Changes between Version 40 and Version 41 of TBR/UserApp/Space/Proba_2
- Timestamp:
- 11/13/18 21:08:00 (5 years ago)
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TBR/UserApp/Space/Proba_2
v40 v41 5 5 PROBA stands for PRoject for !OnBoard Autonomy. The PROBA satellites are among the smallest spacecraft ever to be flown by ESA, but they are making a big impact in the field of space technology. PROBA-2 is the second of the series, building on nearly eight years of successful PROBA-1 experience. 6 6 7 [[Image( https://devel.rtems.org/old_images/Proba-2-in-orbit-rear-view.jpg, 400px)]]7 [[Image(Proba-2-in-orbit-rear-view.jpg, 400px)]] 8 8 9 9 Figure 1: Rear view of PROBA-2 in orbit … … 81 81 onboard. The spacecraft platform provides full redundancy. 82 82 83 [[Image( https://devel.rtems.org/old_images/PROBA2_Auto11.jpeg)]]83 [[Image(PROBA2_Auto11.jpeg)]] 84 84 85 85 Figure 2: PROBA-2 Block Diagram … … 108 108 possible. 109 109 110 [[Image( https://devel.rtems.org/old_images/PROBA2_Auto14.jpeg)]]110 [[Image(PROBA2_Auto14.jpeg)]] 111 111 112 112 Figure 3: PROBA-2 internal structure and accommodation … … 145 145 set of Phoenix GPS receivers provided by DLR. 146 146 147 [[Image( https://devel.rtems.org/old_images/PROBA2_Auto2.jpeg)]]147 [[Image(PROBA2_Auto2.jpeg)]] 148 148 149 149 Figure 4: Phoenix GPS architecture for PROBA-2 … … 339 339 allowing autonomous flare tracking up to 3 times the sun radius. 340 340 341 [[Image( https://devel.rtems.org/old_images/PROBA2_Auto1F.jpeg)]]341 [[Image(PROBA2_Auto1F.jpeg)]] 342 342 343 343 Figure 5: Open view of the main components of SWAP and SWAP Flight Model (image courtesy AMOS S.A.) … … 506 506 507 507 * Provision of daily global coverage of the land masses in the latitudes 35º and 75º North and in the latitudes between 35° and 56° South, with a 90% daily coverage of equatorial zones - and 100% two-daily imaging, during day time, of the land masses in the latitudes between 35º North and 35º South.. 508 [[Image( https://devel.rtems.org/old_images/ProbaV_Auto12.jpeg)]]508 [[Image(ProbaV_Auto12.jpeg)]] 509 509 510 510 Figure 6: Artist's view of the PROBA-V spacecraft (image credit: ESA) 12) 13) … … 524 524 * HMA (Heterogeneous Mission Access) and QA4EO (Quality Assurance for Earth Observation) implementation for user data. Planned interoperability with GSCDA V2 (GMES Space Component Data Access Version 2). 525 525 526 [[Image( https://devel.rtems.org/old_images/ProbaV_Auto11.jpeg)]]526 [[Image(ProbaV_Auto11.jpeg)]] 527 527 528 528 Figure 7: PROBA-V project organization (image credit: ESA, Ref. 9) … … 538 538 The power distribution and conditioning part of ADPMS supplies an unregulated bus, with each equipment having its internal DC/DC converter. The power conditioning system is designed around a Li-ion battery. 539 539 540 [[Image( https://devel.rtems.org/old_images/ProbaV_Auto10.jpeg)]]540 [[Image(ProbaV_Auto10.jpeg)]] 541 541 Figure 8: PROBA-V spacecraft accommodation (image credit: QinetiQ Space) 542 542 … … 595 595 The development of the new X-band transmitter is based almost exclusively on COTS components to achieve at the same time high performances and low recurrent cost. The transmitter also features an innovative functionality with an on-board programmable RF output power from 1-10 W which allows to match finely with the chosen bit rate, and to reduce as much as possible the margins of the link budget and therefore the consumption power. PROBA-V is the first mission to use this newly developed transmitter. The transmitter has a mass of 1 kg, a size of 160 mm x 115 mm x 46 mm, an in-orbit life time of 5 years, and a radiation hardness of 10 krad. Data rates from 10-100 Mbit/s are available. The X-band transmitter was manufactured by TES Electonic Solutions of Bruz, France. 18) 596 596 597 [[Image( https://devel.rtems.org/old_images/ProbaV_AutoF.jpeg)]]597 [[Image(ProbaV_AutoF.jpeg)]] 598 598 599 599 Figure 9: Overview of the transmitter architecture (CNES, TES) 600 600 601 [[Image( https://devel.rtems.org/old_images/ProbaV_AutoE.jpeg)]]601 [[Image(ProbaV_AutoE.jpeg)]] 602 602 603 603 Figure 10: Photo of the X-band transmitter (image credit: CNES, ESA)