TY - GEN A1 - Quarmby, Andrew A1 - Mönnig, Jamal A1 - Mugele, Hendrik A1 - Henschke, Jakob A1 - Kim, MyoungHwee A1 - Cassel, Michael A1 - Engel, Tilman T1 - Biomechanics and lower limb function are altered in athletes and runners with achilles tendinopathy compared with healthy controls: A systematic review T2 - Zweitveröffentlichungen der Universität Potsdam : Humanwissenschaftliche Reihe N2 - Achilles tendinopathy (AT) is a debilitating injury in athletes, especially for those engaged in repetitive stretch-shortening cycle activities. Clinical risk factors are numerous, but it has been suggested that altered biomechanics might be associated with AT. No systematic review has been conducted investigating these biomechanical alterations in specifically athletic populations. Therefore, the aim of this systematic review was to compare the lower-limb biomechanics of athletes with AT to athletically matched asymptomatic controls. Databases were searched for relevant studies investigating biomechanics during gait activities and other motor tasks such as hopping, isolated strength tasks, and reflex responses. Inclusion criteria for studies were an AT diagnosis in at least one group, cross-sectional or prospective data, at least one outcome comparing biomechanical data between an AT and healthy group, and athletic populations. Studies were excluded if patients had Achilles tendon rupture/surgery, participants reported injuries other than AT, and when only within-subject data was available.. Effect sizes (Cohen's d) with 95% confidence intervals were calculated for relevant outcomes. The initial search yielded 4,442 studies. After screening, twenty studies (775 total participants) were synthesised, reporting on a wide range of biomechanical outcomes. Females were under-represented and patients in the AT group were three years older on average. Biomechanical alterations were identified in some studies during running, hopping, jumping, strength tasks and reflex activity. Equally, several biomechanical variables studied were not associated with AT in included studies, indicating a conflicting picture. Kinematics in AT patients appeared to be altered in the lower limb, potentially indicating a pattern of “medial collapse”. Muscular activity of the calf and hips was different between groups, whereby AT patients exhibited greater calf electromyographic amplitudes despite lower plantar flexor strength. Overall, dynamic maximal strength of the plantar flexors, and isometric strength of the hips might be reduced in the AT group. This systematic review reports on several biomechanical alterations in athletes with AT. With further research, these factors could potentially form treatment targets for clinicians, although clinical approaches should take other contributing health factors into account. The studies included were of low quality, and currently no solid conclusions can be drawn. T3 - Zweitveröffentlichungen der Universität Potsdam : Humanwissenschaftliche Reihe - 830 KW - achilles tendinopathy KW - biomechanics KW - neuromuscular KW - kinetics KW - electromyography KW - athletes KW - runners KW - kinematics Y1 - 2023 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-587603 SN - 1866-8364 IS - 830 ER - TY - JOUR A1 - Quarmby, Andrew A1 - Mönnig, Jamal A1 - Mugele, Hendrik A1 - Henschke, Jakob A1 - Kim, MyoungHwee A1 - Cassel, Michael A1 - Engel, Tilman T1 - Biomechanics and lower limb function are altered in athletes and runners with achilles tendinopathy compared with healthy controls: A systematic review JF - Frontiers in Sports and Active Living N2 - Achilles tendinopathy (AT) is a debilitating injury in athletes, especially for those engaged in repetitive stretch-shortening cycle activities. Clinical risk factors are numerous, but it has been suggested that altered biomechanics might be associated with AT. No systematic review has been conducted investigating these biomechanical alterations in specifically athletic populations. Therefore, the aim of this systematic review was to compare the lower-limb biomechanics of athletes with AT to athletically matched asymptomatic controls. Databases were searched for relevant studies investigating biomechanics during gait activities and other motor tasks such as hopping, isolated strength tasks, and reflex responses. Inclusion criteria for studies were an AT diagnosis in at least one group, cross-sectional or prospective data, at least one outcome comparing biomechanical data between an AT and healthy group, and athletic populations. Studies were excluded if patients had Achilles tendon rupture/surgery, participants reported injuries other than AT, and when only within-subject data was available.. Effect sizes (Cohen's d) with 95% confidence intervals were calculated for relevant outcomes. The initial search yielded 4,442 studies. After screening, twenty studies (775 total participants) were synthesised, reporting on a wide range of biomechanical outcomes. Females were under-represented and patients in the AT group were three years older on average. Biomechanical alterations were identified in some studies during running, hopping, jumping, strength tasks and reflex activity. Equally, several biomechanical variables studied were not associated with AT in included studies, indicating a conflicting picture. Kinematics in AT patients appeared to be altered in the lower limb, potentially indicating a pattern of “medial collapse”. Muscular activity of the calf and hips was different between groups, whereby AT patients exhibited greater calf electromyographic amplitudes despite lower plantar flexor strength. Overall, dynamic maximal strength of the plantar flexors, and isometric strength of the hips might be reduced in the AT group. This systematic review reports on several biomechanical alterations in athletes with AT. With further research, these factors could potentially form treatment targets for clinicians, although clinical approaches should take other contributing health factors into account. The studies included were of low quality, and currently no solid conclusions can be drawn. KW - achilles tendinopathy KW - biomechanics KW - neuromuscular KW - kinetics KW - electromyography KW - athletes KW - runners KW - kinematics Y1 - 2023 U6 - https://doi.org/10.3389/fspor.2022.1012471 SN - 2624-9367 PB - Frontiers CY - Lausanne, Schweiz ER - TY - JOUR A1 - Olas, Justyna Jadwiga A1 - Fichtner, Franziska A1 - Apelt, Federico T1 - All roads lead to growth BT - imaging-based and biochemical methods to measure plant growth JF - Journal of experimental botany N2 - Plant growth is a highly complex biological process that involves innumerable interconnected biochemical and signalling pathways. Many different techniques have been developed to measure growth, unravel the various processes that contribute to plant growth, and understand how a complex interaction between genotype and environment determines the growth phenotype. Despite this complexity, the term 'growth' is often simplified by researchers; depending on the method used for quantification, growth is viewed as an increase in plant or organ size, a change in cell architecture, or an increase in structural biomass. In this review, we summarise the cellular and molecular mechanisms underlying plant growth, highlight state-of-the-art imaging and non-imaging-based techniques to quantitatively measure growth, including a discussion of their advantages and drawbacks, and suggest a terminology for growth rates depending on the type of technique used. KW - biomass KW - growth KW - imaging KW - kinematics KW - morphometrics KW - phenomics KW - phenotyping KW - relative expansion rate of growth (RER) KW - relative growth KW - rate (RGR) Y1 - 2019 U6 - https://doi.org/10.1093/jxb/erz406 SN - 0022-0957 SN - 1460-2431 VL - 71 IS - 1 SP - 11 EP - 21 PB - Oxford Univ. Press CY - Oxford ER - TY - THES A1 - Mitzkus, Martin T1 - Spectroscopic surface brightness fluctuations T1 - Spektroskopische Flächenhelligkeitsfluktuationen BT - probing bright evolved stars in unresolved stellar populations BT - Untersuchung von hellen, entwickelten Sternen in unaufgelösten stellaren Populationen N2 - Galaxies evolve on cosmological timescales and to study this evolution we can either study the stellar populations, tracing the star formation and chemical enrichment, or the dynamics, tracing interactions and mergers of galaxies as well as accretion. In the last decades this field has become one of the most active research areas in modern astrophysics and especially the use of integral field spectrographs furthered our understanding. This work is based on data of NGC 5102 obtained with the panoramic integral field spectrograph MUSE. The data are analysed with two separate and complementary approaches: In the first part, standard methods are used to measure the kinematics and than model the gravitational potential using these exceptionally high-quality data. In the second part I develop the new method of surface brightness fluctuation spectroscopy and quantitatively explore its potential to investigate the bright evolved stellar population. Measuring the kinematics of NGC 5102 I discover that this low-luminosity S0 galaxy hosts two counter rotating discs. The more central stellar component co-rotates with the large amount of HI gas. Investigating the populations I find strong central age and metallicity gradients with a younger and more metal rich central population. The spectral resolution of MUSE does not allow to connect these population gradients with the two counter rotating discs. The kinematic measurements are modelled with Jeans anisotropic models to infer the gravitational potential of NGC 5102. Under the self-consistent mass-follows-light assumption none of the Jeans models is able to reproduce the observed kinematics. To my knowledge this is the strongest evidence evidence for a dark matter dominated system obtained with this approach so far. Including a Navarro, Frenk & White dark matter halo immediately solves the discrepancies. A very robust result is the logarithmic slope of the total matter density. For this low-mass galaxy I find a value of -1.75 +- 0.04, shallower than an isothermal halo and even shallower than published values for more massive galaxies. This confirms a tentative relation between total mass slope and stellar mass of galaxies. The Surface Brightness Fluctuation (SBF) method is a well established distance measure, but due to its sensitive to bright stars also used to study evolved stars in unresolved stellar populations. The wide-field spectrograph MUSE offers the possibility to apply this technique for the first time to spectroscopic data. In this thesis I develop the spectroscopic SBF technique and measure the first SBF spectrum of any galaxy. I discuss the challenges for measuring SBF spectra that rise due to the complexity of integral field spectrographs compared to imaging instruments. Since decades, stellar population models indicate that SBFs in intermediate-to-old stellar systems are dominated by red giant branch and asymptotic giant branch stars. Especially the later carry significant model uncertainties, making these stars a scientifically interesting target. Comparing the NGC 5102 SBF spectrum with stellar spectra I show for the first time that M-type giants cause the fluctuations. Stellar evolution models suggest that also carbon rich thermally pulsating asymptotic giant branch stars should leave a detectable signal in the SBF spectrum. I cannot detect a significant contribution from these stars in the NGC 5102 SBF spectrum. I have written a stellar population synthesis tool that predicts for the first time SBF spectra. I compute two sets of population models: based on observed and on theoretical stellar spectra. In comparing the two models I find that the models based on observed spectra predict weaker molecular features. The comparison with the NGC 5102 spectrum reveals that these models are in better agreement with the data. N2 - Galaxien entwickeln sich auf kosmischen Zeitskalen. Um diese Entwicklung zu untersuchen und zu verstehen benutzen wir zwei verschiedene Methoden: Die Analyse der stellaren Population in Galaxien gibt Auskunft über die Sternentstehungsgeschichte und die Erzeugung von schweren Elementen. Die Analyse der Bewegung der Sterne gibt Auskunft über die dynamische Entwicklung, Interaktionen und Kollisionen von Galaxien, sowie die Akkretion von Gas. Die Untersuchung der Galaxienentwicklung ist in den letzten Jahrzehnten zu einem der wichtigsten Bereiche in der modernen Astrophysik geworden und die Einführung der Integral-Feldspektroskopie hat viel zu unserem heutigen Verständnis beigetragen. Die Grundlage dieser Arbeit bilden Spektren von der Galaxie NGC 5102. Die Spektren wurden mit dem Integral-Feldspektrographen MUSE aufgenommen, welcher sich durch ein groß es Gesichtsfeld auszeichnet. Die Daten werden mit zwei unterschiedlichen und sich ergänzenden Methoden analysiert: Im ersten Teil der Arbeit benutze ich etablierte Methoden um die Bewegung der Sterne zu vermessen und daraus das Gravitationspotential der Galaxie abzuleiten. Dieser Teil der Arbeit profitiert insbesondere von der ausgezeichneten Datenqualität. Im zweiten Teil der Arbeit entwickle ich erstmalig eine Methode für die Datenanalyse zur Extraktion von spektroskopischen Flächenhelligkeitsfluktuationen und quantifiziere deren Potential für die Untersuchung der hellen und entwickelten Sterne in Galaxien. Durch die Analyse der Bewegung der Sterne in NGC 5102 habe ich entdeckt, dass diese S0 Galaxie aus zwei entgegengesetzt rotierenden Scheiben besteht. Durch die Kombination von meinen Ergebnissen mit publizierten Messungen der Rotation des HI Gases finde ich, dass dieses in die gleiche Richtung rotiert wie die innere Scheibe. Die Analyse der stellaren Population zeigt starke Gradienten im mittleren Alter und der mittleren Metallizität. Dabei ist die stellare Population im Zentrum jünger und hat eine höhere Metallizität. Die spektrale Auflösung von MUSE reicht nicht aus, um zu untersuchen, ob diese Gradienten in der Population mit den beiden entgegengesetzt rotierenden Scheiben verbunden sind. Um das Gravitationspotential von NGC 5102 zu untersuchen, modelliere ich die gemessene Kinematik mit anisotropen Jeans Modellen. Keines der Modelle in dem ich annehme, dass die Massenverteilung der Verteilung des Lichts folgt, ist in der Lage die gemessene Kinematik zu reproduzieren. Nach meinem Wissen ist dies der bislang stärkste Hinweis auf Dunkle Materie, der mit dieser Methode in einer einzelnen Galaxie bisher erzielt worden ist. Durch das Hinzufügen einer sphärischen Dunkle Materie Komponente in Form eines Navarro, Frenk & White Halos kann die Diskrepanz zwischen Beobachtung und Modell gelöst werden. Fast modelunabhängig lässt sich die Steigung des logarithmischen Dichteprofils der gesamten (sichtbare und dunkle) Materie messen. In dieser massearmen Galaxie finde ich einen Wert von -1.75 +- 0.04. Diese Steigung ist flacher als die eines isotermen Dichteprofils und noch flacher als die Steigungen die für massereiche Galaxien veröffentlicht wurden. Diese Ergebnisse bestätigen eine bisher nur angedeutete Korrelation zwischen der Steigung des Dichteprofils und der stellaren Masse. Flächenhelligkeitsfluktuationen (Surface Brightness Fluctuations, SBF) sind eine etablierte Methode zur Entfernungsbestimmung von Galaxien. SBF werden von den hellsten Sternen in einer Population verursacht und werden daher auch benutzt, um diese Sterne zu untersuchen. MUSE zeichnet sich durch die einmalige Kombination von einem groß en Gesichtsfeld, mit einem guten räumlichen Sampling, und einer spektroskopischen Zerlegung des Lichts über das gesamte Gesichtsfeld aus. Dadurch kann die SBF Methode erstmalig auf Spektren angewendet werden. In dieser Arbeit entwickle ich die Methode der spektroskopischen SBF und messe das erste SBF Spektrum von einer Galaxie. Dabei diskutiere ich insbesondere die Herausforderungen die sich durch die Komplexität von Integral-Feldspektrographen verglichen mit bildgebenden Instrumenten für die SBF Methode ergeben. Seit langem sagen stellare Populationsmodelle voraus, dass die SBF in stellaren Populationen, die älter als etwa 0.5 Gyr sind, von Sternen auf dem roten und dem asymptotischen Riesenast erzeugt werden. Dabei ist insbesondere die Modellierung von Sternen des asymptotischen Riesenastes schwierig, weshalb diese wissenschaftlich besonders interessant sind. Der Vergleich des gemessenen SBF Spektrums von NGC 5102 mit Spektren von Riesensternen zeigt, dass das SBF Spektrum von Sternen mit dem Spektraltyp M dominiert wird. Nach allen Standardmodellen der stellaren Entwicklung sollten auch kohlenstoffreiche Riesensterne vom Spektraltyp C im SBF Spektrum sichtbar sein. Zu dem gemessenen SBF Spektrum tragen diese Sterne aber nicht signifikant bei. Ich habe eine stellar population synthesis Software geschrieben, die zum ersten Mal auch SBF Spektrenmodelle berechnet. Mit dieser Software habe ich zwei verschiedene Versionen von Modellen berechnet: die eine basiert auf beobachteten Sternspektren, die andere auf theoretischen Modellen von Sternspektren. Die Version der SBF Modellspektren, die auf den beobachteten Sternspektren beruht, zeigt schwächere molekulare Absorptionsbanden. Der Vergleich mit dem SBF Spektrum von NGC 5102 zeigt, dass diese Modelle besser zu den Daten passen. KW - galaxy KW - kinematics KW - stellar population KW - Galaxien KW - Kinematik KW - stellare Population Y1 - 2017 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-406327 ER - TY - JOUR A1 - Henschke, Jakob A1 - Kaplick, Hannes A1 - Wochatz, Monique A1 - Engel, Tilman T1 - Assessing the validity of inertial measurement units for shoulder kinematics using a commercial sensor-software system BT - a validation study JF - Health science reports N2 - Background and Aims Wearable inertial sensors may offer additional kinematic parameters of the shoulder compared to traditional instruments such as goniometers when elaborate and time-consuming data processing procedures are undertaken. However, in clinical practice simple-real time motion analysis is required to improve clinical reasoning. Therefore, the aim was to assess the criterion validity between a portable "off-the-shelf" sensor-software system (IMU) and optical motion (Mocap) for measuring kinematic parameters during active shoulder movements. Methods 24 healthy participants (9 female, 15 male, age 29 +/- 4 years, height 177 +/- 11 cm, weight 73 +/- 14 kg) were included. Range of motion (ROM), total range of motion (TROM), peak and mean angular velocity of both systems were assessed during simple (abduction/adduction, horizontal flexion/horizontal extension, vertical flexion/extension, and external/internal rotation) and complex shoulder movements. Criterion validity was determined using intraclass-correlation coefficients (ICC), root mean square error (RMSE) and Bland and Altmann analysis (bias; upper and lower limits of agreement). Results ROM and TROM analysis revealed inconsistent validity during simple (ICC: 0.040-0.733, RMSE: 9.7 degrees-20.3 degrees, bias: 1.2 degrees-50.7 degrees) and insufficient agreement during complex shoulder movements (ICC: 0.104-0.453, RMSE: 10.1 degrees-23.3 degrees, bias: 1.0 degrees-55.9 degrees). Peak angular velocity (ICC: 0.202-0.865, RMSE: 14.6 degrees/s-26.7 degrees/s, bias: 10.2 degrees/s-29.9 degrees/s) and mean angular velocity (ICC: 0.019-0.786, RMSE:6.1 degrees/s-34.2 degrees/s, bias: 1.6 degrees/s-27.8 degrees/s) were inconsistent. Conclusions The "off-the-shelf" sensor-software system showed overall insufficient agreement with the gold standard. Further development of commercial IMU-software-solutions may increase measurement accuracy and permit their integration into everyday clinical practice. KW - diagnostic techniques and procedures KW - kinematics KW - shoulder joint KW - validation study KW - wearable devices Y1 - 2022 U6 - https://doi.org/10.1002/hsr2.772 SN - 2398-8835 VL - 5 IS - 5 SP - 1 EP - 11 PB - Wiley CY - Hoboken ER - TY - GEN A1 - Henschke, Jakob A1 - Kaplick, Hannes A1 - Wochatz, Monique A1 - Engel, Tilman T1 - Assessing the validity of inertial measurement units for shoulder kinematics using a commercial sensor-software system T2 - Zweitveröffentlichungen der Universität Potsdam : Humanwissenschaftliche Reihe N2 - Background and Aims Wearable inertial sensors may offer additional kinematic parameters of the shoulder compared to traditional instruments such as goniometers when elaborate and time-consuming data processing procedures are undertaken. However, in clinical practice simple-real time motion analysis is required to improve clinical reasoning. Therefore, the aim was to assess the criterion validity between a portable "off-the-shelf" sensor-software system (IMU) and optical motion (Mocap) for measuring kinematic parameters during active shoulder movements. Methods 24 healthy participants (9 female, 15 male, age 29 +/- 4 years, height 177 +/- 11 cm, weight 73 +/- 14 kg) were included. Range of motion (ROM), total range of motion (TROM), peak and mean angular velocity of both systems were assessed during simple (abduction/adduction, horizontal flexion/horizontal extension, vertical flexion/extension, and external/internal rotation) and complex shoulder movements. Criterion validity was determined using intraclass-correlation coefficients (ICC), root mean square error (RMSE) and Bland and Altmann analysis (bias; upper and lower limits of agreement). Results ROM and TROM analysis revealed inconsistent validity during simple (ICC: 0.040-0.733, RMSE: 9.7 degrees-20.3 degrees, bias: 1.2 degrees-50.7 degrees) and insufficient agreement during complex shoulder movements (ICC: 0.104-0.453, RMSE: 10.1 degrees-23.3 degrees, bias: 1.0 degrees-55.9 degrees). Peak angular velocity (ICC: 0.202-0.865, RMSE: 14.6 degrees/s-26.7 degrees/s, bias: 10.2 degrees/s-29.9 degrees/s) and mean angular velocity (ICC: 0.019-0.786, RMSE:6.1 degrees/s-34.2 degrees/s, bias: 1.6 degrees/s-27.8 degrees/s) were inconsistent. Conclusions The "off-the-shelf" sensor-software system showed overall insufficient agreement with the gold standard. Further development of commercial IMU-software-solutions may increase measurement accuracy and permit their integration into everyday clinical practice. T3 - Zweitveröffentlichungen der Universität Potsdam : Humanwissenschaftliche Reihe - 809 KW - diagnostic techniques and procedures KW - kinematics KW - shoulder joint KW - validation study KW - wearable devices Y1 - 2023 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-578278 SN - 1866-8364 SP - 1 EP - 11 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - GEN A1 - Gianelli, Claudia A1 - Gentilucci, Maurizio T1 - Editorial: Reaching to Grasp Cognition: Analyzing Motor Behavior to Investigate Social Interactions T2 - Frontiers in psychology KW - kinematics KW - social cognition KW - action observation KW - imitation KW - joint action KW - complementary actions KW - cooperation and competition KW - embodied cognition Y1 - 2018 U6 - https://doi.org/10.3389/fpsyg.2018.01236 SN - 1664-1078 VL - 9 PB - Frontiers Research Foundation CY - Lausanne ER -