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2. Exploring the link between star and planet formation with Ariel

Author

Turrini, Diego, Codella, Claudio, Danielski, Camilla, Fedele, Davide, Fonte, Sergio, Garufi, Antonio, Guarcello, Mario Giuseppe, Helled, Ravit, Ikoma, Masahiro, Kama, Mihkel, Kimura, Tadahiro, Kruijssen, J. M. Diederik, Maldonado, Jesus, Miguel, Yamila, Molinari, Sergio, Nikolaou, Athanasia, Oliva, Fabrizio, Panić, Olja, Pignatari, Marco, Podio, Linda, Rickman, Hans, Schisano, Eugenio, Shibata, Sho, Vazan, Allona, and Wolkenberg, Paulina

Published
2022
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3. Rapid Affinity and Microsomal Stability Ranking of Crude Mixture Libraries of Histone Deacetylase Inhibitors.

Author

Tyagarajan, Sriram, Andrews, Christine L., Beshore, Douglas C., Buevich, Alexei V., Curran, Patrick J., Dandliker, Peter, Greshock, Thomas J., Hoar, Jason, Kim, Alex, Karnachi, Prabha, Knemeyer, Ian, Kozlowski, Joseph, Liu, Jian, Maletic, Milana, Myers, Robert, Rada, Vanessa, Sha, Deyou, Sauvagnat, Berengere, Vachal, Petr, and Wolkenberg, Scott

Published
2024
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10. A chemical survey of exoplanets with ARIEL

Author

Tinetti, Giovanna, Drossart, Pierre, Eccleston, Paul, Hartogh, Paul, Heske, Astrid, Leconte, Jérémy, Micela, Giusi, Ollivier, Marc, Pilbratt, Göran, Puig, Ludovic, Turrini, Diego, Vandenbussche, Bart, Wolkenberg, Paulina, Beaulieu, Jean-Philippe, Buchave, Lars A., Ferus, Martin, Griffin, Matt, Guedel, Manuel, Justtanont, Kay, Lagage, Pierre-Olivier, Machado, Pedro, Malaguti, Giuseppe, Min, Michiel, Nørgaard-Nielsen, Hans Ulrik, Rataj, Mirek, Ray, Tom, Ribas, Ignasi, Swain, Mark, Szabo, Robert, Werner, Stephanie, Barstow, Joanna, Burleigh, Matt, Cho, James, du Foresto, Vincent Coudé, Coustenis, Athena, Decin, Leen, Encrenaz, Therese, Galand, Marina, Gillon, Michael, Helled, Ravit, Morales, Juan Carlos, Muñoz, Antonio García, Moneti, Andrea, Pagano, Isabella, Pascale, Enzo, Piccioni, Giuseppe, Pinfield, David, Sarkar, Subhajit, Selsis, Franck, Tennyson, Jonathan, Triaud, Amaury, Venot, Olivia, Waldmann, Ingo, Waltham, David, Wright, Gillian, Amiaux, Jerome, Auguères, Jean-Louis, Berthé, Michel, Bezawada, Naidu, Bishop, Georgia, Bowles, Neil, Coffey, Deirdre, Colomé, Josep, Crook, Martin, Crouzet, Pierre-Elie, Da Peppo, Vania, Sanz, Isabel Escudero, Focardi, Mauro, Frericks, Martin, Hunt, Tom, Kohley, Ralf, Middleton, Kevin, Morgante, Gianluca, Ottensamer, Roland, Pace, Emanuele, Pearson, Chris, Stamper, Richard, Symonds, Kate, Rengel, Miriam, Renotte, Etienne, Ade, Peter, Affer, Laura, Alard, Christophe, Allard, Nicole, Altieri, Francesca, André, Yves, Arena, Claudio, Argyriou, Ioannis, Aylward, Alan, Baccani, Cristian, Bakos, Gaspar, Banaszkiewicz, Marek, Barlow, Mike, Batista, Virginie, Bellucci, Giancarlo, Benatti, Serena, Bernardi, Pernelle, Bézard, Bruno, Blecka, Maria, Bolmont, Emeline, Bonfond, Bertrand, Bonito, Rosaria, Bonomo, Aldo S., Brucato, John Robert, Brun, Allan Sacha, Bryson, Ian, Bujwan, Waldemar, Casewell, Sarah, Charnay, Bejamin, Pestellini, Cesare Cecchi, Chen, Guo, Ciaravella, Angela, Claudi, Riccardo, Clédassou, Rodolphe, Damasso, Mario, Damiano, Mario, Danielski, Camilla, Deroo, Pieter, Di Giorgio, Anna Maria, Dominik, Carsten, Doublier, Vanessa, Doyle, Simon, Doyon, René, Drummond, Benjamin, Duong, Bastien, Eales, Stephen, Edwards, Billy, Farina, Maria, Flaccomio, Ettore, Fletcher, Leigh, Forget, François, Fossey, Steve, Fränz, Markus, Fujii, Yuka, García-Piquer, Álvaro, Gear, Walter, Geoffray, Hervé, Gérard, Jean Claude, Gesa, Lluis, Gomez, H., Graczyk, Rafał, Griffith, Caitlin, Grodent, Denis, Guarcello, Mario Giuseppe, Gustin, Jacques, Hamano, Keiko, Hargrave, Peter, Hello, Yann, Heng, Kevin, Herrero, Enrique, Hornstrup, Allan, Hubert, Benoit, Ida, Shigeru, Ikoma, Masahiro, Iro, Nicolas, Irwin, Patrick, Jarchow, Christopher, Jaubert, Jean, Jones, Hugh, Julien, Queyrel, Kameda, Shingo, Kerschbaum, Franz, Kervella, Pierre, Koskinen, Tommi, Krijger, Matthijs, Krupp, Norbert, Lafarga, Marina, Landini, Federico, Lellouch, Emanuel, Leto, Giuseppe, Luntzer, A., Rank-Lüftinger, Theresa, Maggio, Antonio, Maldonado, Jesus, Maillard, Jean-Pierre, Mall, Urs, Marquette, Jean-Baptiste, Mathis, Stephane, Maxted, Pierre, Matsuo, Taro, Medvedev, Alexander, Miguel, Yamila, Minier, Vincent, Morello, Giuseppe, Mura, Alessandro, Narita, Norio, Nascimbeni, Valerio, Nguyen Tong, N., Noce, Vladimiro, Oliva, Fabrizio, Palle, Enric, Palmer, Paul, Pancrazzi, Maurizio, Papageorgiou, Andreas, Parmentier, Vivien, Perger, Manuel, Petralia, Antonino, Pezzuto, Stefano, Pierrehumbert, Ray, Pillitteri, Ignazio, Piotto, Giampaolo, Pisano, Giampaolo, Prisinzano, Loredana, Radioti, Aikaterini, Réess, Jean-Michel, Rezac, Ladislav, Rocchetto, Marco, Rosich, Albert, Sanna, Nicoletta, Santerne, Alexandre, Savini, Giorgio, Scandariato, Gaetano, Sicardy, Bruno, Sierra, Carles, Sindoni, Giuseppe, Skup, Konrad, Snellen, Ignas, Sobiecki, Mateusz, Soret, Lauriane, Sozzetti, Alessandro, Stiepen, A., Strugarek, Antoine, Taylor, Jake, Taylor, William, Terenzi, Luca, Tessenyi, Marcell, Tsiaras, Angelos, Tucker, C., Valencia, Diana, Vasisht, Gautam, Vazan, Allona, Vilardell, Francesc, Vinatier, Sabrine, Viti, Serena, Waters, Rens, Wawer, Piotr, Wawrzaszek, Anna, Whitworth, Anthony, Yung, Yuk L., Yurchenko, Sergey N., Osorio, María Rosa Zapatero, Zellem, Robert, Zingales, Tiziano, and Zwart, Frans

Published
2018
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11. The Phase A study of the ESA M4 mission candidate ARIEL

Author

Puig, Ludovic, Pilbratt, Göran, Heske, Astrid, Escudero, Isabel, Crouzet, Pierre-Elie, de Vogeleer, Bram, Symonds, Kate, Kohley, Ralf, Drossart, Pierre, Eccleston, Paul, Hartogh, Paul, Leconte, Jeremy, Micela, Giusi, Ollivier, Marc, Tinetti, Giovanna, Turrini, Diego, Vandenbussche, Bart, and Wolkenberg, Paulina

Published
2018
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15. Intercomparison of radiative forcing calculations of stratospheric water vapour and contrails

Author

Gunnar Myhre, Maria Kvalevåg, Gaby Rädel, Jolene Cook, Keith P. Shine, Hannah Clark, Fernand Karcher, Krzysztof Markowicz, Aleksandra Kardas, Paulina Wolkenberg, Yves Balkanski, Michael Ponater, Piers Forster, Alexandrude Rap, Ruben Leon, and Rodriguez

Subjects
Meteorology. Climatology, QC851-999
Abstract

Seven groups have participated in an intercomparison study of calculations of radiative forcing (RF) due to stratospheric water vapour (SWV) and contrails. A combination of detailed radiative transfer schemes and codes for global-scale calculations have been used, as well as a combination of idealized simulations and more realistic global-scale changes in stratospheric water vapour and contrails. Detailed line-by-line codes agree within about 15 % for longwave (LW) and shortwave (SW) RF, except in one case where the difference is 30 %. Since the LW and SW RF due to contrails and SWV changes are of opposite sign, the differences between the models seen in the individual LW and SW components can be either compensated or strengthened in the net RF, and thus in relative terms uncertainties are much larger for the net RF. Some of the models used for global-scale simulations of changes in SWV and contrails differ substantially in RF from the more detailed radiative transfer schemes. For the global-scale calculations we use a method of weighting the results to calculate a best estimate based on their performance compared to the more detailed radiative transfer schemes in the idealized simulations.

Published
2009
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17. The atmospheric temperatures over Olympus Mons on Mars: An atmospheric hot ring

Author

Wolkenberg, P., Formisano, V., Rinaldi, G., and Geminale, A.

Subjects
Planets -- Atmosphere, Atmospheric circulation, Mars (Planet), Astronomy, Earth sciences
Abstract

To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2009.11.005 Byline: P. Wolkenberg, V. Formisano, G. Rinaldi, A. Geminale Keywords: Mars, Atmosphere, Climate; Mars; Atmospheres; Dynamics Abstract: We study the thermal fields over Olympus Mons separating seasons (northern spring and summer against southern spring and summer) and local time observations (day side versus night side). Temperature vertical profiles retrieved from Planetary Fourier Spectrometer on board Mars Express (PFS-MEX) data have been used. In many orbits (running north to south along a meridian) passing over the top of the volcano there is evidence of a hot air on top of the volcano, of two enhancement of the air temperature both north and south of it and in between a collar of air that is colder than nearby at low altitudes, and warmer than nearby at high altitudes. Mapping together many orbits passing over or near the volcano we find that the hot air has the tendency to form an hot ring around it. This hot structure occurs mostly between LT=10.00 and 15.00 and during the northern summer. Distance of the hot structure from the top of the volcano is about 600km (10[degrees] of latitude). The hot atmospheric region is 300-420km (5-7[degrees]) wide. Hot ring temperature contrasts of about 40K occur at 2km above the surface and decrease to 20K at 5km and to 10K at 10km. The atmospheric circulation over an area of 40[degrees]x40[degrees] (latitudes and longitudes) is affected by the topography and the presence of Olympus Mons (-133[degrees]W,18[degrees]N). We discuss also the thermal stability of the atmosphere over the selected area using the potential temperatures. The temperature field over the top of the volcano shows unstable atmosphere within 10km from the surface. Finally, we interpret the hot temperatures around volcano as an adiabatic compression of down-welling branch coming from over the top of volcano. Different air temperature profiles are observed in the same seasons during the night, or in different seasons. In northern spring-summer during the night the isothermal contours do not show the presence of the volcano until we reach close to the surface very much, where a thermal inversion is observed. The surface temperature shows higher values (by 10K) in correspondence of the scarp (an abrupt altimetry variation of roughly 5km) on south (6[degrees]N) and north (30[degrees]N) sides of volcano. During the southern spring-summer, on the contrary the isothermal curves run parallel to the surface even on top the volcano, just like the GCM have predicted. Author Affiliation: I.F.S.I., INAF, Via Fosso del Cavaliere, Rome, Italy Article History: Received 19 March 2009; Revised 21 October 2009; Accepted 4 November 2009

Published
2010

20. Discovery of an Anion-Dependent Farnesyltransferase Inhibitor from a Phenotypic Screen.

Author

Bukhtiyarova, Marina, Cook, Erica M., Hancock, Paula J., Hruza, Alan W., Shaw, Anthony W., Adam, Gregory C., Barnard, Richard J. O., McKenna, Philip M., Holloway, M. Katharine, Bell, Ian M., Carroll, Steve, Cornella-Taracido, Ivan, Cox, Christopher D., Kutchukian, Peter S., Powell, David A., Strickland, Corey, Trotter, B. Wesley, Tudor, Matthew, Wolkenberg, Scott, and Li, Jing

Published
2021
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22. The science of ARIEL

Author

Tinetti, G., Drossart, P., Eccleston, P., Hartogh, P., Leconte, J., Micela, G., Ollivier, M., Pilbratt, G., Puig, L., Heske, A., Turrini, D., Vandenbussche, B., Wolkenberg, P., University College of London [London] (UCL), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Sonnensystemforschung (MPS), Max-Planck-Gesellschaft, ECLIPSE 2017, Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astronomico di Palermo, Istituto Nazionale di Astrofisica (INAF), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), University of Valencia, Instituut voor Sterrenkunde [Leuven], Catholic University of Leuven - Katholieke Universiteit Leuven (KU Leuven), Space Research Centre of Polish Academy of Sciences (CBK), Polska Akademia Nauk = Polish Academy of Sciences (PAN), Pomies, Marie-Paule, Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), and Agence Spatiale Européenne = European Space Agency (ESA)

Subjects
Astrophysics::Instrumentation and Methods for Astrophysics, [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], [SDU.ASTR.EP] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], Astrophysics::Earth and Planetary Astrophysics
Abstract

International audience; Thousands of exoplanets have now been discovered with a huge range of masses, sizes and orbits: from rocky Earth-size planets to large gas giants grazing the surface of their host star. However, the essential nature of these exoplanets remains largely mysterious: there is no known, discernible pattern linking the presence, size, or orbital parameters of a planet to the nature of its parent star. We have little idea whether the chemistry of a planet is linked to its formation environment, or whether the type of host star drives the physics and chemistry of the planet's birth, and evolution. Progress with these science questions demands a large, unbiased spectroscopic survey of exoplanets. The ESA ARIEL M4 candidate mission has been conceived to conduct such a survey and to explore the nature of exoplanet atmospheres and interiors and, through this, the key factors affecting the formation and evolution of planetary systems.

Published
2017

23. Similarities and Differences of Global Dust Storms in MY 25, 28, and 34.

Author

Wolkenberg, P., Giuranna, M., Smith, M. D., Grassi, D., and Amoroso, M.

Subjects
DUST storms, MARTIAN atmosphere, OBSERVATIONS of Mars, ATMOSPHERIC temperature, SURFACE temperature
Abstract

To better understand the dust cycle on Mars during years with planet‐encircling dust storms, we analyze the last three events that took place in Mars Year (MY) 25, MY 28, and MY 34. Global dust storms that occurred in MY 25 and MY 34 (June 2018) were taking place during equinox, while the MY 28 storm had an onset after perihelion. Before the expansion phase of the MY 25 and MY 34 storms, we find similar regions (northern rim of Hellas, Arabia Terra, and Utopia Planitia) where dust is present. Possible precursor dust storms over Hellas and the southern polar cap edges were observed during MY 28 as a component of background dust activity. These features are not found in equinoctial dust storms on this scale. Dust during the MY 25 and MY 34 storms encircled the entire planet by the similar season (Ls = 193°). The MY 34 storm is characterized by a shorter decay phase compared to the events in MY 25 and MY 28. Dust opacity is correlated with atmospheric temperatures at 0.5 mbar and nighttime surface temperatures, while daytime surface temperatures are anticorrelated with dust opacity. Plain Language Summary: On Mars, one of the most variable atmospheric components is dust. We study it to better understand the cycle of its presence and absence in the Martian atmosphere. One of the particular phenomena of this cycle is the global dust storm that enshrouds the entire planet. Using data measured by two spectrometers, Thermal Infrared Emission Spectrometer onboard the Mars Global Surveyor and Planetary Fourier Spectrometer onboard the Mars Express orbiters, we investigate similarities and differences of the three most recent global dust storms that have occurred on Mars. We find similarities between the two global dust storms that took place in 2001 and 2018 (Mars Year [MY] 25 and 34). They encircled the entire planet in the equinox season. The storms in MY 25 and MY 28 dissipated over a very long timescale compared to the global dust storm of MY 34. Local dust storms in the northern rim of Hellas, Arabia Terra, and Utopia Planitia were observed before the onset of MY 25 and MY 34 global events. Key Points: The three global dust storms considered here have a similar duration of expansion phaseGlobal dust storm in Mars Year (MY) 34 is characterized by a shorter decay phase in comparison with the decay phases in MY 28 and MY 25 stormsRelatively large dust opacities are observed over Hellas and southern polar edge regions long before the onset of MY 28 storm [ABSTRACT FROM AUTHOR]

Published
2020
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25. The Venus nighttime atmosphere as observed by the VIRTIS-M instrument. Average fields from the complete infrared dataset

Author

Grassi, Davide, Politi, Romano, Ignatiev, Nikolai, Plainaki, C., Lebonnois, Sebastien, Wolkenberg, P., Montabone, Luca, Migliorini, Alessandra, Piccioni, Giuseppe, Drossart, Pierre, Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Space Research Institute of the Russian Academy of Sciences (IKI), Russian Academy of Sciences [Moscow] (RAS), Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Space Research Centre of Polish Academy of Sciences (CBK), Polska Akademia Nauk = Polish Academy of Sciences (PAN), Space Science Institute [Boulder] (SSI), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS Paris), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École des Ponts ParisTech (ENPC)-École polytechnique (X)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)

Subjects
[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology, ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2014

26. History in Place: Connecting Teachers and Students with Community History.

Author

Clyne, Jo, Whitworth, Eleanor, and Wolkenberg, Tanya

Subjects
HISTORY education in primary schools, HISTORY education in secondary schools, MUSEUMS
Abstract

The article presents a lesson plan for primary and secondary education which uses museum primary sources for history education.

Published
2014

30. Martian atmosphere as observed by VIRTIS-M on Rosetta spacecraft.

Author

Coradini, A., Grassi, D., Capaccioni, F., Filacchione, G., Tosi, F., Ammannito, E., De Sanctis, M. C., Formisano, V., Wolkenberg, P., Rinaldi, G., Arnold, G., Barucci, M. A., Bellucci, G., Benkhoff, J., Bibring, J. P., Blanco, A., Bockelee-Morvan, D., Capria, M. T., Carlson, R., and Carsenty, U.

Published
2010
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32. Accelerating lead development by microwave-enhanced medicinal chemistry.

Author

Shipe, William D., Wolkenberg, Scott E., and Lindsley, Craig W.

Subjects
DRUG development, PHARMACOLOGY, PHARMACY, ORGANIC synthesis
Abstract

Microwave-assisted organic synthesis (MAOS) addresses the need for accelerated chemical synthesis by providing many advantages over classical thermal conditions. Microwave instruments produced by Biotage, CEM and Milestone enable chemistry to be safely and reproducibly performed on various scales and in a parallel fashion. To illustrate the high utility of this technology for lead development, our Akt kinase program will be described wherein MAOS played a pivotal role in the identification of isozyme-selective Akt inhibitors. [Copyright &y& Elsevier]

Published
2005
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36. Research requires deep knowledge of the modality to be tested.

Author

Stockheimer, Kim Rock, Baltacı, Gül, Forrester, Graceann G., Frassine, Stefano, and Wolkenberg, Andrea

Abstract

A letter to the editor is presented in response to the article "Kinesio Taping does not decrease swelling in acute, lateral ankle sprain of athletes: a randomised trial" by G.S. Nunes in the 2015 issue.

Published
2016
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