CVE-2006-2440

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Summary

CVECVE-2006-2440
StatePUBLIC
Assigner[email protected]
Source PriorityCVE Program / NVD first with legacy fallback
Published2006-05-18 10:02:00 UTC
Updated2017-10-12 01:29:00 UTC
DescriptionHeap-based buffer overflow in the libMagick component of ImageMagick 6.0.6.2 might allow attackers to execute arbitrary code via an image index array that triggers the overflow during filename glob expansion by the ExpandFilenames function.

Risk And Classification

Problem Types: NVD-CWE-Other

NVD Known Affected Configurations (CPE 2.3)

TypeVendorProductVersionUpdateEditionLanguage
Application Imagemagick Imagemagick 6.0.6.2 All All All
Application Imagemagick Imagemagick 6.2.4 All All All
Application Imagemagick Imagemagick 6.0.6.2 All All All
Application Imagemagick Imagemagick 6.2.4 All All All

References

ReferenceSourceLinkTags
Red Hat update for ImageMagick - Advisories - Secunia SECUNIA secunia.com
SGI Advanced Linux Environment 3 Multiple Updates - Advisories - Secunia SECUNIA secunia.com
20070201-01-P SGI patches.sgi.com
Debian -- Security Information -- DSA-1168-1 imagemagick DEBIAN www.debian.org
Support REDHAT www.redhat.com
Repository / Oval Repository OVAL oval.cisecurity.org
Debian update for imagemagick - Secunia.com SECUNIA secunia.com
#345595 - libmagick: array index overflow in DisplayImageCommand - Debian Bug report logs CONFIRM bugs.debian.org Patch
CVE Program record CVE.ORG www.cve.org canonical
NVD vulnerability detail NVD nvd.nist.gov canonical, analysis

Vendor Comments And Credit

OrganizationPublishedContributorStatement
Red Hat2006-09-19Mark J CoxRed Hat is aware of this issue and is tracking it via the following bug: https://bugzilla.redhat.com/bugzilla/show_bug.cgi?id=192278 The Red Hat Security Response Team has rated this issue as having low security impact, a future update may address this flaw. More information regarding issue severity can be found here: http://www.redhat.com/security/updates/classification/ This issue does not affect Red Hat Enterprise Linux 2.1 or 3.

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