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Surprising Sun: A New Step Towards a Complete Picture?
DOI: 10.1103/PhysRevLett.93.211102 Bibcode: 2004PhRvL..93u1102T

García, R. A.; Turck-Chièze, S.; Piau, L. +5 more

Important revisions of the solar model ingredients have appeared recently. We first show that the updated CNO composition suppresses the anomalous position of the Sun in the known galactic enrichment. The following law, He/H=0.075+44.6 O/H in number fraction, is now compatible with all the indicators. We then suggest some directions of investigati…

2004 Physical Review Letters
SOHO 144
Theory and Observations of Slow-Mode Solitons in Space Plasmas
DOI: 10.1103/PhysRevLett.93.125004 Bibcode: 2004PhRvL..93l5004S

Stasiewicz, K.

A generalized model for one-dimensional magnetosonic structures of large amplitude in space plasmas is presented. The model is verified with multipoint measurements on Cluster satellites in the magnetosheath and the boundary layer under conditions of plasma beta (plasma/magnetic pressure) between 0.1 10. We demonstrate good agreement between the m…

2004 Physical Review Letters
Cluster 88
Slow Magnetosonic Solitons Detected by the Cluster Spacecraft
DOI: 10.1103/PhysRevLett.90.085002 Bibcode: 2003PhRvL..90h5002S

Lavraud, B.; Buchert, S.; Gustafsson, G. +4 more

Experimental evidence is provided for the existence of slow-mode magnetosonic solitons in the col­lisionless plasma at the magnetopause boundary layer. The solitons were detected by the fleet of Cluster spacecraft at the dusk flank of the magnetosphere as magnetic field depressions (up to 85%) accom­panied with enhancement of the plasma density an…

2003 Physical Review Letters
Cluster 88
Density-Transition Scale at Quasiperpendicular Collisionless Shocks
DOI: 10.1103/PhysRevLett.91.265004 Bibcode: 2003PhRvL..91z5004B

Bale, S. D.; Horbury, T. S.; Mozer, F. S.

Measurements of a spacecraft floating potential, on the four Cluster spacecraft, are used as a proxy for electron plasma density to study, for the first time, the macroscopic density transition scale at 98crossings of the quasiperpendicular terrestrial bow shock. A timing analysis gives shock speeds and normals; the shock speed is used to convert …

2003 Physical Review Letters
Cluster 78
Determination of Hyperfine-Induced Transition Rates from Observations of a Planetary Nebula
DOI: 10.1103/PhysRevLett.89.281101 Bibcode: 2002PhRvL..89B1101B

Judge, Philip G.; Proffitt, Charles R.; Brage, Tomas

Observations of the planetary nebula NGC3918 made with the STIS instrument on the Hubble Space Telescope reveal the first unambiguous detection of a hyperfine-induced transition 2s2p

3
Po0→2s2
1
S0 in the berylliumlike emission line spectrum of N IV at 1487.89Å. …

2002 Physical Review Letters
eHST 53
Comment on ``Indication, from Pioneer 10/11, Galileo, and Ulysses Data, of an Apparent Anomalous, Weak, Long-Range Acceleration''
DOI: 10.1103/PhysRevLett.83.1892 Bibcode: 1999PhRvL..83.1892K

Katz, J. I.

A Comment on the Letter by John D. Anderson et al., Phys. Rev. Lett. 81, 2858 (1998). The authors of the Letter offer a Reply.

1999 Physical Review Letters
Ulysses 47
Indication, from Pioneer 10/11, Galileo, and Ulysses Data, of an Apparent Anomalous, Weak, Long-Range Acceleration
DOI: 10.1103/PhysRevLett.81.2858 Bibcode: 1998PhRvL..81.2858A

Anderson, John D.; Nieto, Michael Martin; Turyshev, Slava G. +3 more

Radio metric data from the Pioneer 10/11, Galileo, and Ulysses spacecraft indicate an apparent anomalous, constant, acceleration acting on the spacecraft with a magnitude ~8.5×10-8 cm/s2, directed towards the Sun. Two independent codes and physical strategies have been used to analyze the data. A number of potential causes ha…

1998 Physical Review Letters
Ulysses 465
Reexamination of evidence for a radiatively decaying neutrino
DOI: 10.1103/PhysRevLett.58.1581 Bibcode: 1987PhRvL..58.1581M

Murthy, J.; Henry, R. C.

Nonstandard electroweak models permitting relatively rapid neutrino decay, with emission of ultraviolet photons, stimulate new interest in astronomical methods of detection of the emitted photons. We do not support the detection of a step in the cosmic background spectrum that has been reported recently. New and more sensitive measurements are urg…

1987 Physical Review Letters
IUE 6