Matthew Kehrli

ORCID: 0000-0003-1268-676X
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About
Contact & Profiles
Research Areas
  • Stellar, planetary, and galactic studies
  • Astro and Planetary Science
  • Wind Energy Research and Development
  • Astronomical Observations and Instrumentation
  • Marine and coastal ecosystems
  • Air Quality Monitoring and Forecasting
  • Water Quality Monitoring and Analysis
  • Isotope Analysis in Ecology
  • Astronomy and Astrophysical Research
  • Social Acceptance of Renewable Energy
  • Atmospheric Ozone and Climate
  • Gamma-ray bursts and supernovae
  • Global Energy Security and Policy
  • Marine and Offshore Engineering Studies
  • Offshore Engineering and Technologies
  • Integrated Energy Systems Optimization
  • History and Developments in Astronomy
  • Geological and Geochemical Analysis

California Polytechnic State University
2019-2021

Scripps Institution of Oceanography
2021

University of California, San Diego
2021

Research Network (United States)
2020

Abstract The analysis of the spatiotemporal variability wind power remains limited during planning stage an offshore farm. This study provides a framework to investigate how varies along Central California Coast over diurnal and seasonal time scales, which is critical for reliability functionality grid system. We find that in this region peaks evening hours across all seasons maximizes spring summer. timing peak production better aligns with demand than solar land-based production,...

10.1088/2515-7620/ab4ee1 article EN cc-by Environmental Research Communications 2019-10-17

Abstract We report on the stellar occultation by (523764) 2014 WC 510 observed 2018 December 1 UT. This campaign was part of Research and Education Collaborative Occultation Network (RECON), a network small telescopes spread over 2000 km in western USA Canada. Light curves from six stations revealed three groups two or more consecutive flux drops correlated time between adjacent stations. A Bayesian model comparison reveals that with double object occulting star is favored alternative models...

10.3847/psj/abb23d article EN cc-by The Planetary Science Journal 2020-09-01

Abstract A stellar occultation by the extreme large-perihelion trans-Neptunian object (541132) Leleākūhonua (also known provisional designation of 2015 TG 387 ) was predicted Lucky Star project and observed with Research Education Collaborative Occultation Network on 2018 October 20 UT. single detection a nearby nondetection provide constraints for size albedo. When circular profile is assumed, radius <?CDATA $r={110}_{-10}^{+14}$?> km, corresponding to geometric albedo...

10.3847/1538-3881/ab8630 article EN The Astronomical Journal 2020-04-23

We present results from the first recorded stellar occultation by large trans-Neptunian object (174567) Varda that was observed on September 10$^{\rm th}$, 2018. belongs to high-inclination dynamically excited population, and has a satellite, Ilmar\"e, which is half size of Varda. determine albedo constrain its 3D shape density. Thirteen different sites in USA monitored event, five detected an main body. A best-fitting ellipse chords provides instantaneous limb body, geometric computed. The...

10.1051/0004-6361/202038526 article EN cc-by Astronomy and Astrophysics 2020-08-19

In 2019, the Research and Education Collaborative Occultation Network (RECON) obtained multiple-chord occultation measurements of two centaur objects: 2014 YY$_{49}$ on 2019 January 28 2013 NL$_{24}$ September 4. RECON is a citizen-science telescope network designed to observe high-uncertainty occultations by outer solar system objects. Adopting circular models for object profiles, we derive radius $r=16^{+2}_{-1}$km geometric albedo $p_V=0.13^{+0.015}_{-0.024}$ YY$_{49}$, $r=66...

10.3847/psj/abd62a article EN cc-by The Planetary Science Journal 2021-02-01

Abstract In response to the growing interest in offshore wind energy development California, U.S. Bureau of Ocean Energy Management delineated three Call Areas for potential leasing. This study provides a comprehensive characterization and comparison power within two Central California (Diablo Canyon Morro Bay) using 12‐ 15‐MW turbines under different inter‐turbine spacing farm size scenarios. Our analysis shows similar daily seasonal patterns produced Areas, which peak spring during evening...

10.1002/we.2646 article EN Wind Energy 2021-05-11

Non-algal particles and chromophoric dissolved organic matter (CDOM) are two major classes of seawater constituents that contribute substantially to light absorption in the ocean within ultraviolet (UV) visible (VIS) spectral regions. The similarities shape these constituent coefficients, a d ( λ ) g ), respectively, have led their common estimation as single combined non-phytoplankton coefficient, dg optical remote-sensing applications. Given different biogeochemical ecological roles...

10.1364/ao.517706 article EN Applied Optics 2024-04-15

Extending the capabilities of optical remote sensing and inverse algorithms, which have been commonly focused on visible (VIS) range electromagnetic spectrum, to derive properties seawater in ultraviolet (UV) is important advancing understanding various optical, biological, photochemical processes ocean. In particular, existing remote-sensing reflectance models that total spectral absorption coefficient seawater, a(λ), partitioning partition a(λ) into component coefficients phytoplankton,...

10.1364/oe.486354 article EN cc-by Optics Express 2023-04-27
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