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2040 greenhouse gas reduction targets and energy transitions in line with the EU Green Deal. [PDF]
Rodrigues R +11 more
europepmc +1 more source
Temporal Dynamics of Airborne Bacterial and Fungal Communities in Megacity Shanghai: Diel Asynchrony, Environmental Drivers, and Cold Front Perturbations. [PDF]
Wang J, Li L, Wang Y, Sun W, Cheng T.
europepmc +1 more source
Effectiveness and feasibility of residential passive heat adaptation interventions on reducing indoor temperature in low-income communities in Africa: a systematic review. [PDF]
Nakanjako R +8 more
europepmc +1 more source
SWFITEM: Solar Wind Fitting for Investigations of Thermodynamics and Energetics at Mars - A MAVEN dataset. [PDF]
Ramstad R +10 more
europepmc +1 more source
A theory for the origin of the slow solar wind is described. Recent papers have demonstrated that magnetic flux moves across coronal holes as a result of the interplay between the differential rotation of the photosphere and the non-radial expansion of the solar wind in more rigidly rotating coronal holes.
Thomas Zurbuchen +2 more
exaly +3 more sources
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Advances in Space Research, 2004
Abstract The origin and location of the slow wind are interesting subjects on their own and also they are important in the matter of the origin of the fast wind especially if the slow wind originates directly from a coronal hole. We have been studying the solar wind whose speed is comparative to or a little slower than that measured in the ...
Munetoshi Tokumaru +2 more
exaly +2 more sources
Abstract The origin and location of the slow wind are interesting subjects on their own and also they are important in the matter of the origin of the fast wind especially if the slow wind originates directly from a coronal hole. We have been studying the solar wind whose speed is comparative to or a little slower than that measured in the ...
Munetoshi Tokumaru +2 more
exaly +2 more sources
On the Sources of Fast and Slow Solar Wind [PDF]
The slow speed solar wind as measured at the Earth orbit and beyond is characterized by its velocity of ≃400 km s−1, by its coronal composition and by its frozen‐in temperature (from carbon charge‐states) of 1.4–1.6 × 106 K. In contrast the fast speed solar wind is characterized by its velocity of ≃750 km s−1, its nearly photospheric composition and ...
Nathan Schwadron, Landi Enrico
exaly +2 more sources

