Observations of an enhanced convection flow channel for northward turning IMF

Geophysical Research Letters

Volumn 24, Issue 24, 1997, Pages 3137-3140

  Nilsson, H ^a   Yamauchi, M ^a   Mukai, T ^b   Yamamoto, T ^b   Moretto, T ^c  

^a SWEDISH INSTITUTE OF SPACE PHYSICS   (Sweden)

^b JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^c DANISH METEOROLOGICAL INSTITUTE   (Denmark)

Author keywords

[No Author keywords available]

Indexed keywords

GEOMAGNETISM; EARTH (PLANET); IONOSPHERE; MAGNETIC FIELD EFFECTS; MAGNETIC FIELDS; MAGNETOSPHERE; SOLAR SYSTEM;

ENHANCED CONVECTION; FLOW CHANNELS;

CHANNEL FLOW; SPACE RESEARCH;

CONVECTION FLOW CHANNEL;

CONVECTION; FLOW CHANNEL; INTERPLANETARY MAGNETIC FIELD; IONOSPHERE;

EID: 0031390863     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/97GL03254     Document Type: Article

References (4)

1. Cowley, S. W. H., The causes of convection in the Earth's magnetosphere: A review of development during the IMS, Rev. Geophys. Space Phys., 20, 531-565, 1982.
2. Dungey, J. W., Interplanetary magnetic field and the auroral zones, Phys. Rev. Lett., 6, 47-48, 1961.
3. y variations into the polar ionospheres through interplanetary field-aligned currents, J. Geophys. Res., 99, 17309-17322, 1994.
4. Todd, H., S. W. H. Cowley, M. Lockwood, D. M. Willis, and H. Lühr, Response time of the high-latitude dayside ionosphere to sudden changes in the north-south component of the IMF, Planet. Space Sci., 36, 1415-1428, 1988.