Departure of high temperature iron lines from the equilibrium state in flaring solar plasmas

The aim of this study is to clarify if the assumption of ionization equilibrium and a Maxwellian electron energy distribution is valid in flaring solar plasmas. We analyze the 2014 December 20 X1.8 flare, in which the \ion{Fe}{xxi} 187~\AA, \ion{Fe}{xxii} 253~\AA, \ion{Fe}{xxiii} 263~\AA\ and \ion{Fe}{xxiv} 255~\AA\ emission lines were simultaneously observed by the EUV Imaging Spectrometer onboard the Hinode satellite. Intensity ratios among these high temperature Fe lines are compared and departures from isothermal conditions and ionization equilibrium examined. Temperatures derived from intensity ratios involving these four lines show significant discrepancies at the flare footpoints in the impulsive phase, and at the looptop in the gradual phase. Among these, the temperature derived from the \ion{Fe}{xxii}/\ion{Fe}{xxiv} intensity ratio is the lowest, which cannot be explained if we assume a Maxwellian electron distribution and ionization equilibrium, even in the case of a multi-thermal structure. This result suggests that the assumption of ionization equilibrium and/or a Maxwellian electron energy distribution can be violated in evaporating solar plasma around 10MK.

Simulating the formation of a sigmoidal flux rope in AR10977 from SOHO/MDI magnetograms

The modeling technique of Mackay et al. is applied to simulate the coronal magnetic field of NOAA active region AR10977 over a seven day period (2007 December 2-10). The simulation is driven with a sequence of line-of-sight component magnetograms from SOHO/MDI and evolves the coronal magnetic field though a continuous series of non-linear force-free states. Upon comparison with Hinode/XRT observations, results show that the simulation reproduces many features of the active region's evolution. In particular, it describes the formation of a flux rope across the polarity inversion line during flux cancellation. The flux rope forms at the same location as an observed X-ray sigmoid. After five days of evolution, the free magnetic energy contained within the flux rope was found to be 3.9 × 1030 erg. This value is more than sufficient to account for the B1.4 GOES flare observed from the active region on 2007 December 7. At the time of the observed eruption, the flux rope was found to contain 20% of the active region flux. We conclude that the modeling technique proposed in Mackay et al.—which directly uses observed magnetograms to energize the coronal field—is a viable method to simulate the evolution of the coronal magnetic field.

Spontaneous Cirrhosis Regression in an IFN-beta-induced AIH-like Syndrome Following Drug Withdrawal: Art of Facts or Artifacts?

Autoimmune hepatitis (AIH) is a disease of unknown aetiology with drug-induced AIH being the most complex and not fully understood type. We present the case of a 57-year-old female patient with acute icteric hepatitis after interferon-beta-1b (IFNβ-1b) administration for multiple sclerosis (MS). Based on liver autoimmune serology, histology and appropriate exclusion of other liver diseases, a diagnosis of AIH-related cirrhosis was established. Following discontinuation of IFNβ-1b, a complete resolution of biochemical activity indices was observed and the patient remained untreated on her own decision. However, 3 years later, after a course of intravenous methylprednisolone for MS, a new acute transaminase flare was recorded which subsided again spontaneously after 3 weeks. Liver biopsy and elastography showed significant fibrosis regression (F2 fibrosis). To our knowledge, this is the first report showing spontaneous cirrhosis regression in an IFNβ-1b-induced AIH-like syndrome following drug withdrawal, suggesting that cirrhosis might be reversible if the offending fibrogenic stimulus is withdrawn.

Multiwavelength observations of the blazar 1ES 1011+496 in Spring 2008

The BL Lac object 1ES 1011+496 was discovered at Very High Energy (VHE, E>100GeV) γ-rays by MAGIC in spring 2007. Before that the source was little studied in different wavelengths. Therefore a multi-wavelength (MWL) campaign was organized in spring 2008. Along MAGIC, the MWL campaign included the Mets¨ahovi radio observatory, Bell and KVA optical telescopes and the Swift and AGILE satellites. MAGIC observations span from March to May, 2008 for a total of 27.9 hours, of which 19.4 hours remained after quality cuts. The light curve showed no significant variability yielding an integral flux above 200 GeV of (1.3 ± 0.3) × 10^(−11) photons cm^(−2) s^( −1) . The differential VHE spectrum could be described with a power-law function with a spectral index of 3.3 ± 0.4. Both results were similar to those obtained during the discovery. Swift XRT observations revealed an X-ray flare, characterized by a harder-when-brighter trend, as is typical for high synchrotron peak BL Lac objects (HBL). Strong optical variability was found during the campaign, but no conclusion on the connection between the optical and VHE γ-ray bands could be drawn. The contemporaneous SED shows a synchrotron dominated source, unlike concluded in previous work based on non-simultaneous data, and is well described by a standard one–zone synchrotron self–Compton model. We also performed a study on the source classification. While the optical and X-ray data taken during our campaign show typical characteristics of an HBL, we suggest, based on archival data, that 1ES 1011+496 is actually a borderline case between intermediate and high synchrotron peak frequency BL Lac objects.

Uveítes felinas : etiologia e abordagem clínica

Dissertação de Mestrado Integrado em Medicina Veterinária

"Lesion journey" nell'idrosadenite suppurativa: correlazione clinica e ultrasonografica

Introduzione: L'idrosadenite suppurativa (HS) è una malattia immuno-mediata che colpisce i follicoli piliferi situati principalmente nelle aree ricche di ghiandole apocrine. Materiali e metodi: È stato condotto uno studio osservazionale prospettico monocentrico finalizzato a correlare i parametri clinici ed ecografici con: l'evoluzione delle lesioni, la probabilità di riacutizzazione o di andare incontro ad un trattamento chirurgico/laser-CO2. Risultati: Sono stati reclutati sessantuno pazienti con un'età media pari a 29,5 ± 7,5 anni che presentavano un numero basale di 127 noduli infiammatori, 43 ascessi e 62 fistole. Dopo un tempo medio di 77,9 settimane, rispettivamente il 40%, 14%, 8% di noduli, ascessi e fistole erano guariti, il 5%, 30%, 29% persistevano privi di infiammazione, il 47%, 33%, 63 % presentava uno stato infiammatorio, e l'8% e il 23% dei noduli e degli ascessi erano evoluti in fistole. Sono stati registrati 137 episodi di flare nelle lesioni acute (noduli + ascessi) e 54 nelle lesioni croniche (fistole), mentre il numero di interventi procedurali è stato rispettivamente pari a 59 e 50. I fattori predittivi associati ad un'evoluzione sfavorevole (stato infiammatorio o cronicizzazione) per ascessi e noduli sono stati: evidenza ecografica di frammenti piliferi intralesionali, elevato segnale Power Doppler (PD) ed edema all'ecografia, profondità della localizzazione ed interessamento genitale; i predittori associati alle fistole sono stati: profondità della localizzazione, edema e dimensioni della lesione. La probabilità che una lesione acuta venisse sottoposta ad un intervento procedurale è stata correlata a: età, presenza di frammenti piliferi, segnale PD, edema e profondità della localizzazione; per le fistole l'unico predittore indipendente è stato la dimensione. I predittori di riacutizzazione della patologia per ascessi e noduli sono stati: giovane età all'esordio, segnale PD, evidenza ecografica di frammenti follicolari, profondità della localizzazione e dimensioni; per le fistole i predittori sono stati: localizzazione ascellare, profondità della localizzazione, edema e dimensione.