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153. Correspondence

Author

Grande, M., Crocoli, A., Attinà, M. G., Nigro, C., Rulli, F., Milito, G., Rugolotto, S., Sun, M., Ball, T., Boucke, L., de Vries, M., Collins, E. E., Lund, J. N., and Semeraro, D.

Published
2007
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155. ESMO Guidelines: Cancer patient management during the COVID-19 pandemic

Author

Aapro, M., Addeo, A., Acierto, P., Balermpas, P., Berg, T., Berghoff, A., Betella, I., Blay, J. -Y., Bosetti, D. G., Bossi, P., Bouchaab, H., Brandt, J., Buske, C., Caraceni, A., Cardoso, F., Carles, J., Catanese, S., Cherny, N., Colombo, I., Colombo, N., Cortes, J., Criscitiello, C., Curigliano, G., de Azambuja, E., Delagoge, S., Del Grande, M., De Santis, M., Douillard, J. -Y., Dummer, R., Dziadziuszko, R., Escudier, B., Fizazi, K., Fleitas, T., Franceschi, E., Hoeller, C., Gillessen, S., Gonzalez Martin, A., Gralla, R., Grigorescu, A., Gronchi, A., Hassan, A., Hui, D., Jerkeman, M., Jones, R., Jordan, K., Keilholz, U., Kreye, G., Ledermann, J., Loibl, S., Lordick, F., Lorigan, P., Loriot, Y., Machiels, J. -P., Broto, J. M., Mei, U., Michielin, O., Mori, M., Multinu, F., Paluch-Shimon, S., Parker, C., Passaro, A., Pentheroudakis, G., Peters, S., Piazza, C., Porta, C., Powles, T., Preusser, M., Reck, M., Ripamonti, C., Rubach, M., Rukhadze, T., Schmidinger, M., Sensus-Konefka, E., Sessa, C., Shaulov, A., Stacchiotti, S., Stevens, A. -M., Stintzing, S., Szturz, P., Trapani, D., van Akkooi, A., Vecchione, L., van Bommel, F., Vogl, U., Von Garnier, C., Weller, M., Wood, J., Zaccarelli, E., and Zimmermann, C.

Published
2020

156. Is Cisterna Magna Width a Useful First-Trimester Marker of Aneuploidy?

Author

Pauta M, Grande M, Borobio V, Illanes C, Soler A, Nogué L, and Borrell A

Subjects
Posterior fossa, Cisterna magna, Down syndrome, First-trimester marker, Prenatal diagnosis, Aneuploidy, reproductive and urinary physiology
Abstract

OBJECTIVE: To assess whether the cisterna magna (CM) width measured in first-trimester fetuses is a useful marker for aneuploidy detection. METHODS: This was a prospective study in 2 different cohorts in a tertiary referral center. The first cohort comprised 913 fetuses from the general pregnancy population during the period 2012-2016 and was used to construct the CM reference ranges applying the ?-µ-s (LMS) method. The second cohort included 714 high-risk fetuses undergoing chorionic villus sampling during the period 2012-2016. Mean detection rates using the 95th percentile for CM width observed in chromosomal anomaly groups were compared with those obtained in chromosomally normal fetuses. RESULTS: The 50th percentile for CM ranged from 1.66 to 2.75 mm when crown-rump length (CRL) increased from 45 to 84 mm. Among high-risk fetuses, the following chromosomal anomalies were diagnosed in 125 (17%) fetuses: trisomy 21 (n = 63), trisomy 18 or 13 (n = 21), monosomy X (n = 9), submicroscopic anomalies (n = 11), and other anomalies (n = 22). The mean CM width for euploid fetuses was 2.4 mm (1.13 multiples of the median, MoM). While CM width was significantly increased in trisomy 21 (mean 2.7 mm; 1.23 MoM; p > 0.05), no differences were found in the other anomaly groups. Among the 63 fetuses with trisomy 21, a CM width above the 99th percentile was observed in 23 fetuses (37%). CONCLUSIONS: The new reference range for CM width at 11-13 weeks of gestation did not differ from previous studies. In first-trimester fetuses with trisomy 21, CM width appears to be increased, although its value as an ultrasound marker is limited, because of its detection rate of 37%.

Published
2020

157. IMF Direction Derived from Cycloid-Like Ion Distributions Observed by Mars Express

Author

Yamauchi, M., Futaana, Y., Fedorov, A., Dubinin, E., Lundin, R., Sauvaud, J.-A., Winningham, D., Frahm, R., Barabash, S., Holmstrom, M., Woch, J., Fraenz, M., Budnik, E., Borg, H., Sharber, J. R., Coates, A. J., Soobiah, Y., Koskinen, H., Kallio, E., Asamura, K., Hayakawa, H., Curtis, C., Hsieh, K. C., Sandel, B. R., Grande, M., Grigoriev, A., Wurz, P., Orsini, S., Brandt, P., Mckenna-Lawler, S., Kozyra, J., and Luhmann, J.

Published
2006
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158. The Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) for the Mars Express Mission

Author

Barabash, S., Lundin, R., Andersson, H., Brinkfeldt, K., Grigoriev, A., Gunell, H., Holmström, M., Yamauchi, M., Asamura, K., Bochsler, P., Wurz, P., Cerulli-Irelli, R., Mura, A., Milillo, A., Maggi, M., Orsini, S., Coates, A. J., Linder, D. R., Kataria, D. O., Curtis, C. C., Hsieh, K. C., Sandel, B. R., Frahm, R. A., Sharber, J. R., Winningham, J. D., Grande, M., Kallio, E., Koskinen, H., Riihelä, P., Schmidt, W., Säles, T., Kozyra, J. U., Krupp, N., Woch, J., Livi, S., Luhmann, J. G., McKenna-Lawlor, S., Roelof, E. C., Williams, D. J., Sauvaud, J.-A., Fedorov, A., and Thocaven, J.-J.

Published
2006
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159. Auroral Plasma Acceleration Above Martian Magnetic Anomalies

Author

Lundin, R., Winningham, D., Barabash, S., Frahm, R., Brain, D., Nilsson, H., Holmström, M., Yamauchi, M., Sharber, J. R., Sauvaud, J.-A., Fedorov, A., Asamura, K., Hayakawa, H., Coates, A. J., Soobiah, Y., Curtis, C., Hsieh, K. C., Grande, M., Koskinen, H., Kallio, E., Kozyra, J., Woch, J., Fraenz, M., Luhmann, J., Mckenna-Lawler, S., Orsini, S., Brandt, P., and Wurz, P.

Published
2006
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160. The Cassini CAPS Electron Spectrometer

Author

Linder, D. R., primary, Coates, A. J., additional, Woodliffe, R. D., additional, Alsop, C., additional, Johnstone, A. D., additional, Grande, M., additional, Preece, A., additional, Narheim, B., additional, and Young, D. T., additional

Published
2013
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161. Cassini Plasma Spectrometer Investigation

Author

Young, D. T., primary, Barraclough, B. L., additional, Berthelier, J. J., additional, Blanc, M., additional, Burch, J. L., additional, Coates, A. J., additional, Goldstein, R., additional, Grande, M., additional, Hill, T. W., additional, Illiano, J. M., additional, Johnson, M. A., additional, Johnson, R. E., additional, Baragiola, R. A., additional, Kelha, V., additional, Linder, D., additional, McComas, D. J., additional, Narheim, B. T., additional, Nordholt, J. E., additional, Preece, A., additional, Sittler, E. C., additional, Svenes, K. R., additional, Szalai, S., additional, Szegö, K., additional, Tanskanen, P., additional, and Viherkanto, K., additional

Published
2013
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165. The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission

Author

Barabash, S., Sauvaud, J.-A., Gunell, H., Andersson, H., Grigoriev, A., Brinkfeldt, K., Holmström, M., Lundin, R., Yamauchi, M., Asamura, K., Baumjohann, W., Zhang, T.L., Coates, A.J., Linder, D.R., Kataria, D.O., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Fedorov, A., Mazelle, C., Thocaven, J.-J., Grande, M., Koskinen, Hannu E.J., Kallio, E., Säles, T., Riihela, P., Kozyra, J., Krupp, N., Woch, J., Luhmann, J., McKenna-Lawlor, S., Orsini, S., Cerulli-Irelli, R., Mura, M., Milillo, M., Maggi, M., Roelof, E., Brandt, P., Russell, C.T., Szego, K., Winningham, J.D., Frahm, R.A., Scherrer, J., Sharber, J.R., Wurz, P., and Bochsler, P.

Published
2007
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166. The D-CIXS X-ray spectrometer on the SMART-1 mission to the Moon—First results

Author

Grande, M., Kellett, B.J., Howe, C., Perry, C.H., Swinyard, B., Dunkin, S., Huovelin, J., Alha, L., D’Uston, L.C., Maurice, S., Gasnault, O., Couturier-Doux, S., Barabash, S., Joy, K.H., Crawford, I.A., Lawrence, D., Fernandes, V., Casanova, I., Wieczorek, M., Thomas, N., Mall, U., Foing, B., Hughes, D., Alleyne, H., Russell, S., Grady, M., Lundin, R., Baker, D., Murray, C.D., Guest, J., and Christou, A.

Published
2007
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167. SMART-1 after lunar capture: First results and perspectives

Author

Foing, B. H., Racca, G. D., Marini, A., Evrard, E., Stagnaro, L., Almeida, M., Koschny, D., Frew, D., Zender, J., Heather, D., Grande, M., Huovelin, J., Keller, H. U., Nathues, A., Josset, J. L., Malkki, A., Schmidt, W., Noci, G., Birkl, R., Iess, L., Sodnik, Z., and McManamon, P.

Published
2005
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169. First ENA observations at Mars: solar-wind ENAs on the nightside

Author

Brinkfeldt, K., Gunell, H., Brandt, P. C:son, Barabash, S., Frahm, R.A., Winningham, J.D., Kallio, E., Holmstrom, M., Futaana, Y., Ekenback, A., Lundin, R., Andersson, H., Yamauchi, M., Grigoriev, A., Sharber, J.R., Scherrer, J.R., Coates, A.J., Linder, D.R., Kataria, D.O., Koskinen, H., Stiles, T., Riihela, P., Schmidt, W., Kozyra, J., Luhmann, J., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Mars (Planet) -- Observations, Magnetosphere -- Observations, Solar wind -- Observations, Astronomy, Earth sciences
Abstract

We present measurements with an Energetic Neutral Atom (ENA) imager on board Mars Express when the spacecraft moves into Mars eclipse. Solar wind ions charge exchange with the extended Mars exosphere to produce ENAs that can spread into the eclipse of Mars due to the ions' thermal spread. Our measurements show a lingering signal from the Sun direction for several minutes as the spacecraft moves into the eclipse. However, our ENA imager is also sensitive to UV photons and we compare the measurements to ENA simulations and a simplified model of UV scattering in the exosphere. Simulations and further comparisons with an electron spectrometer sensitive to photoelectrons generated when UV photons interact with the spacecraft suggest that what we are seeing in Mars' eclipse are ENAs from upstream of the bow shock produced in charge exchange with solar wind ions with a non-zero temperature. The measurements are a precursor to a new technique called ENA sounding to measure solar wind and planetary exosphere properties in the future. Keywords: Mars; Solar wind; Magnetospheres

Published
2006

170. First ENA observations at Mars: ENA emissions from the martian upper atmosphere

Author

Futaana, Y., Barabash, S., Grigoriev, A., Holmstrom, M., Kallio, E., Brandt, P. C:son, Gunell, H., Brinkfeldt, K., Lundin, R., Andersson, H., Yamauchi, M., McKenna-Lawler, S., Winningham, J.D., Frahm, R.A., Sharber, J.R., Scherrer, J.R., Coates, A.J., Linder, D.R., Kataria, D.O., Sales, T., Riihela, P., Schmidt, W., Koskinen, H., Kozyra, J., Luhmann, J., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Galli, A., Krupp, N., Woch, J., Franz, M., and Asamura, K. Dierker, C.

Subjects
Mars probes -- Observations, Mars (Planet) -- Atmosphere, Mars (Planet) -- Observations, Astronomy, Earth sciences
Abstract

The neutral particle detector (NPD) on board Mars Express has observed energetic neutral atoms (ENAs) from a broad region on the dayside of the martian upper atmosphere. We show one such example for which the observation was conducted at an altitude of 570 km, just above the induced magnetosphere boundary (IMB). The time of flight spectra of these ENAs show that they had energies of 0.2-2 keV/amu, with an average energy of ~1.1 keV/amu. Both the spatial distribution and the energy of these ENAs are consistent with the backscattered ENAs, produced by an ENA albedo process. This is the first observation of backscattered ENAs from the martian upper atmosphere. The origin of these ENAs is considered to be the solar wind ENAs that are scattered back by collision processes in the martian upper atmosphere. The particle flux and energy flux of the backscattered ENAs are 0.9-1.3 x [10.sup.7] [cm.sup.-2] [s.sup.-1] and ~9.5 x [10.sup.9] eV [cm.sup.-2] [s.sup.-l], respectively. Keywords: Mars, atmosphere; Solar wind; Atmospheres, dynamics; Atmospheres, structure; Ionospheres

Published
2006

171. Energetic neutral atoms (ENA) at Mars: properties of the hydrogen atoms produced upstream of the martian bow shock and implications for ENA sounding technique around non-magnetized planets

Author

Kallio, E., Barabash, S., Brinkfeldt, K., Gunell, H., Holmstrom, M., Futaana, Y., Schmidt, W., Sales, T., Koskinen, H., Riihela, P., Lundin, R., Andersson, H., Yamauchi, M., Grigoriev, A., Winningham, J.D., Frahm, R.A., Sharber, J.R., Scherrer, J.R., Coates, A.J., Linder, D.R., Kataria, D.O., Kozyra, J., Luhmann, J.G., Roelof, E., Williams, D., Livi, S., Brandt, P. C:son, Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Monte Carlo method -- Usage, Hydrogen bonding -- Properties, Mars (Planet) -- Atmosphere, Mars (Planet) -- Observations, Astronomy, Earth sciences
Abstract

We have studied the interaction of fast solar wind hydrogen atoms with the martian atmosphere by a three-dimensional Monte Carlo simulation. These energetic neutral hydrogen atoms, H-ENAs, are formed upstream of the martian bow shock. Both H-ENAs scattered and non-scattered from the martian atmosphere/exosphere were studied. The colliding H-ENAs were found to scatter both to the dayside and nightside. On the dayside they contribute to the so-called H-ENA albedo. On the nightside the heated and scattered hydrogen atoms were found also in the martian wake. The density, the energy distribution function and the direction of the velocity of H-ENAs on the nightside are presented. The present study describes a novel 'ENA sounding' technique in which energetic neutral atoms are used to derive information of the properties of planetary exosphere and atmosphere in a similar manner as the solar wind photons are used to derive atmospheric densities by measuring the scattered UV light. A detailed study of the direction and energy of the scattered and non-scattered H-ENAs suggest that the ENA sounding is a method to study the interaction between the planetary atmosphere and the solar wind and to monitor the density, and likely also the magnetization, of the planetary upper atmosphere. Already present-day ENA instrument should be capable to detect the analyzed particle fluxes. Keywords: Mars, atmosphere

Published
2006

172. First ENA observations at Mars: charge exchange ENAs produced in the magnetosheath

Author

Gunell, H., Brinkfeldt, K., Holmstrom, M., Brandt, P. C:son, Barabash, S., Kallio, E., Ekenback, A., Futaana, Y., Lundin, R., Andersson, H., Yamauchi, M., Grigoriev, A., Winningham, J.D., Frahm, R.A., Sharber, J.R., Scherrer, J.R., Coates, A.J., Linder, D.R., Kataria, D.O., Sales, T., Riihela, P., Schmidt, W., Koskinen, H., Kozyra, J., Luhmann, J., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Mars (Planet) -- Environmental aspects, Mars (Planet) -- Observations, Magnetosphere -- Observations, Astronomy, Earth sciences
Abstract

Measurements of energetic neutral atoms (ENA) generated in the magnetosheath at Mars are reported. These ENAs are the result of charge exchange collisions between solar wind protons and neutral oxygen and hydrogen in the exosphere of Mars. The peak of the observed ENA flux is 1.3 x [10.sup.11] [m.sup.-2] [sr.sup.-1] [s.sup.-1]. For the case studied here, i.e., the passage of Mars Express through the martian magnetosheath around 20:15 UT on 3 May 2004, the measurements agree with an analytical model of the ENA production at the planet. It is possible to find parameter values in the model such that the observed peak in the ENA count rate during the spacecraft passage through the magnetosheath is reproduced. Keywords: Mars; Solar wind; Magnetospheres

Published
2006

173. Plasma intrusion above Mars crustal fields--Mars Express ASPERA-3 observations

Author

Franz, M., Winningham, J.D., Dubinin, E., Roussos, E., Woch, J., Barabash, S., Lundin, R., Holmstrom, M., Andersson, H., Yamauchi, M., Grigoriev, A., Frahm, R.A., Sharber, J.R., Scherrer, J.R., Coates, A.J., Soobiah, Y., Linder, D.R., Kataria, D.O., Kallio, E., Sales, T., Riihela, P., Schmidt, W., Koskinen, H.E.J., Kozyra, J., Luhmann, J., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Asamura, K., and Dierker, C.

Subjects
Mars (Planet) -- Observations, Mars probes -- Observations, Magnetosphere -- Observations, Astronomy, Earth sciences
Abstract

Using data of the ASPERA-3 instrument on board the European Mars Express spacecraft we investigate the effect of the martian crustal fields on electrons intruding from the magnetosheath. For the crustal field strength we use published data obtained by the Mars Global Surveyor MAG/ER instrument for a fixed altitude of 400 km. We use statistics on 13 months of 80-100 eV electron observations to show that the electron intrusion altitude determined by a probability measure is approximately linearly dependent on the total field strength at 400 km altitude. We show that on the dayside the mean electron intrusion altitude describes the location of the Magnetic Pile-Up Boundary (MPB) such that we can quantify the effect of the crustal fields on the MPB. On the nightside we quantify the shielding of precipitating electrons by the crustal fields. PACS: 96.30.Gc; 94.05.-a; 96.12.Jt Keywords: Mars; Magnetospheres

Published
2006

174. Numerical interpretation of high-altitude photoelectron observations

Author

Liemohn, Michael W., Frahm, R.A., Winningham, J.D., Ma, Y., Barabash, S., Lundin, R., Kozyra, J.U., Nagy, A.F., Bougher, S.M., Bell, J., Brain, D., Mitchell, D., Luhmann, J., Holmstrom, M., Andersson, H., Yamauchi, M., Grigoriev, A., McKenna-Lawler, S., Sharber, J.R., Scherrer, J.R., Jeffers, S.J., Coates, A.J., Linder, D.R., Kataria, D.O., Kallio, E., Koskinen, H., Sales, T., Riihela, P., Schmidt, W., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Mars (Planet) -- Observations, Photoelectron spectroscopy -- Observations, Ionosphere -- Spectra, Astronomy, Earth sciences
Abstract

The Electron Spectrometer (ELS) instrument of the ASPERA-3 package on the Mars Express satellite has recorded photoelectron energy spectra up to apoapsis (~10,000 km altitude). The characteristic photoelectron shape of the spectrum is sometimes seen well above the ionosphere in the evening sector across a wide range of near-equatorial latitudes. Two numerical models are used to analyze the characteristics of these high-altitude photoelectrons. The first is a global, multi-species MHD code that produces a 3-D representation of the magnetic field and bulk plasma parameters around Mars. It is used here to examine the possibility of magnetic connectivity between the high-altitude flanks of the martian ionosheath and the subsolar ionosphere. It is shown that some field lines in this region are draped interplanetary magnetic lines while others are open field lines (connected to both the IMF and the crustal magnetic field sources). The second model is a kinetic electron transport model that calculates the electron velocity space distribution along a selected, non-uniform, magnetic field line. It is used here to simulate the high-altitude ELS measurements. It is shown that the photoelectrons are essentially confined to the source cone, as governed by magnetic field inhomogeneity along the field line. Reasonable agreement is shown between the data and the model results, and a method is demonstrated for inferring properties of the local and photoelectron source region magnetic field from the ELS measurements. Specifically, the number of sectors in which photoelectrons are measured is a function of the magnetic field intensity ratio and the field's angle with respect to the detector plane. In addition, the sector of the photoelectron flux peak is a function of the magnetic field azimuthal angle in the detector plane. Keywords: Mars; Magnetospheres; Ionospheres; Magnetic fields

Published
2006

175. Observations of magnetic anomaly signatures in Mars Express ASPERA-3 ELS data

Author

Soobiah, Y., Coates, A.J., Linder, D.R., Kataria, D.O., Winningham, J.D., Frahm, R.A., Sharber, J.R., Scherrer, J.R., Barabash, S., Lundin, R., Holmstrom, M., Andersson, H., Yamauchi, M., Grigoriev, A., Kallio, E., Koskinen, H., Sales, T., Riihela, P., Schmidt, W., Kozyra, J., Luhmann, J., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Solar wind -- Observations, Magnetic fields -- Observations, Mars (Planet) -- Atmosphere, Mars (Planet) -- Observations, Astronomy, Earth sciences
Abstract

Mars Express (MEX) Analyser of Space Plasmas and Energetic Atoms (ASPERA-3) data is providing insights into atmospheric loss on Mars via the solar wind interaction. This process is influenced by both the interplanetary magnetic field (IMF) in the solar wind and by the magnetic 'anomaly' regions of the martian crust. We analyse observations from the ASPERA-3 Electron Spectrometer near to such crustal anomalies. We find that the electrons near remanent magnetic fields either increase in flux to form intensified signatures or significantly reduce in flux to form plasma voids. We suggest that cusps intervening neighbouring magnetic anomalies may provide a location for enhanced escape of planetary plasma. Initial statistical analysis shows that intensified signatures are mainly a dayside phenomenon whereas voids are a feature of the night hemisphere. Keywords: Magnetic fields; Solar wind; Mars

Published
2006

176. Carbon dioxide photoelectron energy peaks at Mars

Author

Frahm, R.A., Winningham, J.D., Sharber, J.R., Scherrer, J.R., Jeffers, S.J., Coates, A.J., Linder, D.R., Kataria, D.O., Lundin, R., Barabash, S., Holmstrom, M., Andersson, H., Yamauchi, M., Grigoriev, A., Kallio, E., Sales, T., Riihela, P., Schmidt, W., Koskinen, H., Kozyra, J.U., Luhmann, J.G., Roelof, E.C., Williams, D.J., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaudk, J.-A., Fedorov, A., Thocaven, J.J., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Carbon dioxide -- Environmental aspects, Electron spectroscopy -- Observations, Mars (Planet) -- Atmosphere, Mars (Planet) -- Composition, Mars (Planet) -- Observations, Astronomy, Earth sciences
Abstract

The ELectron Spectrometer (ELS) from the Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) flown on the Mars Express spacecraft has an 8% energy resolution, combined with the capability to oversample the martian electron distribution. This makes possible the resolution and identification of electrons generated as a result of the He 304 [Angstrom] ionization of C[O.sub.2] at the martian exobase on the dayside of the planet. Ionospheric photoelectrons were observed during almost every pass into the ionosphere and C[O.sub.2] photoelectron peaks were identified near the terminator. Atmospherically generated C[O.sub.2] photoelectrons are also observed at 10,000 km altitude in the martian tail near the inner magnetospheric boundary. Observations over a wide range of spacecraft orbits showed a consistent presence of photoelectrons at locations along the inner magnetospheric boundary and in the ionosphere, from an altitude of 250 to 10,000 km. Keywords: Mars; Ionospheres; Atmospheres; Magnetospheres

Published
2006

177. First ENA observations at Mars: subsolar ENA jet

Author

Futaana, Y., Barabash, S., Grigoriev, A., Holmstrom, M., Kallio, E., Brandt, P. C:son, Gunell, H., Brinkfeldt, K., Lundin, R., Andersson, H., Yamauchi, M., McKenna-Lawler, S., Winningham, J.D., Frahm, R.A., Sharber, J.R., Scherrer, J.R., Coates, A.J., Linder, D.R., Kataria, D.O., Sales, T., Riihela, P., Schmidt, W., Koskinen, H., Kozyra, J., Luhmann, J., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Mars (Planet) -- Observations, Magnetosphere -- Observations, Solar wind -- Observations, Astronomy, Earth sciences
Abstract

The Neutral Particle Detector (NPD), an Energetic Neutral Atom (ENA) sensor of the Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) on board Mars Express, detected intense fluxes of ENAs emitted from the subsolar region of Mars. The typical ENA fluxes are (4-7) x [10.sup.5] [cm.sup.-2] [sr.sup.-1] [s.sup.-1] in the energy range 0.3-3 keV. These ENAs are likely to be generated in the subsolar region of the martian exosphere. As the satellite moved away from Mars, the ENA flux decreased while the field of view of the NPD pointed toward the subsolar region. These decreases occurred very quickly with a time scale of a few tens of seconds in two thirds of the orbits. Such a behavior can be explained by the spacecraft crossing a spatially constrained ENA jet, i.e., a highly directional ENA emission from a compact region of the subsolar exosphere. This ENA jet is highly possible to be emitted conically from the subsolar region. Such directional ENAs can result from the anisotropic solar wind flow around the subsolar region, but this can not be explained in the frame of MHD models. Keywords: Mars, atmosphere; Solar wind; Magnetospheres

Published
2006

178. Electron oscillations in the induced martian magnetosphere

Author

Winningham, J.D., Frahm, R.A., Sharber, J.R., Coates, A.J., Linder, D.R., Soobiah, Y., Kallio, E., Espley, J.R., Lundin, R., Barabash, S., Holmstrom, M., Andersson, H., Yamauchi, M., Grigoriev, A., Scherrer, J.R., Jeffers, S.J., Kataria, D.O., Kozyra, J.U., Luhmann, J.G., Roelof, E.C., Williams, D.J., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Koskinen, H., Sales, T., Riihela, P., Schmidt, W., Grande, M., Carter, M., Sauvaud, J.-A., Fedorov, A., Thocaven, J.-J., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Magnetosphere -- Observations, Solar oscillations -- Observations, Mars (Planet) -- Environmental aspects, Mars (Planet) -- Observations, Astronomy, Earth sciences
Abstract

The Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) experiment flown on the Mars Express (MEX) spacecraft includes the Electron Spectrometer (ELS) as part of its complement. The ELS instrument measures the differential electron flux spectrum in a 128-level logarithmic energy sweep within a time period of 4 s. The orbital path of MEX traverses the martian sheath, cusps, and tail where ELS recorded periodic electron intensity oscillations. These oscillations comprised periodic variations of up to an order of magnitude (peak to valley) in energy flux, with the largest amplitudes in the tens to hundreds of eV range. The observed oscillations displayed periods ranging from minutes down to the instrument sweep resolution of 4 s. In the cases analyzed here, the frequency of the integrated electron energy flux typically peaked between 0.01 and 0.02 Hz. This frequency range is nearly the same as the typical [O.sup.+] gyrofrequency in the magnetosheath, calculated using magnetometer data from Mars Global Surveyor. Due to the motion of the spacecraft, it is unclear if the wave structures observed were permanent standing waves or rather constituted waves propagating past the spacecraft. Keywords: Mars; Magnetosphere

Published
2006

179. Solar wind plasma protrusion into the martian magnetosphere: ASPERA-3 observations

Author

Dubinin, E., Winningham, D., Franz, M., Woch, J., Lundin, R., Barabash, S., Fedorov, A., Frahm, R., Sharber, J.R., Coates, A.J., Krupp, N., Sauvaud, J.-A., Holmstrom, M., Andersson, H., Yamauchi, M., Grigoriev, A., Thocaven, J.-J., Asamura, K., Curtis, C., Hsieh, K.S., Sandel, B., Koskinen, H., Kallio, E., Riihela, P., Schmidt, W., Sales, T., Kozyra, J., Luhmann, J., McKenna-Lawler, S., Cerulli-Irelli, R., Orsini, S., Maggi, M., Roelof, E., Williams, D., Livi, S., Wurz, P., Bochsler, P., Dierker, C., Grande, M., and Carter, M.

Subjects
Solar wind -- Observations, Magnetosphere -- Observations, Mars (Planet) -- Environmental aspects, Mars (Planet) -- Observations, Astronomy, Earth sciences
Abstract

The ASPERA-3 experiment onboard the Mars Express spacecraft revealed, near the wake boundary of Mars, a spatially narrow, strip-like plasma structure composed of magnetosheath-like electrons and planetary ions. The peak electron energy often exceeds the peak energy at the bow shock that indicates a significant heating (acceleration) during the structure formation. It is shown that this structure is formed during efficient plasma penetration into the martian magnetosphere in the region near the terminator. The penetration of sheath electrons and their gradual heating (acceleration) is accompanied by a change of the ion composition from a solar wind plasma to a planetary plasma dominated by oxygen ions. A possible mechanism of plasma inflow to the magnetosphere is discussed. Keywords: Mars; Magnetospheres

Published
2006

180. Structure of the martian wake

Author

Fedorov, A., Budnik, E., Sauvaud, J.-A., Mazelle, C., Barabash, S., Lundin, R., Acuna, M., Holmstrom, M., Grigoriev, A., Yamauchi, M., Andersson, H., Thocaven, J.-J, Winningham, D., Frahm, R., Sharber, J.R., Scherrer, J., Coastes, A.J., Linder, D.R., Kataria, D.O., Kallio, E., Koskines, H., Sales, T., Riihela, P., Schmidt, W., Kozyra, J., Luhmann, J., Roeloff, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Heavy ions -- Observations, Magnetosphere -- Observations, Mars (Planet) -- Atmosphere, Mars (Planet) -- Observations, Astronomy, Earth sciences
Abstract

We present the first results from the ion mass analyzer IMA of the ASPERA-3 instrument on-board of Mars Express. More than 200 orbits for May 2004-September 2004 time interval have been selected for the statistical study of the distribution of the atmospheric origin ions in the planetary wake. This study shows that the martian magnetotail consists of two different ion regimes. Planetary origin ions of the first regime form the layer adjacent to the magnetic pile-up boundary. These ions are accelerated to energy greater than 2000 eV and exhibit a gradual decreasing of energy down to the planetary tail. The second plasma regime is observed in the planetary shadow. The heavy ions (considered as planetary ones) are accelerated to the energy of the solar wind protons. Obviously the acceleration mechanism is different for the different plasma regimes. Study of two plasma regimes in the frame referred to the interplanetary magnetic field (IMF) direction (we used MGS magnetometer data to obtain the IMF clock angle) clearly shows their spatial anisotropy. The monoenergetic plasma in the planetary shadow is observed only in the narrow angular sector around the positive direction of the interplanetary electric field. Keywords: Mars; Magnetospheres

Published
2006

181. Mass composition of the escaping plasma at Mars

Author

Carlsson, E., Fedorov, A., Barabash, S., Budnik, E., Grigoriev, A., Gunell, H., Nilsson, H., Sauvaud, J.-A., Lundin, R., Futaana, Y., Holmstrom, M., Andersson, H., Yamauchi, M., Winningham, J.D., Frahm, R.A., Sharber, J.R., Scherrer, J., Coates, A.J., Linder, D.R., Kataria, D.O., Kallio, E., Koskinen, H., Sales, T., Riihela, P., Schmidt, W., Kozyra, J., Luhmann, J., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Thocaven, J.J., McKenna-Lawler, S., Orsini, S., Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Mars (Planet) -- Observations, Ionospheric research, Astronomy, Earth sciences
Abstract

Data from the Ion Mass Analyzer (IMA) sensor of the ASPERA-3 instrument suite on Mars Express have been analyzed to determine the mass composition of the escaping ion species at Mars. We have examined 77 different ion-beam events and we present the results in terms of flux ratios between the following ion species: C[O.sup.+.sub.2]/[O.sup.+] and [O.sup.+.sub.2]/[O.sup.+]. The following ratios averaged over all events and energies were identified: C[O.sup.+.sub.2]/[O.sup.+] = 0.2 and [O.sup.+.sub.2]/[O.sup.+] = 0.9. The values measured are significantly higher, by a factor of 10 for [O.sup.+.sub.2]]/[O.sup.+], than a contemporary modeled ratio for the maximum fluxes which the martian ionosphere can supply. The most abundant ion species was found to be [O.sup.+], followed by [O.sup.+.sub.2] and C[O.sup.+.sub.2]. We estimate the loss of C[O.sup.+.sub.2] to be 4.0 x [10.sup.24] s-1 (0.29 kg[s.sup.-1]) by using the previous measurements of Phobos-2 in our calculations. The dependence of the ion ratios in relation to their energy ranges we studied, 0.3-3.0 keV, indicated that no clear correlation was found. Keywords: Ionospheres; Mars, atmosphere

Published
2006

182. Electric fields within the martian magnetosphere and ion extraction: ASPERA-3 observations

Author

Dubinin, E., Lundin, R., Franz, M., Woch, J., Barabash, S., Fedorov, A., Winningham, D., Krupp, N., Sauvaud, J.-A., Holmstrom, M., Andersson, H., Yamauchi, M., Grigoriev, A., Thocaven, J.-J., Frahm, R., Sharber, J., Asamura, K., Coates, A., Curtis, C., Hsieh, K.S., Sandel, B., Koskinen, H., Kallio, E., Riihela, P., Schmidt, W., Sales, T., Kozyra, J., Luhmann, J., McKennan-Lawler, S., Cerulli-Irelli, R., Orsini, S., Maggi, M., Roelof, E., Williams, D., Livi, S., Wurz, P., Bochsler, P., Dierker, C., Grande, M., and Carter, M.

Subjects
Mars (Planet) -- Environmental aspects, Mars (Planet) -- Observations, Magnetosphere -- Observations, Ionosphere -- Observations, Astronomy, Earth sciences
Abstract

Observations made by the ASPERA-3 experiment onboard the Mars Express spacecraft found within the martian magnetosphere beams of planetary ions. In the energy (E/q)-time spectrograms these beams are often displayed as dispersive-like, ascending or descending (whether the spacecraft moves away or approach the planet) structures. A linear dependence between energy gained by the beam ions and the altitude from the planet suggests their acceleration in the electric field. The values of the electric field evaluated from ion energization occur close to the typical values of the interplanetary motional electric field. This suggests an effective penetration of the solar wind electric field deep into the martian magnetosphere or generation of large fields within the magnetosphere. Two different classes of events are found. At the nominal solar wind conditions, a 'penetration' occurs near the terminator. At the extreme solar wind conditions, the boundary of the induced magnetosphere moves to a more dense upper atmosphere that leads to a strong scavenging of planetary ions from the dayside regions. Keywords: Mars; Solar wind; Magnetospheres; Ionospheres; Magnetic fields

Published
2006

183. Ionospheric plasma acceleration at Mars: ASPERA-3 results

Author

Lundin, R., Winningham, D., Barabash, S., Frahm, R.A., Andersson, H., Holmstrom, M., Grigoriev, A., Yamauchi, M., Borg, H., Sharber, J.R., Sauvaud, J.-A., Fedorov, A., Budnik, E., Thocaven, J.-J., Asamura, K., Hayakawa, H., Coates, A.J., Linder, D.R., Kataria, D.O., Curtis, C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., Reading, D.H., Koskinen, H., Kallio, E., Riihela, P., Schmidt, W., Sales, T., Kozyra, J., Krupp, N., Woch, J., Franz, M., Luhmann, J., McKennan-Lawler, S., Cerulli-Irelli, R., Orsini, S., Maggi, M., Roelof, E., Williams, D., Livi, S., Brandt, P.C:son, Wurz, P., and Bochsler, P.

Subjects
Mars (Planet) -- Observations, Ionospheric research -- Observations, Mars probes -- Observations, Astronomy, Earth sciences
Abstract

The Analyzer of Space Plasma and Energetic Atoms (ASPERA) on-board the Mars Express spacecraft (MEX) measured penetrating solar wind plasma and escaping/accelerated ionospheric plasma at very low altitudes (250 km) in the dayside subsolar region. This implies a direct exposure of the martian topside atmosphere to solar wind plasma forcing leading to energization of ionospheric plasma. The ion and electron energization and the ion outflow from Mars is surprisingly similar to that over the magnetized Earth. Narrow 'monoenergetic' cold ion beams, ion beams with broad energy distributions, sharply peaked electron energy spectra, and bidirectional streaming electrons are particle features also observed near Mars. Energized martian ionospheric ions ([O.sup.+], [O.sup.+.sub.2], C[O.sup.+.sub.2], etc.) flow in essentially the same direction as the external sheath flow. This suggests that the planetary ion energization couples directly to processes in the magnetosheath/solar wind. On the other hand, the beam-like distribution of the energized plasma implies more indirect energization processes like those near the Earth, i.e., energization in a magnetized environment by waves and/or parallel (to B) electric fields. The general conditions for martian plasma energization are, however, different from those in the Earth's magnetosphere. Mars has a weak intrinsic magnetic field and solar wind plasma may therefore penetrate deep into the dense ionospheric plasma. Local crustal magnetization, discovered by Acuna et al. [Acuna, M.J., Connerey, J., Ness, N., Lin, R., Mitchell, D., Carlsson, C., McFadden, J., Anderson, K., Reme, H., Mazelle, C., Vignes, D., Wasilewski, P., Cloutier, P., 1999. Science 284, 790-793], provide some dayside shielding against the solar wind. On the other hand, multiple magnetic anomalies may also lead to 'hot spots' facilitating ionospheric plasma energization. We discuss the ASPERA-3 findings of martian ionospheric ion energization and present evidences for two types of plasma energization processes responsible for the low- and mid-altitude plasma energization near Mars: magnetic field-aligned acceleration by parallel electric fields and plasma energization by low frequency waves. Keywords: Mars, atmosphere; Ionospheres; Magnetospheres

Published
2006

184. Ion escape at Mars: comparison of a 3-D hybrid simulation with Mars Express IMA/ASPERA-3 measurements

Author

Kallio, E., Fedorov, A., Budnik, E., Sales, T., Janhunen, P., Schmidt, W., Koskinen, H., Riihela, P., Barabash, S., Lundin, R., Holmstrom, M., Gunell, H., Brinkfeldt, K., Futaana, Y., Andersson, H., Yamauchi, M., Grigoriev, A., Sauvaud, J.-A., Thocaven, J.-J., Winningham, J.D., Frahm, R.A., Sharber, J.R., Scherrer, J.R., Coates, A.J., Linder, D.R., Kataria, D.O., Kozyra, J., Luhmann, J.G., Roelof, E., Williams, D., Livi, S., Curtis, C.C., Hsieh, K.C., Sandel, B.R., Grande, M., Carter, M., McKenna-Lawler, S., Orsini, S, Cerulli-Irelli, R., Maggi, M., Wurz, P., Bochsler, P., Krupp, N., Woch, J., Franz, M., Asamura, K., and Dierker, C.

Subjects
Mars (Planet) -- Observations, Ionospheric electron density -- Measurement, Solar wind -- Research, Astronomy, Earth sciences
Abstract

We have analysed ion escape at Mars by comparing ASPERA-3/Mars Express ion measurements and a 3-D quasi-neutral hybrid model. As Mars Express does not have a magnetometer onboard, the analysed IMA data are from an orbit when the IMF clock angle was possible to determine from the magnetic field measurements of Mars Global Surveyor. We found that fast escaping planetary ions were observed at the place which, according to the 3-D model, is anticipated to contain accelerated heavy ions originating from the martian ionosphere. The direction of the interplanetary magnetic field was found to affect noticeably which regions can be magnetically connected to Mars Express and to the overall 3-D Mars-solar wind interaction. Keywords: Mars, atmosphere; Ionospheres

Published
2006

190. POROSITY QUANTIFICATION OF ADDITIVE MANUFACTURED TI6AL4V AND COCRW ALLOYS PRODUCED BY L-PBF.

Author

BIDULSKÝ, R., PETROUŠEK, P., BIDULSKÁ, J., HUDÁK, R., ŽIVČÁK, J., and ACTIS GRANDE, M.

Subjects
PORE size (Materials), ALLOYS, IMAGE analysis
Abstract

The main aim of the present paper is to evaluate the porosity and mechanical properties of Ti6Al4v and CoCrW alloys produced by Laser Powder Bed Fusion (L-PBF) as an additive manufacturing (AM) technology. Ti6Al4v and CoCrW alloys are attractive for medical application. the complex examination of porosity for these alloys needs the quantification of morphological and dimensional characteristics. Quantification of porosity was realized on non-etched samples. Quantitative image analysis was used to describe the dimensional and morphological porosity characteristics. the pores were evaluated by image pro plus software. the results show the significant inhomogeneity of the morphology and distribution, as well as the pore size in the investigated materials and underline the importance of pore structure for the controlling mechanism of the mechanical response. [ABSTRACT FROM AUTHOR]

Published
2022
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191. In situ dust measurements in the inner Saturnian system

Author

Srama, R., Kempf, S., Moragas-Klostermeyer, G., Helfert, S., Ahrens, T.J., Altobelli, N., Auer, S., Beckmann, U., Bradley, J.G., Burton, M., Dikarev, V.V., Economou, T., Fechtig, H., Green, S.F., Grande, M., Havnes, O., Hillier, J.K., Horanyi, M., Igenbergs, E., Jessberger, E.K., Johnson, T.V., Krüger, H., Matt, G., McBride, N., Mocker, A., Lamy, P., Linkert, D., Linkert, G., Lura, F., McDonnell, J.A.M., Möhlmann, D., Morfill, G.E., Postberg, F., Roy, M., Schwehm, G.H., Spahn, F., Svestka, J., Tschernjawski, V., Tuzzolino, A.J., Wäsch, R., and Grün, E.

Published
2006
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193. Medium energy neutral atom (MENA) imager for the IMAGE mission

Author

Pollock, C.J., Asamura, K., Baldonado, J., Balkey, M.M., Barker, P., Burch, J.L., Korpela, E.J., Cravens, J., Dirks, G., Fok, M.-C., Funsten, H.O., Grande, M., Gruntman, M., Hanley, J., Jahn, J.-M., Jenkins, M., Lampton, M., Marckwordt, M., McComas, D.J., Mukai, T., Penegor, G., Pope, S., Ritzau, S., Schattenburg, M.L., Scime, E., Skoug, R., Spurgeon, W., Stecklein, T., Storms, S., Urdiales, C., Valek, P., van Beek, J.T.M., Weidner, S.E., Wüest, M., Young, M.K., and Zinsmeyer, C.

Published
2000
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198. Impact of early oseltamivir treatment on outcome in critically ill patients with 2009 pandemic influenza A

Author

Rodríguez, Alejandro, Díaz, Emili, Martín-Loeches, Ignacio, Sandiumenge, Alberto, Canadell, Laura, Díaz, Juan J., Figueira, Juan C., Marques, Asunción, Álvarez-Lerma, Francisco, Vallés, Jordi, Baladín, Bárbara, García-López, Fernando, Suberviola, Borja, Zaragoza, Rafael, Trefler, Sandra, Bonastre, Juan, Blanquer, José, Rello, Jordi, Cobo, Pedro, Martins, Javier, Carbayo, Cecilia, Robles-Musso, Emilio, Cárdenas, Antonio, Fierro, Javier, Fernández, Dolores Ocaña, Sierra, Rafael, Jesús Huertos, M, Carlos Pozo, Juan, Guerrero, R., Márquez, Enrique, Rodríguez-Carvajal, Manuel, Jareño, Antonio, Pomares, José, Ballesteros, José Luis, Fernández, Yolanda, Lobato, Francisco, Prieto, José F., Albofedo-Sánchez, José, Martínez, Pilar, Díaz Castellanos, Miguel Angel, Sevilla, Guillermo, Garnacho-Montero, José, Hinojosa, Rafael, Fernández, Esteban, Loza, Ana, León, Cristóbal, Arenzana, Angel, Ocaña, Dolores, Navarrete, Inés, Zaheri Beryanaki, Medhi, Sánchez, Ignacio, Avellanas, Manuel Luis, Lander, Arantxa, Ramírez de Arellano, S. Garrido, Marquina Lacueva, M. I., Luque, Pilar, González, Ignacio, Montón, Jose M, Dorado Regil, Paloma, Iglesias, Lisardo, Pascual González, Carmen, Quiroga, García-Rodríguez, Águeda, Socias, Lorenzo, Ibánez, Pedro, Borges-Sa, Marcío, Socias, Antonia, Del Castillo, A., Jordà Marcos, Ricard, Bonell, José M., Amestarán, Ignacio, Ruiz-Santana, Sergio, Díaz, Juan José, Sisón, Hernández, David, Trujillo, Ana, Regalado, Luis, Lorente, Leonardo, Martín, Mar, Martínez, Sergio, Cáceres, J. J., Suberviola, Borja, Ugarte, P., García-López, Fernando, Álvaro Alonso, Angel, Pasilla, Antonio, Gómez Grande, M Luisa, Albaya, Antonio, Canabal, Alfonso, Marina, Luis, Simón, Almudena, María Añón, José, López Messa, Juan B., López Pueyo, M Jesús, Ferreras, Zulema, Macias, Santiago, Ángel Berezo, José, Varela, Jesús Blanco, Ojeda, A. Andaluz, Terrero, Antonio Álvarez, Tena Ezpeleta, Fabiola, Paez, Zulema, García, Álvaro, Catalán, Rosa M, Ferrer, Miquel, Torres, Antoni, Barbadillo, Sandra, Cabré, Lluís, Rovira, Assumpta, Álvarez-Lerma, Francisco, Vázquez, Antonia, Nolla, Joan, Fernández, Francisco, Cervelló, Joaquim Ramón, Mañéz, Rafael, Ballús, J., Granada, Rosa M, Vallés, Jordi, Ortíz, Marta, Guía, C., Arméstar, Fernando, Páez, Joaquim, Almirall, Jordi, Balanzo, Xavier, Rello, Jordi, Arnau, Elena, Llopart, Lluis, Palomar, Mercedes, Catalán, Iñaki, Sirvent, Josep M, Ferri, Cristina, de Arbina, Nerea López, Badía, Mariona, Valverdú-Vidal, Montserrat, Barcenilla, Fernando, Magret, Mònica, Esteban, M. F., Luna, José, Nava, Juan M, de Molina, J. González, Josic, Zoran, Gurri, Francisco, Rodríguez, Alejandro, Lisboa, Thiago, de Mendoza, Diego, Trefler, Sandra, María Díaz, Rosa, Mesalles, Eduard, José, Juliá-Narváez, Fernández-Zapata, Alberto, Recio, Teresa, Arrascaeta, Abilio, García-Ramos, M José, Gallego, Elena, Bueno, Fernándo, Díaz, Mercedes, Cordero, M Lourdes, Pastor, José A., Álvarez–Rocha, Luis, Vila, Dolores, Lamas, Ana Díaz, Pérez, Javier Blanco, Ortiz Piquer, M., Merayo, Eleuterio, López-Ciudad, Victor Jose, Cortez, Juan, Vilaboy, Eva, Saborido, Eva Maria, González, Raul José, Freita, Santiago, López, Ana María, Canabal, Julio, Ferres, Enrique, Monzón, José Luis, Goñi, Félix, Del Nogal Sáez, Frutos, Blasco Navalpotro, M., García-Torrejón, M Carmen, Pérez–Calvo, César, López, Diego, Arnaiz, Luis, Sánchez-Alonso, S., Velayos, Carlos, del Río, Francisco, González, Miguel Ángel, Martín, María Cruz, Molina, José M, Montejo, Juan Carlos, Catalán, Mercedes, Albert, Patricia, de Pablo, Ana, Guerrero, José Eugenio, Peyrat, Jaime Benitez, Cerdá, Enrique, Alvarez, Manuel, Pey, Carlos, Rodríguez, Montse, Palencia, Eduardo, Caballero, Rafael, Vaquero, Concepción, Mariscal, Francisco, García, S., Carrasco, Nieves, Prieto, Isidro, Liétor, A., Ramos, R., Galván, Beatríz, Figueira, Juan C., Soriano, M. Cruz, Galdós, P., Balandin Moreno, Bárbara, del Cabo, Fernández, Hermosa, Cecilia, Gordo, Federico, Algora, Alejandro, Paredes, Amparo, Cambronero, J. A., Gómez-Rosado, Sonia, Prado López, Luis Miguel, Martínez, Sofía, Abad, F. Felices, Martínez, Mariano, Butí, Sergio Manuel, Gil Rueda, Bernardo, García, Francisco, Macaya, Laura, Maraví-Poma, Enrique, Jimenez Urra, I., Macaya Redin, L., Tellería, A., Insansti, Josu, González, Nagore, Marco, Pilar, Vidaur, Loreto, Santamaría, B., Vergara, Juan Carlos, Iruretagoyena Amiano, Jose Ramon, Manzano, Alberto, Arenal, Carlos Castillo, Olaechea, Pedro María, Blanquer, José, Reig Valero, Roberto, Belenger, A., Altaba, Susana, Álvarez-Sánchez, Bernabé, Alberto Picos, Santiago, Sánchez-Miralles, Ángel, Bonastre, Juan, Palamo, M., Cebrian, Javier, Cuñat, José, Romero, Belén, Zaragoza, Rafael, Paricio, Virgilio, Marques, Asunción, Sánchez-Morcillo, S., Tormo, S., Latour, J., Ángel García, M., and Ribas, Antoli

Published
2011
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