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 (6 hours) calibration observation of Uranus affected for 90 min by |
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 1 hour of science. |
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 (140 min) eclipses. |
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 | 82 min lost due to problems on instrument start-up. |
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 for all instruments. |
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 | 90 min of science lost as orbit geometry causes VILSPA antenna to point |
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). |