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The 3-dimensional radio mapping experiment /SBH/ on ISEE-CThe 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).
Document ID
19780065152
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Knoll, R.
(Observatoire de Paris-Meudon France)
Epstein, G.
(Observatoire de Paris-Meudon France)
Hoang, S.
(Observatoire de Paris-Meudon France)
Huntzinger, G.
(Observatoire de Paris-Meudon France)
Steinberg, J. L.
(Meudon, Observatoire, Meudon Hauts-de-Seine, France)
Fainberg, J.
(Observatoire de Paris-Meudon France)
Grena, F.
(Observatoire de Paris-Meudon France)
Stone, R. G.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Mosier, S. R.
(NSF Washington, D.C., United States)
Date Acquired
August 9, 2013
Publication Date
July 1, 1978
Publication Information
Publication: IEEE Transactions on Geoscience Electronics
Volume: GE-16
Subject Category
Spacecraft Instrumentation
Accession Number
78A49061
Distribution Limits
Public
Copyright
Other

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