them in the most distant parts of the universe. Using a Monte Carlo method of stellar population synthesis (the Scenario Machine), we
Publikováno v:
Astrophysics and Space Science. 231:389-392
Assuming that gamma-ray bursts (GRB) originate from binary neutron star (NS) or black holes (BH) merging in distant galaxies, theoretical logN-logS distributions for gamma-ray bursts (GRB) are calculated using the compact binaries coalescence rates c
Publikováno v:
1998 Conference on Precision Electromagnetic Measurements Digest (Cat. No.98CH36254).
The Large Hadron Collider (LHC) is CERN's next particle accelerator project, scheduled to be commissioned in 2005. The project requires accurate current measurements above 10 kA. Calibration heads have been developed in collaboration with industry to
Autor:
S. Okoye, C. R. Tolbert, M. Capaccioli, A. A. Boyarchuk, G. Krishna, Yoshihide Kozai, Masaki Morimoto, Richard M. West, E.P.J. van den Heuvel, G. F. Smith, S. Wang, J. Sahade, J. Zhao, S. Nha, M. Othman, M. S. Roberts, H. F. Haupt, S. H. Ye, B. Caccin, J. R. Ducati, P. M. Routly, D. M. Chitre, D. A. MacRae, V. Straizys, R. D. Cannon, Kam-Ching Leung, H. E. Jorgensen, Govind Swarup, A. Florsch, S. Ninkovic
Publikováno v:
Transactions of the International Astronomical Union. 24:421-422
Thirty five grants were made during the triennium October 1, 1996 to September 30, 1999. The astronomer, home country, and host country are listed below.
Publikováno v:
Scopus-Elsevier
Evolution of the coalescence rate of double neutron stars (NS) and neutron star -- black hole (BH) binaries are computed for model galaxies with different star formation rates. Assuming gamma-ray bursts (GRB) to originate from NS+NS or NS+BH merging
Publikováno v:
Wind Energy Science, Vol 2, Pp 211-228 (2017)
Understanding uncertainties in wind resource assessment associated with the use of the output from numerical weather prediction (NWP) models is important for wind energy applications. A better understanding of the sources of error reduces risk and
Externí odkaz:
https://doaj.org/article/ff95b73c1b8b48d6a602d3b07b57ff3c
Autor:
M. Kelly, H. E. Jørgensen
Publikováno v:
Wind Energy Science, Vol 2, Pp 189-209 (2017)
In this work we relate uncertainty in background roughness length (z0) to uncertainty in wind speeds, where the latter are predicted at a wind farm location based on wind statistics observed at a different site. Sensitivity of predicted winds to r
Externí odkaz:
https://doaj.org/article/160a3bd1fda74042ad00aef9ff158a20
Autor:
H. E. Jorgensen, P. R. Jorden, I. G. van Breda, William B. Sparks, P. J. Rudd, Jasper Wall, D. J. Thorne
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 217:87-98
On presente des observations CCD et une procedure numerique adaptees a la localisation des bandes de poussiere dans les galaxies elliptiques. On l'applique a 31 galaxies elliptiques brillantes pour decouvrir que huit d'entre elles presentent des indi
Autor:
D. McNally, E. V. Konovich, D. G. Wentzel, L. Houziaux, H. E. Jorgensen, J. Kleczek, E. A. Müller, M. Rigutti, T. L. Swihart
Publikováno v:
Transactions of the International Astronomical Union. 16:207-217