Results 171 to 180 of about 3,493 (285)
Infrared polarimetry of dark clouds - II. Magnetic field structure in the Ophiuchi dark cloud [PDF]
S. Sato +7 more
openaire +1 more source
Exploiting Aeolus winds in a regional numerical weather prediction model
Aeolus measured winds have proven to be beneficial for global models. However, demonstrating positive impact for limited‐area models has been a challenge so far. For the first time, we have demonstrated a statistically significant positive impact of Aeolus winds in a limited‐area model by using the 4DVar data assimilation technique and the most recent ...
Gert‐Jan Marseille +3 more
wiley +1 more source
A two micron polarization survey toward dark clouds
A near infrared (2.2 micron) polarization survey of about 190 sources was conducted toward nearby dark clouds. The sample includes both background field stars and embedded young stellar objects. The aim is to determine the magnetic field structure in the
Gatley, I. +3 more
core
Abstract The presence of Arctic clouds plays a crucial role in the evolution of the surface temperature of Arctic sea ice. However, large biases in cloud representation remain in state‐of‐the‐art weather and climate models. In this study, we use observational data from the one‐year Arctic ship campaign Multi‐disciplinary drifting Observatory for the ...
Luise Schulte +5 more
wiley +1 more source
Small-Target Ship Detection with Joint Spatio-Temporal Features Across Multiple Frames. [PDF]
Qian Y, Hu Z, Zhang B, Yang W, Chen Q.
europepmc +1 more source
ERA5 hourly 325‐m and 1512‐m (a) convergence and (b) vertical motion (actually pressure change with sign reversed to compare with convergence) over Sable Island around the time of an event. The mist (green) and fog (red) occurrences at the surface station are shown at the bottom of the figures. A 325‐m fitted line convergence was positive for the first
Clive E. Dorman +8 more
wiley +1 more source
The Spitzer Survey of Cygnus-X and Infrared Dark Clouds
International audienceThe Cygnus-X region contains a massive star formation complex with the richest known concentration of massive protostars and the largest OB associations in the nearest 2 kpc.
Joseph L., Hora +9 more
core +1 more source
Assimilation of AMSU‐A all‐sky observations can be increased up to fivefold if spatial observation‐error correlations are accounted for properly. New correlation estimates derived using data from ECMWF and the UK Met Office reveal that correlation length‐scales are between 75 and 150 km for AMSU‐A channels peaking in the troposphere. This is attributed
Rishabh Bhatt +9 more
wiley +1 more source
Large-amplitude variability driven by giant dust storms on a planetary-mass companion. [PDF]
Tan X +19 more
europepmc +1 more source

