Sub-Coulomb Stripping in the 124Sn(d,p)125Sn Reaction

Powell, D.L.; Dallimore, P.J.; Davidson, W.F.

doi:10.1071/ph710793

Cited by 6 publications

(1 citation statement)

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“…Type III bursts are usually weakly circularly polarized with H emission having a lower degree of polarization than F emission (e.g. McLean 1971;Suzuki & Sheridan 1977;Suzuki & Dulk 1985). made a thorough analysis of polarization characteristics of 997 bursts, finding the average degree of polarization of F-H pairs was 0.35 and 0.11 respectively while structureless bursts only had a polarization of 0.06.…”

Section: Polarizationmentioning

confidence: 99%

A review of solar type III radio bursts

Reid

Ratcliffe

2014

Res. Astron. Astrophys.

341

217

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Solar type III radio bursts are an important diagnostic tool in the understanding of solar accelerated electron beams. They are a signature of propagating beams of nonthermal electrons in the solar atmosphere and the solar system. Consequently, they provide information on electron acceleration and transport, and the conditions of the background ambient plasma they travel through. We review the observational properties of type III bursts with an emphasis on recent results and how each property can help identify attributes of electron beams and the ambient background plasma. We also review some of the theoretical aspects of type III radio bursts and cover a number of numerical efforts that simulate electron beam transport through the solar corona and the heliosphere.

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Section: Polarizationmentioning

confidence: 99%

A review of solar type III radio bursts

Reid

Ratcliffe

2014

Res. Astron. Astrophys.

341

217

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Number-projected three-quasiparticle description of the odd Sn isotopes

1978

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An account is given of the description of the low-energy properties of the odd Sn nuclei in terms of number projected one-(1 q.p.) and three-quasiparticle (3 q.p.) states. The shell model space for the neutrons consists of one major shell. A simple Gaussian force is used as an effective interaction. Its strength and the single-particle energies, which are the only parameters, are derived in a consistent way from spectroscopic data on the onequasiparticle states. We find that the spectra can be well interpreted in terms of l q.p. and 3q.p. states. Branching ratios of gamma decay, one-nucleon transfer spectroscopic factors, electric and magnetic moments show generally good agreement with the experimental data. For halflives and mixing ratios, which are most sensitive to details of the 3 q.p. components, the agreement is less, but all have the correct order of magnitude.

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