The relationship between the IMF B(y) and the distant tail (150-238 Re) lobe and plasmasheet B(y) fields

Details The relationship between the IMF B(y) and the distant tail (150-238 Re) lobe and plasmasheet B(y) fields The relationship between the IMF B(y) and the distant tail (150-238 Re) lobe and plasmasheet B(y) fields

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984georl..11.1082t&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 11, Oct. 1984, p. 1082-1085. NASA-supported research.

Computer Science

Sound

47

Geomagnetic Tail, Interplanetary Magnetic Fields, Plasma Layers, Space Plasmas, Atmospheric Models, Earth Magnetosphere, International Sun Earth Explorer 3, Plasma Pressure, Satellite Sounding

Scientific paper

The relationships between the Solar Magnetospheric (SM) y-component of the interplanetary magnetic field (IMF) and the lobe and plasmasheet magnetic fields have been studied for the two ISEE-3 deep tail passes. It is found that for positive sector IMFs, 13 percent of the interplanetary magnetic field penetrates into the aberrated north-dawn and south-dusk lobe quadrants, and about the same amount in the north-dusk and south-dawn lobe quadrants for negative sector IMFs. For the above cases, field penetration is significantly less for opposite polarity IMFs. The former results are generally consistent with open magnetospheric models, but the latter (the lack of response in certain quadrants) are unexplained by theory at this time. If the magnitude of the plasmasheet B(y) fields are related to plasma pressure anisotropies, very small anisotropies of about 1.01 are expected.

Affiliated with

Also associated with

No associations

Rating

The relationship between the IMF B(y) and the distant tail (150-238 Re) lobe and plasmasheet B(y) fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The relationship between the IMF B(y) and the distant tail (150-238 Re) lobe and plasmasheet B(y) fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The relationship between the IMF B(y) and the distant tail (150-238 Re) lobe and plasmasheet B(y) fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1227850