Opprettet av
Nicolas Martin
{$ ',' | translate $}
Zoe Young
Gjennomgått av
Mason Taylor
{$ ',' | translate $}
Jeff Morrison
Sist oppdatert 01/11/2025
EMU gratis to coulomb (C)
Konverteringstabell
| EMU gratis | Coulomb (C) |
|---|---|
| 0.001 | {$ $parent.$ctrl.customFormatted(0.01) $} C |
| 0.01 | {$ $parent.$ctrl.customFormatted(0.1) $} C |
| 0.1 | {$ $parent.$ctrl.customFormatted(1.0) $} C |
| 1 | {$ $parent.$ctrl.customFormatted(10.0) $} C |
| 2 | {$ $parent.$ctrl.customFormatted(20.0) $} C |
| 3 | {$ $parent.$ctrl.customFormatted(30.0) $} C |
| 4 | {$ $parent.$ctrl.customFormatted(40.0) $} C |
| 5 | {$ $parent.$ctrl.customFormatted(50.0) $} C |
| 6 | {$ $parent.$ctrl.customFormatted(60.0) $} C |
| 7 | {$ $parent.$ctrl.customFormatted(70.0) $} C |
| 8 | {$ $parent.$ctrl.customFormatted(80.0) $} C |
| 9 | {$ $parent.$ctrl.customFormatted(90.0) $} C |
| 10 | {$ $parent.$ctrl.customFormatted(100.0) $} C |
| 20 | {$ $parent.$ctrl.customFormatted(200.0) $} C |
| 30 | {$ $parent.$ctrl.customFormatted(300.0) $} C |
| 40 | {$ $parent.$ctrl.customFormatted(400.0) $} C |
| 50 | {$ $parent.$ctrl.customFormatted(500.0) $} C |
| 60 | {$ $parent.$ctrl.customFormatted(600.0) $} C |
| 70 | {$ $parent.$ctrl.customFormatted(700.0) $} C |
| 80 | {$ $parent.$ctrl.customFormatted(800.0) $} C |
| 90 | {$ $parent.$ctrl.customFormatted(900.0) $} C |
| 100 | {$ $parent.$ctrl.customFormatted(1000.0) $} C |
| 1000 | {$ $parent.$ctrl.customFormatted(10000.0) $} C |
Populære konverteringer
Populære konverteringer
| Units | Symbols |
|---|---|
| Coulomb Megacoulomb | C MC |
| Coulomb Kilocoulomb | C kC |
| Coulomb Millicoulomb | C mC |
| Coulomb Mikrocoulomb | C µC |
| Coulomb Nanocoulomb | C nC |
| Coulomb Picoculomb | C pC |
| Coulomb Abcoulomb | C abC |
| Coulomb EMU gratis | — |
| Coulomb Statcoulomb | C stC |
| Coulomb ESU gratis | — |
| Coulomb Franklin | C Fr |
| Coulomb Ampere-time | C A*h |
| Coulomb Ampere-minutt | C A*min |
| Coulomb Ampere-sekund | C A*s |
| Coulomb Faraday (basert på karbon 12) | — |
| Coulomb Elementær ladning | C e |