Ionization Efficiency in the Dayside Ma...

Neutral densities, ionization rates, and ionization efficiencies for CO2 (blue) and O (r...

Ionization Efficiency in the Dayside Ma...

Altitude profiles of CO2 (left) and O (right) ionization efficiencies for the 240 nomina...

Ionization Efficiency in the Dayside Ma...

Diurnal (top) and solar cycle (bottom) variations of CO2 (blue) and O (red) ionization e...

Ionization Efficiency in the Dayside Ma...

Distribution of CO2 ionization efficiency at the top of the dayside Martian upper atmosp...

Optimal Target Stars in the Search for ...

Relative benefit Δ of an ideal search strategy as a function of stellar mass. The blue c...

Optimal Target Stars in the Search for ...

Relative benefit Δ for a direct-imaging search strategy as a function of stellar mass. T...

Optimal Target Stars in the Search for ...

Relative benefit Δ for a transmission spectroscopy search strategy as a function of stel...

A Long Decay of X-Ray Flux and Spectral...

Left: XMM-Newton PN spectra for GSN 069  along with the best-fitted models (top panel)....

A Long Decay of X-Ray Flux and Spectral...

Upper panel: historical flux light curve in the 0.2–2 keV for GSN 069. The Swift data a...

A Long Decay of X-Ray Flux and Spectral...

Upper panel: the best-fitting χ2 values are plotted against the actual time of TDE from ...

A Long Decay of X-Ray Flux and Spectral...

Upper panel: joint 68% (dotted) and 99% (solid) confidence contours of the blackbody tem...

von Kármán–Howarth Equation for Hall Ma...

Power spectral densities of (red) the magnetic field, (blue) the proton velocity field, ...

von Kármán–Howarth Equation for Hall Ma...

Second-order structure functions of (red) the magnetic field, (blue) the proton velocity...

von Kármán–Howarth Equation for Hall Ma...

Exact law in hybrid simulations βi = 1/16, βi = 1/2, and βi = 4: The cascade rate, ϵ*, n...

Models of Tidally Induced Gas Filaments...

Orbit of the SMC around the LMC in the model with a 9:1 mass ratio. The orbit before ent...

Models of Tidally Induced Gas Filaments...

Tidal interaction between SMC and LMC before infall to the MW potential in the model wit...

Models of Tidally Induced Gas Filaments...

MS in gas according to our simulation with a 9:1 LMC–SMC mass ratio. The top three panel...

Models of Tidally Induced Gas Filaments...

Dynamical age of the Stream in the model with a 9:1 mass ratio color-coded by time since...

Models of Tidally Induced Gas Filaments...

MS in the stellar component according to our simulation with a 9:1 LMC–SMC mass ratio. T...

Models of Tidally Induced Gas Filaments...

Line-of-sight velocity (in the frame of the local standard of rest) to the MS in the 9:1...

Models of Tidally Induced Gas Filaments...

Representation in Magellanic Stream coordinates for interactions with different mass rat...

Models of Tidally Induced Gas Filaments...

Percentage of material stripped from both Clouds during their mutual interaction. The da...

A Short-term ESPERTA-based Forecast Too...

Intensity time profiles for the 41 “Hit” (correctly predicted) ≥S2 > 10 MeV proton event...

A Short-term ESPERTA-based Forecast Too...

ESPERTA probability contours for the prediction of ≥S1 SPEs for three solar longitude ba...

A Short-term ESPERTA-based Forecast Too...

ESPERTA probability contours for prediction of ≥S2 SPEs for three solar longitude bands....