This is a summary list of special events and conflicts between instruments that occurred during the Operational Phase of the mission (some of which have already been mentioned):
| Revolution | Event |
| 79 | First revolution after PV Phase. |
| 94 | PHT-FCS1/TRS2 change in illumination behaviour/brightness increase. |
| 116 | AOCS calibration led to shorter science window. Some loss of |
| science due to system crash. | |
| 137 | ISO pointing performance tests using ISOCAM. |
| 152 | Soft geomagnetic disturbance with no impact on science. |
| 161 | Tests of the SWS virtual fourth aperture. |
| 173 | Tests of LWS parallel mode. |
| 196 | As soon as AOS was achieved at the start of the revolution, it was seen |
| that ISO had gone to survival mode and that both the Earth warning | |
| and forbidden regions had been traversed by ISO - | |
| ISO had viewed the Earth for about 2 minutes. All temperatures were | |
| out of range (high) and all scientific operations for the revolution | |
| were therefore suspended. | |
| 197 | Recovery procedures implemented. |
| 198 | Normal operations resumed within 36 hours. No damage was done to the |
| satellite. | |
| 204 | LWS switch-off rolled back 60 minutes. |
| 217 | Some LWS tests made during the revolution to verify a command changing |
| the LWS biases. | |
| 220 | Many small problems affecting a large number of observations. First there |
| were problems with the PPM (Earth constraint was approached closely), | |
| then a guide star was not found, and PHT-P2 suffered from latch-up problems | |
| 242 | Over four hours of observations lost due to problems with the Goldstone |
| antenna. | |
| 256 | Goldstone problems led to loss of over one hour observations. |
| 263 | Goldstone problems led to loss of over one hour observations. |
| 264 | ISOCAM and SWS measurements made for ISO pointing tests. Special |
| ISOCAM mode had to be used for the one hour test. | |
| 267-268 | Goldstone problems led to loss of over ten hours observations. |
| 274 | Spacecraft problems (automatic on-board reset) led to the loss of half the |
| revolution. | |
| 290 | Improved SSO tracking algorithm implemented. |
| 294 | The opening of the science window was delayed by 2h 30m due to a |
| planned delta-V maneouver (to keep the phase of the orbit correct) and | |
| second DLCM, both at the start of the revolution. | |
| 301 | Nearly six hours of science lost due to spacecraft problems. |
| 317 | Long ( |
| short Goldstone dropout. | |
| 327 | Improved Sun ephemerides. |
| 330 | Goldstone problems led to 5 observations (80 min) lost. |
| 343 | Loss of communications with ISO for 45 min from Goldstone due to |
| high winds. | |
| 356 | Tests of LWS wheel subsystem plus minor Goldstone problems. |
| 364 | ISO went into survival mode at the start of the revolution, leading to |
| a loss of two hours science. | |
| 365 | Some Goldstone problems leading to loss of 85 min science time. |
| 368 | STR calibration updated. |
| 372 | Goldstone power failure led to the loss of 5 hours observing. Satellite |
| went into perigee with ISOCAM in wrong mode. |
| Revolution | Event |
| 373 | No anomaly observed with ISOCAM, but one hour observing lost due to |
| one minute of loss of contact with the satellite. | |
| 378 | LWS activities halted until further notice due to FP interchange wheel |
| problem (positioning difficulties). Next two revolutions could not be | |
| replanned. This time was devoted to LWS observations, that were lost. | |
| 384 | Straylight rejection measurements for SWS. |
| 398 | Many telemetry problems due to a thunderstorm around Madrid and |
| Goldstone problems led to the loss of over 100 min science time. | |
| 410-412 | Tests of ground system for the 366 day year problem (1996 was a leap |
| year). On revolution 411 this caused the loss of one hour of science. | |
| 413 | Telemetry problems in Madrid and Goldstone caused the loss of two hours |
| of science. | |
| 417 | Various problems caused the loss of just over one hour of science. |
| 432-435 | Manual LWS checks and tests were made to try and solve the wheel problem. |
| 442 | LWS operations re-start with one test observation completed successfully. |
| 447 | Real re-start of LWS operations with 30 observations completed nominally. |
| 452 | Sun ephemerides recalculated four times per revolution, instead of once |
| per revolution to improve ISO pointing accuracy. | |
| 470 | Lots of minor Goldstone problems lead to the loss of |
| 484 | Lots of problems at handover leading to 67 min science lost. |
| 522 | Loss of over six hours science due to LWS problems (microprocessor and reset). |
| 528 | Non-nominal behaviour of SWS led to the loss of 78 min science. |
| 566 | Loss of 75 min of science due to a CTV problem. |
| 571 | CAM-CVF observations in the Mission Data Base temporarily `blocked' |
| from the automatic scheduling routines to prevent the strong increase in | |
| band 3 dark currents observed in SWS observations performed | |
| in the following 30 min. | |
| 575 | Loss of 100 min science time (SWS observation) due to non-availability |
| of Goldstone. | |
| 578 | Fire alarm drill on station, Instrument Controller left post as per procedure. |
| No events happened during this time. | |
| 602 | Almost four hours of science lost due to spacecraft attitude problems - |
| one observation was up to 1.5 degrees off. | |
| 603 | Many problems with PHT-P2 latch-ups affecting 85 min science. |
| Science observations using PHT-P2 detector suspended. | |
| 613 | Start of PHT-P2 latch-up tests. Also, many telemetry drops but little impact |
| on the science time. | |
| 614 | Lots of telemetry drops due to a thunderstorm around VILSPA. |
| 620 | Two hours of observations lost due to Goldstone problems. |
| 623 | Two hours of observations lost due to Goldstone problems. |
| 637-641 | 400 min of PHT science time affected or lost due to PHT-P2 latch-up |
| problem. | |
| 646 | Loss of 81 min science time due to Goldstone problems. |
| 659 | End of PHT-P2 latch-up tests. |
| 661-662 | PHT straylight tests during eclipse. |
| 664 | Start of long ( |
| 668 | Loss of 90 min of observations due to Goldstone problems. |
| 672-673 | Special PHT straylight measurements during eclipses. |
| 676 | Automatic scheduling of CAM-CVF observations resumed. Mission |
| Planning software was updated so that SWS observations were not | |
| scheduled any more until after 30 min of a CAM-CVF measurement. | |
| 678 | Last revolution for which the eclipses lasted longer than 140 min. |
| Revolution | Event |
| 684 | Resumption of PHT-P2 observations. |
| 688 | 200 min observation lost due to Goldstone problems. |
| 719 | LWS wheel tests. |
| 721 | |
| 722 | Solar flare caused loss of most of the science time due to enhanced |
| glitch rate. | |
| 732 | 284 min science lost due to Goldstone problems. |
| 756 | Problems with guide stars caused 60 min of science to be lost. |
| 757 | Third DLCM and an orbit correction maneouvre carried out at the start of |
| the revolution. | |
| Problems with Goldstone led to the loss of 185 min science. | |
| 764 | OTF set to 2 |
| 777 | 100 min of science lost due to a combination of errors, plus on the 1997-1998 |
| year change the wrong year entered in the system. | |
| 843-844 | |
| directly at the Sun (ISO in the VILSPA-Sun line). | |
| 851 | Problems with a guide star (blemish on CCD) causes 4h 45m of science |
| to be lost. | |
| 875 | Liquid helium depletion at 21:07 zulu on 8 April 1998. |
| 876-880 | Some SWS observations carried out as bands 1 and 2 are still useable. |
| 881-887 | Start of SWS post-He observations. SWS used all these revolutions. |
| 888-907 | SWS observations interleaved with the Technology Test Phase (TTP). |