Mr. Dean Yeoman Profile

Dean Yeoman

Optoelectronics Engineer at European Space Agency - ESTEC

SPIE Involvement:

Author

Publications (3)

Proceedings Article | 27 August 2024 Presentation + Paper

High-performance infrared detector developments at the European Space Agency

Nick Nelms, Kyriaki Minoglou, Brian Shortt, Alessandra Ciapponi, Dean Yeoman, Matthew Soman, Anna Eiden, Toncho Ivanov, Mustapha Zahir, Michal Miler, Thibaut Prod'homme, Luc Boucher, Joerg Ter Haar

Proceedings Volume 13103, 131030B (2024) https://doi.org/10.1117/12.3012032

KEYWORDS: Sensors, Detector development, Charge-coupled devices, Detector arrays, Infrared detectors, Readout integrated circuits, CCD image sensors, Short wave infrared radiation, Indium gallium arsenide, Silicon

Read Abstract +

Proceedings Article | 13 December 2020 Presentation + Paper

Radiation damage testing status of the CCDs for the SMILE SXI

Steven Parsons, David Hall, Andrew Holland, Peter Verhoeve, Steven Sembay, George Randall, Oliver Hetherington, Dean Yeoman, Thomas Buggey, Matthew Soman

Proceedings Volume 11454, 114540Q (2020) https://doi.org/10.1117/12.2560337

KEYWORDS: Radiation effects, Charge-coupled devices, Cryogenics, Solar processes, Magnetosphere, X-rays, Space operations, Satellite imaging, Satellites, X-ray imaging

Read Abstract +

The joint European Space Agency and Chinese Academy of Sciences Solar wind Magnetosphere Ionosphere Link Explorer mission (SMILE) aims to develop a global scale understanding of the interaction between the solar weather and the Earth’s magnetosphere-ionosphere. The soft X-ray imager (SXI) is one of the instruments on board and will observe photons emitted in the 200 eV to 2000 eV energy range from the solar wind charge exchange process using two large 4510 x 4510 pixel CCD370s as a focal plane. The CCD370s take their design and qualification heritage from similar sensors being used in the PLATO mission, with specific modifications to optimize their performance in this soft X-ray energy range. SMILE will orbit Earth in a highly elliptical orbit and will pass through the radiation belts every 52 hours. The trapped and solar protons present will gradually damage the CCDs throughout the 3-year mission and degrade their performance. To understand the impact the damage has on the devices a series of proton radiation campaigns are being undertaken. These campaigns are being performed with flight-like SMILE CCDs, and functionally similar PLATO devices, with follow-up characterization across from -130 to -85 °C. The most recent irradiation campaign has been completed using a PLATO CCD280 kept below -85 °C for irradiation and characterization, and the results show that the measured parallel charge transfer inefficiency varies with temperature between 1x10^-4 and 4x10^-4 in unbinned full-frame readout mode. The effect of temperature annealing up to -85 °C on the parallel charge transfer inefficiency has also been assessed and shows that no temperature-dependent annealing of the radiation-induced damage has been observed. A similar behavior is expected to be seen in the SMILE devices, albeit with an anticipated improvement by a factor 3-4 due to the modifications made to the design. Thus, results indicate the SMILE CCD370s will meet the performance requirements of the SMILE SXI instrument.

Proceedings Article | 13 December 2020 Presentation + Paper

Processing x-ray data on board the SMILE SXI

George Randall, Steven Parsons, David Hall, Thomas Buggey, Oliver Hetherington, Mark Leese, Andrew Holland, Dean Yeoman, Matthew Soman

Proceedings Volume 11454, 114540T (2020) https://doi.org/10.1117/12.2560339

KEYWORDS: X-rays, Solar processes, Imaging systems, X-ray imaging, Space operations, Data modeling, Magnetosphere, Ultraviolet radiation, Plasma, Ions

Read Abstract +

View contact details

UPDATE YOUR PROFILE

Is this your profile? Update it now.

Sign into your SPIE.org account

Don’t have a profile and want one?

Create an account on SPIE.org

Keywords/Phrases

Search In:

Publication Years