000485890 001__ 485890 000485890 005__ 20250715180046.0 000485890 0247_ $$2doi$$a10.1016/j.actaastro.2022.05.024 000485890 0247_ $$2ISSN$$a0094-5765 000485890 0247_ $$2ISSN$$a1879-2030 000485890 0247_ $$2datacite_doi$$a10.3204/PUBDB-2022-06918 000485890 0247_ $$2altmetric$$aaltmetric:129422089 000485890 0247_ $$2WOS$$aWOS:000810036200005 000485890 0247_ $$2openalex$$aopenalex:W4281853378 000485890 037__ $$aPUBDB-2022-06918 000485890 041__ $$aEnglish 000485890 082__ $$a520 000485890 1001_ $$0P:(DE-HGF)0$$aBauer, Waldemar$$b0$$eCorresponding author 000485890 245__ $$aIn orbit testing of SOLID debris detector 000485890 260__ $$aAmsterdam [u.a.]$$bElsevier Science$$c2022 000485890 3367_ $$2DRIVER$$aarticle 000485890 3367_ $$2DataCite$$aOutput Types/Journal article 000485890 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1669196843_28613 000485890 3367_ $$2BibTeX$$aARTICLE 000485890 3367_ $$2ORCID$$aJOURNAL_ARTICLE 000485890 3367_ $$00$$2EndNote$$aJournal Article 000485890 520__ $$aThe number of artificial objects in space increases due to past and present space activities. To analyse the quantity of the small (diameter >100 μm up to cm) space debris and meteoroids, an innovative in-situ impact detection method has been developed at DLR (German Aerospace Center) in Bremen, Germany. The method Solar panel-based Impact Detector “SOLID” uses solar panels for impact detection. Since solar panels provide large detection areas and exist on nearly all satellites, this method enables for the collection of large amounts of data in different orbits. An impacting object generates a permanent damage on a panel. The damage can be determined during analysis scan as well as confirmed or refuted in the frame of subsequent scans of the panels. Those properties of the sensor system can significantly improve the amount as well as the quality of measurement data to be used for environmental model validation. The SOLID method was successfully verified on ground by Hypervelocity Impact (HVI) tests at Fraunhofer EMI, Freiburg, Germany. The ability of the detection method SOLID for impact detection of space debris and meteoroids was clearly demonstrated on ground. Since July 2017, the SOLID sensor system is placed in a 600 km Sun-synchronous orbit on the microsatellite mission TechnoSat of Technische Universität Berlin (TUB). Four solar panels equipped with SOLID technology are installed on the satellite for in-orbit testing and environmental exploration. The total detection area of all panels is about 0.0755 m$^2$. The system was designed to detect space debris or meteoroid objects with a diameter larger than 100 μm. In total 15,570,047 scans were performed over the four years in space. By means of measurement data changes were identified on one panel. However, so far, the telemetry data shows no clear evidence for an impact. 000485890 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0 000485890 588__ $$aDataset connected to CrossRef, Journals: bib-pubdb1.desy.de 000485890 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0 000485890 7001_ $$00000-0003-0401-5157$$aBraun, Vitali$$b1 000485890 7001_ $$0P:(DE-HGF)0$$aWerner, Philipp$$b2 000485890 7001_ $$aMontenegro, Sergio$$b3 000485890 7001_ $$0P:(DE-H253)PIP1091899$$aBarschke, Merlin$$b4 000485890 7001_ $$00000-0003-2287-2910$$aRomberg, Oliver$$b5 000485890 7001_ $$0P:(DE-HGF)0$$aDilger, Erik$$b6 000485890 773__ $$0PERI:(DE-600)2014614-0$$a10.1016/j.actaastro.2022.05.024$$gVol. 197, p. 235 - 245$$p235 - 245$$tActa astronautica$$v197$$x0094-5765$$y2022 000485890 8564_ $$uhttps://bib-pubdb1.desy.de/record/485890/files/1-s2.0-S009457652200220X-main.pdf$$yRestricted 000485890 8564_ $$uhttps://bib-pubdb1.desy.de/record/485890/files/ActaAstron.197%282022%29235.pdf$$yPublished on 2022-08-01. Available in OpenAccess from 2023-08-01. 000485890 8564_ $$uhttps://bib-pubdb1.desy.de/record/485890/files/1-s2.0-S009457652200220X-main.pdf?subformat=pdfa$$xpdfa$$yRestricted 000485890 8564_ $$uhttps://bib-pubdb1.desy.de/record/485890/files/ActaAstron.197%282022%29235.pdf?subformat=pdfa$$xpdfa$$yPublished on 2022-08-01. Available in OpenAccess from 2023-08-01. 000485890 909CO $$ooai:bib-pubdb1.desy.de:485890$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire 000485890 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1091899$$aDeutsches Elektronen-Synchrotron$$b4$$kDESY 000485890 9131_ $$0G:(DE-HGF)POF4-613$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vMatter and Radiation from the Universe$$x0 000485890 9141_ $$y2022 000485890 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)0160$$2StatID$$aDBCoverage$$bEssential Science Indicators$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)1160$$2StatID$$aDBCoverage$$bCurrent Contents - Engineering, Computing and Technology$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)0530$$2StatID$$aEmbargoed OpenAccess 000485890 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bACTA ASTRONAUT : 2019$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)0113$$2StatID$$aWoS$$bScience Citation Index Expanded$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)9900$$2StatID$$aIF < 5$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bASC$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2021-02-04 000485890 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2021-02-04 000485890 9201_ $$0I:(DE-H253)ZEU-EXP_AT-20120731$$kZEU-EXP/AT$$lAstroteilchenphysik$$x0 000485890 9201_ $$0I:(DE-H253)Z_GA-20210408$$kZ_GA$$lGammaastronomie$$x1 000485890 980__ $$ajournal 000485890 980__ $$aVDB 000485890 980__ $$aUNRESTRICTED 000485890 980__ $$aI:(DE-H253)ZEU-EXP_AT-20120731 000485890 980__ $$aI:(DE-H253)Z_GA-20210408 000485890 9801_ $$aFullTexts