Other
Scientific paper
Jul 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978itge...16..199k&link_type=abstract
IEEE Transactions on Geoscience Electronics, vol. GE-16, July 1978, p. 199-204.
Other
26
International Sun Earth Explorer 3, Interplanetary Magnetic Fields, Radio Observation, Solar Wind, Spaceborne Experiments, Type 3 Bursts, Data Processing, Earth Magnetosphere, Lines Of Force, Magnetic Field Configurations, Magnetic Measurement, Preamplifiers, Radio Observation, Satellite-Borne Instruments, Solar Corona
Scientific paper
The SBH experiment on ISEE-C will provide maps of the large scale structure of the interplanetary magnetic field from ten solar radii altitude to the earth orbit, in and out of the ecliptic. The SBH instrument will track type III solar radio bursts at 24 frequencies in the range 30 kHz-2 MHz thus providing the positions of 24 points along the line of force which guides the electrons producing the radio radiation. The antennas are two dipoles: one (90 m long) in the spin plane, the other (15 m long) along the spin axis. The receiver was designed for high sensitivity (0.3 microV in 3 kHz BW), high intermodulation rejection (80 dB/1 microV input for order 2 products), large dynamic range (70 dB), high selectivity (-30-dB response 6.5 kHz away from the center frequency of 10.7 MHz for the 3 kHz BW channels), and high reliability (expected orbital life: 3 years).
Epstein Gabriel
Fainberg Joe
Grena F.
Hoang Sang
Huntzinger Gerard
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