Résultats de la recherche - (( (temperature OR temperaturas) decrease ) OR ( temperatura decrease ))*

X-ray Polarisation in Magnetar Atmospheres -- Effects of Mode Conversion par Kelly, Ruth M. E., Zane, Silvia, Turolla, Roberto, Taverna, Roberto

Table des matières: “… atmospheric models under varying conditions of magnetic field strength/orientation, effective temperature…”
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The polarization of the boundary layer around weakly magnetized neutron stars in X-ray binaries par Farinelli, R., Waghmare, A., Ducci, L., Santangelo, A.

Table des matières: “… temperature of the boundary layer of these systems in a soft state, the polarization degree was less then 0.5…”
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The Plasma $β$ in quiet Sun Regions: Multi-Instrument View par Rodríguez-Gómez, Jenny M., Kuckein, Christoph, Manrique, Sergio J. Gonzalez, Saqri, Jonas, Veronig, Astrid, Gomöry, Peter, Podladchikova, Tatiana

Table des matières: “… heights through the solar atmosphere based on multi-height observational data. We obtained temperature…”
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General Relativistic Hydrodynamics in Discrete Spacetime: Perfect Fluid Accretion onto Static and Spinning Black Holes par Gorard, Jonathan

Table des matières: “… in Gravitas, we discover that the mass/energy and momentum accretion rates both decrease monotonically…”
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Investigation of the Thermal Structure in the Atmospheric Boundary Layer During Evening Transition and the Impact of Aerosols on Radiative Cooling par Singh, Suryadev Pratap, Rafiuddin, Mohammad, Banerjee, Subham, R, Sreenivas K

Table des matières: “… with decreases in downward and upward longwave flux, soil sensible heat flux, wind speed, and turbulent kinetic…”
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Dynamical properties of magnetized low angular momentum accretion flow around a Kerr black hole par Dihingia, Indu K., Mizuno, Yosuke

Table des matières: “… the highest density, pressure, and temperature near the black hole, making it easier to observe. We find…”
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The ALMA Legacy survey of Class 0/I disks in Corona australis, Aquila, chaMaeleon, oPhiuchus north, Ophiuchus, Serpens (CAMPOS). I. Evolution of Protostellar disk radii par Hsieh, Cheng-Han, Arce, Héctor G., Maureira, María José, Pineda, Jaime E., Segura-Cox, Dominique, Mardones, Diego, Dunham, Michael M., Arun, Aiswarya

Table des matières: “…, the fraction of large disks with sizes above 60\,au decreases as the protostar evolves from Class 0 to Class I…”
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Temporal genomics help in deciphering neutral and adaptive patterns in the contemporary evolution of kelp populations par Reynes, Lauric, Fouqueau, Louise, Aurelle, D., Mauger, Stéphane, Destombe, Christophe, Valero, Myriam

Table des matières: “… with changes in sea surface temperature (SST) along latitudinal gradients. This finding suggests that SST may…”
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An improved correction of radial-velocity systematic for the SOPHIE spectrograph par Grouffal, S., Santerne, A., Hara, N. C., Boisse, I., Coez, S., Heidari, N., Sulis, S.

Table des matières: “… Observatory using a few instrument's housekeeping data, such as the internal pressure and temperature…”
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Stellar Characterization and a Chromospheric Activity Analysis of a K2 Sample of Planet-Hosting Stars par Loaiza-Tacuri, V., Cunha, Katia, Smith, Verne V., Quispe-Huaynasi, F., Costa-Almeida, Ellen, Ghezzi, Luan, Melendez, Jorge

Table des matières: “…Effective temperatures, surface gravities, and iron abundances were derived for 109 stars observed…”
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Electric field induction in quark-gluon plasma due to thermoelectric effects par Singh, Kamaljeet, Dey, Jayanta, Sahoo, Raghunath

Table des matières: “… in determining the induced field. Additionally, we account for the temperature evolution of QGP using different…”
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Seasonal and longitudinal variability in Io's SO2 atmosphere from 22 years of IRTF/TEXES observations par Giles, Rohini S., Spencer, John R., Tsang, Constantine C. C., Greathouse, Thomas K., Lellouch, Emmanuel, López-Valverde, Miguel A.

Table des matières: “… hemisphere can plausibly be explained by the daily Jupiter eclipses, which decrease the surface temperature…”
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Local aging effects in PuB$_{4}$: Growing inhomogeneity and slow dynamics of local-field fluctuations probed by $^{239}$Pu NMR par Blackwell, Seth B., Yamamoto, Riku, Thomas, Sean M., Dioguardi, Adam P., Cary, Samantha K., Kozimor, Stosh A., Bauer, Eric D., Ronning, Filip, Hirata, Michihiro

Table des matières: “…}$, and a signal intensity that decreases linearly by 20 % per year. The spin-spin relaxation time $T_{2…”
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Sulphur dioxide in the mid-infrared transmission spectrum of WASP-39b par Powell, Diana, Feinstein, Adina D., Lee, Elspeth K. H., Zhang, Michael, Tsai, Shang-Min, Taylor, Jake, Kirk, James, Bell, Taylor, Barstow, Joanna K., Gao, Peter, Bean, Jacob L., Blecic, Jasmina, Chubb, Katy L., Crossfield, Ian J. M., Jordan, Sean, Kitzmann, Daniel, Moran, Sarah E., Morello, Giuseppe, Moses, Julianne I., Welbanks, Luis, Yang, Jeehyun, Zhang, Xi, Ahrer, Eva-Maria, Bello-Arufe, Aaron, Brande, Jonathan, Casewell, S. L., Crouzet, Nicolas, Cubillos, Patricio E., Demory, Brice-Olivier, Dyrek, Achrène, Flagg, Laura, Hu, Renyu, Inglis, Julie, Jones, Kathryn D., Kreidberg, Laura, López-Morales, Mercedes, Lagage, Pierre-Olivier, Valdés, Erik A. Meier, Miguel, Yamila, Parmentier, Vivien, Piette, Anjali A. A., Rackham, Benjamin V., Radica, Michael, Redfield, Seth, Stevenson, Kevin B., Wakeford, Hannah R., Aggarwal, Keshav, Alam, Munazza K., Batalha, Natalie M., Batalha, Natasha E., Benneke, Björn, Berta-Thompson, Zach K., Brady, Ryan P., Caceres, Claudio, Carter, Aarynn L., Désert, Jean-Michel, Harrington, Joseph, Iro, Nicolas, Line, Michael R., Lothringer, Joshua D., MacDonald, Ryan J., Mancini, Luigi, Molaverdikhani, Karan, Mukherjee, Sagnick, Nixon, Matthew C., Oza, Apurva V., Palle, Enric, Rustamkulov, Zafar, Sing, David K., Steinrueck, Maria E., Venot, Olivia, Wheatley, Peter J., Yurchenko, Sergei N.

Table des matières: “… process in high temperature exoplanet atmospheres. This is due to the low ($<$1 ppb) abundance of SO$_2…”
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Magic silicon dioxide for widely tunable integrated photonics par Lopez-Rodriguez, Bruno, Sharma, Naresh, Li, Zizheng, van der Kolk, Roald, van der Boom, Jasper, Scholte, Thomas, Chang, Jin, Groblacher, Simon, Zadeh, Iman Esmaeil

Table des matières: “… heater. In addition, the low-temperature deposition of our silicon dioxide cladding can be combined…”
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Three-Dimensional Venus Cloud Structure Simulated by a General Circulation Model par Shao, Wencheng D., Mendonça, João M., Dai, Longkang

Table des matières: “… is overestimated above the clouds due to efficient transport in the cloud region. The cloud top decreases…”
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Microphysical Prescriptions for Parameterized Water Cloud Formation on Ultra-cool Substellar Objects par Mang, James, Morley, Caroline V., Robinson, Tyler D., Gao, Peter

Table des matières: “…, these icy clouds change the emergent spectra, temperature structure, and albedo of the substellar atmosphere…”
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Radiation Resilience of $β$-Ga$_2$O$_3$ Schottky Barrier Diodes Under High Dose Gamma Radiation par Khan, Saleh Ahmed, Saha, Sudipto, Singisetti, Uttam, Bhuiyan, A F M Anhar Uddin

Table des matières: “… reaching up to 5 Mrad (Si). Initial exposure of the diodes to 1 Mrad resulted in a significant decrease…”
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Observation of Thermal Deuteron-Deuteron Fusion in Ion Tracks par Czerski, K., Dubey, R., Kowalska, A., Das, G. Haridas, Kaczmarski, M., Targosz-Sleczka, N., Valat, M.

Table des matières: “… high beam currents at very low energies. The experimental thick target yield, decreasing over seven…”
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Optical signatures of interlayer electron coherence in a bilayer semiconductor par Liu, Xiaoling, Leisgang, Nadine, Dolgirev, Pavel E., Zibrov, Alexander A., Sung, Jiho, Wang, Jue, Taniguchi, Takashi, Watanabe, Kenji, Walther, Valentin, Park, Hongkun, Demler, Eugene, Kim, Philip, Lukin, Mikhail D.

Table des matières: “… between the excitons, which increases with electron density and decreases with temperature. We argue…”
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