@article{VollmerMoellmann2011, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter}, title = {High Speed - Slow Motion: Technik digitaler Hochgeschwindigkeitskameras}, series = {In: Physik in unserer Zeit 42 (2011) 3, 144- 148}, journal = {In: Physik in unserer Zeit 42 (2011) 3, 144- 148}, doi = {10.1002/piuz.201101270}, pages = {144 -- 148}, year = {2011}, abstract = {Moderne Hochgeschwindigkeitskameras arbeiten digital. Ihre CMOS- oder CCD-Sensoren erm{\"o}glichen hohe Bildwiederholraten. Bei professionelleren Systemen l{\"a}sst sich dabei die Integrationszeit, also die Belichtungszeit der Einzelbilder, unabh{\"a}ngig von der Bildwiederholrate einstellen. F{\"u}r die hohe Aufnahmegeschwindigkeit sorgt ein zweistufiger Prozess. Ein sehr schneller interner Speicher nimmt die Bilddaten zuerst auf, dann schreibt eine Ausleseelektronik diese in einen externen Speicher. Neben teuren Profisystemen w{\"a}chst inzwischen das Segment an preiswerten Amateurkameras mit High-Speed-Option.}, language = {de} } @article{VollmerMoellmann2008, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter}, title = {Thermographie : Grundlagen, Forschung und moderne Anwendungen in Industrie und Technik}, series = {In: Praxis der Naturwissenschaften - Physik in der Schule 57 (2008) 8, 5-14}, journal = {In: Praxis der Naturwissenschaften - Physik in der Schule 57 (2008) 8, 5-14}, pages = {5 -- 14}, year = {2008}, language = {de} } @article{VollmerMoellmann2008, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter}, title = {Infrarotkameras: es gibt mehr zu sehen als unsere Augen wahrnehmen}, series = {In: Naturwissensschaftliche Rundschau 61 (2008) 11, 557—565}, journal = {In: Naturwissensschaftliche Rundschau 61 (2008) 11, 557—565}, pages = {557 -- 565}, year = {2008}, language = {de} } @article{VollmerMoellmannArnold2008, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter and Arnold, Frank}, title = {Ins eigene Segel blasen. M{\"u}nchhausen-Effekt und Schubumkehr}, series = {In: Physik in unserer Zeit 39 (2008) 5, 241-245}, journal = {In: Physik in unserer Zeit 39 (2008) 5, 241-245}, doi = {10.1002/piuz.200801172}, pages = {241 -- 245}, year = {2008}, abstract = {Kann man sich mit seinem Segelboot fortbewegen, indem man ins eigene Segel bl{\"a}st? Der Impulssatz erlaubt diesen an M{\"u}nchhausen erinnernden Effekt. Das demonstriert ein vereinfachtes Gedankenexperiment, bei dem der Segler durch den Werfer eines Balls und das Segel durch eine starre Wand ersetzt wird. Allerdings ergibt die naive Theorie, die Luftmolek{\"u}le als ball{\"a}hnliche Korpuskeln auffasst, einen zu hohen Impuls des reflektierten Luftstroms. Eine realistische Beschreibung liefert die moderne Str{\"o}mungstheorie. Ihre Resultate sind experimentell erfolgreich umsetzbar. Technisch angewendet wird das Prinzip in der Schubumkehr von Flugzeugtriebwerken.}, language = {de} } @article{VollmerMoellmannKarstaedt2004, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter and Karst{\"a}dt, Detlef}, title = {Microwave oven experiments with metals and light sources}, series = {In: Physics Education 39 (2004), 500-508}, journal = {In: Physics Education 39 (2004), 500-508}, pages = {500 -- 508}, year = {2004}, abstract = {Don't put metal objects in the microwave' is common safety advice. But why? Here we describe demonstration experiments involving placing household metallic objects in a microwave oven. These allow a better understanding of the interaction of microwaves with materials. Light bulbs and discharge lamps can also be used in instructive demonstrations.}, language = {en} } @article{VollmerMoellmannKarstaedt2004, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter and Karst{\"a}dt, Detlef}, title = {More experiments with microwave ovens}, series = {In: Physics education 39 (2004) 4, 346 - 351}, journal = {In: Physics education 39 (2004) 4, 346 - 351}, pages = {346 -- 351}, year = {2004}, abstract = {Microwave ovens can be used to perform exciting demonstrations that illustrate a variety of physics topics. Experiments discussed here show superheating, visualize the inhomogeneous heating that takes place in a microwave and also show how to use a mobile phone to detect radiation leaking from the oven. Finally eggs can give some spectacular (though messy) explosions. In all cases please note the safety advice given.}, language = {en} } @article{VollmerMoellmann2008, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter}, title = {Michelson Interferometer for your kitchen table}, series = {In: The Physics Teacher 46 (2008), 114-117}, journal = {In: The Physics Teacher 46 (2008), 114-117}, issn = {0031-921x}, pages = {114 -- 117}, year = {2008}, language = {en} } @article{VollmerMoellmannArnold2007, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter and Arnold, F.}, title = {Locomotion by blowing into the sail of a sailboat? From a basic physics question to thrust reversal of jet airplanes}, series = {In: Physics Education 42 (2007), 369-377}, journal = {In: Physics Education 42 (2007), 369-377}, issn = {0031-9120}, pages = {369 -- 377}, year = {2007}, language = {en} } @article{VollmerMoellmann2007, author = {Vollmer, Michael and M{\"o}llmann, Klaus-Peter}, title = {Infrared thermal imaging as a tool in university physics education}, series = {In: European Journal of Physics 28 (2007), S37-S50}, journal = {In: European Journal of Physics 28 (2007), S37-S50}, pages = {37 -- 50}, year = {2007}, language = {en} } @article{MoellmannVollmer2006, author = {M{\"o}llmann, Klaus-Peter and Vollmer, Michael}, title = {Measurements and predictions of the illuminance during a solar eclipse}, series = {In: European journal of physics 27 (2006), 1299-1314}, journal = {In: European journal of physics 27 (2006), 1299-1314}, pages = {1299 -- 1314}, year = {2006}, abstract = {Measurements of illuminance during a solar eclipse are presented. The data are compared to theoretical predictions, based on a geometrical model for obscuration. The model assumes a straight and uniform motion of the sun and moon as well as a spherical shape of both, i.e. it neglects any effects of limb darkening. Furthermore, the sun's disk is assumed to have homogeneous luminosity, i.e. any luminosity variations due to sun spots are neglected. Input parameters are the duration of the eclipse, the duration of totality, the impact parameter, i.e. the distance between the two trajectories of sun and moon, and the sizes of sun and moon. The model applies to all types of eclipses, partial, annular and total.}, language = {en} }