Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Proton flow measurements in the magnetotail plasma sheet made with Imp 6

Journal Article · · J. Geophys. Res., v. 81, no. 1, pp. 227-234
Patterns of proton flow in the magnetotail plasma sheet are described. They are derived from observed anisotropies of the flux of protons measured with the Los Alamos Scientific Laboratory (LASL) plasma probe on Imp 6. These observations, made in the geocentric distance range rapprox. =25--32 R/subE/, are entirely consistent with those made at rapprox. =18 R/subE/ with Vela satellites and reported earlier. In particular, the substorm thinning and thickening of the plasma sheet are seen and are accompanied by antisunward, then sunward, flow of plasma as they are at the Vela orbit. During one substorm the Goddard Space Flight Center magnetometer on the satellite clearly showed the Z component of the magnetic field in the plasma sheet to be southward throughout the expansion phase, while antisunward flow prevailed, and then to become suddenly northward again as the flow turned sunward at the substorm's recovery. This observation of the magnetic field behavior provides important confirmation of the view, regarding neutral line formation and movement during substorms, that has been established earlier on the basis of plasma flow measurements made by the Vela satellites. A dawn-to-dusk cross-tail proton flow comprising a proton current of approx.10$sup 7$ protons/cm$sup 2$ -s(approx.1.6x10$sup -12$ A/cm$sup 2$) was observed as the magnetometer indicated that the satellite was crossing the magnetic 'neutral sheet.' This observation further supports an earlier suggestion that dawn-to-dusk cross-tail proton flows, measured occasionally with the Vela satellites, constituted the magnetotail neutral sheet current. (AIP)
Research Organization:
Los Alamos Scientific Laboratory, University of California, Los Alamos, New Mexico 87544
Sponsoring Organization:
USDOE
NSA Number:
NSA-33-027188
OSTI ID:
4006210
Journal Information:
J. Geophys. Res., v. 81, no. 1, pp. 227-234, Journal Name: J. Geophys. Res., v. 81, no. 1, pp. 227-234; ISSN JGREA
Country of Publication:
United States
Language:
English

Similar Records

Magnetotail plasma flow measured by Vela 4A
Journal Article · Sat Sep 01 00:00:00 EDT 1973 · J. Geophys. Res., v. 78, no. 25, pp. 5463-5476 · OSTI ID:4322497

Timing of energetic proton enhancements relative to magnetospheric substorm activity and its implication for substorm theories
Journal Article · Sat Feb 28 23:00:00 EST 1981 · J. Geophys. Res.; (United States) · OSTI ID:6315741

Correlated observations of two auroral substorms from an aircraft and from a Vela satellite
Journal Article · Tue Jun 01 00:00:00 EDT 1976 · J. Geophys. Res.; (United States) · OSTI ID:7356374