Response of the equatorial and polar magnetosphere to the very tenuous solar wind on May 11, 1999

Geophysical Research Letters

Volumn 27, Issue 23, 2000, Pages 3773-3776

  Farrugia, C J ^a   Singer, H J ^b   Evans, D ^b   Berdichevsky, D ^c,d   Scudder, J D ^e   Ogilvie, K W ^d   Fitzenreiter, R J ^d   Russell, C T ^f  

^a UNIVERSITY OF NEW HAMPSHIRE   (United States)

^b NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d RAYTHEON COMPANY   (United States)

^e UNIVERSITY OF IOWA   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ATMOSPHERIC DENSITY; EARTH (PLANET); MAGNETIC MOMENTS; MAGNETOSPHERE; ORBITS; RAIN; STORMS;

ELECTRON PRECIPITATION; EQUATORIAL; GEOSTATIONARY ORBIT; POLAR MAGNETOSPHERE; SOLAR WIND;

GEOPHYSICS; SOLAR WIND;

SOLAR WIND;

ELECTRON PRECIPITATION; GEO-STATIONARY ORBITS; NORTH-SOUTH ASYMMETRY; NORTHERN HEMISPHERES; SIMULTANEOUS PRECIPITATION; SOLAR WIND DENSITY; SOLAR WIND PARAMETERS; SUBSTORM ACTIVITY;

EID: 0034483794     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL003800     Document Type: Article

References (10)

1. Polar cap x-rays and electrons under low-density solar wind conditions: Coordinated PIXIE and DMSP observations On May 11
2. Magnetosphere on May 11, 1999, the day the solar wind almost disappeared: I. Current systems
3. Magnetosphere on May 11, 1999, the day the solar wind almost disappeared: II. Magnetic pulsations in space and on the ground
4. Polar rain: Solar coronal electrons in the earth's magnetosphere
5. Low energy polar cap electrons during quiet times
6. Bidirectional solar wind electron heat flux and hemispherically symmetric polar rain
7. The variation of reconnection rate at the dayside magnetopause and cusp ion precipitation
8. Long-period polar rain variations, solar wind and hemispherically symmetric polar rain
9. Solar-cycle variation of low density solar wind during more than 3 solar cycles
10. Statistical properties of particle precipitation in the polar cap during intervals of northward interplanetary magnetic field