Differences in Convection Following Initiation Fig. 3: As in Fig. 2, but at ten days after convective initiation. Differences in Convection Following Initiation.
1 GALEX Angular Correlation Function … or about the Galactic extinction effects.
By Alicia Thompson
HST/WFPC2 F606W
Differences in Convection Following Initiation
Bayesian f lux reconstruction in one and two bands
Green Events
Geomagnetic field
Geomagnetic field Inclination Fig S1. Long-wavelength part of the geomagnetic field at Earth’s surface (International Geomagnetic Reference Model, IGRF.
Differential cross section in deuteron-proton elastic scattering at 1.25 GeV/u
