Abstract

We are studying the development of space-flight compatible room-temperature electronics for the Lynx x-ray microcalorimeter (LXM) of the Lynx mission. The baseline readout technique for the LXM is microwave SQUID multiplexing. The key modules at room temperature are the RF electronics module and the digital electronics and event processor (DEEP). The RF module functions as frequency converters and mainly consists of local oscillators and I/Q mixers. The DEEP performs demultiplexing and event processing, and mainly consists of field-programmable gate arrays, ADCs, and DACs. We designed the RF electronics and DEEP to be flight ready, and estimated the power, size, and mass of those modules. There are two boxes each for the RF electronics and DEEP for segmentation, and the sizes of the boxes are 13 in: × 13 in: × 9 in: for the RF electronics and 15.5 in: × 11.5 in: × 9.5 in: for the DEEP. The estimated masses are 25.1 kg∕box for the RF electronics box and 24.1 kg∕box for the DEEP box. The maximum operating power for the RF electronics is 141 W or 70.5 W∕box, and for the DEEP box is 615 W or 308 W∕box. The overall power for those modules is 756 W. We describe the detail of the designs as well as the approaches to the estimation of resources, sizes, masses, and powers.

Highlights

  • The Lynx mission concept is one of four flagship missions being studied for consideration in the 2020 Astrophysics Decadal Survey.[1]

  • In microwave SQUID multiplexing, hundreds of sensor signals are fed into RF-SQUIDs that are inductively coupled to superconducting microwave resonators spread over a frequency range of several gigahertz and are read out using a single pair of coaxial cables

  • We present a design for the RF electronics and digital electronics and event processor (DEEP) that meets the notional requirements of each subsystem using technology that should be available in the near future

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Summary

Introduction

The Lynx mission concept is one of four flagship missions being studied for consideration in the 2020 Astrophysics Decadal Survey.[1]. The Lynx x-ray microcalorimeter[2] (LXM), one of three instruments the spacecraft carries, is an imaging spectrometer, which will provide 3-eV spectral energy resolution over the 0.2 to 7 keV energy band for 5 0 × 5 0 field of view (FOV) with 1′′ pixels. We present a design for the RF electronics and DEEP that meets the notional requirements of each subsystem using technology that should be available in the near future. These designs are based on several currently available stateof-the-art readout systems developed for ground applications.

Microwave SQUID Multiplexing Readout System Overview
MHz 40 MHz
50 L 90 deg shift RI
RF Electronics
Digital Electronics and Event Processor
ADC and DAC
FPGA Design
Tone generation and channelization
Microwave SQUID multiplexer demodulator
Event processing
FPGA Resource Estimation
Power and Mass Estimation
Tone Tracking
Resource Reduction
Thermal Loading and Radiation Hardness
Findings
Summary
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