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1. Solar Flare Data from the Berkeley-Illinois-Maryland Array [BIMA]
The BIMA array is a 3-element radio interferometer. Flare observations at 86 GHz with high spatial resolution were obtained during the Flares 22/MAX'91 campaign of December 1991/Jnauary 1992. Times ...

2. The SWICS/MASS/STICS (SMS) Instrument Package on WIND [WIND_SMS]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...

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