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authorDan McGee <dan@archlinux.org>2010-10-07 15:09:07 +0200
committerDan McGee <dan@archlinux.org>2010-10-07 15:09:07 +0200
commit82f3b02f602b8244047ab12f38dadc42f416bd2d (patch)
tree4ed2ffe599ee459313da2e71b2347cdaebf78a40 /templates
parent2e299273e2462775cf3ecd4f93715678575319fd (diff)
downloadarchweb-82f3b02f602b8244047ab12f38dadc42f416bd2d.tar.gz
archweb-82f3b02f602b8244047ab12f38dadc42f416bd2d.tar.xz
Factor check completion pct into mirror score
Use it as the divisor in our slightly longer equation. Signed-off-by: Dan McGee <dan@archlinux.org>
Diffstat (limited to 'templates')
-rw-r--r--templates/mirrors/status.html5
1 files changed, 3 insertions, 2 deletions
diff --git a/templates/mirrors/status.html b/templates/mirrors/status.html
index d2e4537..47ba9b7 100644
--- a/templates/mirrors/status.html
+++ b/templates/mirrors/status.html
@@ -36,8 +36,9 @@
retrieval time. A high standard deviation can indicate an unstable or
overloaded mirror.</li>
<li><em>Mirror Score:</em> A very rough calculation for ranking
- mirrors. It is currently calculated as <tt>hours delay + average
- duration + standard deviation</tt>. Lower is better.</li>
+ mirrors. It is currently calculated as <tt>(hours delay + average
+ duration + standard deviation) / completion percentage</tt>. Lower
+ is better.</li>
</ul>
<p>The final table on this page is an error log, which shows any errors
that occurred while contacting mirrors. This only shows errors that