Fix spelling (American English, not British English)

nasa-gcn · Feb 18, 2025 · f3f23c1 · f3f23c1
1 parent eae948a
commit f3f23c1
Showing 1 changed file with 6 additions and 6 deletions.
diff --git a/app/routes/missions.svom/route.mdx b/app/routes/missions.svom/route.mdx
@@ -26,7 +26,7 @@ import logo from './logo_svom_black.svg'
 
 The [Space-based multi-band astronomical Variable Objects Monitor (SVOM)](https://www.svom.eu/en/the-svom-mission/) is a French-Chinese mission, result of a collaboration between the two national space agencies, [China National Space Administration (CNSA)](https://www.cnsa.gov.cn/english/index.html) and [Centre national d'études spatiales (CNES)](https://cnes.fr/en/projects/svom). SVOM is dedicated to the study of the most powerful transient phenomena, with a particular emphasis on gamma-ray bursts (GRBs).
 
-The SVOM spacecraft carries four multi-wavelength instruments: ECLAIRs, Gamma Ray burst Monitor (GRM), Microchannel X-ray Telescope (MXT) and Visual Telescope (VT). ECLAIRs and GRM can detect gamma-ray transient sources in real-time with localisation capabilities for ECLAIRs. SVOM can transfer the alerts in near real-time with a typical latency of less than 30s and perform autonomous slew to allow x-ray and optical follow-up of the source with the smaller field of view instruments: MXT and VT.
+The SVOM spacecraft carries four multi-wavelength instruments: ECLAIRs, Gamma Ray burst Monitor (GRM), Microchannel X-ray Telescope (MXT) and Visual Telescope (VT). ECLAIRs and GRM can detect gamma-ray transient sources in real-time with localization capabilities for ECLAIRs. SVOM can transfer the alerts in near real-time with a typical latency of less than 30s and perform autonomous slew to allow x-ray and optical follow-up of the source with the smaller field of view instruments: MXT and VT.
 
  <div className="overflow-table">
 
@@ -63,11 +63,11 @@ Each of the four instruments has its own dedicated topic to stream notices with
 | Notice Type                                | Content                                                              | Latency       |
 | ------------------------------------------ | -------------------------------------------------------------------- | ------------- |
 | `grm-trigger`                              | GRM trigger notice with possible rough localization                  | ~15 sec       |
-| `eclairs-wakeup`                           | ECLAIRs localisation of a GRB candidate                              | ~15 sec       |
-| `eclairs-catalog`                          | ECLAIRs localisation of a flaring source from the on-board catalogue | ~15 sec       |
+| `eclairs-wakeup`                           | ECLAIRs localization of a GRB candidate                              | ~15 sec       |
+| `eclairs-catalog`                          | ECLAIRs localization of a flaring source from the on-board catalogue | ~15 sec       |
 | `slewing` /<br/>`not-slewing` <sup>1</sup> | Platform slew status and target coordinates                          | ~1-8&nbsp;min |
-| <pre>`mxt-initial_qf#`<sup>2</sup></pre>   | MXT localisation of a found counterpart (only if platform slews)     | ~3 min        |
-| <pre>`mxt-update_qf#`<sup>2</sup></pre>    | MXT updated localisation (qf > mxt-initial_qf)                       | ~3 min        |
+| <pre>`mxt-initial_qf#`<sup>2</sup></pre>   | MXT localization of a found counterpart (only if platform slews)     | ~3 min        |
+| <pre>`mxt-update_qf#`<sup>2</sup></pre>    | MXT updated localization (qf > mxt-initial_qf)                       | ~3 min        |
 
  </div>
 
@@ -76,7 +76,7 @@ the slew threshold (in a maximum time window of 8 min) or if the slew was not
 possible. The reason is specified in the notice parameters.
 
 <sup>2</sup> the value of the quality factor `qf` indicates the accuracy
-of the localisation:
+of the localization:
  - `qf1`&#8594; 120'' < R90 < 300''<br/>
  - `qf2`&#8594; 60'' < R90 < 120''<br/>
  - `qf3`&#8594; 30'' < R90 < 60''<br/>