Results 51 to 60 of about 1,126,700 (167)

PROSWIN: Probabilistic Solar Wind Speed Forecasting Using Deep Distributional Regression From Solar Images

AGU Advances, Volume 7, Issue 8, November 2026.
Abstract Accurately predicting fast solar wind conditions is challenging, as uncertainties are large and unquantified by traditional single‐value prediction models. In particular, the risks of high‐speed solar wind streams (HSSs), which can cause damage to technological infrastructure, cannot be reliably assessed without probabilistic forecasts.
Daniel Collin, Yuri Shprits, Luca Chiarabini, Stefan J. Hofmeister, Nadja Klein, Guillermo Gallego   +5 more
wiley   +1 more source

Unusually complex phase of dense nitrogen at extreme conditions

, 2018
This dataset contains DFT enthalpies (PBE and PBE+TS), Raman spectra and AIRSS search generators supporting the paper "Unusually Complex Phase of Dense Nitrogen at Extreme Conditions" published in Nature Communications.Martinez-Canales, Miguel. (2018). i-
School of Physics and Astronomy, Martinez-Canales, Miguel   +1 more
core   +1 more source

Surface Modification of Solids by Extreme Ultraviolet and Plasma Treatment [PDF]

, 2018
In this paper, results of surface modification, using a laser-produced plasma source of extreme ultraviolet, and the extreme ultraviolet induced low temperature plasmas, are presented.
W. Skrzeczanowski, Fiedorowicz, H., Wachulak, P., J. Czwartos, Czwartos, J., P. Wachulak, A. Bartnik, J. Kostecki, R. Jarocki, Bartnik, A., H. Fiedorowicz, Jarocki, R., Kostecki, J., Skrzeczanowski, W.   +13 more
core   +1 more source

Are Coronal Loops Projection Effects?

The Astrophysical Journal
We report results of an in-depth numerical investigation of three-dimensional projection effects that could influence the observed loop-like structures in an optically thin solar corona.
Vadim M. Uritsky, James A. Klimchuk
doaj   +1 more source

When Laboratory Studies of Plumes Shed the Veil of the Enceladus' Interior

Journal of Geophysical Research: Planets, Volume 131, Issue 11, November 2026.
Abstract Since the discovery by Cassini of plumes of water vapor and icy particles erupting from the South Polar Terrain (SPT) of Enceladus, numerous numerical models have been proposed to explain the mechanism driving these plumes, and how they relate to the thermodynamic conditions inside the underlying crevasses.
Yaël R. A. Bourgeois, Stéphanie M. Cazaux, Fabrizio Giordano   +2 more
wiley   +1 more source

Employing partially coherent, compact gas-discharge sources for coherent diffractive imaging with extreme ultraviolet light

, 2015
Coherent diffractive imaging (CDI) and related techniques enable a new type of diffraction-limited high-resolution extreme ultraviolet (EUV) microscopy.
Juschkin, L., Miao, Jianwei, Grützmacher, D., Jianwei Miao, Odstrčil, M., Brocklesby, W. S., D. Rudolf, W. S. Brocklesby, R. Bresenitz, D. Grützmacher, J. Bußmann, Odstrčil, Michal, Brocklesby, William S., Juschkin, Larissa, Bußmann, J., Brocklesby, W.S., Bresenitz, R., Rudolf, Denis, Rudolf, D., L. Juschkin, Miao, J., M. Odstrčil, Bußmann, Johannes   +22 more
core   +1 more source

3D mask effects in high NA EUV imaging

, 2022
Art. 109570Z, 13 S.Understanding, characterization and management of 3D mask effects, including non-telecentricity, contrast fading and best focus shifts, become increasingly important for the performance optimization of future extreme ultraviolet (EUV ...
Evanschitzky, P., Fliervoet, T., Erdmann, A., Setten, E. van, Bottiglieri, G.   +4 more
core   +1 more source

Empirical Prediction of Plasma Emission Measure Distributions and X-Ray/Extreme-ultraviolet Spectra of Late-type Stars

The Astrophysical Journal
High-energy emission spectra from the outer atmospheres of late-type stars represent an important feature of the stellar activity in several contexts, such as the photoevaporation and photochemistry of planetary atmospheres or the modeling of irradiated ...
A. Maggio, I. Pillitteri, J. Sanz-Forcada, G. Micela   +3 more
doaj   +1 more source

Global Ionospheric Responses to Four X‐Class Solar Flares in November 2025

Space Weather, Volume 24, Issue 11, November 2026.
Abstract We investigate global ionospheric responses to four X‐class solar‐disk flares that occurred in November 2025 from the same solar active region, using multi‐instrument observations including GNSS, ionosonde, geomagnetic and GOES solar irradiance data. Pronounced dayside TEC enhancements are observed for three flares (#2 X1.2, #3 X5.1, and #4 X4.
Lei Liu, Shasha Zou
wiley   +1 more source

The Effect of Field Line Tracing Height on Wang‐Sheeley‐Arge Solar Wind Predictions at Earth

Space Weather, Volume 24, Issue 11, November 2026.
Abstract A key component of the widely used Wang‐Sheeley‐Arge model is the tracing of magnetic field lines in the solar corona, as that largely determines the modeled open/closed field regions and in turn the predicted large‐scale solar wind structure. However, small closed field regions interspersed among the open field lines inside coronal holes (CHs)
Satabdwa Majumdar, Martin A. Reiss, Pete Riley, Charles N. Arge   +3 more
wiley   +1 more source