Zobrazeno 1 - 10
of 14 470
pro vyhledávání: '"Heinemann, P"'
Autor:
Bouvet, Pierre, Bevilacqua, Carlo, Ambekar, Yogeshwari, Antonacci, Giuseppe, Au, Joshua, Caponi, Silvia, Chagnon-Lessard, Sophie, Czarske, Juergen, Dehoux, Thomas, Fioretto, Daniele, Fu, Yujian, Guck, Jochen, Hamann, Thorsten, Heinemann, Dag, Jähnke, Torsten, Jean-Ruel, Hubert, Kabakova, Irina, Koski, Kristie, Koukourakis, Nektarios, Krause, David, Cavera III, Salvatore La, Landes, Timm, Li, Jinhao, Margueritat, Jeremie, Mattarelli, Maurizio, Monaghan, Michael, Overby, Darryl R., Perez-Cota, Fernando, Pontecorvo, Emanuele, Prevedel, Robert, Ruocco, Giancarlo, Sandercock, John, Scarcelli, Giuliano, Scarponi, Filippo, Testi, Claudia, Török, Peter, Vovard, Lucie, Weninger, Wolfgang, Yakovlev, Vladislav, Yun, Seok-Hyun, Zhang, Jitao, Palombo, Francesca, Bilenca, Alberto, Elsayad, Kareem
Brillouin Light Scattering (BLS) spectroscopy is a non-invasive, non-contact, label-free optical technique that can provide information on the mechanical properties of a material on the sub-micron scale. Over the last decade it has seen increased app
Externí odkaz:
http://arxiv.org/abs/2411.11712
Autor:
Heinemann, Lena, Jaus, Alexander, Marinov, Zdravko, Kim, Moon, Spadea, Maria Francesca, Kleesiek, Jens, Stiefelhagen, Rainer
Within this work, we introduce LIMIS: The first purely language-based interactive medical image segmentation model. We achieve this by adapting Grounded SAM to the medical domain and designing a language-based model interaction strategy that allows r
Externí odkaz:
http://arxiv.org/abs/2410.16939
The main hurdle of planet formation theory is the metre-scale barrier. One of the most promising ways to overcome it is via the streaming instability (SI). Unfortunately, the mechanism responsible for the onset of this instability remains mysterious.
Externí odkaz:
http://arxiv.org/abs/2408.07441
Autor:
Asai, Shoji, Ballarino, Amalia, Bose, Tulika, Cranmer, Kyle, Cyr-Racine, Francis-Yan, Demers, Sarah, Geddes, Cameron, Gershtein, Yuri, Heeger, Karsten, Heinemann, Beate, Hewett, JoAnne, Huber, Patrick, Mahn, Kendall, Mandelbaum, Rachel, Maricic, Jelena, Merkel, Petra, Monahan, Christopher, Murayama, Hitoshi, Onyisi, Peter, Palmer, Mark, Raubenheimer, Tor, Sanchez, Mayly, Schnee, Richard, Seidel, Sally, Seo, Seon-Hee, Thaler, Jesse, Touramanis, Christos, Vieregg, Abigail, Weinstein, Amanda, Winslow, Lindley, Yu, Tien-Tien, Zwaska, Robert
This is the report from the 2023 Particle Physics Project Prioritization Panel (P5) approved by High Energy Physics Advisory Panel (HEPAP) on December 8, 2023. The final version was made public on May 8, 2024 and submitted to DOE SC and NSF MPS.
Externí odkaz:
http://arxiv.org/abs/2407.19176
Autor:
Adan, Danyer Perez, Banos, Luis Ignacio Estevez, Cass, Tony, Felkers, Bjoern, Guzman, Fernando, Hartmann, Thomas, Heinemann, Beate, Jung, Hannes, Kemp, Yves, Lehner, Frank, Nicklaus, Jürgen, Menendez, David Gutierrez, Rodriguez, Sandra Consuegra, Trapaga, Cesar Garcia, Vaillant, Lidice, Walker, Rodney
In August 2023, IT experts and scientists came together for a workshop to discuss the possibilities of building a computer cluster fully on renewable energies, as a test-case at Havana University in Cuba. The discussion covered the scientific needs f
Externí odkaz:
http://arxiv.org/abs/2404.07665
Autor:
Piantschitsch, I., Terradas, J., Soubrie, E., Heinemann, S. G., Hofmeister, S. J., Soler, R., Temmer, M.
The geometry of a coronal hole (CH) affects the density profile of the reflected part of an incoming global coronal wave (CW). In this study, we perform for the first time magnetohydrodynamic (MHD) simulations of fast-mode MHD waves interacting with
Externí odkaz:
http://arxiv.org/abs/2403.06614
Autor:
Heinemann, Stephan G., Owens, Mathew J., Temmer, Manuela, Turtle, James A., Arge, Charles N., Henney, Carl J., Pomoell, Jens, Asvestari, Eleanna, Linker, Jon A., Downs, Cooper, Caplan, Ronald M., Hofmeister, Stefan J., Scolini, Camilla, Pinto, Rui F., Madjarska, Maria S.
Coronal holes are recognized as the primary sources of heliospheric open magnetic flux (OMF). However, a noticeable gap exists between in-situ measured OMF and that derived from remote sensing observations of the Sun. In this study, we investigate th
Externí odkaz:
http://arxiv.org/abs/2402.12805
High-speed solar wind streams (HSSs) interact with the preceding ambient solar wind to form Stream Interaction Regions (SIRs), which are a primary source of recurrent geomagnetic storms. However, HSSs may also encounter and subsequently interact with
Externí odkaz:
http://arxiv.org/abs/2402.08065
Autor:
Carcaboso, F., Dumbovic, M., Kay, C., Lario, D., Jian, L. K., Wilson III, L. B., Gómez-Herrero, R., Temmer, M., Heinemann, S. G., Nieves-Chinchilla, T., Veronig, A. M.
A fast and wide Coronal Mass Ejection (CME) erupted from the Sun on 2012-03-13. Its interplanetary counterpart was detected in situ two days later by STEREO-A and near-Earth spacecraft. We suggest that at 1 au the CME extended at least 110$^\circ$ in
Externí odkaz:
http://arxiv.org/abs/2401.17501
This study addresses the critical need for high signal-to-noise ratio in optical detection methods for biological sample discrimination under low-photon-flux conditions to ensure accuracy without compromising sample integrity. We explore polarization
Externí odkaz:
http://arxiv.org/abs/2401.10789