AS7690 Mirai Communication Network Inc. 🇯🇵 JP
Announcing 10 prefixes, seen at the RIS collectors.
IPv4 prefixes
9
38,912 (152 × /24)
IPv6 prefixes
1
1 × /32
Upstreams
2
transit providers observed
Peers
5
settlement-free adjacencies
Downstreams
2
transit customers observed
Customer cone
3
ASes reachable through it
Registry and operator data
- AS number
- AS7690
- Name
- Mirai Communication Network Inc.
- Organisation
- Mirai Communication Network inc.,
- Country
- 🇯🇵 JP
- RIR
- APNIC
- Allocated
- 1997-11-13
- Network type
- NSP
- Traffic levels
- 10-20Gbps
- Scope
- Asia Pacific
- Peering policy
- Open
- IRR as-set
- AS-MIRAI
- Website
- https://www.mirai.ad.jp/
- PeeringDB
- net/5565
- Exchanges
- 5
RPKI coverage of this AS
Its own announcements, validated against the current ROA set
Upstreams
Networks seen providing transit to this one
| Network | Country | Cone | IPv4 prefixes | Paths | Source |
|---|---|---|---|---|---|
| AS2497 Internet Initiative Japan Inc. | 🇯🇵 JP | 28,464 | 244 | 275 | CAIDA |
| AS10010 TOKAI Communications Corporation | 🇯🇵 JP | 94 | 186 | 122 | CAIDA |
Peers
Adjacencies that look settlement-free rather than transit
| Network | Country | Cone | IPv4 prefixes | Paths | Source |
|---|---|---|---|---|---|
| AS6939 Hurricane Electric LLC | 🇺🇸 US | 56,494 | 236 | 41 | CAIDA |
| AS20485 TransTeleCom JSC | 🇷🇺 RU | 28,474 | 85 | 6 | CAIDA |
| AS9304 HGC Global Communications Limited | 🇭🇰 HK | 25,250 | 1,763 | 2 | CAIDA |
| AS24482 SG.GS | 🇸🇬 SG | 20,686 | 45 | 9 | CAIDA |
| AS17639 Converge ICT Solutions Inc. | 🇵🇭 PH | 243 | 567 | 7 | CAIDA |
Downstreams
Networks this one appears to provide transit to
| Network | Country | Cone | IPv4 prefixes | Paths | Source |
|---|---|---|---|---|---|
| AS18076 Institute of Advanced Media Arts and Sciences | 🇯🇵 JP | 0 | 1 | 31 | CAIDA |
| AS9591 National Institute for Fusion Science | 🇯🇵 JP | 0 | 2 | 8 | CAIDA |
Relationships marked inferred come from where the two networks sit on the AS paths the collectors see, which is a guess and is wrong for some of them. The rest are stated by CAIDA's published inference over a much wider set of collectors.