Spin determination of isobaric analogue resonances in209Bi and207Bi by proton polarization measurements

1969 ◽  
Vol 221 (5) ◽  
pp. 494-497 ◽  
Author(s):  
S. Fiarman ◽  
N. Marquardt
Keyword(s):  
Proton Polarization ◽  
Polarization Measurements ◽  
Isobaric Analogue ◽  
Spin Determination

Proton polarization measurements near isobaric analogue resonances in 145Eu

1969 ◽  
Vol 131 (2) ◽  
pp. 267-272 ◽  
Author(s):  
S. Fiarman ◽  
E.J. Ludwig ◽  
L.S. Michelman ◽  
A.B. Robbins
Keyword(s):  
Proton Polarization ◽  
Polarization Measurements ◽  
Isobaric Analogue

Spin determination of deeply-bound hole states from ( $$\vec d$$ ,3He) reactions

1980 ◽  
Vol 297 (4) ◽  
pp. 307-309 ◽  
Author(s):  
A. Stuirbrink ◽  
G. J. Wagner ◽  
K. T. Kn�pfle ◽  
Liu Ken Pao ◽  
G. Mairle ◽  
...  
Keyword(s):  
Spin Determination

Spin determination of the 12C + 12C resonance at Ec.m. = 6.25 MeV

1977 ◽  
Vol 67 (3) ◽  
pp. 262-264 ◽  
Author(s):  
W. Galster ◽  
W. Treu ◽  
P. Dück ◽  
H. Fröhlich ◽  
H. Voit
Keyword(s):  
Spin Determination

WISE data and sparse photometry used for shape reconstruction of asteroids

2015 ◽  
Vol 10 (S318) ◽  
pp. 170-176 ◽  
Author(s):  
Josef Ďurech ◽  
Josef Hanuš ◽  
Victor M. Alí-Lagoa ◽  
Marco Delbo ◽  
Dagmara A. Oszkiewicz
Keyword(s):  
Rotation Period ◽  
Shape Reconstruction ◽  
Physical Models ◽  
Inversion Method ◽  
Wide Field ◽  
Reflected Light ◽  
Space Data ◽  
Spin Determination ◽  
Infrared Survey

AbstractAsteroid disk-integrated sparse-in-time photometry can be used for determination of shapes and spin states of asteroids by the lightcurve inversion method. To clearly distinguish the correct solution of the rotation period from other minima in the parameter space, data with good photometric accuracy are needed. We show that if the low-quality sparse photometry obtained from ground-based astrometric surveys is combined with data from the Wide-field Infrared Survey Explorer (WISE) satellite, the correct rotation period can be successfully derived. Although WISE observed in mid-IR wavelengths, we show that for the period and spin determination, these data can be modelled as reflected light. The absolute fluxes are not required since only relative variation of the flux over the rotation is sufficient to determine the period. We also discuss the potential of combining all WISE data with the Lowell photometric database to create physical models of thousands of asteroids.

Spin Determination of Intermediate Structure in the Subthreshold Fission ofNp237

1973 ◽  
Vol 8 (6) ◽  
pp. 2352-2363 ◽  
Author(s):  
G. A. Keyworth ◽  
J. R. Lemley ◽  
C. E. Olsen ◽  
F. T. Seibel ◽  
J. W. T. Dabbs ◽  
...  
Keyword(s):  
Intermediate Structure ◽  
Spin Determination

scholarly journals Precision, absolute proton polarization measurements at 200 MeV beam energy

2011 ◽  
Vol 295 ◽  
pp. 012132 ◽  
Author(s):  
A Zelenski ◽  
G Atoian ◽  
A Bogdanov ◽  
D Raparia ◽  
M Runtso ◽  
...  
Keyword(s):  
Beam Energy ◽  
Proton Polarization ◽  
Polarization Measurements
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