CVE-2003-0456
UnknownEPSS 2.76%
Last modified
CVE-2003-0456 is a vulnerability of currently unknown severity. VisNetic WebSite 3.5 allows remote attackers to obtain the full pathname of the server via a request containing a folder that does not exist, which leaks the pathname in an error message, as demonstrated using _vti_bin/fpcount.exe.. EPSS estimates a 2.76% chance of exploitation in the next 30 days.
Description
VisNetic WebSite 3.5 allows remote attackers to obtain the full pathname of the server via a request containing a folder that does not exist, which leaks the pathname in an error message, as demonstrated using _vti_bin/fpcount.exe.
Metrics
Weakness Enumeration
Affected Software
| Vendor | Product | Versions |
|---|---|---|
| Deerfield | Visnetic Website | 3.5.13 |
| Deerfield | Visnetic Website | 3.5.15 |
| Deerfield | Visnetic Website | 3.5.17 |
References
- http://archives.neohapsis.com/archives/vulnwatch/2003-q3/0002.htmlExploit, Patch, Vendor Advisory
- http://www.securityfocus.com/bid/8075Patch, Vendor Advisory
- http://archives.neohapsis.com/archives/vulnwatch/2003-q3/0002.htmlExploit, Patch, Vendor Advisory
- http://www.securityfocus.com/bid/8075Patch, Vendor Advisory
Timeline
- Published
- Last Modified
- Status
- Modified
Frequently Asked Questions
What is CVE-2003-0456?
VisNetic WebSite 3.5 allows remote attackers to obtain the full pathname of the server via a request containing a folder that does not exist, which leaks the pathname in an error message, as demonstrated using _vti_bin/fpcount.exe.
How severe is CVE-2003-0456?
Severity scoring for CVE-2003-0456 is pending analysis. The EPSS model estimates a 2.76% probability of exploitation in the next 30 days.
How do I fix CVE-2003-0456?
Check the vendor references and advisories linked above for patched versions and mitigation guidance. You can also run a Strix scan to test if your systems are affected.
Are you affected by CVE-2003-0456?
Run a free Strix scan to check your systems for this vulnerability.
Scan your code nowSource: NVD / NIST
