A modeling strategy that is adapted to the study of synchrotron-self-absorbed plasmoids that was developed for the quasar Mrk 231 by Reynolds et al. is applied to the microquasar GRS 1915+105. The major flare from 1993 December shows spectral evidence of three such self-absorbed components. The analysis yields an estimate of the power that is required to eject the plasmoids from the central engine that is independent of other estimates that exist in the literature for different flares. The technique has an advantage since the absorbed spectrum contains an independent constraint provided by the optical depth at each epoch of observation. The modeling procedure presented here self-consistently determines the dimensions of the radio-emitting plasma from the spectral shape. Thus, structural dimensions are determined analytically that can be much smaller than interferometer beamwidths. A synthesis of the time evolution of the components allows one to address the fundamental uncertainties in previous estimates. First, the plasma is not protonic, but comprises an electron-positron gas. The minimum electron energy is determined to be less than six times the electron rest-mass energy. The analysis also indicates that the plasmoids are ejected from the central engine magnetically dominated. The temporal behavior is one of magnetic energy conversion to mechanical energy as the plasmoids approach equipartition. The time-dependent models bound the impulsive energy flux, Q, required to eject the individual major flare plasmoids from the central engine to, 4.1 × 1037 erg s–1 Q 6.1 × 1038 erg s–1.
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