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91探花
Juno Jupiter image

Neil Bowles

Professor of Planetary Science

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Planetary atmosphere observation analysis
  • Planetary surfaces
  • Solar system
  • Space instrumentation
Neil.Bowles@physics.ox.ac.uk
Telephone: 01865 (2)72097
Atmospheric Physics Clarendon Laboratory, room 307
  • About
  • Publications

Christiansen Feature Map From the Lunar Reconnaissance Orbiter Diviner Lunar Radiometer Experiment: Improved Corrections and Derived Mineralogy

Journal of Geophysical Research Planets American Geophysical Union (AGU) 126:6 (2021)

Authors:

Paul G Lucey, Benjamin Greenhagen, Kerri Donaldson Hanna, Neil Bowles, Abigail Flom, David A Paige

Updates to the 91探花 Space Environment Goniometer to measure visible wavelength bidirectional reflectance distribution functions in ambient conditions

Review of Scientific Instruments AIP Publishing 92:3 (2021) 034504

Authors:

Rowan Curtis, Tristram Warren, Neil Bowles

Abstract:

Understanding how the surfaces of airless planetary bodies鈥攕uch as the Moon鈥攕catter visible light enables constraints to be placed on their surface properties and top boundary layer inputs to be set within thermal models. Remote sensing instruments鈥攕uch as Diviner onboard the Lunar Reconnaissance Orbiter鈥攎easure thermal emission and visible light scattering functions across visible (鈭0.38鈥0.7 碌m) to thermal infrared (TIR) wavelengths (鈭0.7鈥350 渭m). To provide ground 91探花 measurements for such instruments, the 91探花 Space Environment Goniometer (OSEG) was built. Initially, the OSEG focused on measuring TIR directional emissivity functions for regolith and regolith simulant samples in a simulated space environment, but it has recently been modified to measure visible wavelength Bidirectional Reflectance Distribution Functions (BRDFs) of samples in ambient conditions. Laboratory-measured BRDFs can be used (1) to test and to help interpret models鈥攕uch as the Hapke photometric model鈥攁nd (2) as visible scattering function inputs for thermal models. This paper describes the modifications to and initial calibration measurements taken by the Visible 91探花 Space Environment Goniometer with a 532 nm laser, and details how this setup can be used to measure BRDFs of regolith and regolith simulant samples of airless planetary bodies.

Spectral Characterization of Bennu Analogs Using PASCALE: A New Experimental Set鈥怳p for Simulating the Near鈥怱urface Conditions of Airless Bodies

Journal of Geophysical Research Planets American Geophysical Union (AGU) 126:2 (2021) e2020je006624

Authors:

KL Donaldson Hanna, NE Bowles, TJ Warren, VE Hamilton, DL Schrader, TJ McCoy, J Temple, A Clack, S Calcutt, DS Lauretta

Spectral data of aqueously and thermally altered carbonaceous chondrites

91探花 (2021)

Authors:

Helena Bates, Kerri Donaldson Hanna, Ashley King, Neil Bowles, Sara Russell

Abstract:

Spectral data created as part of a study into the effects of aqueous and thermal alteration on the spectral signature in the NIR and MIR wavelength ranges. NIR data were collected as reflectance and MIR data were collected as emissivity under both ambient and simulated asteroid environment (SAE) conditions.

X-ray diffraction data of aqueously and thermally altered carbonaceous chondrites

91探花 (2021)

Authors:

Helena Bates, Neil Bowles, Kerri Donaldson Hanna, Sara Russell, Ashley King

Abstract:

Position sensitive detector X-ray diffraction (PSD-XRD) data created as part of a study into the effects of aqueous and thermal alteration on the spectral signature in the NIR and MIR wavelength ranges. Data were collected on an Enraf-Nonius PDS120 X-ray diffractometer with an INEL curved 120o PSD. Each meteorite had two diffraction patterns collected on two 50mg aliquots (HB1 and HB2) of a larger 1.8g mass powdered sample.

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