The Black Hole Explorer: Back End Electronics
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arXiv
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| Autori principali: | , , , , , , , , , , , , , , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| author | Srinivasan, Ranjani Weintroub, Jonathan Raffanti, Rick Bilyeu, Bryan Gauron, Thomas Test, John Richards, Elliot Fernandez, Manuel Freeman, Mark Cheimets, Peter Gendelman, Mauricio Haworth, Kari Houston, Janice Johnson, Michael D. Mamani, Emilia Marrone, Daniel Pola, Ariel L. Wang, Jade |
| author_facet | Srinivasan, Ranjani Weintroub, Jonathan Raffanti, Rick Bilyeu, Bryan Gauron, Thomas Test, John Richards, Elliot Fernandez, Manuel Freeman, Mark Cheimets, Peter Gendelman, Mauricio Haworth, Kari Houston, Janice Johnson, Michael D. Mamani, Emilia Marrone, Daniel Pola, Ariel L. Wang, Jade |
| contents | This paper describes specification and early design of back end signal processing subsystems for the Black Hole Explorer (BHEX) Very Long Baseline Interferometry (VLBI) space telescope. The "back end" consists of two subsystems. First, the block downconverter (BDC) is a heterodyne system that performs a frequency translation of the analog signal from IF to baseband and amplifies and filters it for digitization. Second, the digital back end (DBE) samples the analog signal with an analog-to-digital converters (ADC) and digitally processes the data stream formatting them to the VLBI "VDIF" standard and converting to Ethernet packets for 100 gigabit-per-second (Gb/s) Ethernet transport to the optical downlink system. Both the BDC and the DBE for BHEX support eight channels of 4.096 GHz bandwidth each, for a total processed bandwidth of 32.768 GHz. The BHEX back end benefits from mature terrestrial back end heritage, described in some detail. The BHEX back end itself is in the early stages of design, with requirements, interface specifications, and component trade studies well advanced. The aim is to build a prototype using terrestrial grade parts which are available in functionally identical space grade equivalents, and to use this prototype to advance the back end Technology Readiness Level (TRL) preparing for a Small Explorer (SMEX) proposal in 2025. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_10103 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The Black Hole Explorer: Back End Electronics Srinivasan, Ranjani Weintroub, Jonathan Raffanti, Rick Bilyeu, Bryan Gauron, Thomas Test, John Richards, Elliot Fernandez, Manuel Freeman, Mark Cheimets, Peter Gendelman, Mauricio Haworth, Kari Houston, Janice Johnson, Michael D. Mamani, Emilia Marrone, Daniel Pola, Ariel L. Wang, Jade Instrumentation and Methods for Astrophysics This paper describes specification and early design of back end signal processing subsystems for the Black Hole Explorer (BHEX) Very Long Baseline Interferometry (VLBI) space telescope. The "back end" consists of two subsystems. First, the block downconverter (BDC) is a heterodyne system that performs a frequency translation of the analog signal from IF to baseband and amplifies and filters it for digitization. Second, the digital back end (DBE) samples the analog signal with an analog-to-digital converters (ADC) and digitally processes the data stream formatting them to the VLBI "VDIF" standard and converting to Ethernet packets for 100 gigabit-per-second (Gb/s) Ethernet transport to the optical downlink system. Both the BDC and the DBE for BHEX support eight channels of 4.096 GHz bandwidth each, for a total processed bandwidth of 32.768 GHz. The BHEX back end benefits from mature terrestrial back end heritage, described in some detail. The BHEX back end itself is in the early stages of design, with requirements, interface specifications, and component trade studies well advanced. The aim is to build a prototype using terrestrial grade parts which are available in functionally identical space grade equivalents, and to use this prototype to advance the back end Technology Readiness Level (TRL) preparing for a Small Explorer (SMEX) proposal in 2025. |
| title | The Black Hole Explorer: Back End Electronics |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2406.10103 |