Zobrazeno 1 - 10
of 11 955
pro vyhledávání: '"Rempel A"'
Autor:
Griesemer, Tina, Ximenes, Rui Franqueira, Izquierdo, Gonzalo Arnau, Santillana, Ignacio Aviles, Brehm, Thomas, Terricabras, Adria Gallifa, Höll, Stefan, Jacobsson, Richard, Kaiser, Marco, Kuchar, Roman, Fontenla, Ana Teresa Pérez, Rempel, Alexey, De Frutos, Oscar Sacristan, Schienbein, Marcel, Sgobba, Stefano, Calviani, Marco
The Beam Dump Facility (BDF) is a planned fixed-target installation in CERN's North Area, set to start operating in 2031. A proton beam of 400 GeV/c will be delivered in 1 s pulses of 4e13 protons every 7.2 s, amounting to 4e19 protons on target (PoT
Externí odkaz:
http://arxiv.org/abs/2410.01964
On 2024 May 10/11, the strongest geomagnetic storm since November 2003 has occurred, with a peak Dst index of -412 nT. The storm was caused by NOAA Active Region (AR) 13664, which was the source of a large number of coronal mass ejections and flares,
Externí odkaz:
http://arxiv.org/abs/2409.08124
Autor:
Vikhorev, Alexandr V., Rempel, Michael M., Polesskaya, Oksana O., Savelev, Ivan V., Myakishev-Rempel, Max V.
Transposable elements (TEs) constitute a significant portion of eukaryotic genomes, yet their role in chromatin organization remains poorly understood. This study investigates the distribution patterns of TEs around chromatin ligation points (LPs) id
Externí odkaz:
http://arxiv.org/abs/2408.11079
Autor:
Santos, J. M. da Silva, Molnar, M., Milić, I., Rempel, M., Reardon, K., Rodríguez, J. de la Cruz
Accurately assessing the balance between acoustic wave energy fluxes and radiative losses is critical for understanding how the solar chromosphere is thermally regulated. We investigate the energy balance in the chromosphere by comparing deposited ac
Externí odkaz:
http://arxiv.org/abs/2408.15908
Autor:
Yang, Kai E., Tarr, Lucas A., Rempel, Matthias, Dodds, S. Curt, Jaeggli, Sarah A., Sadowski, Peter, Schad, Thomas A., Cunnyngham, Ian, Liu, Jiayi, Glaser, Yannik, Sun, Xudong
The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will provide high-resolution, multi-line spectropolarimetric observations that are poised to revolutionize our understanding of the Sun. Given the massive data volume, novel i
Externí odkaz:
http://arxiv.org/abs/2407.20309
In this paper, we study the Cauchy problem for the linear plate equation with mass term and its applications to semilinear models. For the linear problem we obtain $L^p-L^q$ estimates for the solutions in the full range $1\leq p\leq q\leq \infty$, an
Externí odkaz:
http://arxiv.org/abs/2406.17211
Autor:
Rodriguez, Sebastian, Dumpala, Sri Harsha, Dikaios, Katerina, Rempel, Sheri, Uher, Rudolf, Oore, Sageev
Current automatic depression detection systems provide predictions directly without relying on the individual symptoms/items of depression as denoted in the clinical depression rating scales. In contrast, clinicians assess each item in the depression
Externí odkaz:
http://arxiv.org/abs/2406.16000
Generating Synthetic Rainfall Fields by R-vine Copulas Applied to Seamless Probabilistic Predictions
Publikováno v:
Quarterly Journal of the Royal Meteorological Society, 150(762), 3078-3098 (2024)
Many post-processing methods improve forecasts at individual locations but remove their correlation structure, which is crucial for predicting larger-scale events like total precipitation amount over areas such as river catchments that are relevant f
Externí odkaz:
http://arxiv.org/abs/2404.13487
Autor:
Bahauddin, Shah Mohammad, Fischer, Catherine E., Rast, Mark P., Milic, Ivan, Woeger, Friedrich, Rempel, Matthias, Keys, Peter H., Rimmele, Thomas R.
We present an interpretation of the recent Daniel K. Inouye Solar Telescope (DKIST) observations of propagating wavefronts in the lower solar atmosphere. Using MPS/University of Chicago MHD (MURaM) radiative magnetohydrodynamic simulations spanning s
Externí odkaz:
http://arxiv.org/abs/2403.13987
Autor:
Mani, Prasad, Hanson, Chris S., Dhanpal, Siddarth, Hanasoge, Shravan, Das, Srijan Bharati, Rempel, Matthias
Magnetic flux emergence from the convection zone into the photosphere and beyond is a critical component of the behaviour of large-scale solar magnetism. Flux rarely emerges amid field-free areas at the surface, but when it does, the interaction betw
Externí odkaz:
http://arxiv.org/abs/2403.00295