Ion-sound model of microwave spikes with fast shocks in the reconnection region

A new model for solar spike bursts is considered based on the interaction o f Langmuir waves with ion-sound waves: l + s --> t. Such a mechanism can op erate in shock fronts, propagating from a magnetic reconnection region. New observations of microwave millisecond spikes are discussed. They have been observed in two events: 4 November 1997 between 05:52-06:10 UT and 28 Nove mber 1997 between 05:00-05:10 UT using the multichannel spectrograph in the range 2.6-3.8 GHz of Beijing AO. Yohkoh/SXT images in the AR and SOHO EIT images testify to a reconstruction of bright loops after the escape of a CM E. A fast shock front might be manifested as a very bright line in T-e SXT maps (up to 20 MK) above dense structures in emission measure (EM) maps. Mo reover one can see at the moment of spike emission (for the 28 November 199 7 event) an additional maximum at the loop top on the HXR map in the AR as principal evidence of fast shock propagation. The model gives the ordinary mode of spike emission. Sometimes we observed a different polarization of m icrowave spikes that might be connected with the depolarization of the emis sion in the transverse magnetic field and rather in the vanishing magnetic field in the middle of the QT region. Duration and frequency band of isolat ed spikes are connected with parameters of fast particle beams and shock fr ont. Millisecond microwave spikes are probably a unique manifestation of fl are fast shocks in the radio emission.