CNN-based local features for navigation near an asteroid

This article addresses the challenge of vision-based proximity navigation in asteroid exploration missions and on-orbit servicing. Traditional feature extraction methods struggle with the significant appearance variations of asteroids due to limited scattered light. To overcome this, we propose a lightweight feature extractor specifically tailored for asteroid proximity navigation, designed to be robust to illumination changes and affine transformations. We compare and evaluate state-of-the-art feature extraction networks and three lightweight network architectures in the asteroid context. Our proposed feature extractors and their evaluation leverages both synthetic images and real-world data from missions such as NEAR Shoemaker, Hayabusa, Rosetta, and OSIRIS-REx. Our contributions include a trained feature extractor, incremental improvements over existing methods, and a pipeline for training domain-specific feature extractors. Experimental results demonstrate the effectiveness of our approach in achieving accurate navigation and localization. This work aims to advance the field of asteroid navigation and provides insights for future research in this domain

Hybrid simulations of the proton precipitation patterns onto the upper atmosphere of Mars

We study the dependence of proton precipitation patterns onto the Martian upper atmosphere on altitude, proton energy, proton origin, and in a lesser extent, solar zenith angle, using the HYB-Mars model, a 3D quasineutral hybrid model. We find that the flux of precipitating protons has a strong altitude dependence: on the dayside, the flux of precipitating protons decreases substantially when the altitude over Mars decreases. We also find that the contribution of exospheric protons to the deposition is significant and its spatial distribution is not identical to that of the solar wind protons. In addition, the low energy proton population comes mainly from the newborn planetary protons. The energized pick-up protons and solar wind protons contribute to the higher energy proton population. The study also confirms that the proton precipitation is highly asymmetric with respect to the direction of the convection electric field in the solar wind. The study implies that the Martian induced magnetosphere protects the upper atmosphere effectively against proton precipitation

Oxygen Ion Escape From Venus Is Modulated by Ultra‐Low Frequency Waves

We study the solar wind‐driven, nonthermal escape of O+ ions from Venus in a global hybrid simulation. In the model, a well‐developed ion foreshock forms ahead of the Venusian quasi‐parallel bow shock under nominal upstream conditions. Large‐scale magnetosonic ultra‐low frequency (ULF) waves at 20‐ to 30‐s period are excited and convect downstream along the foreshock with the solar wind. We show that the foreshock ULF waves transmit through the bow shock in the downstream region and interact with the planetary ion acceleration, causing 25% peak‐to‐peak fluctuations in the O+ escape rate. These results demonstrate the importance of upstream plasma waves on the energization and escape of heavy ions from the planetary atmospheres.Key PointsA global hybrid simulation predicts fluctuations in the O+ escape from VenusThe fluctuations are associated with the foreshock ULF waves, which modulate the acceleration of heavy pickup ionsUpstream waves need to be taken into account in the interpretation of heavy ion erosion from unmagnetized planetsPeer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/155962/1/grl60648_am.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/155962/2/grl60648-sup-0001-Figure_SI-S01.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/155962/3/grl60648.pd

Sympatric Ixodes-tick species : pattern of distribution and pathogen transmission within wild rodent populations

The generalist tick Ixodes ricinus is the most important vector for tick-borne pathogens (TBP), including Borrelia burgdorferi sensu lato, in Europe. However, the involvement of other sympatric Ixodes ticks, such as the specialist vole tick I. trianguliceps, in the enzootic circulations of TBP remains unclear. We studied the distribution of I. ricinus and I. trianguliceps in Central Finland and estimated the TBP infection likelihood in the most common rodent host in relation with the abundance of the two tick species. Ixodes trianguliceps was encountered in all 16 study sites whereas I. ricinus was frequently observed only at a quarter of the study sites. The abundance of I. ricinus was positively associated with open water coverage and human population density around the study sites. Borrelia burgdorferi s. l.-infected rodents were found only in sites where I. ricinus was abundant, whereas the occurrence of other TBP was independent of I. ricinus presence. These results suggest that I. trianguliceps is not sufficient, at least alone, in maintaining the circulation of B. burgdorferi s. l. in wild hosts. In addition, anthropogenic factors might affect the distribution of I. ricinus ticks and, hence, their pathogens, thus shaping the landscape of tick-borne disease risk for humans.Peer reviewe

A case study of proton precipitation at Mars:Mars Express observations and hybrid simulations

Using the data from the Analyzer of Space Plasma and Energetic Atoms (ASPERA-3) experiment on board Mars Express and hybrid simulations, we have investigated the entry of protons into the Martian induced magnetosphere. We discuss one orbit on the dayside with observations of significant proton fluxes at altitudes down to 260 km on 27 February 2004. The protons observed below the induced magnetosphere boundary at an altitude of less than 700 km have energies of a few keV, travel downward, and precipitate onto the atmosphere. The measured energy flux and particle flux are 10^8–10^9 eV cm^−2 s^−1 and 10^5–10^6 H^+ cm^−2 s^−1, respectively. The proton precipitation occurs because the Martian magnetosheath is small with respect to the heated proton gyroradius in the subsolar region. The data suggest that the precipitation is not permanent but may occur when there are transient increases in the magnetosheath proton temperature. The higher-energy protons penetrate deeper because of their larger gyroradii. The proton entry into the induced magnetosphere is simulated using a hybrid code. A simulation using a fast solar wind as input can reproduce the high energies of the observed precipitating protons. The model shows that the precipitating protons originate from both the solar wind and the planetary exosphere. The precipitation extends over a few thousand kilometers along the orbit of the spacecraft. The proton precipitation does not necessarily correlate with the crustal magnetic anomalies

Auroral imaging with combined Suomi 100 nanosatellite and ground-based observations: A case study

Auroras can be regarded as the most fascinating manifestation of space weather and they are continuously observed by ground-based and, nowadays more and more, also by space-based measurements. Investigations of auroras and geospace comprise the main research goals of the Suomi 100 nanosatellite, the first Finnish space research satellite, which has been measuring the Earth's ionosphere since its launch on Dec. 3, 2018. In this work, we present a case study where the satellite's camera observations of an aurora over Northern Europe are combined with ground-based observations of the same event. The analyzed image is, to the authors' best knowledge, the first auroral image ever taken by a cubesat. Our data analysis shows that a satellite vantage point provides complementary, novel information of such phenomena. The 3D auroral location reconstruction of the analyzed auroral event demonstrates how information from a 2D image can be used to provide location information of auroras under study. The location modelling also suggests that the Earth's limb direction, which was the case in the analyzed image, is an ideal direction to observe faint auroras. Although imaging on a small satellite has some large disadvantages compared with ground-based imaging (the camera cannot be repaired, a fast moving spinning satellite), the data analysis and modelling demonstrate how even a small 1-Unit (size: 10 cm x 10 cm x 10 cm) CubeSat and its camera, build using cheap commercial off-the-shelf components, can open new possibilities for auroral research, especially, when its measurements are combined with ground-based observations.Comment: Accepted manuscript 34 pages, 17 figure

12. Pääsuunnittelijakoulutuksen tutkielmat

Pääsuunnittelijakoulutus on suunnittelun ja johtamisen koulutusohjelma, jonka tavoitteena on tukea pääsuunnittelutehtävissä toimivien asiantuntijoiden edellytyksiä ja valmiuksia vastata tulevaisuuden osaamisvaatimuksiin. Julkaisu sisältää 12. pääsuunnittelijakoulutuksen tutkielmat: (1) Renni Haroma: Arkkitehdin vaikutusmahdollisuudet pääsuunnittelijana KVR-urakassa; tehtävät ja vastuut, sekä onnistuneen lopputuloksen varmistaminen (2) Pontus Högström: Rakennuttajan ja pääsuunnittelijan vastuut pienrakennushankkeessa (3) Outi Jääskeläinen: Pääsuunnittelija kunnallisessa rakennusinvestointihankkeessa (4) Tuomo Kallio: Tietomalli pääsuunnittelijan työkaluna - Muuttuvat ohjeet ja määräykset (5) Sami Karvinen: Rakennesuunnittelija pääsuunnittelijana - Tehtävän erityispiirteet (6) Pauli Koivisto: Pääsuunnittelijan tehtäviä korjausrakentamiskohteissa (7) Mika Kurth: Pääsuunnittelu tietomallihankkeessa - Pääsuunnittelijan, arkkitehdin ja tietomallikoordinaattorin roolit (8) Niklas Mahlberg: Kokemuksia yhteispohjoismaisesta rakennushankkeesta - Case: Teatteri- ja konserttitalo Kilden, Kristiansand, Norja (9) Joni Räisänen: Tietomallintaminen; haasteet ja mahdollisuudet - Tietomallintaminen pääsuunnittelijavetoisessa hankkeessa - Case: Alberga Business Park (10) Sebastian Rönnblad: Pääsuunnittelu tilaajan näkökulmasta (11) Esa Sallinen: Sosiaalinen toimilupa toimitilahankkeessa - vaikutukset pääsuunnittelijan rooliin (12) Kimmo Severinkangas: Pääsuunnittelijan ja rakentamiseen ryhtyvän tehtävä- ja vastuujako vesivoimalaitoksen rakennushankkeessa - Case: Suunnitteilla oleva Sierilän vesivoimalaitoshanke (13) Erki Valdre: Pääsuunnittelun riskienhallinta - Laatujärjestelmä riskienhallintavälineenä (14) Riitta Vesala: Verkostojohtamis- ja esimiestaidot pääsuunnittelijan tehtävässä

Radar—CubeSat Transionospheric HF Propagation Observations: Suomi 100 Satellite and EISCAT HF Facility

Radio waves provide a useful diagnostic tool to investigate the properties of the ionosphere because the ionosphere affects the transmission and properties of high frequency (HF) electromagnetic waves. We have conducted a transionospheric HF-propagation research campaign with a nanosatellite on a low-Earth polar orbit and the EISCAT HF transmitter facility in Tromsø, Norway, in December 2020. In the active measurement, the EISCAT HF facility transmitted sinusoidal 7.953 MHz signal which was received with the High frEquency rAdio spectRomEteR (HEARER) onboard 1 Unit (size: 10 × 10 × 10 cm) Suomi 100 space weather nanosatellite. Data analysis showed that the EISCAT HF signal was detected with the satellite's radio spectrometer when the satellite was the closest to the heater along its orbit. Part of the observed variations seen in the signal was identified to be related to the heater's antenna pattern and to the transmitted pulse shapes. Other observed variations can be related to the spatial and temporal variations of the ionosphere and its different responses to the used transmission frequencies and to the transmitted O- and X-wave modes. Some trends in the observed signal may also be associated to changes in the properties of ionospheric plasma resulting from the heater's electromagnetic wave energy. This paper is, to authors' best knowledge, the first observation of this kind of “self-absorption” measured from the transionospheric signal path from a powerful radio source on the ground to the satellite-borne receiver