Zobrazeno 1 - 10
of 13 403
pro vyhledávání: '"MANDAL, S"'
Yes
The purpose of this research is to establish the necessary and sufficient conditions for food safety and security during pandemic outbreaks, focusing on the case of COVID-19 to ensure resilience of the food supply chain. The study emphasises
The purpose of this research is to establish the necessary and sufficient conditions for food safety and security during pandemic outbreaks, focusing on the case of COVID-19 to ensure resilience of the food supply chain. The study emphasises
Externí odkaz:
http://hdl.handle.net/10454/19666
Coronal loops generally trace magnetic lines of force in the upper solar atmosphere. Understanding the loop morphology and its temporal evolution has implications for coronal heating models that rely on plasma heating due to reconnection at current s
Externí odkaz:
http://arxiv.org/abs/2411.16943
Resistive Plate Chamber (RPC) is one of the most commonly used detectors in high energy physics experiments for triggering and tracking because of its good efficiency ($\textgreater$~90\%) and time resolution ($\sim$~1-2~ns). Generally, bakelite whic
Externí odkaz:
http://arxiv.org/abs/2408.07336
Autor:
De, S., Mandal, S., Sen, Sanket, Sen, Arnab, Gopal, R., Ltaief, L. Ben, Turchini, S., Catone, D., Zema, N., Coreno, M., Richter, R., Mudrich, M., Sharma, V., Krishnan, S. R.
The three-body dissociation dynamics of the dicationic camphor molecule (C$_{10}$H$_{16}$O$^{2+}$) resulting from Auger decay are investigated using soft X-ray synchrotron radiation. A photoelectron-photoion-photoion coincidence (PEPIPICO) method, a
Externí odkaz:
http://arxiv.org/abs/2406.08502
Autor:
Mandal, S., Chatterjee, S., Sen, A., Gope, S., Dhani, S., Hegde, A. C., Chatterjee, M., Das, S., Biswas, S.
Gas Electron Multiplier (GEM) is one of the mostly used gaseous detectors in the High Energy Physics (HEP) experiments. GEMs are widely used as tracking devices due to their high-rate handling capability and good position resolution. An initiative is
Externí odkaz:
http://arxiv.org/abs/2401.11104
Autor:
Nölke, J. D., Solanki, S. K., Hirzberger, J., Peter, H., Chitta, L. P., Kahil, F., Valori, G., Wiegelmann, T., Suárez, D. Orozco, Albert, K., Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Rodríguez, J. Blanco, Gandorfer, A., Germerott, D., Guerrero, L., Gutierrez-Marques, P., Kolleck, M., Iniesta, J. C. del Toro, Volkmer, R., Woch, J., Fiethe, B., Cama, J. M. Gómez, Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Rubio, L. R. Bellot, Calchetti, D., Carmona, M., Deutsch, W., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., Parejo, P. García, Blesa, J. L. Gasent, Gizon, L., Grauf, B., Heerlein, K., Korpi-Lagg, A., Lange, T., Jiménez, A. López, Maue, T., Meller, R., Vacas, A. Moreno, Müller, R., Nakai, E., Schmidt, W., Schou, J., Schühle, U., Sinjan, J., Staub, J., Strecker, H., Torralbo, I., Berghmans, D., Kraaikamp, E., Rodriguez, L., Verbeeck, C., Zhukov, A. N., Auchere, F., Buchlin, E., Parenti, S., Janvier, M., Barczynski, K., Harra, L., Schwanitz, C., Cuadrado, R. Aznar, Mandal, S., Teriaca, L., Long, D., Smith, P.
Publikováno v:
A&A 678, A196 (2023)
Extreme ultraviolet (EUV) observations of the quiet solar atmosphere reveal extended regions of weak emission compared to the ambient quiescent corona. The magnetic nature of these coronal features is not well understood. We study the magnetic proper
Externí odkaz:
http://arxiv.org/abs/2309.09789
Autor:
Ltaief, L. Ben, Sishodia, K., Richter, R., Bastian, B., Asmussen, J. D., Mandal, S., Pal, N., Medina, C., Krishnan, S. R., von Haeften, K., Mudrich, M.
Interatomic Coulombic decay (ICD) processes play a crucial role in weakly bound complexes exposed to intense or high-energy radiation. Using large helium nanodroplets, we demonstrate that ICD is efficient even when the droplets are irradiated by weak
Externí odkaz:
http://arxiv.org/abs/2308.14674
Autor:
Chitta, L. P., Zhukov, A. N., Berghmans, D., Peter, H., Parenti, S., Mandal, S., Cuadrado, R. Aznar, Schühle, U., Teriaca, L., Auchère, F., Barczynski, K., Buchlin, É., Harra, L., Kraaikamp, E., Long, D. M., Rodriguez, L., Schwanitz, C., Smith, P. J., Verbeeck, C., Seaton, D. B.
Publikováno v:
Science 381, 867-872 (2023)
Coronal holes are areas on the Sun with open magnetic field lines. They are a source region of the solar wind, but how the wind emerges from coronal holes is not known. We observed a coronal hole using the Extreme Ultraviolet Imager on the Solar Orbi
Externí odkaz:
http://arxiv.org/abs/2308.13044
Autor:
Chitta, L. P., Solanki, S. K., Iniesta, J. C. del Toro, Woch, J., Calchetti, D., Gandorfer, A., Hirzberger, J., Kahil, F., Valori, G., Suárez, D. Orozco, Strecker, H., Appourchaux, T., Volkmer, R., Peter, H., Mandal, S., Cuadrado, R. Aznar, Teriaca, L., Schühle, U., Berghmans, D., Verbeeck, C., Zhukov, A. N., Priest, E. R.
Publikováno v:
ApJL 956, L1 (2023)
Arch-like loop structures filled with million Kelvin hot plasma form the building blocks of the quiet-Sun corona. Both high-resolution observations and magnetoconvection simulations show the ubiquitous presence of magnetic fields on the solar surface
Externí odkaz:
http://arxiv.org/abs/2308.10982
Autor:
Antolin, P., Dolliou, A., Auchère, F., Chitta, L. P., Parenti, S., Berghmans, D., Cuadrado, R. Aznar, Barczynski, K., Gissot, S., Harra, L., Huang, Z., Janvier, M., Kraaikamp, E., Long, D. M., Mandal, S., Peter, H., Rodriguez, L., Schühle, U., Smith, P. J., Solanki, S. K., Stegen, K., Teriaca, L., Verbeeck, C., West, M. J., Zhukov, A. N., Appourchaux, T., Aulanier, G., Buchlin, E., Delmotte, F., Gilles, J. M., Haberreiter, M., Halain, J. -P., Heerlein, K., Hochedez, J. -F., Gyo, M., Poedts, S., Rochus, P.
Publikováno v:
A&A 676, A112 (2023)
Coronal rain is the most dramatic cooling phenomenon of the solar corona and an essential diagnostic tool for the coronal heating properties. A puzzling feature of the solar corona, besides the heating, is its EUV filamentary structure and variabilit
Externí odkaz:
http://arxiv.org/abs/2305.11691