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S. M. White, M. R. Kundu (University of Maryland)
The 10-element BIMA array will be used in to image solar flares at millimeter wavelengths during campaign periods in the upcoming solar maximum. Since millimeter emission in the impulsive phase of flares comes from electrons with energies typically in excess of 1 MeV, these observations complement observations of lower energy electrons at other wavelengths. Recent BIMA flare data will be presented and plans for the near future will be discussed.
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