148 results on '"Gizon, A"'
Search Results
2. Dynamics of Large-Scale Solar Flows
- Author
-
Hotta, Hideyuki, primary, Bekki, Yuto, additional, Gizon, Laurent, additional, Noraz, Quentin, additional, and Rast, Mark, additional
- Published
- 2023
- Full Text
- View/download PDF
3. Metal-rich stars are less suitable for the evolution of life on their planets
- Author
-
Shapiro, Anna V., primary, Brühl, Christoph, additional, Klingmüller, Klaus, additional, Steil, Benedikt, additional, Shapiro, Alexander I., additional, Witzke, Veronika, additional, Kostogryz, Nadiia, additional, Gizon, Laurent, additional, Solanki, Sami K., additional, and Lelieveld, Jos, additional
- Published
- 2023
- Full Text
- View/download PDF
4. HiRISE - High-Resolution Imaging and Spectroscopy Explorer - Ultrahigh resolution, interferometric and external occulting coronagraphic science
- Author
-
Erdélyi, Robertus, primary, Damé, Luc, additional, Fludra, Andrzej, additional, Mathioudakis, Mihalis, additional, Amari, T., additional, Belucz, B., additional, Berrilli, F., additional, Bogachev, S., additional, Bolsée, D., additional, Bothmer, V., additional, Brun, S., additional, Dewitte, S., additional, de Wit, T. Dudok, additional, Faurobert, M., additional, Gizon, L., additional, Gyenge, N., additional, Korsós, M. B., additional, Labrosse, N., additional, Matthews, S., additional, Meftah, M., additional, Morgan, H., additional, Pallé, P., additional, Rochus, P., additional, Rozanov, E., additional, Schmieder, B., additional, Tsinganos, K., additional, Verwichte, E., additional, Zharkov, S., additional, Zuccarello, F., additional, and Wimmer-Schweingruber, R., additional
- Published
- 2022
- Full Text
- View/download PDF
5. Habitability of the early Earth: liquid water under a faint young Sun facilitated by strong tidal heating due to a closer Moon
- Author
-
Heller, René, primary, Duda, Jan-Peter, additional, Winkler, Max, additional, Reitner, Joachim, additional, and Gizon, Laurent, additional
- Published
- 2021
- Full Text
- View/download PDF
6. How to Estimate the Far-Side Open Flux Using STEREO Coronal Holes
- Author
-
Heinemann, Stephan G., primary, Temmer, Manuela, additional, Hofmeister, Stefan J., additional, Stojakovic, Aleksandar, additional, Gizon, Laurent, additional, and Yang, Dan, additional
- Published
- 2021
- Full Text
- View/download PDF
7. A journey of exploration to the polar regions of a star: probing the solar poles and the heliosphere from high helio-latitude
- Author
-
Harra, Louise, primary, Andretta, Vincenzo, additional, Appourchaux, Thierry, additional, Baudin, Frédéric, additional, Bellot-Rubio, Luis, additional, Birch, Aaron C., additional, Boumier, Patrick, additional, Cameron, Robert H., additional, Carlsson, Matts, additional, Corbard, Thierry, additional, Davies, Jackie, additional, Fazakerley, Andrew, additional, Fineschi, Silvano, additional, Finsterle, Wolfgang, additional, Gizon, Laurent, additional, Harrison, Richard, additional, Hassler, Donald M., additional, Leibacher, John, additional, Liewer, Paulett, additional, Macdonald, Malcolm, additional, Maksimovic, Milan, additional, Murphy, Neil, additional, Naletto, Giampiero, additional, Nigro, Giuseppina, additional, Owen, Christopher, additional, Martínez-Pillet, Valentín, additional, Rochus, Pierre, additional, Romoli, Marco, additional, Sekii, Takashi, additional, Spadaro, Daniele, additional, Veronig, Astrid, additional, and Schmutz, W., additional
- Published
- 2021
- Full Text
- View/download PDF
8. Rossby Waves in Astrophysics
- Author
-
Eyal Heifetz, Luca Biancofiore, Aaron C. Birch, Jose Luis Ballester, Ramon Oliver, M. Albekioni, O. M. Umurhan, Ron Yellin-Bergovoy, Laurent Gizon, Teimuraz V. Zaqarashvili, Y. Bekki, Eka Gurgenashvili, Leon Ofman, Scott W. McIntosh, Mausumi Dikpati, Bastian Proxauf, A. F. Lanza, Biancofiore, Luca, and AUT
- Subjects
Angular momentum ,010504 meteorology & atmospheric sciences ,Context (language use) ,Astrophysics ,01 natural sciences ,Atmosphere ,Planet ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Magnetohydrodynamic waves ,Solar system planets ,010303 astronomy & astrophysics ,Physics::Atmospheric and Oceanic Physics ,0105 earth and related environmental sciences ,Physics ,Astrophysical Processes ,Astrophysical discs ,Astrophysics::Instrumentation and Methods for Astrophysics ,Sun ,Rossby wave ,Astronomy and Astrophysics ,Stars ,Rossby waves ,Planetary science ,Space and Planetary Science ,Astrophysics::Earth and Planetary Astrophysics - Abstract
Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined.
- Published
- 2021
9. Accurate Short-Characteristics Radiative Transfer in A Numerical Tool for Astrophysical RESearch (ANTARES)
- Author
-
Kostogryz, Nadiia M., primary, Kupka, Friedrich, additional, Piskunov, Nikolai, additional, Fabbian, Damian, additional, Krüger, Daniel, additional, and Gizon, Laurent, additional
- Published
- 2021
- Full Text
- View/download PDF
10. Rossby Waves in Astrophysics
- Author
-
Zaqarashvili, T. V., primary, Albekioni, M., additional, Ballester, J. L., additional, Bekki, Y., additional, Biancofiore, L., additional, Birch, A. C., additional, Dikpati, M., additional, Gizon, L., additional, Gurgenashvili, E., additional, Heifetz, E., additional, Lanza, A. F., additional, McIntosh, S. W., additional, Ofman, L., additional, Oliver, R., additional, Proxauf, B., additional, Umurhan, O. M., additional, and Yellin-Bergovoy, R., additional
- Published
- 2021
- Full Text
- View/download PDF
11. Interpreting the Helioseismic and Magnetic Imager (HMI) Multi-Height Velocity Measurements
- Author
-
Robert F. Stein, Sebastien Couvidat, Aaron C. Birch, Bernhard Fleck, Sanja Danilovic, Laurent Gizon, Robert H. Cameron, Björn Löptien, and Kaori Nagashima
- Subjects
Physics ,Convection ,Phase (waves) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Scale height ,Astrophysics ,01 natural sciences ,Cutoff frequency ,010101 applied mathematics ,Atmosphere ,Wavelength ,Astrophysics - Solar and Stellar Astrophysics ,Space and Planetary Science ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,0101 mathematics ,Effective height ,010303 astronomy & astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) ,Line (formation) - Abstract
The Solar Dynamics Observatory/Helioseismic and Magnetic Imager (SDO/HMI) filtergrams, taken at six wavelengths around the Fe I 6173.3 {\AA} line, contain information about the line-of-sight velocity over a range of heights in the solar atmosphere. Multi-height velocity inferences from these observations can be exploited to study wave motions and energy transport in the atmosphere. Using realistic convection simulation datasets provided by the STAGGER and MURaM codes, we generate synthetic filtergrams and explore several methods for estimating Dopplergrams. We investigate at which height each synthetic Dopplergram correlates most strongly with the vertical velocity in the model atmospheres. On the basis of the investigation, we propose two Dopplergrams other than the standard HMI-algorithm Dopplergram produced from HMI filtergrams: a line-center Dopplergram and an average-wing Dopplergram. These two Dopplergrams correlate most strongly with vertical velocities at the heights of 30 - 40 km above (line-center) and 30 - 40 km below (average-wing) the effective height of the HMI-algorithm Dopplergram. Therefore, we can obtain velocity information from two layers separated by about a half of a scale height in the atmosphere, at best. The phase shifts between these multi-height Dopplergrams from observational data as well as those from the simulated data are also consistent with the height-difference estimates in the frequency range above the photospheric acoustic cutoff frequency., Comment: accepted for publication in Solar Physics
- Published
- 2014
12. Fragile Detection of Solar g $g$ -Modes by Fossat et al.
- Author
-
Schunker, Hannah, primary, Schou, Jesper, additional, Gaulme, Patrick, additional, and Gizon, Laurent, additional
- Published
- 2018
- Full Text
- View/download PDF
13. Global-scale equatorial Rossby waves as an essential component of solar internal dynamics
- Author
-
Löptien, Björn, primary, Gizon, Laurent, additional, Birch, Aaron C., additional, Schou, Jesper, additional, Proxauf, Bastian, additional, Duvall, Thomas L., additional, Bogart, Richard S., additional, and Christensen, Ulrich R., additional
- Published
- 2018
- Full Text
- View/download PDF
14. Comparison of Travel-Time and Amplitude Measurements for Deep-Focusing Time–Distance Helioseismology
- Author
-
Pourabdian, Majid, primary, Fournier, Damien, additional, and Gizon, Laurent, additional
- Published
- 2018
- Full Text
- View/download PDF
15. Experimental evidence for signature inversion in 132La from a revisited level scheme
- Author
-
Timar, J., Sohler, D., Nyako, B.M., Zolnai, L., Dombradi, Zs., Paul, E.S., Boston, A.J., Fox, C., Nolan, P.J., Sampson, J.A., Scraggs, H.C., Walker, A., Gizon, J., Gizon, A., Bazzacco, D., Lunardi, S., Petrache, C.M., Astier, A., Buforn, N., Bednarczyk, P., Kintz, N., Wyss, R., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
- Subjects
Physics ,Nuclear and High Energy Physics ,Spins ,Isotope ,010308 nuclear & particles physics ,Hadron ,Nuclear structure ,Parity (physics) ,Inversion (meteorology) ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,0103 physical sciences ,Nuclear fusion ,Atomic physics ,010306 general physics ,Spin (physics) - Abstract
Matière Nucléaire; The decay out of the πh 11/2νh 11/2 band to the known low-energy levels in 132La was studied using the reaction 100Mo + 36S at 160 MeV beam energy. The low-energy level scheme has been further developed and unambiguous spin and parity values have been assigned to the levels connecting the band to the 6- isomeric state. According to the new level scheme the spins in the πh 11/2νh 11/2 band are shifted up by one unit compared to the earlier tentative experimental values. The obtained new spins prove the existence of signature inversion in 132La and give further support to the spin assignments made for the πh 11/2νh 11/2 bands in the neighbouring odd-odd La isotopes from level energy systematics. (Springer)
- Published
- 2003
16. Excited states of 154Tm
- Author
-
F. Farget, P. Paris, J. Genevey, D. Santos, J. Gizon, A. Płochocki, D. Barnéoud, C. Foin, A. Gizon, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), and Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,010308 nuclear & particles physics ,Hadron ,State (functional analysis) ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,Electron spectroscopy ,medicine.anatomical_structure ,Recoil ,Excited state ,0103 physical sciences ,medicine ,Level structure ,Nuclear fusion ,Atomic physics ,010306 general physics ,Nucleus - Abstract
A high-spin level structure of the nucleus 154Tm has been established for the first time up to 6.14 MeV. The 118Sn + 40Ca reaction at 205 MeV associated with the recoil shadow method was used to identify the I π = (19)+ isomeric state at 2.74 MeV. In-beam γ-ray and conversion electron spectroscopy have been applied on the 144Sm(14N, 4n)154Tm reaction at 95 MeV to build the level scheme. The level structure of 154Tm is compared to other structures observed in N = 85 neighbouring nuclei. (Springer)
- Published
- 2002
17. New investigation of the decay of the high-spin isomer in 151Er
- Author
-
J. Genevey, J. Gizon, D. Barnéoud, D. Santos, C. Foin, F. Farget, A. Płochocki, A. Gizon, C. F. Liang, D. Bucurescu, P. Paris, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,010308 nuclear & particles physics ,0103 physical sciences ,Hadron ,Conversion coefficients ,Nuclear fusion ,Electron ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,Atomic physics ,010306 general physics ,Spin (physics) ,01 natural sciences - Abstract
The decay of the T 1/2 = 420 ns isomer in 151Er has been reinvestigated. The multipolarities of the decaying transitions have been established by measuring the electron conversion coefficients. An I π = 67/2− assignment is proposed for this isomer with a π[h 11 2/4 d 3 2/1 d 5 2/−1 ]⊗ν[f 7/2 h 9/2 h 11 2/−1 ] configuration.
- Published
- 2000
18. New insight in the level structure of 153Er
- Author
-
M. Ashgar, J. Gizon, A. Płochocki, A. Gizon, D. Barnéoud, C. Foin, F. Farget, J. Genevey, P. Paris, D. Santos, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,21.10.Pc ,23.20.Lv ,27.70.+q ,Hadron ,SHELL model ,Parity (physics) ,02 engineering and technology ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,010402 general chemistry ,021001 nanoscience & nanotechnology ,01 natural sciences ,Electron spectroscopy ,0104 chemical sciences ,medicine.anatomical_structure ,medicine ,Level structure ,Nuclear fusion ,Atomic physics ,0210 nano-technology ,Nucleus ,Excitation - Abstract
The high-spin level structure of the 153Er nucleus has been reinvestigated by in-beam %-ray and electron spectroscopy with (14N,pxn) reaction. Excitation energies, spin and parity assignments are unambiguously established for the two lowest isomers T1/2 380 ns and T1/2\simeq 10 ns. The characteristics of the third one (T1/2 250 ns) at 5.2 MeV are still questionable but its main decay modes are better known. An extension of the level scheme is proposed up to 8.4 MeV.Experimental results have been discussed in terms of shell model multiplets and compared with the other structures observed in N=85 neighbouring nuclei.
- Published
- 2000
19. Terminating high-spin bands in 101Rh
- Author
-
A. Gizon, A. J. Boston, D. Bucurescu, J. Timár, D. T. Joss, E. S. Paul, N. J. O’Brien, A. T. Semple, B. M. Nyakó, A. V. Afanasjev, Ingemar Ragnarsson, L. Zolnai, J. Gizon, C. M. Parry, Gh. Căta-Danil, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,Normalization property ,Spin states ,010308 nuclear & particles physics ,Hadron ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,Formalism (philosophy of mathematics) ,medicine.anatomical_structure ,0103 physical sciences ,medicine ,Nuclear fusion ,Neutron ,Atomic physics ,010306 general physics ,Nucleus - Abstract
High spin states of 101Rh have been populated using the reaction 70Zn+36S at 130 MeV. γ-rays were detected with the EUROGAM2 array. New high-spin bands have been observed in this nucleus up to 45/2−, 57/2− and 65/2+ states. They have been interpreted using the Nilsson-Strutinsky cranking formalism as terminating configurations. Two of the bands were observed up to the predicted terminating states which are built up from g9/2 protons as well as d5/2, g7/2 and h11/2 neutrons relative to a 90Zr core.
- Published
- 1999
20. Fourier Analysis of Gapped Time Series: Improved Estimates of Solar and Stellar Oscillation Parameters
- Author
-
T. Stahn and Laurent Gizon
- Subjects
Physics ,Oscillation ,Astrophysics (astro-ph) ,Phase (waves) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics ,Asteroseismology ,Convolution ,symbols.namesake ,Quality (physics) ,Space and Planetary Science ,Fourier analysis ,Frequency domain ,Harmonic ,symbols ,Statistical physics - Abstract
Quantitative helio- and asteroseismology require very precise measurements of the frequencies, amplitudes, and lifetimes of the global modes of stellar oscillation. It is common knowledge that the precision of these measurements depends on the total length (T), quality, and completeness of the observations. Except in a few simple cases, the effect of gaps in the data on measurement precision is poorly understood, in particular in Fourier space where the convolution of the observable with the observation window introduces correlations between different frequencies. Here we describe and implement a rather general method to retrieve maximum likelihood estimates of the oscillation parameters, taking into account the proper statistics of the observations. Our fitting method applies in complex Fourier space and exploits the phase information. We consider both solar-like stochastic oscillations and long-lived harmonic oscillations, plus random noise. Using numerical simulations, we demonstrate the existence of cases for which our improved fitting method is less biased and has a greater precision than when the frequency correlations are ignored. This is especially true of low signal-to-noise solar-like oscillations. For example, we discuss a case where the precision on the mode frequency estimate is increased by a factor of five, for a duty cycle of 15%. In the case of long-lived sinusoidal oscillations, a proper treatment of the frequency correlations does not provide any significant improvement; nevertheless we confirm that the mode frequency can be measured from gapped data at a much better precision than the 1/T Rayleigh resolution., Comment: Accepted for publication in Solar Physics Topical Issue "Helioseismology, Asteroseismology, and MHD Connections"
- Published
- 2008
21. Band terminations in valence-space and core-excited configurations in102Pd
- Author
-
D. T. Joss, E. S. Paul, J. Gizon, Gh. Câta-Danil, D. Santos, B. M. Nyakó, Ingemar Ragnarsson, L. Zolnai, N. J. O’Brien, A. T. Semple, János Timár, A. J. Boston, A. Gizon, J. Genevey, A. V. Afanasjev, and C. M. Parry
- Subjects
Physics ,Nuclear and High Energy Physics ,Valence (chemistry) ,Excited state ,Hadron ,General Physics and Astronomy ,Level structure ,Molecular physics - Abstract
The level structure of102Pd has been investigated using the Eurogam Phase2 array. Termination of rotational bands has been observed atI=28− andI=32+, and tentatively atI=38+ andI=42+. Three other bands evolving towards termination have also been identified. These terminating bands are explained in terms of valence-space and core-excited configurations.
- Published
- 1997
22. Structure of low-spin states in the doubly-odd 182Ir nucleus
- Author
-
A. Gizon, B. Roussière, J. Obert, D. Hojman, F. Ibrahim, F. Le Blanc, J. Sauvage, A. Knipper, J. Oms, J. Genevey, A. Wojtasiewicz, María Angélica Cardona, G. Marguier, Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), ISOLDE, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,Spin states ,010308 nuclear & particles physics ,Hadron ,Parity (physics) ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,21.10.Hw, 23.20.Lv, 23.20.Nx, 27.70.+q ,Excited state ,0103 physical sciences ,Quasiparticle ,Nuclear fusion ,Level structure ,Atomic physics ,010306 general physics ,Ground state - Abstract
Published online 7 August 2007; Low-spin states of $^{182}Ir$ were populated through the $\beta^+/EC$ decay of $^{182}Pt$. Two strong $E2$ transitions were observed for the first time: a 25.7keV transition in $^{182}Ir$ and a 34.0keV transition in Re of probable mass A = 178. Spin and parity, $I^\pi = 3^+$, are firmly assigned to the $^{182}Ir$ ground state (g.s.). For the excited states, the parity is established and the spin determined or restricted. These assignments support most of the interpretations of the level structure previously suggested. The systematics for the known $5^+ \to 3^+$ transitions in $\pi h_{9/2} \bigotimes ν 1/2^-[521]$ bands is presented. Using a semi-microscopic two-quasiparticle axial-rotor coupling model, particle configurations have been attributed or suggested for most of the coupled states lying at low energy in $^{182}Ir$.
- Published
- 2007
23. Helioseismology of Time-Varying Flows Through The Solar Cycle
- Author
-
Laurent Gizon
- Subjects
Physics ,Convection ,Sunspot ,Astronomy and Astrophysics ,Atmospheric sciences ,Meridional circulation ,Physics::Fluid Dynamics ,Convection zone ,Space and Planetary Science ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Differential rotation ,Helioseismology ,Variation (astronomy) ,Physics::Atmospheric and Oceanic Physics - Abstract
Flows in the upper convection zone are measured by helioseismology on a wide variety of scales. These include differential rotation and meridional circulation, local flows around complexes of magnetic activity and sunspots, and convective flows. The temporal evolution of flows through cycle 23 reveals connections between mass motions in the solar interior and the large-scale characteristics of the magnetic cycle. Here I summarize the latest observations and their implications. Observations from local helioseismology suggest that subsurface flows around active regions introduce a solar-cycle variation in the meridional circulation.
- Published
- 2004
24. Measuring Stellar Differential rotation with asteroseismology
- Author
-
Laurent Gizon and Sami K. Solanki
- Subjects
Rotation period ,Physics ,Stellar rotation ,Equator ,Astronomy ,Astronomy and Astrophysics ,Angular velocity ,Astrophysics ,Rotation ,Asteroseismology ,Stars ,Space and Planetary Science ,Astrophysics::Solar and Stellar Astrophysics ,Differential rotation ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics::Galaxy Astrophysics - Abstract
The variation of rotation with latitude is poorly known on stars other than the Sun. Several indirect techniques, photometric and spectroscopic, have been used to search for departure from rigid rotation for sufficiently fast rotators. Here we investigate the possibility of measuring stellar differential rotation for solar-type stars through asteroseismology. Rotationally split frequencies of global oscillation provide information about rotation at different latitudes depending on the azimuthal order, m, of the mode of pulsation. We present a method to estimate differential rotation based on the realization that the m =± 1a ndm =± 2 components of quadrupole oscillations can be observed simultaneously in asteroseismology. Rotational frequency splittings can be inverted to provide an estimate of the difference in stellar angular velocity between the equator and 45 ◦ latitude. The precision of the method, assessed through Monte Carlo simulations, depends on the value of the mean rotation and on the inclination angle between the rotation axis and the line of sight.
- Published
- 2004
25. The 130Nd↦130Pr↦130Ce decay chain revisited
- Author
-
P. Paris, A. Płochocki, J. Inchaouh, J. Genevey, I. Penev, C. F. Liang, A. Gizon, and D. Barnéoud
- Subjects
Physics ,Nuclear and High Energy Physics ,010308 nuclear & particles physics ,Branching fraction ,Hadron ,01 natural sciences ,Internal conversion ,Excited state ,0103 physical sciences ,Decay chain ,Atomic physics ,010306 general physics ,Nucleon ,Ground state ,Radioactive decay - Abstract
An investigation of low-lying energy levels of 130Pr and 130Ce has been made via β-decay. The radioactive parent nuclei were produced via 94,96Mo + 40Ca reactions at 6.8 MeV/nucleon and transported by a He-jet system. Gamma-γ-t, γ-X-t, γ-e--t coincidence measurements were performed. Internal conversion coefficients have been measured with a magnetic spectrometer. The new β-decay half-life of 130Nd has been determined to be 21(3) s. A partial level scheme of 130Pr at low-spin has been constructed. The β-decay of 130Pr to 130Ce suggests the existence of three β-instable isomeric states in 130Pr, while only one half-life T 1/2 = 40(4) s has been measured. Based on the present work and low-lying excited states in neighbouring odd-mass nuclei, the spins and parities of isomeric states in 130Pr are proposed to be 2+, (4,5)+ and (7,8±). The ground state in 130Pr is still undetermined.
- Published
- 2001
26. Low-spin states of doubly odd 182Au
- Author
-
J. C. Putaux, J. Sauvage, R. Béraud, P. Kilcher, G. Cata-Danil, C. Richard-Serre, J. Oms, G. Marguier, B. Roussière, A. Gizon, J. Obert, Nicole Collaborations, A. Knipper, J. Genevey, A. Wojtasiewicz, F. Le Blanc, F. Ibrahim, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), ISOLDE, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,Spin states ,010308 nuclear & particles physics ,Electron spectra ,Hadron ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,7. Clean energy ,Coincidence ,Spectral line ,0103 physical sciences ,Quasiparticle ,Nuclear fusion ,Atomic physics ,Nuclear Experiment ,010306 general physics - Abstract
Low-spin states of 184Au have been studied using the β+/EC decay of 184Hg. γ-ray and conversion-electron singles spectra were recorded with 184Hg mass-separated sources. For γ-γ-t and X-γ-t coincidence measurements, mercury nuclei were produced in the 148Sm + 40Ar reaction and transported by a He-jet system. The electron spectra were recorded from 184Hg sources produced at ISOLDE. A level scheme of 184Au including 48 transitions is proposed. The experimental results are interpreted in the frame of a semi-microscopic axial-rotor-plus-two-quasiparticle model developed in the context of the HF+BCS approximation.
- Published
- 2001
27. Seismic tomography of the near solar surface
- Author
-
Laurent Gizon, R. M. Larsen, and Thomas L. Duvall
- Subjects
Surface (mathematics) ,Physics ,Photosphere ,Sunspot ,Penumbra ,Flow (psychology) ,Astronomy and Astrophysics ,Geophysics ,Astrophysics ,Surface gravity ,Space and Planetary Science ,Seismic tomography ,Supergranulation ,Helioseismology ,Seismology ,Geology - Abstract
Surface gravity waves have been used to probe flows in the two megameters beneath the photosphere using the techniques of time-distance helioseismology. The results suggest that supergranule velocities are smaller than at the surface. The outward flow outside a sunspot penumbra (the moat) is observed, as is an inward flow in the region beyond the moat.
- Published
- 2000
28. [Untitled]
- Author
-
J. Sauvage, G. Marguier, J.C. Putaux, A. Wojtasiewicz, A. Gizon, B. Roussière, A. Knipper, J. Genevey, J. Obert, J. Oms, D. Forkel-Wirth, F. Le Blanc, F. Ibrahim, P. Kilcher, C. Richard-Serre, J. Lettry, and D. Hojman
- Subjects
Physics ,010308 nuclear & particles physics ,education ,Resolution (electron density) ,High resolution ,Elementary particle ,Fermion ,Electron ,equipment and supplies ,01 natural sciences ,mental disorders ,0103 physical sciences ,Energy transformation ,Atomic physics ,010306 general physics ,Spectrograph ,Lepton - Abstract
High-resolution measurements of low-energy conversion electrons have been performed in odd and odd–odd nuclei with masses around A=182. The experimental setup, a magnetic spectrograph coupled to a specific tape transport system, is described. Three experiments have been performed and the main results are presented.
- Published
- 2000
29. Five-quasiparticle bands in 127Ba
- Author
-
Dewald, A., Schmidt, A., Alexius, G., Vogel, O., Chakrawarthy, R. S., Bazzacco, D., von Brentano, P., Gizon, A., Gizon, J., Lunardi, Santo, Napoli, D. R., Pavan, Pietro, Rossi Alvarez, C., Wiedenh, I., x000F6, Ver, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,Spin states ,Spins ,010308 nuclear & particles physics ,Hadron ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,Nuclear physics ,0103 physical sciences ,Quasiparticle ,Nuclear fusion ,Atomic physics ,Nuclear Experiment ,010306 general physics ,Beam energy - Abstract
High spin states in 127Ba have been investigated with the fusion–evaporation reaction 96Zr(36S,5n)127Ba at a beam energy of 150 MeV with the GASP-spectrometer at INFN in Legnaro, Italy. The level scheme could be extended to high spins resulting in the observation of five-quasiparticle states. Altogether 15 band structures were placed in the level scheme.
- Published
- 1998
30. Coexistence of terminating bands and more collective bands in theA ∼ 100 region of nuclei
- Author
-
I. Ragnarsson, A. V. Afanasjev, and J. Gizon
- Subjects
Nuclear and High Energy Physics - Published
- 1996
31. Coexistence of terminating bands and more collective bands in the A ∼ 100 region of nuclei
- Author
-
J. Gizon, Ingemar Ragnarsson, and A. V. Afanasjev
- Subjects
Physics ,Nuclear and High Energy Physics ,Normalization property ,Spins ,Nuclear fusion ,Nanotechnology ,Atomic physics ,Ground state - Abstract
Nilsson-Strutinsky cranking calculations on A ≥ 100 Ru and Pd nuclei suggest that, contrary to other mass regions, it should be possible to follow the ground state rotational bands to their termination at spins just above I = 30ℏ and then also to observe other bands which terminate at higher spins.
- Published
- 1996
32. The EChO science case
- Author
-
Tinetti, Giovanna, primary, Drossart, Pierre, additional, Eccleston, Paul, additional, Hartogh, Paul, additional, Isaak, Kate, additional, Linder, Martin, additional, Lovis, Christophe, additional, Micela, Giusi, additional, Ollivier, Marc, additional, Puig, Ludovic, additional, Ribas, Ignasi, additional, Snellen, Ignas, additional, Swinyard, Bruce, additional, Allard, France, additional, Barstow, Joanna, additional, Cho, James, additional, Coustenis, Athena, additional, Cockell, Charles, additional, Correia, Alexandre, additional, Decin, Leen, additional, de Kok, Remco, additional, Deroo, Pieter, additional, Encrenaz, Therese, additional, Forget, Francois, additional, Glasse, Alistair, additional, Griffith, Caitlin, additional, Guillot, Tristan, additional, Koskinen, Tommi, additional, Lammer, Helmut, additional, Leconte, Jeremy, additional, Maxted, Pierre, additional, Mueller-Wodarg, Ingo, additional, Nelson, Richard, additional, North, Chris, additional, Pallé, Enric, additional, Pagano, Isabella, additional, Piccioni, Guseppe, additional, Pinfield, David, additional, Selsis, Franck, additional, Sozzetti, Alessandro, additional, Stixrude, Lars, additional, Tennyson, Jonathan, additional, Turrini, Diego, additional, Zapatero-Osorio, Mariarosa, additional, Beaulieu, Jean-Philippe, additional, Grodent, Denis, additional, Guedel, Manuel, additional, Luz, David, additional, Nørgaard-Nielsen, Hans Ulrik, additional, Ray, Tom, additional, Rickman, Hans, additional, Selig, Avri, additional, Swain, Mark, additional, Banaszkiewicz, Marek, additional, Barlow, Mike, additional, Bowles, Neil, additional, Branduardi-Raymont, Graziella, additional, du Foresto, Vincent Coudé, additional, Gerard, Jean-Claude, additional, Gizon, Laurent, additional, Hornstrup, Allan, additional, Jarchow, Christopher, additional, Kerschbaum, Franz, additional, Kovacs, Géza, additional, Lagage, Pierre-Olivier, additional, Lim, Tanya, additional, Lopez-Morales, Mercedes, additional, Malaguti, Giuseppe, additional, Pace, Emanuele, additional, Pascale, Enzo, additional, Vandenbussche, Bart, additional, Wright, Gillian, additional, Zapata, Gonzalo Ramos, additional, Adriani, Alberto, additional, Azzollini, Ruymán, additional, Balado, Ana, additional, Bryson, Ian, additional, Burston, Raymond, additional, Colomé, Josep, additional, Crook, Martin, additional, Di Giorgio, Anna, additional, Griffin, Matt, additional, Hoogeveen, Ruud, additional, Ottensamer, Roland, additional, Irshad, Ranah, additional, Middleton, Kevin, additional, Morgante, Gianluca, additional, Pinsard, Frederic, additional, Rataj, Mirek, additional, Reess, Jean-Michel, additional, Savini, Giorgio, additional, Schrader, Jan-Rutger, additional, Stamper, Richard, additional, Winter, Berend, additional, Abe, L., additional, Abreu, M., additional, Achilleos, N., additional, Ade, P., additional, Adybekian, V., additional, Affer, L., additional, Agnor, C., additional, Agundez, M., additional, Alard, C., additional, Alcala, J., additional, Allende Prieto, C., additional, Alonso Floriano, F. J., additional, Altieri, F., additional, Alvarez Iglesias, C. A., additional, Amado, P., additional, Andersen, A., additional, Aylward, A., additional, Baffa, C., additional, Bakos, G., additional, Ballerini, P., additional, Banaszkiewicz, M., additional, Barber, R. J., additional, Barrado, D., additional, Barton, E. J., additional, Batista, V., additional, Bellucci, G., additional, Belmonte Avilés, J. A., additional, Berry, D., additional, Bézard, B., additional, Biondi, D., additional, Błęcka, M., additional, Boisse, I., additional, Bonfond, B., additional, Bordé, P., additional, Börner, P., additional, Bouy, H., additional, Brown, L., additional, Buchhave, L., additional, Budaj, J., additional, Bulgarelli, A., additional, Burleigh, M., additional, Cabral, A., additional, Capria, M. T., additional, Cassan, A., additional, Cavarroc, C., additional, Cecchi-Pestellini, C., additional, Cerulli, R., additional, Chadney, J., additional, Chamberlain, S., additional, Charnoz, S., additional, Christian Jessen, N., additional, Ciaravella, A., additional, Claret, A., additional, Claudi, R., additional, Coates, A., additional, Cole, R., additional, Collura, A., additional, Cordier, D., additional, Covino, E., additional, Danielski, C., additional, Damasso, M., additional, Deeg, H. J., additional, Delgado-Mena, E., additional, Del Vecchio, C., additional, Demangeon, O., additional, De Sio, A., additional, De Wit, J., additional, Dobrijévic, M., additional, Doel, P., additional, Dominic, C., additional, Dorfi, E., additional, Eales, S., additional, Eiroa, C., additional, Espinoza Contreras, M., additional, Esposito, M., additional, Eymet, V., additional, Fabrizio, N., additional, Fernández, M., additional, Femenía Castella, B., additional, Figueira, P., additional, Filacchione, G., additional, Fletcher, L., additional, Focardi, M., additional, Fossey, S., additional, Fouqué, P., additional, Frith, J., additional, Galand, M., additional, Gambicorti, L., additional, Gaulme, P., additional, García López, R. J., additional, Garcia-Piquer, A., additional, Gear, W., additional, Gerard, J.-C., additional, Gesa, L., additional, Giani, E., additional, Gianotti, F., additional, Gillon, M., additional, Giro, E., additional, Giuranna, M., additional, Gomez, H., additional, Gomez-Leal, I., additional, Gonzalez Hernandez, J., additional, González Merino, B., additional, Graczyk, R., additional, Grassi, D., additional, Guardia, J., additional, Guio, P., additional, Gustin, J., additional, Hargrave, P., additional, Haigh, J., additional, Hébrard, E., additional, Heiter, U., additional, Heredero, R. L., additional, Herrero, E., additional, Hersant, F., additional, Heyrovsky, D., additional, Hollis, M., additional, Hubert, B., additional, Hueso, R., additional, Israelian, G., additional, Iro, N., additional, Irwin, P., additional, Jacquemoud, S., additional, Jones, G., additional, Jones, H., additional, Justtanont, K., additional, Kehoe, T., additional, Kerschbaum, F., additional, Kerins, E., additional, Kervella, P., additional, Kipping, D., additional, Koskinen, T., additional, Krupp, N., additional, Lahav, O., additional, Laken, B., additional, Lanza, N., additional, Lellouch, E., additional, Leto, G., additional, Licandro Goldaracena, J., additional, Lithgow-Bertelloni, C., additional, Liu, S. J., additional, Lo Cicero, U., additional, Lodieu, N., additional, Lognonné, P., additional, Lopez-Puertas, M., additional, Lopez-Valverde, M. A., additional, Lundgaard Rasmussen, I., additional, Luntzer, A., additional, Machado, P., additional, MacTavish, C., additional, Maggio, A., additional, Maillard, J.-P., additional, Magnes, W., additional, Maldonado, J., additional, Mall, U., additional, Marquette, J.-B., additional, Mauskopf, P., additional, Massi, F., additional, Maurin, A.-S., additional, Medvedev, A., additional, Michaut, C., additional, Miles-Paez, P., additional, Montalto, M., additional, Montañés Rodríguez, P., additional, Monteiro, M., additional, Montes, D., additional, Morais, H., additional, Morales, J. C., additional, Morales-Calderón, M., additional, Morello, G., additional, Moro Martín, A., additional, Moses, J., additional, Moya Bedon, A., additional, Murgas Alcaino, F., additional, Oliva, E., additional, Orton, G., additional, Palla, F., additional, Pancrazzi, M., additional, Pantin, E., additional, Parmentier, V., additional, Parviainen, H., additional, Peña Ramírez, K. Y., additional, Peralta, J., additional, Perez-Hoyos, S., additional, Petrov, R., additional, Pezzuto, S., additional, Pietrzak, R., additional, Pilat-Lohinger, E., additional, Piskunov, N., additional, Prinja, R., additional, Prisinzano, L., additional, Polichtchouk, I., additional, Poretti, E., additional, Radioti, A., additional, Ramos, A. A., additional, Rank-Lüftinger, T., additional, Read, P., additional, Readorn, K., additional, Rebolo López, R., additional, Rebordão, J., additional, Rengel, M., additional, Rezac, L., additional, Rocchetto, M., additional, Rodler, F., additional, Sánchez Béjar, V. J., additional, Sanchez Lavega, A., additional, Sanromá, E., additional, Santos, N., additional, Sanz Forcada, J., additional, Scandariato, G., additional, Schmider, F.-X., additional, Scholz, A., additional, Scuderi, S., additional, Sethenadh, J., additional, Shore, S., additional, Showman, A., additional, Sicardy, B., additional, Sitek, P., additional, Smith, A., additional, Soret, L., additional, Sousa, S., additional, Stiepen, A., additional, Stolarski, M., additional, Strazzulla, G., additional, Tabernero, H. M., additional, Tanga, P., additional, Tecsa, M., additional, Temple, J., additional, Terenzi, L., additional, Tessenyi, M., additional, Testi, L., additional, Thompson, S., additional, Thrastarson, H., additional, Tingley, B. W., additional, Trifoglio, M., additional, Martín Torres, J., additional, Tozzi, A., additional, Turrini, D., additional, Varley, R., additional, Vakili, F., additional, de Val-Borro, M., additional, Valdivieso, M. L., additional, Venot, O., additional, Villaver, E., additional, Vinatier, S., additional, Viti, S., additional, Waldmann, I., additional, Waltham, D., additional, Ward-Thompson, D., additional, Waters, R., additional, Watkins, C., additional, Watson, D., additional, Wawer, P., additional, Wawrzaszk, A., additional, White, G., additional, Widemann, T., additional, Winek, W., additional, Wiśniowski, T., additional, Yelle, R., additional, Yung, Y., additional, and Yurchenko, S. N., additional
- Published
- 2015
- Full Text
- View/download PDF
33. Interpretation of Helioseismic Travel Times
- Author
-
Burston, Raymond, primary, Gizon, Laurent, additional, and Birch, Aaron C., additional
- Published
- 2015
- Full Text
- View/download PDF
34. The alpha decay study of223Th (T 1/2=0.6 s)
- Author
-
V. Barci, A. Gizon, D. Barneou, R. Béraud, J. Genevey, Ch. Briançon, C. F. Liang, P. Paris, Raymond K. Sheline, and J. Blachot
- Subjects
Physics ,Nuclear and High Energy Physics ,Spins ,media_common.quotation_subject ,Parity (physics) ,Asymmetry ,medicine.anatomical_structure ,Atomic orbital ,medicine ,Nuclear fusion ,Alpha decay ,Atomic physics ,Ground state ,Nucleus ,media_common - Abstract
The219Ra levels, fed by the α-decay of223Th, have been studied by anα−γ coincidence experiment. AK=1/2+ band, based on the 7/2+ ground state, with a large decoupling parameter a=−5.5 is proposed. Three levels with spins 5/2, 9/2, 7/2 and lowα-hindrance factors around 140 keV, can be considered as members of aK=5/2+ band, perturbed by the Coriolis coupling of configurations arising from theg9/2 shell. TheseK =1/2+ and 5/2+ orbitals are expected forN=131 in the reflection asymmetry model with ɛ2≃ɛ3−0.1. How-ever no evidence was found for the corresponding negative parity bands in this transitional nucleus.
- Published
- 1992
35. Local Helioseismology
- Author
-
Laurent Gizon and Aaron Birch
- Subjects
Space and Planetary Science ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Astronomy and Astrophysics - Published
- 2005
36. The PLATO 2.0 mission
- Author
-
Rauer, H., primary, Catala, C., additional, Aerts, C., additional, Appourchaux, T., additional, Benz, W., additional, Brandeker, A., additional, Christensen-Dalsgaard, J., additional, Deleuil, M., additional, Gizon, L., additional, Goupil, M.-J., additional, Güdel, M., additional, Janot-Pacheco, E., additional, Mas-Hesse, M., additional, Pagano, I., additional, Piotto, G., additional, Pollacco, D., additional, Santos, Ċ., additional, Smith, A., additional, Suárez, J.-C., additional, Szabó, R., additional, Udry, S., additional, Adibekyan, V., additional, Alibert, Y., additional, Almenara, J.-M., additional, Amaro-Seoane, P., additional, Eiff, M. Ammler-von, additional, Asplund, M., additional, Antonello, E., additional, Barnes, S., additional, Baudin, F., additional, Belkacem, K., additional, Bergemann, M., additional, Bihain, G., additional, Birch, A. C., additional, Bonfils, X., additional, Boisse, I., additional, Bonomo, A. S., additional, Borsa, F., additional, Brandão, I. M., additional, Brocato, E., additional, Brun, S., additional, Burleigh, M., additional, Burston, R., additional, Cabrera, J., additional, Cassisi, S., additional, Chaplin, W., additional, Charpinet, S., additional, Chiappini, C., additional, Church, R. P., additional, Csizmadia, Sz., additional, Cunha, M., additional, Damasso, M., additional, Davies, M. B., additional, Deeg, H. J., additional, Díaz, R. F., additional, Dreizler, S., additional, Dreyer, C., additional, Eggenberger, P., additional, Ehrenreich, D., additional, Eigmüller, P., additional, Erikson, A., additional, Farmer, R., additional, Feltzing, S., additional, Oliveira Fialho, F. de, additional, Figueira, P., additional, Forveille, T., additional, Fridlund, M., additional, García, R. A., additional, Giommi, P., additional, Giuffrida, G., additional, Godolt, M., additional, da Silva, J. Gomes, additional, Granzer, T., additional, Grenfell, J. L., additional, Grotsch-Noels, A., additional, Günther, E., additional, Haswell, C. A., additional, Hatzes, A. P., additional, Hébrard, G., additional, Hekker, S., additional, Helled, R., additional, Heng, K., additional, Jenkins, J. M., additional, Johansen, A., additional, Khodachenko, M. L., additional, Kislyakova, K. G., additional, Kley, W., additional, Kolb, U., additional, Krivova, N., additional, Kupka, F., additional, Lammer, H., additional, Lanza, A. F., additional, Lebreton, Y., additional, Magrin, D., additional, Marcos-Arenal, P., additional, Marrese, P. M., additional, Marques, J. P., additional, Martins, J., additional, Mathis, S., additional, Mathur, S., additional, Messina, S., additional, Miglio, A., additional, Montalban, J., additional, Montalto, M., additional, P. F. G. Monteiro, M. J., additional, Moradi, H., additional, Moravveji, E., additional, Mordasini, C., additional, Morel, T., additional, Mortier, A., additional, Nascimbeni, V., additional, Nelson, R. P., additional, Nielsen, M. B., additional, Noack, L., additional, Norton, A. J., additional, Ofir, A., additional, Oshagh, M., additional, Ouazzani, R.-M., additional, Pápics, P., additional, Parro, V. C., additional, Petit, P., additional, Plez, B., additional, Poretti, E., additional, Quirrenbach, A., additional, Ragazzoni, R., additional, Raimondo, G., additional, Rainer, M., additional, Reese, D. R., additional, Redmer, R., additional, Reffert, S., additional, Rojas-Ayala, B., additional, Roxburgh, I. W., additional, Salmon, S., additional, Santerne, A., additional, Schneider, J., additional, Schou, J., additional, Schuh, S., additional, Schunker, H., additional, Silva-Valio, A., additional, Silvotti, R., additional, Skillen, I., additional, Snellen, I., additional, Sohl, F., additional, Sousa, S. G., additional, Sozzetti, A., additional, Stello, D., additional, Strassmeier, K. G., additional, Švanda, M., additional, Szabó, Gy. M., additional, Tkachenko, A., additional, Valencia, D., additional, Van Grootel, V., additional, Vauclair, S. D., additional, Ventura, P., additional, Wagner, F. W., additional, Walton, N. A., additional, Weingrill, J., additional, Werner, S. C., additional, Wheatley, P. J., additional, and Zwintz, K., additional
- Published
- 2014
- Full Text
- View/download PDF
37. Magnetic Flux Transport at the Solar Surface
- Author
-
Jiang, J., primary, Hathaway, D. H., additional, Cameron, R. H., additional, Solanki, S. K., additional, Gizon, L., additional, and Upton, L., additional
- Published
- 2014
- Full Text
- View/download PDF
38. Helioseismology with Solar Orbiter
- Author
-
Löptien, Björn, primary, Birch, Aaron C., additional, Gizon, Laurent, additional, Schou, Jesper, additional, Appourchaux, Thierry, additional, Blanco Rodríguez, Julián, additional, Cally, Paul S., additional, Dominguez-Tagle, Carlos, additional, Gandorfer, Achim, additional, Hill, Frank, additional, Hirzberger, Johann, additional, Scherrer, Philip H., additional, and Solanki, Sami K., additional
- Published
- 2014
- Full Text
- View/download PDF
39. Interpreting the Helioseismic and Magnetic Imager (HMI) Multi-Height Velocity Measurements
- Author
-
Nagashima, Kaori, primary, Löptien, Björn, additional, Gizon, Laurent, additional, Birch, Aaron C., additional, Cameron, Robert, additional, Couvidat, Sebastien, additional, Danilovic, Sanja, additional, Fleck, Bernhard, additional, and Stein, Robert, additional
- Published
- 2014
- Full Text
- View/download PDF
40. Propagating Linear Waves in Convectively Unstable Stellar Models: A Perturbative Approach
- Author
-
Papini, E., primary, Gizon, L., additional, and Birch, A. C., additional
- Published
- 2013
- Full Text
- View/download PDF
41. Erratum to: Helioseismology of Sunspots: A Case Study of NOAA Region 9787
- Author
-
T. Stahn, Robert P. Cameron, Markus Roth, Sarbani Basu, Aaron C. Birch, S. Zharkov, Thomas L. Duvall, D. C. Braun, Hannah Schunker, Jason Jackiewicz, Laurent Gizon, Charles S. Baldner, R. S. Bogart, Michael Thompson, and Shravan M. Hanasoge
- Subjects
Sunspot ,Planetary science ,Meteorology ,Space and Planetary Science ,Astronomy ,Astronomy and Astrophysics ,Helioseismology ,Geology - Published
- 2010
42. Band structures in doubly-odd 100Rh
- Author
-
D. T. Joss, József Tímár, E. S. Paul, A. T. Semple, A. Gizon, B. M. Nyakó, J. Gizon, L. Zolnai, A. J. Boston, N. J. O’Brien, C. M. Parry, Gh. Căta-Danil, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,Spin states ,010308 nuclear & particles physics ,Hadron ,State (functional analysis) ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,0103 physical sciences ,Nuclear fusion ,Level structure ,Atomic physics ,010306 general physics ,Excitation ,Energy (signal processing) - Abstract
High spin states of 100Rh have been populated using the reaction 70Zn+36S at 130 MeV. γ-rays were detected with the EUROGAM2 array. The level structure of 100Rh has been extended up to 14.41 MeV excitation energy. Several band structures are observed. A band based on a Iπ=8− state is developed up to the Iπ=24− level. It is assigned as the πg 9/2 −5νh 11/2 configuration.
- Published
- 1998
43. Excited states of 154Tm
- Author
-
Foin, C., primary, Gizon, A., additional, Genevey, J., additional, Gizon, J., additional, Paris, P., additional, Farget, F., additional, Santos, D., additional, Barnéoud, D., additional, and Płochocki, A., additional
- Published
- 2002
- Full Text
- View/download PDF
44. High-spin states in the 96Tc nucleus
- Author
-
Bucurescu, D., primary, Căta-Danil, Gh., additional, Căta-Danil, I., additional, Ivaşcu, M., additional, Mărginean, N., additional, Rusu, C., additional, Stroe, L., additional, Ur, C.A., additional, Gizon, A., additional, Gizon, J., additional, Nyakó, B., additional, Timár, J., additional, Zolnai, L., additional, Boston, A.J., additional, Joss, D.T., additional, Paul, E.S., additional, Semple, A.T., additional, and Parry, C.M., additional
- Published
- 2001
- Full Text
- View/download PDF
45. Level structure of 123Cs observed from 123Ba decay and described using the IBFM and CQPC models
- Author
-
Gizon, A., primary, Weiss, B., additional, Paris, P., additional, Liang, C. F., additional, Genevey, J., additional, Gizon, J., additional, Barci, V., additional, Căta-Danil, Gh., additional, Dionisio, J. S., additional, Lagrange, J. M., additional, Pautrat, M., additional, Vanhorenbeeck, J., additional, Vieu, Ch., additional, Zolnai, L., additional, Arias, J. M., additional, Barea, J., additional, and Droste, Ch., additional
- Published
- 2000
- Full Text
- View/download PDF
46. New investigation of the decay of the high-spin isomer in 151Er
- Author
-
Foin, C., primary, Gizon, A., additional, Barnéoud, D., additional, Genevey, J., additional, Gizon, J., additional, Santos, D., additional, Farget, F., additional, Paris, P., additional, Liang, C. F., additional, Bucurescu, D., additional, and Płochocki, A., additional
- Published
- 2000
- Full Text
- View/download PDF
47. New insight in the level structure of
- Author
-
Foin, C., primary, Farget, F., additional, Gizon, A., additional, Santos, D., additional, Barnéoud, D., additional, Genevey, J., additional, Gizon, J., additional, Paris, P., additional, Ashgar, M., additional, and Płochocki, A., additional
- Published
- 2000
- Full Text
- View/download PDF
48. Configuration assignments and decay of 126La high-spin bands
- Author
-
Timár, J., primary, Gizon, A., additional, Paris, P., additional, Genevey, J., additional, Gizon, J., additional, Hannachi, F., additional, Liang, C.F., additional, Lopez-Martens, A., additional, Merdinger, J.C., additional, Nyakó, B.M., additional, Weiss, B., additional, and Zolnai, L., additional
- Published
- 2000
- Full Text
- View/download PDF
49. High spin band structures in104Cd
- Author
-
Birger Fogelberg, Bo Cederwall, A. Johnson, Lars-Olov Norlin, R.A. Bark, A. Gizon, S. Törmänen, D. Seweryniak, S. Mitarai, M. Piiparinen, E. Adamides, J. Kownacki, Dan Jerrestam, R. Julin, A. Atac, J. Gizon, Ramon Wyss, Ari Virtanen, Andras Kerek, R. Schubart, E. Ideguchi, Claes Fahlander, H. Grawe, Wlodzimierz Klamra, S. Juutinen, G. Sletten, Johan Nyberg, and W. Kaczmarczyk
- Subjects
Physics ,Nuclear and High Energy Physics ,Spin states ,Nuclear fusion ,Heavy ion ,Detector array ,Atomic physics ,Nuclear Experiment - Abstract
High spin states in Cd-104 have been investigated by means of heavy ion induced reactions using the Nordball detector array. The level scheme constructed from yy-coincidences is dominated by three ...
- Published
- 1995
50. High spin states in 128Ba
- Author
-
Vogel, O., primary, Chakrawarthy, R.S., additional, Dewald, A., additional, Petkov, P., additional, Jessen, K., additional, Gableske, J., additional, von Brentano, P., additional, Bazzacco, D., additional, Gizon, A., additional, Gizon, J., additional, Lunardi, S., additional, Napoli, D.R., additional, Pavan, P., additional, Rossi Alvarez, C., additional, and Wiedenhöver, I., additional
- Published
- 1999
- Full Text
- View/download PDF
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.