CRIS - Normal Operation. CRIS is not designed to operate during solar energetic particle events. EPAM - Normal Operation. EPAM continues to work well. RTSW data was valid during the July 14-16 event. Almost all of the data during the recent large events are correct. The possible exceptions are a few hours surrounding the shock passage on July 15. At that time our count rates rose to about 200,000 counts per second and there may have been some saturation effects in the data. We have been actively studying the design to try to understand how it responded during these very highest fluxes. We are confident that the higher energy channels and the composition channels are correct. However, the lowest 3 or 4 energy channels for ions and electrons are still being looked at. MAG - Normal Operation - MAG is working just fine. RTSW data was valid during the July 14-16 event. SEPICA - SEPICA is presently generating science data on half of Fan 3. Diagnostic tests are in progress to determine the cause of anomalies with several data channels required to produce good science from the other half of Fan 3. The science data within SEPICA will be redirected to a spare portion of instrument memory to test the possibility that the existing memory has been damaged. A procedure to perform this step is in final test, and may be upoaded to the instrument this week. Fan pressures have been stable for approximately eight months. Fan 2 is still just below the threshold for operation, and Fan 3 is at a completely nominal pressure. SIS - Normal Operation. Because of the large geometry factor of the instrument, SIS count rates were saturated for several days during the July 14 event, rendering the RTSW data invalid for the period. Detector thresholds were raised in order to reduce the count rates. However, raising these thresholds causes NOAA RTSW data processing software to calculate incorrect fluxes. The thresholds were lowered when particle intensities dropped sufficiently. The SIS team is considering various options for improving the instrument response to events like this in the future. SIS continued to return pulse-height data during the event, and analysis of these data is underway. SWEPAM - Normal Operation. No changes to instrument operation in recent months. July 14 event: Such a large flare produces copious energetic particles at sufficiently high energies that they penetrate the spacecraft and instrument and make spurious counts in the CEM detectors. The effect of the high background counts was to cause a breakdown in the SWEPAM algorithm which chooses the energy range to measure. Because of the high counts, the instrument always measured the lowest possible energy range (~250 eV to 1.8 keV). During the July 14 event, the solar wind speed was sufficiently high that this energy range did not include the main solar wind proton beam (peak seen at energies ranging from 2 to >5 keV). The instrument was happy and healthy, it just was looking in the wrong place. The SWEPAM RTSW data was not valid for ~36 hours during the July 14 event because of this effect. However, SWEPAM also has a mode which measures the full energy range (250 eV to ~17 keV) once each half hour. These data do show the solar wind peak, and we should eventually be able to solar solar wind moments from them. SWICS/SWIMS - Normal Operation. SWICS and SWIMS are just fine, with no anomalies whatsoever. In May of this year the level of the SWICS Post Acceleration Power Supply was increased to about 26.1 kV (from its previous 22.8 kV) and it has operated there without incident since then. The higher voltage level increases the energy range of SWICS measurements. Except for extremely high count rates, there were also no anomalies during the solar storm period of July 14-16, 2000. ULEIS - Since April 3, 2000 one of the two redundant TOF systems in ULEIS (TOF-1) has not returned reliable data. Therefore the ULEIS team has turned off the high voltage on the TOF-1 system to minimize the risk of high voltage discharge. The command was executed on June 19, 2000. The ULEIS team has found that the mass resolution from the remaining TOF-2 system is quite good, and isotopes such as 3He and 22Ne are still resolved.