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<rfc xmlns:xi="http://www.w3.org/2001/XInclude" category="info" docName="draft-many-tiptop-ip-architecture-00" ipr="trust200902" obsoletes="" updates="" submissionType="IETF" xml:lang="en" version="3">
  <front>
    <title abbrev="IP in Deep Space">An Architecture for IP in Deep Space</title>
    <seriesInfo name="Internet-Draft" value="draft-many-tiptop-ip-architecture-00"/>
    <author fullname="Marc Blanchet" initials="MB">
      <organization>Viagenie</organization>
      <address>
        <postal>
          <country>Canada</country>
        </postal>
        <email>marc.blanchet@viagenie.ca</email>
      </address>
    </author>
    <author fullname="Wesley Eddy" initials="WE">
      <organization>MTI Systems</organization>
      <address>
        <postal>
          <country>USA</country>
        </postal>
        <email>wes@mti-systems.com</email>
      </address>
    </author>
    <author fullname="Tony Li" initials="TL">
      <organization>Juniper Networks</organization>
      <address>
        <postal>
          <country>USA</country>
        </postal>
        <email>tony.li@tony.li</email>
      </address>
    </author>
    <area>Internet</area>
    <workgroup>Internet Engineering Task Force</workgroup>
    <keyword>dtn</keyword>
    <keyword>quic</keyword>
    <keyword>space</keyword>
    <keyword>deep space</keyword>
    <keyword>ip</keyword>
    <keyword>dns</keyword>
    <keyword>routing</keyword>
    <abstract>
      <t>
	Deep space communications involve long delays (e.g., Earth to
	Mars is 4-24 minutes) and intermittent communications, because
	of orbital dynamics. The IP protocol stack used on Earth's Internet is
	based on assumptions of shorter delays and mostly uninterrupted
	communications. This document describes the architecture of the
	IP protocol stack tailored for its use in deep space. It
	involves buffering IP packets in IP forwarders facing
	intermittent links
	and adjusting transport protocol configuration and application
	protocol timers. This architecture applies to the Moon, Mars, or
	general interplanetary networking.
      </t>
    </abstract>
  </front>
  <middle>
    <section anchor="intro">
      <name>Introduction</name>
      <t>
	Deep space communications involve long delays (e.g., Earth to
	Mars is 4-20 minutes) and intermittent communications, because
	of orbital dynamics. Up to now, communications have been done on
	a layer-2 point-to-point basis, with sometimes the use of
	relays, but no layer-3 networking has been in use. <xref target="RFC4838"/> reports an assessment done around 25 years
	ago concluding that the IP protocol stack was not suitable for
	deep space networking. This result led to the definition of a
	completely new protocol stack based on a store-and-forward
	paradigm implemented in the Bundle Protocol(BP) <xref target="RFC9171"/> and its various components, such as
	convergence-layer adapters (<xref target="RFC9174"/>, <xref target="RFC7122"/>) and BP Security (BPSEC) <xref target="RFC9172"/>.
      </t>
      <t>More recently, space agencies plan to deploy IP
      networks on celestial bodies, such as the Moon <xref target="ioag"/> or Mars<xref target="ioag-mars"/>, on the
      surface and in orbital vicinity, using layer 2 technologies such
      as Wi-Fi or 5G. On the surface, the plan is to have a dense
      network around facilities and habitats.</t>
      <t>Mission concepts are also based on a cluster of multiple network nodes nearby at Lagrange points.</t>
      <t>
	A previous document <xref target="I-D.many-deepspace-ip-assessment"/> revisited the
	initial assessment of not using IP and concluded that the IP
	stack is viable in deep space, given the IP stack evolution
	that happened since the original evaluation.</t>
      <t>This document
	defines an architecture to use IP in deep space networking. IP
	in deep space means running IP over deep space layer-2 links,
	a reliable transport over IP, applications protocols over that
	transport, and applying proper routing, security, and network
	management on that IP network. Reusing the whole IP stack in
	deep space enables the reuse of all protocols, tools, and
	software currently used on the Internet. However, as one might
	already argue, many components of the IP stack cannot be used
	as is and therefore requires careful configuration and
	deployment considerations that are discussed in this document.
      </t>
      <t>
	Delay-Tolerant Networking (DTN), also known as Delay and
	Disruption-Tolerant Networking, has been used to identify the
	problem space, and since the solution was based on the Bundle
	protocol, DTN has also been associated with the Bundle
	protocol. This document tries to solve the DTN problem using
	the Internet Protocol stack. Therefore, in this document, the
	DTN keyword is used to name the problem space, not the Bundle
	protocol solution.
      </t>
      <t>
	Since the Moon is a few light seconds away from Earth, it is
	possible to configure and run various IP-based protocols and
	applications to make it "work". Mars with a much longer delay
	is more difficult. This
	framework would also work for longer delays, such as reaching
	Jupiter or the whole Solar System Internet (SSI), but it is
	not specifically discussed. This document uses "deep space"
	extensively as opposed to "space" which often includes
	earth-orbiting communications, which are not covered in this
	document. Even if the definition of deep space per the ITU
	does not include the Moon, this document applies to IP
	networks on the Moon.
      </t>
      <t>It should also be noted that DTN and BP were also designed
      for non-space use cases. While this document focuses on the deep
      space use case, it shall work for the other use cases of BP, but
      these use cases are outside of the scope of this document.</t>
      <t>As with the Bundle protocol, this framework proposes to use
      IP in deep space with a similar store-and-forward
      paradigm. Therefore, the IP layer has to deal with the fact that
      a destination may not be currently reachable and that IP packets
      could be stored for an unusual amount of time, such as minutes,
      hours, or days, in the forwarding device waiting for reachability back
      because of a new
      link-up  opportunity. The transport layer should be able to work
      with long and variable delays, including intermittent
      communications. The application protocols and the applications
      themselves should be properly set to wait a longer time than on
      the current Internet to receive a response to a query. Finally, all network services such as routing, security, naming, and network management should also be adapted to this new context. This document is structured around these layers.</t>
      <t>The key characteristics of space communications and networking, its use case and its requirements are discussed in another document<xref target="I-D.many-tiptop-usecase"/>.</t>
      <section>
        <name>Document and Discussion Location</name>
        <t>The source of this document is located at https://github.com/marcblanchet/draft-deepspace-ip-architecture. Comments or changes are welcomed using a PR or an issue.</t>
        <t>This subject should be discussed on the deepspace@ietf.org mailing list.</t>
      </section>
    </section>
    <section anchor="layer2">
      <name>Layer 2 in Deep Space</name>
      <section anchor="layer2surface">
        <name>Celestial Body Surface</name>
        <t>The Interagency Operations Advisory Group (IOAG) <xref target="ioag"/> has defined the communications architecture
	for the Moon and Mars. On the celestial body surface, it is planned to use 3GPP and Wi-Fi link layer protocols. IP will be used over these link layers.</t>
      </section>
      <section anchor="layer2ccsds">
        <name>Deep Space Links</name>
        <t>Deep space links typically use the Consultative Committee
	for Space Data Standards (CCSDS) <xref target="CCSDSWEB"/>
	standards for link layers, such as Telecommand (TC) <xref target="CCSDS_TC"/>, Telemetry (TM) <xref target="CCSDS_TM"/>,
	Advanced Orbiting Systems (AOS) <xref target="CCSDS_AOS"/>,
	Proximity1 (Prox1) <xref target="CCSDS_PROX1"/> or the Unified
	Space Data Link Protocol (USLP) <xref target="CCSDS_USLP"/>. CCSDS has defined a generic
	encapsulation mechanism for the payloads for all these link
	layer protocols with IP as an encapsulated protocol
	<xref target="IPoverCCSDSSpaceLinks"/> <xref target="SANAIPEHeaderRegistry"/>. Therefore, IP packets can be transported over any CCSDS link layers.</t>
      </section>
      <section anchor="layer2orbit">
        <name>Celestial Body Orbits</name>
        <t>For celestial body orbits, IOAG has planned the use of CCSDS
	link layer protocols. However, as on Earth, it may be possible
	to use 6G-NTN technology around celestial bodies, such as in
	lunar or Martian orbits. 6G-NTN technologies use IP as its
	layer 3 technology.</t>
      </section>
    </section>
    <section anchor="ip">
      <name>Internet Protocol</name>
      <t>IPv4 or IPv6 packets can be carried as is over long delays
      and disruptions, as IP has no notion of time. Originally,
      the Time To Live (TTL) field of IPv4 was defined based on time
      <xref target="STD5"/>, but it has been effectively implemented
      as a hop count, which was renamed as "Hop Count" in IPv6 <xref target="STD86"/>. Nothing needs to be changed to the IP protocol or its packet format.</t>
      <section>
        <name>IP Forwarding and Store-and-Forward</name>
        <t>
	  For deep space applications, an IP packet may need to be
	  stored temporarily over much longer periods than are typical
	  for the Internet when the next hop is currently unreachable
	  or undefined, which can happen due to orbital dynamics. This
	  is commonly referred to as "store-and-forward" and bears no
	  relationship to the same term when used regarding
	  switch architectures.
	</t>
        <t>
	  This store and forward mechanism may be implemented at layer
	  2 as is currently done by the Mars orbiters. In this case,
	  the frames are stored, regardless of payload type.  In this
	  case, IP packets are unaware of the store-and-forward and no
	  changes are needed in the IP forwarding function.  The L2
	  network is just behaving as a point-to-point link with a
	  large and variable latency.
	</t>
        <t>
	  If an IP forwarder has an interface on an intermittent link, and that link is down,
      some destinations may become unreachable when there is no alternate route. In this case,
	  the forwarder store the packets locally instead of dropping them. This might be implemented as a deep queue with
	  active queue management (AQM) <xref target="RFC7567"/>. When the
	  route to the destination is back, on the same link or a different link, maybe minutes or hours
	  later, the stored packets can be transmitted.
	</t>
        <t>
	  This store-and-forward mechanism requires proper
	  provisioning of storage for the
	  target deployment and usage. If the storage is full, then
      packets must be dropped. The choice of which packets
	  to drop depends on the policies configured on the node, which may be a
	  function of traffic class, source or destination IP
	  addresses, flow labels, or other parameters. An example is
	  described in <xref target="I-D.blanchet-tvr-forwarding"/>.
	</t>
      </section>
      <section anchor="headercompression">
        <name>Header Compression</name>
        <t>
	  Deep space links are point-to-point links and bandwidth in
	  space is very valuable, so header compression is very effective. Static Context Header Compression (SCHC) <xref target="I-D.ietf-schc-architecture"/> is a header
	  compression technique that relies on rules in a static
	  context and is, therefore, more efficient for deep
	  space. SCHC should be considered on a deep space
	  point-to-point link or a string of L2 links.
	</t>
      </section>
    </section>
    <section>
      <name>IP Addressing and Routing</name>
      <section title="Addressing">
        <t>
      The IP address space is a hierarchical namespace where
      ranges of addresses are encoded as "prefixes".  Individual
      domains advertise prefixes to the broader Internet
      and assign these addresses internally. Prefixes may be
      aggregated into less-specific prefixes, which makes the
      routing subsystem more efficient by decreasing overhead.
    </t>
        <t>
      Space networks provide a unique opportunity to provide
      extremely efficient routing by assigning a unique prefix or
      block of addresses per celestial body and its proximal
      orbits. Management of the IP address space is currently
      documented in <xref target="RFC7020"/>, but this only covers
      continental regions and does not provide for addressing for
      space.
    </t>
        <t>
      Address space for outer space should be managed by a
      Regional Internet Registry (RIR) and blocks of address space
      should be allocated for each celestial body of
      interest. Space service providers should use prefixes
      assigned by this RIR.
    </t>
      </section>
      <section title="Routing">
        <t>
	Existing routing protocols require proof of
	liveness between protocol partners, implemented through
	the periodic exchange of packets between partners. This is
	impractical on long-delay or intermittent links, so a PCE
	<xref target="RFC4655"/> based approach seems appropriate for
	those domains possibly supplemented by contact plan schedules<xref target="I-D.ietf-tvr-schedule-yang"/>. Interconnection between
	domains can still be done with BGP <xref target="RFC4271"/>,
	but long-delay or intermittent links should be
	avoided. Domains straddling such links must provide
	proxy advertisements for prefixes reachable across such links.
      </t>
        <t>
	Optimal routing for domains with intermittent links is out of
	scope for this document.
      </t>
        <t>
	On the surface of celestial bodies and in proximal orbit,
	traditional protocols are applicable and should be used (e.g.,
	<xref target="RFC9717"/>).
      </t>
      </section>
    </section>
    <section>
      <name>Transport</name>
      <section anchor="udp">
        <name>UDP</name>
        <t>UDP <xref target="RFC768"/> has no notion of time and,
	therefore can be used as-is in deep space. Hence, protocols using UDP transport can be used in space as-is, if they do not rely on time or can be configured with timeouts appropriate in deep space.</t>
      </section>
      <section anchor="quic-section">
        <name>QUIC</name>
        <t>QUIC <xref target="RFC9000"/> like most IP transport protocols
	implements congestion control mechanisms, which, based on
	various metrics such as calculated delays or packet loss, pace
	the rate of sending packets at the source node to decrease the
	perceived congestion in the network. QUIC supports many new
	features suitable and useful in deep space such as 1 RTT for
	connection establishment and security, mobility, 0 RTT,
	streams, user space, etc. [TLI: This sentence needs more words
	to explain these references.]</t>
        <t>Current implementations of QUIC typically set various
	transport configuration parameters suitable for the Internet
	environment, expecting an RTT to be in the hundreds of milliseconds
	and a normally always-connected network. Therefore, QUIC
	stacks using default configurations will not work in deep
	space. However, studies and simulations <xref target="quic-sim"/> showed that with proper configuration of
	parameters, QUIC stacks can support the delays and disruptions
	in deep space. <xref target="I-D.many-deepspace-quic-profile"/> describes how to
	properly configure a QUIC stack for deep space applications,
	where QUIC is unaware of disruptions. If the transport is
	aware of the disruptions, further optimizations are possible.</t>
        <t>Having multiple streams and applications within a single
	QUIC connection is valuable and useful for deep space. A
	ground station may set up the initial QUIC connection with a spacecraft and then carry all needed applications and streams over that same connection for the whole duration of the mission.</t>
        <t>Session keys and certificate lifetimes together with certificate validation and trust chain anchors need to be carefully configured and handled.</t>
        <t>QUIC proxies <xref target="I-D.ietf-masque-quic-proxy"/>
	can be used at the edge of space to isolate, apply policies, or
	optimize traffic at the ingress/egress to a celestial body network.</t>
      </section>
      <section>
        <name>Other Transports</name>
        <t>Other transports such as TCP <xref target="RFC9293"/>, SCTP
	<xref target="RFC9260"/>, DCCP <xref target="RFC4340"/> and others were not investigated for their suitability in space.</t>
      </section>
    </section>
    <section anchor="http-section">
      <name>HTTP</name>
      <t>HTTP by itself has no notion of time. An HTTP request and
      response may take minutes or hours to be completed. However,
      current infrastructure and software on the Internet have various time-related configurations that will not work well in the deep space context.</t>
      <t>HTTP headers containing time, such as Cache-Control and
      Expires <xref target="RFC9111"/>, should not be used or if used,
      must be set to large enough values to cover the longest delay so
      that expiration does not happen before the actual data arrives
      at the destination. As with any HTTP application and content on
      the Internet, these headers should be set properly based on the
      deployment use case, which is even more important for deep
      space. Similarly, when continuous content transfer is used, as
      with 100-Continue <xref target="RFC9110"/>, proper values for
      headers should be set.</t>
      <t>HTTP clients and servers typically have default timeouts that
      should be modified. For example, curl <xref target="curl"/> has the "-m" option for this use
      case. Similarly, HTTP server implementations have various
      timeout configuration variables that must be set
      properly. Testing with HTTP client Curl and HTTP server nginx
      and an introduced network delay of minutes, hours and days showed<xref target="quic-sim"/> that HTTP
      communications work well with basic configuration changes.</t>
      <t>HTTP applications themselves must be developed using an asynchronous pattern and if they have timeouts, they should be adjusted appropriately.</t>
      <t>Internet websites are designed with the assumption of
      hundreds of milliseconds delay and relatively always connected,
      where pages contain multiple queries to get further resources,
      media, queries to web services, and downloading additional code
      and frameworks. This could work in theory in space, but it will
      not be optimal, as multiple queries will be generated and
      therefore take multiple RTT before the whole page is received
      complete. This issue can be mitigated by using various
      techniques such as Web Assembly <xref target="wasm"/> or
      pre-caching. Moreover, it could be possible to have simple HTML
      pages with no or very few references and no media content 
      that was not locally cached. An example would be a rover on Mars presenting an HTTP server with a base and bare HTML page to offer basic info on its status (maybe all in text) and some additional detailed pages, most likely also in base HTML text. However, it is foreseen that most applications based on QUIC-HTTP transport in deep space would be using REST or similar asynchronous patterns and not typical web browsing.</t>
      <t>Caching should be used extensively on space networks to maximize local fetching. Preemptive caching by pre-populating caches with data that shall be used locally on the celestial body network shall be done as much as possible to provide better response time on the local celestial body network.</t>
      <t>QPACK <xref target="RFC9204"/> should be considered for higher bandwidth efficiency.</t>
    </section>
    <section>
      <name>Network services</name>
      <section anchor="dns">
        <name>Naming</name>
        <t>
	  For small-scale deployments, one can use IP addresses
	  directly or a mapping from a name to an IP address such as
	  /etc/hosts.  However, this does not provide easy dynamic
	  updates, scaling by hierarchy, service discovery,
	  authentication of records, etc. Therefore, the Domain Name
	  System (DNS) shall be considered early on in the space
	  deployment. However, naming hierarchy and infrastructure
	  must be carefully designed to avoid name resolution over
	  deep space links, given that answers may come after minutes
	  or hours. There are clear advantages of having the space
	  name hierarchy anchored to the current Internet root, as it
	  enables DNSSEC through the same security infrastructure
	  currently used and deployed. Using the same root also does
	  not require new policies. A new TLD or a new root is way
	  more complicated and does not bring any significant value
	  compared to using the current domain tree.</t>
        <t>Care must be taken to manage key lifecycles and resource
	record lifetimes. <xref target="I-D.many-dnsop-dns-isolated-networks"/> discusses the
	various methods and the naming hierarchy that should be used in space.</t>
      </section>
      <section>
        <name>Network Management</name>
        <t>NETCONF <xref target="RFC6241"/> and RESTCONF <xref target="RFC8040"/> shall be used with proper configuration
	values to avoid timeouts and appropriate transport. NETCONF
	over QUIC transport <xref target="I-D.ietf-netconf-over-quic"/> or RESTCONF over HTTP over QUIC transport shall be configured with appropriate QUIC transport parameters as discussed in <xref target="quic-section"/>.</t>
        <t>While being declared historic in IETF, SNMP<xref target="RFC1157"/> runs over UDP and has no notion of time. Therefore, with proper configuration of client timeout, it can be used as is to manage nodes and services in deep space.</t>
      </section>
    </section>
    <section anchor="IANA">
      <name>IANA Considerations</name>
      <t>This memo includes no request to IANA.</t>
    </section>
    <section anchor="Security">
      <name>Security Considerations</name>
      <t>Using the current IP protocol stack in deep space inherits
      all the work on privacy, cryptography, key management,
      firewalls, and scrutiny of protocols that are deployed on the
      Internet. As an example, TLS has been more carefully examined
      than almost any other secure transport protocol. Moreover, given
      that no changes are made in the protocols, this architecture
      does not bring new security issues on the protocols themselves. Deep space security
      requirements are different than on the existing Internet, but nothing has been found to prevent the conformance of the IP protocol stack to those requirements.</t>
      <t>As it is currently planned, the deep space network shall be
      isolated from the current Internet by an "air gap", to disable
      any direct communications from the Internet to deep space. Moreover, destination IP prefix filtering shall be used to restrict the traffic to only the relevant one for each link. Note that this shall also be implemented in the routing control plane, but additional security might be appropriate to further protect the deep space links.</t>
      <t>Each celestial network edge device shall have firewall rules
      to prevent inappropriate traffic from entering deep space
      links. If communications from Mars may only occur to Earth, but
      not to the Moon, then appropriate filtering based on destination
      IP prefixes shall be used.</t>
      <t>Storage in IP forwarders may become full by normal traffic or by malicious traffic that could become a denial-of-service attack.
          Appropriate policies and measures should be put in place in those forwarders to drop packets in advance to avoid the depletion of storage space and to mitigate such attacks.</t>
    </section>
  </middle>
  <back>
    <references>
      <name>References</name>
      <references>
        <name>Informative References</name>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.768.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.1157.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.4271.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.4340.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.4655.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.4838.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.6241.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.7020.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.7122.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.7567.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.8040.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9000.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9110.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9111.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9171.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9172.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9174.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9204.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9260.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9293.xml"/>
        <xi:include href="https://www.rfc-editor.org/refs/bibxml/reference.RFC.9717.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml9/reference.STD.0005.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml9/reference.STD.0086.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.blanchet-tvr-forwarding.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.ietf-masque-quic-proxy.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.ietf-netconf-over-quic.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.ietf-schc-architecture.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.ietf-tvr-schedule-yang.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.many-deepspace-ip-assessment.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.many-tiptop-usecase.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.many-deepspace-quic-profile.xml"/>
        <xi:include href="https://bib.ietf.org/public/rfc/bibxml3/reference.I-D.many-dnsop-dns-isolated-networks.xml"/>
        <reference anchor="IPoverCCSDSSpaceLinks" target="https://public.ccsds.org/Pubs/702x1b1c2.pdf">
          <front>
            <title>IP OVER CCSDS SPACE LINKS, Blue Book 702</title>
            <author>
              <organization>Consultative Committee on Space Data Systems(CCSDS)</organization>
            </author>
            <date year="2012" month="September"/>
          </front>
        </reference>
        <reference anchor="SANAIPEHeaderRegistry" target="https://sanaregistry.org/r/ipe_header/">
          <front>
            <title>Internet Protocol Extension Header</title>
            <author/>
          </front>
        </reference>
        <reference anchor="CCSDS_AOS" target="https://public.ccsds.org/Pubs/732x0b4.pdf">
          <front>
            <title>AOS Space Data Link Protocol, Blue Book 732.0-B-4</title>
            <author>
              <organization>Consultative Committee on Space Data Systems(CCSDS)</organization>
            </author>
            <date year="2021" month="October"/>
          </front>
        </reference>
        <reference anchor="CCSDS_TM" target="https://public.ccsds.org/Pubs/132x0b3.pdf">
          <front>
            <title>TM Space Data Link Protocol, Blue Book 132.0-B-3</title>
            <author>
              <organization>Consultative Committee on Space Data Systems(CCSDS)</organization>
            </author>
            <date year="2021" month="October"/>
          </front>
        </reference>
        <reference anchor="CCSDS_TC" target="https://public.ccsds.org/Pubs/232x0b4e1c1.pdf">
          <front>
            <title>TC Space Data Link Protocol, Blue Book 232.0-B-4</title>
            <author>
              <organization>Consultative Committee on Space Data Systems(CCSDS)</organization>
            </author>
            <date year="2021" month="October"/>
          </front>
        </reference>
        <reference anchor="CCSDS_PROX1" target="https://public.ccsds.org/Pubs/211x0b6e1.pdf">
          <front>
            <title>Proximity-1 Space Link Protocol—Data Link Layer, Blue Book 211.0-B-6</title>
            <author>
              <organization>Consultative Committee on Space Data Systems(CCSDS)</organization>
            </author>
            <date year="2020" month="July"/>
          </front>
        </reference>
        <reference anchor="CCSDS_USLP" target="https://public.ccsds.org/Pubs/732x1b2s.pdf">
          <front>
            <title>Unified Space Data Link Protocol, Blue Book 732.1-B-2</title>
            <author>
              <organization>Consultative Committee on Space Data Systems(CCSDS)</organization>
            </author>
            <date year="2021" month="October"/>
          </front>
        </reference>
        <reference anchor="wasm" target="https://github.com/webassembly/spec">
          <front>
            <title>WebAssembly Specifications</title>
            <author>
              <organization>World Wide Web Consortium(W3C)</organization>
            </author>
          </front>
        </reference>
        <reference anchor="ioag" target="https://www.ioag.org/Public%20Documents/Lunar%20communications%20architecture%20study%20report%20FINAL%20v1.3.pdf">
          <front>
            <title>The Future Lunar Communications Architecture, Report of the Interagency Operations Advisory Group</title>
            <author>
              <organization>Lunar Communications Architecture Working Group, Interagency Operations Advisory Group</organization>
            </author>
            <date year="2022" month="January"/>
          </front>
        </reference>
        <reference anchor="ioag-mars" target="https://www.ioag.org/Public%20Documents/MBC%20architecture%20report%20final%20version%20PDF.pdf">
          <front>
            <title>The Future
                Mars Communications Architecture, Report of the Interagency Operations Advisory Group
                </title>
            <author>
              <organization>Mars and Beyond Communications Architecture Working Group, Interagency Operations Advisory Group</organization>
            </author>
            <date year="2022" month="February"/>
          </front>
        </reference>
        <reference anchor="curl" target="https://curl.se">
          <front>
            <title>Curl</title>
            <author/>
          </front>
        </reference>
        <reference anchor="CCSDSWEB" target="https://ccsds.org">
          <front>
            <title>Consultative Committee for Space Data Systems</title>
            <author>
              <organization>CCSDS</organization>
            </author>
          </front>
        </reference>
        <reference anchor="quic-sim" target="https://deepspaceip.github.io/meetings/ietf120/ietf120-deepspaceip-simulation-results.pdf">
          <front>
            <title>Deep Space IP:
            Some simulation results</title>
            <author fullname="Marc Blanchet" initials="M." surname="Blanchet">
              <organization>Viagenie</organization>
            </author>
            <date month="July" year="2024"/>
          </front>
        </reference>
      </references>
    </references>
    <section anchor="Acknowledgements" numbered="false">
      <name>Acknowledgements</name>
      <t>This work started by reassessing the use of the whole IP stack in the context of deep space discussed in <xref target="I-D.many-deepspace-ip-assessment"/> where early contributors are acknowledged.</t>
      <t>This document and its underlying work has been reviewed and discussed by many, who have provided valuable feedback and comments, including disagreements, and made an overall more solid document. These people are, in no specific order: Padme Pillay-Esnault, Marius Feldmann, Britta Hale.</t>
    </section>
  </back>
</rfc>
