DON27BZ02-NV016: D-Region Ionosphere Specification for HF Propagation

Part of the DoW SBIR/STTR FY27 Release 2 topic list. Browse all 83 topics by industry or service.

Topic DON27BZ02-NV016 from the DoW SBIR 2027 BAA, Release 2. Pre-release now; proposals due January 6, 2027, 12:00 PM ET.

Quick answer

DON27BZ02-NV016 is a Department of the Navy SBIR topic seeking measurement techniques, modeling methods, or both that improve specification and forecast of the D-region ionosphere for HF absorption and VLF propagation. It follows a standard Phase I feasibility, Phase II prototype structure. Proposals are due January 6, 2027, 12:00 PM ET.

Book a Free Fit Call

Solicitation at a glance

  • Topic number: DON27BZ02-NV016
  • Official title: Improved Ionosphere D-region Specification for High Frequency Propagation
  • Agency: Department of the Navy
  • Program: SBIR (DoW SBIR 2027 BAA, Release 2)
  • Award type: Phase I (see topic text for Phase II)
  • Award amount: Phase I base up to $200,000 plus an option up to $115,000. Source: Navy Release 2 instructions in DSIP.
  • CMMC level: Level 2 (Self)
  • ITAR: No
  • Technology areas: None
  • Pre-release (direct TPOC contact allowed): November 4 to December 2, 2026, 8:00 AM ET
  • Opens in DSIP: December 2, 2026, 8:00 AM ET
  • Proposals due: January 6, 2027, 12:00 PM ET
  • Official source: DSIP Topics app (search DON27BZ02-NV016)

BW&CO's take

What the Department of the Navy wants

HF and VLF skywave systems depend on the D-region ionosphere (about 60 to 90 km altitude), which is hard to measure and poorly captured by current models. IRI is weak at high latitudes and at night, D-RAP focuses on solar flares, and NIMO adds the D-region only in post processing. The Navy wants better specification of electron density in the 60-70 km and 80-90 km bands, within 10% error or better than existing models 75% of the time, at a 5 to 15 minute cadence and 5 degree resolution. Phase II delivers either a prototype instrument with a low-latency data feed or near-real-time model software, validated with ray-trace simulation.

Who is a good fit

  • Ionospheric remote sensing of the D-region, such as VLF or HF sounding methods, with data at low (< 30 degrees) or high (> 60 degrees) latitudes
  • Data assimilation or physics-based ionosphere modeling experience, ideally familiarity with NIMO, IDA-4D, IRI, or D-RAP
  • HF and VLF propagation and ray-trace simulation tools to quantify improvement over current models
  • Ability to run a measurement system or model in near-real-time with operationally relevant data sources

Watch-outs

  • The topic asks approaches to demonstrate improvement over existing models in both the 60-70 km and 80-90 km regions, with stated targets (10% electron density error or improvement 75% of the time).
  • Solar flare absorption alone is not the target. The topic emphasizes day-to-day variability and high-latitude nighttime conditions that current models miss.
  • Phase I must include a detailed operational implementation plan with enough evidence to justify claims of skill improvement.
  • The topic metadata lists CMMC Level 2 (Self). It is not marked as ITAR-restricted in the topic metadata.

Think your company fits DON27BZ02-NV016? Talk with BW&CO before the January 6 deadline.

Plan Your DON27BZ02-NV016 Submission

Official topic text (verbatim from DSIP)

The text in this section is copied word for word from the official DSIP topic as published on November 4, 2026. DSIP is the official source and topics can be amended. Always confirm the current version at dodsbirsttr.mil before you submit. Our commentary above is BW&CO's interpretation, not Government guidance.

Title

Improved Ionosphere D-region Specification for High Frequency Propagation

Objective

Develop tools and/or techniques to improve characterization of the D-region ionosphere sufficient for skillful ionosphere model specification and forecast over climatology and that demonstrate the impact of improved methodology on ionosphere accuracy for use by high frequency (HF) and very low frequency (VLF) signal propagation tools.

Description

HF and VLF skywave propagation depend on knowledge of the altitudinal structure of the ionosphere for reliable system operation. The D-region ionosphere, a region typically between 60-90 km altitude above the Earth’s surface, is particularly challenging to predict with sufficient fidelity for skywave mission planning because the region is difficult to measure with in situ measurements. Remote sensing methods provide a limited dataset from which to develop detailed physical and assimilative models that can reliably produce the regional behavior on a day-to-day basis.

Operational models like the D-Region Absorption Product (D-RAP) produce maps of outage areas as a function of radio frequency (RF) to inform HF system users of anticipated degradation or blackouts due to radiation increases. These predictions primarily address HF absorption due to solar X-ray flares at low and mid-latitudes and do not address the VLF propagation use case. While solar X-ray flares are important effects with Navy relevance, the effects of flares typically only last for a few hours and occur 10-20 times a year. For sufficient use in HF absorption and VLF propagation applications, a D-region ionosphere is required to capture seasonal, solar cycle, and day-to-day variability at all latitudes in addition to solar flare phenomenology.

The intended capability is improved D-region specification and forecast in the 60-70 km and 80-90 km altitude regions for VLF propagation and HF absorption, particularly day-to-day variability and in the high latitude regions at night.

Climatological models like the International Reference Ionosphere (IRI) produce an altitude profile at D-region altitudes. The IRI model is based on about a hundred historical rocket profiles, so it captures some of the basic day/night, latitudinal, and seasonal variations in the D-region ionosphere but the model does not capture day-to-day variations or solar X-ray flare events. The model may be sufficient for some HF propagation applications but has been shown to be severely deficient in the high latitude region and during nighttime. In addition, the observations used to create the model do not accurately capture the shape of the lower D-region, which is required for VLF propagation applications.

The Next-generation Ionospheric Model for Operations (NIMO) is an assimilative geospace model developed to address operational USN space weather needs in the ionosphere. NIMO harnesses contributions from both near real-time data and state-of-the-art implementation of ionospheric theory to provide hindcasts, nowcasts, and forecasts for operational or research purposes. NIMO is currently configured to assimilate various types of electron density measurements through the Ionospheric Data Assimilation Four-Dimensional (IDA-4D) data assimilation schema. The D-region is not included in the data assimilation process but is simply added in post processing to the bottom of the electron density grid. The D-region model includes influence from changes in the solar conditions, but uses a climatological model for the neutral atmosphere, so it does not capture the day-to-day variability that is seen in the ionosphere.

Key performance Metrics/Goals:

Techniques to improve the global specification and forecast of the D-region ionosphere is sought with particular emphasis on the low latitudes (< 30 degrees) and high latitudes (> 60 degrees). Note: Any measurement techniques should provide measurements or any model should ingest measurements of the D-region and demonstrate improvement over existing models in two key altitude regions: 60-70 km altitude and 80-90 km altitude, which are required for VLF propagation and HF absorption, respectively.

Key parameters include

  1. Specify electron density in the 60-70km and 80-90km regions within 10% error. Alternatively, an improvement 75% of the time over existing models is sought.
  2. Specification at a temporal cadence of 5-15 minutes
  3. Specification at a spatial resolution of 5 degrees in latitude and longitude

Technical concepts may include developing prototype concept improvements to measurement techniques and systems, developing improvements to data exploitation and modeling, or a combination of the two.

Phase I

Develop a technical concept for improvements to D-region specification. Establish the feasibility of the concept. Provide required Phase I deliverables that include a detailed plan of operational implementation with sufficient evidence to justify claims of skill improvement.

Phase II

Develop a prototype system that improves state-of-the-art forecasting for D-region morphology and validate the results in an operationally relevant environment. Depending on the nature of the Phase I concept demonstration, deliver a functioning prototype instrument demonstrated in an operationally relevant environment with low-latency data-feed or a functioning model software package that exploits operationally relevant data sources in near-real-time. Validate either solution using an appropriate ray-trace simulation tool that demonstrates improved performance over current state-of-the-art systems. Prepare a Phase III commercialization/transition plan.

Phase III Dual Use Applications

Deliver and integrate a new D-region model concept or data exploitation methodology into the NIMO for USN operational ionosphere prediction needs. Transition new measurement systems to an appropriate operator. Note: Delivery of the measurement system will be dependent upon the intended operational mode and target environment.

References

  1. Akmaev, R. A., et al. "DRAP model validation: I. Scientific report." Technical Report (2010). https://www.ngdc.noaa.gov/stp/drap/DRAP-V-Report1.pdf

  2. Bilitza, D., Pezzopane, M., Truhlik, V., Altadill, D., Reinisch, B. W. and Pignalberi, A. “The International Reference Ionosphere model: A review and description of an ionospheric benchmark.” Reviews of Geophysics, 60, e2022RG000792, 2022. https://doi.org/10.1029/2022RG000792

  3. Burrell, A. G. et al. “Next-generation Ionospheric Model for Operations – validation and demonstration for space weather and research.” Ann. Geophys., 44, 2026, pp. 303-329. https://doi.org/10.5194/angeo-44-303-2026, 2026.

Keywords

Ionosphere; D-region; space weather; very low frequency; VLF; high frequency; HF; skywave propagation; radar; communication

Frequently asked questions

What is DON27BZ02-NV016?

It is a Department of the Navy SBIR topic to develop tools or techniques that improve characterization, specification, and forecast of the D-region ionosphere for use by HF and VLF signal propagation tools.

When is DON27BZ02-NV016 due?

Proposals are due January 6, 2027, 12:00 PM ET. DSIP pre-release began November 4, 2026, and direct contact with the topic authors is allowed only until the topic opens on December 2, 2026, 8:00 AM ET.

Is this a Phase I or Direct-to-Phase II topic?

The topic describes a standard Phase I to develop and establish feasibility of a technical concept, followed by Phase II prototype development and validation in an operationally relevant environment. It does not state that it is Direct-to-Phase II.

What performance targets does the Navy set?

Specify electron density in the 60-70 km and 80-90 km regions within 10% error, or improve on existing models 75% of the time, at a temporal cadence of 5 to 15 minutes and a spatial resolution of 5 degrees in latitude and longitude.

Book a Free Fit Call

Previous
Previous

DON27BZ02-NV017: Expeditionary Water Quality Sensors

Next
Next

DON27BZ02-NV015: High-Sensitivity TMR Magnetometers