NASA SBIR 2020-I Solicitation

Proposal Summary


PROPOSAL NUMBER:
 20-1- S1.08-6766
SUBTOPIC TITLE:
 Suborbital Instruments and Sensor Systems for Earth Science Measurements
PROPOSAL TITLE:
 Hyperspectral VSF and Polarization Instrument
SMALL BUSINESS CONCERN (Firm Name, Mail Address, City/State/Zip, Phone)
Photonics Automation Specialties LLC
1402 East Manlove Sreet #43
Tucson, AZ 85719
(520) 286-6545

Principal Investigator (Name, E-mail, Mail Address, City/State/Zip, Phone)

Name:
Xiyao Zhang
E-mail:
xiyao.zhang@photonicsautomation.com
Address:
4643 N Mountain Quail Rd Tucson, AZ 85719 - 6207
Phone:
(919) 723-8277

Business Official (Name, E-mail, Mail Address, City/State/Zip, Phone)

Name:
Gerard Knight-Rubino
E-mail:
jerry.rubino@photonicsautomation.com
Address:
1402 E Manlove St #43 Tucson, AZ 85719 - 6348
Phone:
(520) 286-6545
Estimated Technology Readiness Level (TRL) :
Begin: 1
End: 4
Technical Abstract (Limit 2000 characters, approximately 200 words)

An In situ polarized hyperspectral UV-Vis volume scattering function (VSF) instrument (ocean submersible to 300 m) covering the angular range close to 0 degrees and as far as 180 degrees (with  ≤2 degree angular resolution) with an ability to measure (at least) horizontal and vertical aspects of linear polarization is proposed herein.

To date, there have been several implementations of VSF instruments that capture a portion of these requirements, but none that completely capture them.  The current state of the art instrument for capturing polarized VSF utilizes a single wavelength and a scanning head to capture light intensity at angles along the beam.

Therefore, we propose an innovative instrument design using approximately 180 optical fiber positions laid out in a concentric circle pointing to the small volume of water being measured. Each fiber will feed into a multichannel spectrometer (spectrograph) which can take all the spectra in a single acquisition.  This way, spectra at all scattering angles can be collected simultaneously, which greatly reduces the overall measurement time. In additional to the much faster speed, the proposed scheme also offers the following advantages over the current state of the art instrument design:

    1) There will be no moving parts outside of the main instrument housing, which makes it easier to be sealed, more robust and portable;
    2) Instead of collecting scattered light at different points along the laser beam, the proposed design looks at the same small volume of water.
    3) Because the optical path lengths for all scattering angles are the same in the proposed new instrument  The overall simple and symmetric geometry (e.g. the identical optical path lengths at different angles) will make calibration easier and improve accuracy.

 

Potential NASA Applications (Limit 1500 characters, approximately 150 words)
    1. As part of future development, we could combine the volume scattering function and absorption spectral measurements together. We could also miniaturize the design;
    2. We could further make the instrument space mission worthy (with different specs if necessary) for the exploration of the other ocean worlds in the solar system;
Potential Non-NASA Applications (Limit 1500 characters, approximately 150 words)
    1. Oceanography: fluorescence analysis of seawater. 
    2. Mineral Analysis: by analyzing absorption lines in the water spectra, we can potentially see the elemental composition of the water and its angular components;
    3. Photonics: analysis of the spectral, radiant, and polarimetric variation of light sources;
    4. Optics: direct optical characterization of birefringent materials;
Duration: 6

Form Generated on 06/29/2020 21:12:56