Italian GP 1988
Monza
Nopeimmat kierrokset
| Sija | Nro | Kuljettaja | Kans. | Auto | Kierr. | Aika | Ero
|
|---|
| 1. | 27 | Michele Alboreto | ITA | Ferrari | 44 | 1.29,070 |
|
| 2. | 28 | Gerhard Berger | AUT | Ferrari | 47 | 1.29,113 | +0,043
|
| 3. | 12 | Ayrton Senna | BRA | McLaren-Honda | 29 | 1.29,569 | +0,499
|
| 4. | 11 | Alain Prost | FRA | McLaren-Honda | 27 | 1.29,642 | +0,572
|
| 5. | 19 | Alessandro Nannini | ITA | Benetton-Ford | 33 | 1.30,248 | +1,178
|
| 6. | 18 | Eddie Cheever | USA | Arrows-Megatron | 42 | 1.30,452 | +1,382
|
| 7. | 17 | Derek Warwick | GBR | Arrows-Megatron | 43 | 1.30,504 | +1,434
|
| 8. | 16 | Ivan Capelli | ITA | March-Judd | 37 | 1.30,971 | +1,901
|
| 9. | 20 | Thierry Boutsen | BEL | Benetton-Ford | 34 | 1.31,543 | +2,473
|
| 10. | 6 | Riccardo Patrese | ITA | Williams-Judd | 26 | 1.31,704 | +2,634
|
| 11. | 1 | Nelson Piquet | BRA | Lotus-Honda | 11 | 1.31,803 | +2,733
|
| 12. | 15 | Maurício Gugelmin | BRA | March-Judd | 27 | 1.31,832 | +2,762
|
| 13. | 10 | Bernd Schneider | GER | Zakspeed | 24 | 1.32,054 | +2,984
|
| 14. | 36 | Alex Caffi | ITA | Dallara-Ford | 19 | 1.32,735 | +3,665
|
| 15. | 2 | Satoru Nakajima | JPN | Lotus-Honda | 11 | 1.32,804 | +3,734
|
| 16. | 22 | Andrea de Cesaris | ITA | Rial-Ford | 20 | 1.33,007 | +3,937
|
| 17. | 5 | Jean-Louis Schlesser | FRA | Williams-Judd | 39 | 1.33,179 | +4,109
|
| 18. | 4 | Julian Bailey | GBR | Tyrrell-Ford | 40 | 1.33,203 | +4,133
|
| 19. | 9 | Piercarlo Ghinzani | ITA | Zakspeed | 10 | 1.33,476 | +4,406
|
| 20. | 25 | René Arnoux | FRA | Ligier-Judd | 42 | 1.33,486 | +4,416
|
| 21. | 30 | Philippe Alliot | FRA | Lola-Ford | 28 | 1.33,581 | +4,511
|
| 22. | 14 | Philippe Streiff | FRA | AGS-Ford | 31 | 1.33,898 | +4,828
|
| 23. | 23 | Pierluigi Martini | ITA | Minardi-Ford | 8 | 1.34,420 | +5,350
|
| 24. | 29 | Yannick Dalmas | FRA | Lola-Ford | 15 | 1.34,723 | +5,653
|
| 25. | 24 | Luis Pérez-Sala | ESP | Minardi-Ford | 11 | 1.35,020 | +5,950
|
| 26. | 21 | Nicola Larini | ITA | Osella | 2 | 1.38,570 | +9,500
|
