0000000001290921

AUTHOR

T. Lange

showing 4 related works from this author

Development of quadrupole collectivity in the neutron-rich Ni, Zn, Ge, and Se isotopes

2003

An experiment was performed to study the collective properties of neutron-rich Ni, Zn, Ge, and Se isotopes. Of particular interest is the vicinity of the N = 50 and Z = 28 shell closures. For most neutron-rich nuclei in this region of the chart of nuclei the B(E2) values of the transitions from the ground to the first excited 2+ states are unknown. This information would give valuable insight into the changes in nuclear structure when going to more neutron-rich nuclei.

PhysicsIsotopes of seleniumIsotopes of germaniumExcited stateNuclear TheoryQuadrupoleIsotopes of zincNuclear structureNeutronCoulomb excitationAtomic physicsNuclear Experiment
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The polarimetric and helioseismic imager on solar orbiter

2020

This paper describes the Polarimetric and Helioseismic Imager on the Solar Orbiter mission (SO/PHI), the first magnetograph and helioseismology instrument to observe the Sun from outside the Sun-Earth line. It is the key instrument meant to address the top-level science question: How does the solar dynamo work and drive connections between the Sun and the heliosphere? SO/PHI will also play an important role in answering the other top-level science questions of Solar Orbiter, as well as hosting the potential of a rich return in further science. SO/PHI measures the Zeeman effect and the Doppler shift in the FeI 617.3nm spectral line. To this end, the instrument carries out narrow-band imaging…

Solar Telescope010504 meteorology & atmospheric sciencesphotosphere [Sun]FiltegramsHighly elliptical orbitFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionTelescopeOrbiterPhotospherelaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHelioseismologySolar dynamo010303 astronomy & astrophysicsSun: magnetic fieldsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesSun: helioseismologyPhysics[PHYS]Physics [physics]PhotosphereEllipsometrypolarimeters [Instrumentation]Spacecraftbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyinstrumentation: polarimetersSun: photosphereHeliosismologiaAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiestechniques: polarimetricmagnetic fields [Sun]Space and Planetary Sciencetechniques: imaging spectroscopyAstrophysics of Galaxies (astro-ph.GA)Physics::Space PhysicsHelioseismologyAstrophysics::Earth and Planetary AstrophysicsbusinessAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HeliosphereEl·lipsometria
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Coulomb breakup of 23O

2005

Abstract The ground-state structure of the near-drip-line nucleus 23O has been investigated in a one-neutron Coulomb breakup reaction. Differential cross sections d σ / d E * for electromagnetic excitation of 23O projectiles (422 MeV/nucleon) incident on a lead target have been obtained from the measurement of the momenta of all breakup products including γ rays. The analysis of the deduced dipole-transition probability into the continuum infers a 2 s 1 / 2 ⊗ O 22 ( 0 + ) ground state configuration with a spectroscopic factor of 0.77(10) and thus a ground-state spin I π ( O 23 ) = 1 / 2 + , resolving earlier conflicting experimental findings. Final-state interaction is of significant influe…

PhysicsNuclear and High Energy PhysicsNuclear TheoryCoulombScattering lengthNeutron scatteringAtomic physicsNuclear ExperimentNucleonGround stateBreakupExcitationSpin-½Physics Letters B
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Performance Analysis of the SO/PHI Software Framework for On-board Data Reduction

2019

The Polarimetric and Helioseismic Imager (PHI) is the first deep-space solar spectropolarimeter, on-board the Solar Orbiter (SO) space mission. It faces: stringent requirements on science data accuracy, a dynamic environment, and severe limitations on telemetry volume. SO/PHI overcomes these restrictions through on-board instrument calibration and science data reduction, using dedicated firmware in FPGAs. This contribution analyses the accuracy of a data processing pipeline by comparing the results obtained with SO/PHI hardware to a reference from a ground computer. The results show that for the analyzed pipeline the error introduced by the firmware implementation is well below the requirem…

Astrophysics - Solar and Stellar AstrophysicsAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstrophysics::Solar and Stellar AstrophysicsComputerSystemsOrganization_SPECIAL-PURPOSEANDAPPLICATION-BASEDSYSTEMSAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)
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