Two-component proton spectra in the inner Saturnian magnetosphere
Journal Article
·
· Geophys. Res. Lett.; (United States)
The Low Energy Charged Particle (LECP) experiment onboard the Voyager-2 spacecraft performed extensive measurements of energetic (approx.28 keV< or approx. =E/sub p/< or approx. =150 MeV; approx.22 keV< or approx. =E/sub e/< or approx. =20 MeV) protons and electrons during spacecraft passage through the inner magnetosphere of Saturn in August 1981. Analysis of the measurements inside the orbits of Enceladus and Mimas reveals the presence of a two-component proton spectrum consisting of a low-energy population at < or approx. =500 keV identified for the first time and described by dj/dE = KE/sup 2.5/, and a high-energy part at E> or approx. =16 MeV whose spectral form is similar to that expected from cosmic ray neutron albedo decay (CRAND), as previously inferred by the Pioneer-11 investigators from integral measurements. In addition, there exist large fluxes of high (> or approx. =1.5 MeV) and low (22 to 35 keV) energy electrons (approx.3.5 x 10/sup 5/ and approx.1.1 x 10/sup 5/ cm/sup -2/sec/sup -1/sr/sup -1/, respectively) throughout this region. The pitch angle distribution of low energy protons changes from a simple sin/sup 2/3/ ..cap alpha.. dependence to one where intensities near 90/sup 0/ become depleted as the spacecraft approached the planet's ring plane at approx.2.88 R/sub S/. It is likely that the pitch angle depletion is due to proton interactions with the tenuous G-ring. These observations also resolve a number of uncertainties regarding the presence of energetic protons and electrons inside the orbits of Enceladus and Mimas, arising from the analysis of Pioneer-11 measurements.
- Research Organization:
- Applied Physics Laboratory, The Johns Hopkins University, Laurel, Maryland 20707
- OSTI ID:
- 6574194
- Journal Information:
- Geophys. Res. Lett.; (United States), Journal Name: Geophys. Res. Lett.; (United States) Vol. 9:10; ISSN GPRLA
- Country of Publication:
- United States
- Language:
- English
Similar Records
General characteristics of hot plasma and energetic particles in the Saturnian magnetosphere: Results from the Voyager spacecraft
Electrons and cosmic ray produced protons in Saturn's inner magnetosphere
Injection of cosmic ray secondaries into the inner Saturnian magnetosphere 1. Protons from the CRAND process
Journal Article
·
Mon Oct 31 23:00:00 EST 1983
· J. Geophys. Res.; (United States)
·
OSTI ID:5123741
Electrons and cosmic ray produced protons in Saturn's inner magnetosphere
Technical Report
·
Mon Dec 31 23:00:00 EST 1984
·
OSTI ID:5939474
Injection of cosmic ray secondaries into the inner Saturnian magnetosphere 1. Protons from the CRAND process
Journal Article
·
Mon Jan 31 23:00:00 EST 1983
· J. Geophys. Res.; (United States)
·
OSTI ID:6213334
Related Subjects
640107* -- Astrophysics & Cosmology-- Planetary Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ATMOSPHERES
ELECTRONS
ELEMENTARY PARTICLES
ENERGY SPECTRA
FERMIONS
FLUX DENSITY
INCLINATION
LEPTONS
PLANETARY ATMOSPHERES
PLANETARY MAGNETOSPHERES
PLANETS
PROTON SPECTRA
SATURN PLANET
SPACE VEHICLES
SPECTRA
VEHICLES
VOYAGER SPACE PROBES
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ATMOSPHERES
ELECTRONS
ELEMENTARY PARTICLES
ENERGY SPECTRA
FERMIONS
FLUX DENSITY
INCLINATION
LEPTONS
PLANETARY ATMOSPHERES
PLANETARY MAGNETOSPHERES
PLANETS
PROTON SPECTRA
SATURN PLANET
SPACE VEHICLES
SPECTRA
VEHICLES
VOYAGER SPACE PROBES