Two Years of Experience in Implementation of the mobiREH Remote Rehabilitation System Supporting Patients and Physiotherapists

The aim of this work is to characterise the process of developing the mobiREH telemedical rehabilitation system which was created as a result of cooperation between the mReh start-up team and the scientific team from the Academy of Physical Education in Kraków. The most significant global and local challenges for rehabilitative health services are: the increasing number of patients awaiting rehabilitation, the increasing waiting time for rehabilitation, and the decreasing number of medical specialists. A mobiREH rehabilitation system is a system that supports home based rehabilitation and helps resolve these problems. The system consists of (a) a mobile application, (b) wearable sensors for patients, and (c) a web-based platform for medical specialists

Slope Map of the Moon’s South Pole (85°S to Pole)

This map is based on data collected by the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter (LRO). The map shows slopes derived from the LOLA 10-m elevation product (NASA Goddard Space Flight Center; Smith et al., 2010; Smith et al., 2017). The slope is represented with four traditional colors 0° to 5° (bright green), 5° to 10° (dark green), 10° to 15° (yellow), and >15° (red). A second version of the map, with colors that may be attractive to those with color blindness, is also available: 0° to 5° (blue), 5° to 10° (darker blue), 10° to 15° (yellow), and >15° (red). The map covers the region from latitude 85°S to the pole on the rim of Shackleton crater. Slope data are overlain on a derived hillshade with solar azimuth 45°W and solar elevation 45°.A product of the Exploration Science Summer Intern Program: Harish, Venkata Satya Kumar Animireddi, Natasha Barrett, Sarah Boazman, Aleksandra Gawronska, Cosette Gilmour, Samuel Halim, Kathryn McCanaan, Jahnavi Shah, and David Kring.Version

Slope Map between Shackleton and de Gerlache Craters, Lunar South Pole

This map is based on data collected by the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter (LRO). The map shows slopes derived from the LOLA 5-m elevation product (NASA Goddard Space Flight Center; Smith et al., 2010; Smith et al., 2017). The slope is represented with four traditional colors 0° to 5° (bright green), 5° to 10° (dark green), 10° to 15° (yellow), and >15° (red). A second version of the map, with colors that may be attractive to those with color blindness, is also available: 0° to 5° (blue), 5° to 10° (darker blue), 10° to 15° (yellow), and >15° (red). The map covers the region between Shackleton and de Gerlache craters. Slope data are overlain on a derived hillshade with solar azimuth 45°W and solar elevation 45°.A product of the Exploration Science Summer Intern Program: Harish, Venkata Satya Kumar Animireddi, Natasha Barrett, Sarah Boazman, Aleksandra Gawronska, Cosette Gilmour, Samuel Halim, Kathryn McCanaan, Jahnavi Shah, and David Kring.Version

The Distribution and Accessibility of Geologic Targets near the Lunar South Pole and Candidate Artemis Landing Sites

Transformative lunar science will be driven by the accessibility, recovery, and return to Earth of geological specimens. Isolated boulders, rock exposures, and rocky craters at the lunar south pole all provide opportunities for geologic characterization and sampling of the lunar crust. Here, we present the results of orbital geological mapping of the region surrounding the south pole using Lunar Reconnaissance Orbiter Narrow Angle Camera images (0.5–2 m pixel−1). We mapped the distribution of isolated boulders (86,896), rocky craters (3556), and rock exposures (7553) around potential Artemis landing sites 001 and 004 (NASA 2020), which are within or near one of the Artemis III candidate landing regions. We found that boulder abundance decreases with increasing distance from the rim of Shackleton crater. From that correlation, we infer that most of the boulders and rock exposures near Shackleton were deposited as ejecta by the Shackleton impact, and by later the reworking of that material during smaller impact events. We additionally assessed the accessibility of the mapped features, and documented geologic targets located on shallow (<15°) slopes, including those on the Shackleton crater rim and on the "Connecting Ridge" between Shackleton and Henson crater. Such targets could be sampled by a future mission to the lunar south pole region. Our catalog of mapped features is made available to the lunar community

Topographic Contour Map of the Moon's South Pole Ridge

Lunar Reconnaissance Orbiter Lunar Orbiter Laser Altimeter (LOLA) 5-m elevation product over derived hillshade with solar azimuth 45° W and solar elevation 45°. High elevation: red and orange; Low elevation: purple and white

Slope Map of the Moon's South Pole Ridge

Lunar Reconnaissance Orbiter Lunar Orbiter Laser Altimeter (LOLA) 5-m elevation product over derived hillshade with solar azimuth 45° and solar elevation 45°. High elevation: red and orange; Low elevation: purple and white

Slope Map of the Moon’s South Pole (85°S to Pole)

This map is based on data collected by the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter (LRO). The map shows slopes derived from the LOLA 10-m elevation product (NASA Goddard Space Flight Center; Smith et al., 2010; Smith et al., 2017). The slope is represented with four traditional colors 0° to 5° (light green), 5° to 10° (bright green), 10° to 15° (dark green), 15° to 20° (yellow), and >20° (red). The map covers the region from latitude 85°S to the pole on the rim of Shackleton crater. Slope data are overlain on a derived hillshade with solar azimuth 45°W and solar elevation 45°.Center for Lunar Science and ExplorationA product of the Exploration Science Summer Intern Program: Harish, Venkata Satya Kumar Animireddi, Natasha Barrett, Sarah Boazman, Aleksandra Gawronska, Cosette Gilmour, Samuel Halim, Kathryn McCanaan, Jahnavi Shah, and David Kring

Slope Map between Shackleton and de Gerlache Craters, Lunar South Pole

This map is based on data collected by the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter (LRO). The map shows slopes derived from the LOLA 5-m elevation product (NASA Goddard Space Flight Center; Smith et al., 2010; Smith et al., 2017). The slope is represented with four traditional colors 0° to 5° (bright green), 5° to 10° (dark green), 10° to 15° (yellow), and >15° (red). A second version of the map, with colors that may be attractive to those with color blindness, is also available: 0° to 5° (blue), 5° to 10° (darker blue), 10° to 15° (yellow), and >15° (red). The map covers the region between Shackleton and de Gerlache craters. Slope data are overlain on a derived hillshade with solar azimuth 45°W and solar elevation 45°.A product of the Exploration Science Summer Intern Program: Harish, Venkata Satya Kumar Animireddi, Natasha Barrett, Sarah Boazman, Aleksandra Gawronska, Cosette Gilmour, Samuel Halim, Kathryn McCanaan, Jahnavi Shah, and David Kring.Version

Slope Map of the Moon's South Pole (85°S to Pole)

This map is based on data collected by the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter (LRO). The map shows slopes derived from the LOLA 10-m elevation product (NASA Goddard Space Flight Center; Smith et al., 2010; Smith et al., 2017). The slope is represented with four traditional colors 0° to 5° (bright green), 5° to 10° (dark green), 10° to 15° (yellow), and >15° (red). A second version of the map, with colors that may be attractive to those with color blindness, is also available: 0° to 5° (blue), 5° to 10° (darker blue), 10° to 15° (yellow), and >15° (red). The map covers the region from latitude 85°S to the pole on the rim of Shackleton crater. Slope data are overlain on a derived hillshade with solar azimuth 45°W and solar elevation 45°.A product of the Exploration Science Summer Intern Program: Harish, Venkata Satya Kumar Animireddi, Natasha Barrett, Sarah Boazman, Aleksandra Gawronska, Cosette Gilmour, Samuel Halim, Kathryn McCanaan, Jahnavi Shah, and David Kring.Version