#### Filter Results:

#### Publication Year

1997

2016

#### Publication Type

#### Co-author

#### Publication Venue

#### Key Phrases

Learn More

- A. C. Haza, A. Griffa, P. Martin, A. Molcard, T. M. Özgökmen, A. C. Poje +5 others
- 2007

[1] A high-resolution numerical model of the Adriatic Sea is used to predict Lagrangian coherent structure boundaries, quantified by finite-size Lyapunov exponents (FSLE), for flow features in the region of the Gargano Peninsula during the course of the Dynamics of the Adriatic in Real Time (DART) observational program. FSLE fields computed from two-day… (More)

- M Frailis, E Franceschi, S Galeotta, K Ganga, C Gauthier, M Giard +11 others
- 2013

We analyse the implications of the Planck data for cosmic inflation. The Planck nominal mission temperature anisotropy measurements, combined with the WMAP large-angle polarization, constrain the scalar spectral index to n s = 0.9603 ± 0.0073, ruling out exact scale invariance at over 5σ. Planck establishes an upper bound on the tensor-to-scalar ratio at r… (More)

- Ganga, M Giard, Y Giraud-Héraud, J González-Nuevo, D Marinucci, M Maris +14 others
- 2013

The Planck nominal mission cosmic microwave background (CMB) maps yield unprecedented constraints on primordial non-Gaussianity (NG). Using three optimal bispectrum estimators, separable template-fitting (KSW), binned, and modal, we obtain consistent values for the primordial local, equilateral, and orthogonal bispectrum amplitudes, quoting as our final… (More)

- F Boulanger, M Bucher, C Burigana, S Galli, K Ganga, C Gauthier +21 others
- 2015

The Planck full mission cosmic microwave background (CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity (NG). Using three classes of optimal bispectrum estimators — separable template-fitting (KSW), binned, and modal — we obtain consistent values for the primordial local, equilateral, and… (More)

- P A R Ade, N Aghanim, Z Ahmed, R W Aikin, K D Alexander, M Arnaud +270 others
- Physical review letters
- 2015

We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400 deg^{2} patch of sky centered on RA 0 h, Dec. -57.5°. The combined maps reach a depth of 57 nK deg in Stokes Q and U in a band centered at 150 GHz. Planck has observed the full sky in polarization at seven… (More)

- H. Zohm, J. Adamek, C. Angioni, G. Antar, C. V. Atanasiu, M. Balden +84 others
- 2006

ASDEX Upgrade was operated with fully W-covered wall in 2007 and 2008. Stationary H-modes at the ITER target values and improved H-modes with H up to 1.2 were run without any boronisation. The boundary conditions set by the full W-wall (high enough ELM frequency, high enough central heating and low enough power density arriving at the target plates) require… (More)

Commercial grating-tuned single-mode extended-cavity semiconductor lasers (ECLDs) can be tuned over 100 nm near 1.55mum . This continuous tuning with no mode hopping requires delicate factory adjustments and high mechanical stability so that the wavelength precision is kept as high as possible and the mismatch between the lasing wavelength and the… (More)

- K M Huffenberger, G Hurier, A H Jaffe, T R Jaffe, D J Marshall, P G Martin +4 others
- 2015

We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is dominated by free-free and spinning dust emission, whereas the polarized intensity is dominated by synchrotron emission. The Commander component-separation tool has been used to separate the various… (More)

- G. Fiksel, A. F. Almagri, J. K. Anderson, F. Bonomo, M. T. Borchardt, D. L. Brower +43 others
- 2008

We report on results achieved in the MST reversed-field pinch in the following three key areas. In the area of plasma confinement and beta we have achieved improved-confinement plasmas with simultaneously high T e ≈ 2 keV and high T i > 1 keV at MST's highest current capability ∼ 0.5 MA. Both temperatures increase with plasma current. In addition, we have… (More)