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Relativistic Reduced-Mass and Recoil Corrections to Vacuum Polarization in Muonic Hydrogen, Muonic Deuterium and Muonic Helium Ions
Relativistic Reduced-Mass Recoil Corrections Vacuum Polarization Muonic Hydrogen Muonic Deuterium Muonic Helium Ions
2011/8/3
Relativistic Reduced-Mass and Recoil Corrections to Vacuum Polarization in Muonic Hydrogen, Muonic Deuterium and Muonic Helium Ions.
Charge stripping accumulation of light heavy ions in HIRFL-CSR main ring
heavy-ion accelerator accumulation stripping injection
2009/8/17
The charge stripping injection method has been adopted for the accumulation of light heavy ions in HIRFL-CSR. This method has some special requirements for the accelerating particles, and at the same ...
Multiple Spacecraft Observations of Energetic Ions During a High Solar Wind Pressure Event
The spacecraft the solar wind pressure the polar satellites high-energy particles the solar wind speed
2017/3/23
On 28 June 1999 the Wind spacecraft (near the forward libration point) observed a large solar wind pressure spike from 0445 UT to 0600 UT. The Polar satellite at 7 hours magnetic local time detected a...
Comparison of Energetic Ions in Cusp and Outer Radiation Belt
Large diamagnetic cavities smooth high tip region charged particle energy the ionosphere the solar wind particles
2017/3/23
Recently, large diamagnetic cavities with a size of as large as 6 Re have been observed in the dayside high-altitude cusp regions. Associated with these cavities are charged particles with energies fr...
Comment on "Origins of energetic ions in the cusp" by K. J. Trattner et al
High-energy ion bow shock acceleration tips detect ion high-energy particles
2017/3/23
The paper by Trattner et al. [2001, hereinafter referred to as TETAL] reanalyzes the data of Chen et al. [1998, hereinafter referred to as CFS] and attempts to prove two statements: first, that the en...
Comment on "MeV magnetosheath ions energized at the bow shock" by S.-W. Chang et al
Storm events ion the bow shock energy as much as magnetic sheath measuring magnetic sheath the bow shock
2017/3/23
From a study of the 4 May 1998 storm event, Chang et al. [2001] (hereinafter referred to as CETAL01) suggested that "ions are accelerated at the quasi-parallel bow shock to energies as high as 1 MeVan...
The Geomagnetic Cusps as Seen in High Charge State Shocked Solar Wind Ions Observed with S/C POLAR during April 2001
High charge state high energy heavy ion the solar wind protons ion polar spacecraft
2017/3/23
We present a method of polar cusp identification using high charge state energetic heavy ions. There is reason to think that these ions constitute shocked solar wind protons and heavier ions such as H...
Energetic Oxygen Ions of Ionospheric Origin Observed in the Cusp
Polar satellites ionosphere power law ion
2017/3/23
On 8/27/96 from 8 to 10:36 UT the POLAR satellite crossed the dayside cusp and observed very energetic ionospheric O<+2 ions which had a magnetic moment spectrum, M(E) that followed a power law. Later...
Energetic Ions in the High Latitude Boundary Layer of the Magnetosphere
Quick cluster ion spectrometer flight energy detection system the incident energy ions high-energy ion the magnetosphere
2017/3/23
The RAPID/CLUSTER is an advanced ion spectrometer with a position sensitive time-of-flight (T) and energy (E) detection system which determines the mass of incident energetic ions. The energy range ex...
Features of Energetic Ions Near the Compressed Magnetosphere
During geomagnetic storm the magnetosphere the wind the equatorial belt high altitude ion
2017/3/23
A possible cusp acceleration mechanism has been investigated during a major geomagnetic storm on May 4, 1998 when the magnetosphere was compressed and eroded. At 5:00–12:05 UT, the WIND spacecraft was...
Features of the Compound Multiplicity of the Interactions of 24Mg and 28Si Ions with Emulsion Nuclei at 4.5A GeV/c
24Mg Emulsion Nuclei 28Si Ions
2010/4/15
The present paper deals with the interactions of 24Mg and 28Si nuclei at 4.5A GeV/c with emulsion. Some characteristics of the compound multiplicity given by the numerical sum of grey and shower parti...