Comet 1P/Halley multifluid MHD model for the Giotto fly-by

The interaction of comets with the solar wind has been the focus of many studies including numerical modeling. We compare the results of our multifluid MHD simulation of comet 1P/Halley to data obtained during the flyby of the European Space Agency's Giotto spacecraft in 1986. The model solves the full set of MHD equations for the individual fluids representing the solar wind protons, the cometary light and heavy ions, and the electrons. The mass loading, charge-exchange, dissociative ion-electron recombination, and collisional interactions between the fluids are taken into account. The computational domain spans over several million kilometers, and the close vicinity of the comet is resolved to the details of the magnetic cavity. The model is validated by comparison to the corresponding Giotto observations obtained by the Ion Mass Spectrometer, the Neutral Mass Spectrometer, the Giotto magnetometer experiment, and the Johnstone Plasma Analyzer instrument. The model shows the formation of the bow shock, the ion pile-up, and the diamagnetic cavity and is able to reproduce the observed temperature differences between the pick-up ion populations and the solar wind protons. We give an overview of the global interaction of the comet with the solar wind and then show the effects of the Lorentz force interaction between the different plasma populations.

Plasma environment of a weak comet – Predictions for Comet 67P/Churyumov–Gerasimenko from multifluid-MHD and Hybrid models

The interaction of a comet with the solar wind undergoes various stages as the comet’s activity varies along its orbit. For a comet like 67P/Churyumov–Gerasimenko, the target comet of ESA’s Rosetta mission, the various features include the formation of a Mach cone, the bow shock, and close to perihelion even a diamagnetic cavity. There are different approaches to simulate this complex interplay between the solar wind and the comet’s extended neutral gas coma which include magnetohydrodynamics (MHD) and hybrid-type models. The first treats the plasma as fluids (one fluid in basic single fluid MHD) and the latter treats the ions as individual particles under the influence of the local electric and magnetic fields. The electrons are treated as a charge-neutralizing fluid in both cases. Given the different approaches both models yield different results, in particular for a low production rate comet. In this paper we will show that these differences can be reduced when using a multifluid instead of a single-fluid MHD model and increase the resolution of the Hybrid model. We will show that some major features obtained with a hybrid type approach like the gyration of the cometary heavy ions and the formation of the Mach cone can be partially reproduced with the multifluid-type model.

Self-consistent multifluid MHD simulations of Europa's exospheric interaction with Jupiter's magnetosphere

The Jovian moon, Europa, hosts a thin neutral gas atmosphere, which is tightly coupled to Jupiter's magnetosphere. Magnetospheric ions impacting the surface sputter off neutral atoms, which, upon ionization, carry currents that modify the magnetic field around the moon. The magnetic field in the plasma is also affected by Europa's induced magnetic field. In this paper we investigate the environment of Europa using our multifluid MHD model and focus on the effects introduced by both the magnetospheric and the pickup ion populations. The model self-consistently derives the electron temperature that governs the electron impact ionization process, which is the major source of ionization in this environment. The resulting magnetic field is compared to measurements performed by the Galileo magnetometer, the bulk properties of the modeled thermal plasma population is compared to the Galileo Plasma Subsystem observations, and the modeled surface precipitation fluxes are compared to Galileo Ultraviolet Spectrometer observations. The model shows good agreement with the measured magnetic field and reproduces the basic features of the plasma interaction observed at the moon for both the E4 and the E26 flybys of the Galileo spacecraft. The simulation also produces perturbations asymmetric about the flow direction that account for observed asymmetries.

In vitro study to simulate the intracardiac magnetohydrodynamic effect

PURPOSE Blood flow causes induced voltages via the magnetohydrodynamic (MHD) effect distorting electrograms (EGMs) made during magnetic resonance imaging. To investigate the MHD effect in this context MHD voltages occurring inside the human heart were simulated in an in vitro model system inside a 1.5 T MR system. METHODS The model was developed to produce MHD signals similar to those produced by intracardiac flow and to acquire them using standard clinical equipment. Additionally, a new approach to estimate MHD distortions on intracardiac electrograms is proposed based on the analytical calculation of the MHD signal from MR phase contrast data. RESULTS The recorded MHD signals were similar in magnitude to intracardiac signals that would be measured by an electrogram of the left ventricle. The dependency of MHD signals on magnetic field strength and electrode separation was well reflected by an analytical model. MHD signals reconstructed from MR flow data were in excellent agreement with the MHD signal measured by clinical equipment. CONCLUSION The in vitro model allows investigation of MHD effects on intracardiac electrograms. A phase contrast MR scan was successfully applied to characterize and estimate the MHD distortion on intracardiac signals allowing correction of these effects. Magn Reson Med, 2014. © 2014 Wiley Periodicals, Inc.

Kinetic simulation of neutral∕ionized gas and electrically charged dust in the coma of comet 67P∕Churyumov-Gerasimenko

The cometary coma is a unique phenomenon in the solar system being a planetary atmosphere influenced by little or no gravity. As a comet approaches the sun, the water vapor with some fraction of other gases sublimate, generating a cloud of gas, ice and other refractory materials (rocky and organic dust) ejected from the surface of the nucleus. Sublimating gas molecules undergo frequent collisions and photochemical processes in the near‐nucleus region. Owing to its negligible gravity, comets produce a large and highly variable extensive dusty coma with a size much larger than the characteristic size of the cometary nucleus. The Rosetta spacecraft is en route to comet 67P/Churyumov‐Gerasimenko for a rendezvous, landing, and extensive orbital phase beginning in 2014. Both, interpretation of measurements and safety consideration of the spacecraft require modeling of the comet’s dusty gas environment. In this work we present results of a numerical study of multispecies gaseous and electrically charged dust environment of comet Chyuryumov‐Gerasimenko. Both, gas and dust phases of the coma are simulated kinetically. Photolytic reactions are taken into account. Parameters of the ambient plasma as well as the distribution of electric/magnetic fields are obtained from an MHD simulation [1] of the coma connected to the solar wind. Trajectories of ions and electrically charged dust grains are simulated by accounting for the Lorentz force and the nucleus gravity.

Modeled Interaction of Comet 67P/Churyumov-Gerasimenko with the Solar Wind Inside 2 AU

Periodic comets move around the Sun on elliptical orbits. As such comet 67P/Churyumov-Gerasimenko (hereafter 67P) spends a portion of time in the inner solar system where it is exposed to increased solar insolation. Therefore given the change in heliocentric distance, in case of 67P from aphelion at 5.68 AU to perihelion at ~1.24 AU, the comet’s activity—the production of neutral gas and dust—undergoes significant variations. As a consequence, during the inbound portion, the mass loading of the solar wind increases and extends to larger spatial scales. This paper investigates how this interaction changes the character of the plasma environment of the comet by means of multifluid MHD simulations. The multifluid MHD model is capable of separating the dynamics of the solar wind ions and the pick-up ions created through photoionization and electron impact ionization in the coma of the comet. We show how two of the major boundaries, the bow shock and the diamagnetic cavity, form and develop as the comet moves through the inner solar system. Likewise for 67P, although most likely shifted back in time with respect to perihelion passage, this process is reversed on the outbound portion of the orbit. The presented model herein is able to reproduce some of the key features previously only accessible to particle-based models that take full account of the ions’ gyration. The results shown herein are in decent agreement to these hybrid-type kinetic simulations.

Detection of Malnutrition in Patients Undergoing Maintenance Haemodialysis: A Quantitative Data Analysis on 12 Parameters

Background Protein-energy-malnutrition (PEM) is common in people with end stage kidney disease (ESKD) undergoing maintenance haemodialysis (MHD) and correlates strongly with mortality. To this day, there is no gold standard for detecting PEM in patients on MHD. Aim of Study The aim of this study was to evaluate if Nutritional Risk Screening 2002 (NRS-2002), handgrip strength measurement, mid-upper arm muscle area (MUAMA), triceps skin fold measurement (TSF), serum albumin, normalised protein catabolic rate (nPCR), Kt/V and eKt/V, dry body weight, body mass index (BMI), age and time since start on MHD are relevant for assessing PEM in patients on MHD. Methods The predictive value of the selected parameters on mortality and mortality or weight loss of more than 5% was assessed. Quantitative data analysis of the 12 parameters in the same patients on MHD in autumn 2009 (n = 64) and spring 2011 (n = 40) with paired statistical analysis and multivariate logistic regression analysis was performed. Results Paired data analysis showed significant reduction of dry body weight, BMI and nPCR. Kt/Vtot did not change, eKt/v and hand grip strength measurements were significantly higher in spring 2011. No changes were detected in TSF, serum albumin, NRS-2002 and MUAMA. Serum albumin was shown to be the only predictor of death and of the combined endpoint “death or weight loss of more than 5%”. Conclusion We now screen patients biannually for serum albumin, nPCR, Kt/V, handgrip measurement of the shunt-free arm, dry body weight, age and time since initiation of MHD.

Una bella roba. ‘Novellare’ als Erzählkonzept in Boccaccios ›Decameron‹

Der narrative Entwurf von Boccaccios ›Decameron‹ und Boccaccios theoretische Reflexionen über das Erzählen stehen klar im Fluchtpunkt der horazischen Lehre des prodesse et delectare. Vor diesem Horizont entwickelt Boccaccio sein Konzept des novellare, das einerseits ein ‚Wiedererzählen’ (analog zu mhd. erniuwen) beinhaltet und andererseits zu einer neuen Autonomie des Erzählens vorstößt. Beobachten lässt sich dieser Vorgang des Erneuerns weniger in Boccaccios theoretischen Ausführungen (etwa im Schlusswort des ›Decameron‹ oder in den ›Genealogie deorum gentilium‹) als in seiner dichterischen Praxis. Als Schlüsseltext wird im Vortrag die Novelle von der duldsamen Griselda herangezogen, die das ›Decameron‹ beschließt und die mit den Worten una bella roba endet. Das ‚schöne Kleid’ ist einerseits traditionelle Dichtungsmetapher (im Horizont des investire bzw. integumentum), andererseits intradiegetischer Bestandteil des Erzähl-‚Stoffs’ der Novelle. Bei Boccaccio dürfte das Gewand der Griselda, zusammen mit deren wiederholt thematisierter Nacktheit, dazu dienen, eine in die Novelle verpackte stoische Lehre zu vergegenwärtigen, diese in eine Erzählung ‚einzukleiden’. Das Kleid der Griselda wird so zur ‚Pathosformel’ (in der Begrifflichkeit A. Warburgs) bzw. zum ‚Faltenwurf’ (in der Begrifflichkeit G. Didi-Hubermans), mithin zur Verkörperung eines ‚neuen Erzählens’, das sich (im Gegensatz etwa zu Dante) von metaphysischen Entwürfen emanzipiert und in der Autonomie sprachlicher Kunstfertigkeit, bis an die Grenzen des Erzählbaren gehend und didaktische Ansprüche überwindend, die Möglichkeiten literarischer Darstellung ausreizt. Von den Zeitgenossen wurde dieses Experiment zwar wahrgenommen, in seinen Dimensionen aber nur ansatzweise erkannt. Symptomatisch für diese Form der Rezeption ist Petrarcas lateinische Übersetzung der ›Griselda‹-Novelle (›Seniles‹, XVII,3), wobei der Verfasser – seinerseits die Kleidermetaphorik bemühend – das Übersetzen als ein stilo alio retexere auffasst und seine Version den (wohl vorwiegend männlich intendierten Lesern) als auf Gott hin orientierte Lehre anempfiehlt: ut legentes ad imitandam saltem femine constantiam excitarem, ut [...] hoc prestare Deo nostro audeant. Diese Rückführung von Boccaccios erzählerischem Wagnis ins Didaktische zeigt sich auch in der Rezeption von Petrarcas Übersetzung, durch welche die Novelle im Europa des 14. und 15. Jahrhunderts weite Verbreitung fand: In einer der Haupthandschriften von Chaucers ›Canterbury Tales‹, dem Hengwrt Manuscript (Aberystwyth, National Library of Wales), wird die auf der ›Griselda‹-Novelle aufbauende Erzählung des Scholaren (›The Clerk’s Tale‹) mit Bestandteilen aus Petrarcas Übersetzung glossiert; in einer Handschrift aus dem Besitz des Nürnberger Humanisten Hartmann Schedel (München, Bayerische Staatsbibliothek, Clm 504) wird Petrarcas Konzept des stilo alio retexere erläutert als: claram facere, nudare [...], aperire, wobei hier die in Boccaccios Novelle intradiegetisch enthaltene Spannung von ‚Einkleidung’ und ‚Nacktheit’ auf einer lehrhaften Ebene fortwirkt.