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Numerical Simulation of VLF Antennas in Space Plasma

ID: SF241-0016 • Type: SBIR / STTR Topic • Match:  85%
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Description

OUSD (R&E) CRITICAL TECHNOLOGY AREA(S): Space Technology The technology within this topic is restricted under the International Traffic in Arms Regulation (ITAR), 22 CFR Parts 120-130, which controls the export and import of defense-related material and services, including export of sensitive technical data, or the Export Administration Regulation (EAR), 15 CFR Parts 730-774, which controls dual use items. Offerors must disclose any proposed use of foreign nationals (FNs), their country(ies) of origin, the type of visa or work permit possessed, and the statement of work (SOW) tasks intended for accomplishment by the FN(s) in accordance with the Announcement. Offerors are advised foreign nationals proposed to perform on this topic may be restricted due to the technical data under US Export Control Laws. OBJECTIVE: Develop a multi-scale 3D numerical Electro-Magnetic (EM) plasma simulation capable of resolving a real electric dipole antenna (cm width and 100 m length) or magnetic loop antenna (cm wire, 20 m diameter) as well as the electromagnetic radiation produced by the antenna with km scale wavelengths. DESCRIPTION: Energetic electrons (100 - 2000 keV), due to either natural process or a High Altitude Nuclear Explosion, HANE, become trapped in the Earth's magnetic field where they are a threat to satellites in low Earth orbit. One technique for removing these electrons is to mimic nature with electromagnetic (EM) Whistler waves that are known to scatter electrons onto trajectories aligned with the magnetic field, where they are lost into the atmosphere [Starks, 2020]. The recent DSX (Demonstration and Science Experiment) mission [Johnston, 2023] successfully demonstrated transmission by an 80 m dipole antenna and reception by a remote satellite. While DSX was able to measure the dissipated power, it was unable to quantify the efficiency of radiation versus local dissipation i.e., plasma heating. Since follow-on systems must be precision engineered for a required size, weight, and power, this topic calls for a numerical model capable of representing antenna concepts in realistic detail while modeling both the local plasma response and the distant radiation including the wave mode. Whistler waves can exist in a range of modes from electrostatic (ES) to electromagnetic (EM). Current thinking holds that EM waves are more effective at modifying the electron pitch angle since the magnetic interaction consumes no energy; while antennas that are small compared to the free space VLF wavelength (100 km) preferentially excite ES waves due to the high index of refraction that matches the wavelength in plasma to the antenna size. Current antenna concepts include: the electric dipole such as with DSX, the magnetic loop antenna, the magnetic rod antenna; and engineered plasma modification for such (near the antenna) to produce non-linear beat wave interference and conversion from ES to EM radiation [Sotnikov, 2018]. The end product will be a computer plasma model capable of aiding the design of a space-based antenna immersed in the low or near Earth plasma. This model will be capable of simulating the performance of the recent DSX antenna, a 100A 20 m diameter magnetic loop, and a compact magnetic rod producing a similar dipole moment. While the usual SBIR rights will apply to the model, so also will the government's limited right to effectively use the model following conclusion of the SBIR effort. PHASE I: In Phase I, the contractor will identify and demonstrate the numerical methods to be used, and at conclusion have demonstrated the viability of the approach. This effort is expected to be computationally intensive so a limited demonstration will be acceptable i.e., it will not be necessary to obtain production levels of super-computer access. Never-the-less, since super-computing is an anticipated requirement, such capability must be convincingly demonstrated PHASE II: During Phase-II, the capability to effectively model one or more antenna concepts is expected, and a fully functional design tool should be delivered at the conclusion of Phase-II. PHASE III DUAL USE APPLICATIONS: In Phase-III the antenna-plasma design tool will be used to design candidate systems for the radiation of radios waves at Very Low Frequency. REFERENCES: Starks, M. J., et.al. 2020, J. Geophys. Res. Space Physics, 125, doi: 10.1029/2019JA027029.; Johnston, W. R., et al. (2023). J.Geophys. Res.: Space Physics,128, doi: 10.1029/2022JA030771; Sotnikov V., et al 2018, Plasma Phys. Control. Fusion 60 044014; KEYWORDS: Radiation Belt Remediation; High Altitude Nuclear Explosion; Particle-In-Cell,

Overview

Response Deadline
Feb. 7, 2024 Past Due
Posted
Nov. 29, 2023
Open
Jan. 3, 2024
Set Aside
Small Business (SBA)
Place of Performance
Not Provided
Source
Alt Source

Program
SBIR Phase I / II
Structure
Contract
Phase Detail
Phase I: Establish the technical merit, feasibility, and commercial potential of the proposed R/R&D efforts and determine the quality of performance of the small business awardee organization.
Phase II: Continue the R/R&D efforts initiated in Phase I. Funding is based on the results achieved in Phase I and the scientific and technical merit and commercial potential of the project proposed in Phase II. Typically, only Phase I awardees are eligible for a Phase II award
Duration
6 Months - 1 Year
Size Limit
500 Employees
On 11/29/23 Department of the Air Force issued SBIR / STTR Topic SF241-0016 for Numerical Simulation of VLF Antennas in Space Plasma due 2/7/24.

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