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T1  - The Temporal and Spatial Scales of Density Structures Released in the Slow Solar Wind During Solar Activity Maximum 
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UR  - http://hdl.handle.net/10138/230196 
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A1  - Sanchez-Diaz, E.; Rouillard, A. P.; Davies, J. A.; Lavraud, B.; Pinto, R. F.; Kilpua, E. 
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Y1  - 2017 
LA  - eng 
AB  - In a recent study, we took advantage of a highly tilted coronal neutral sheet to show that density structures, extending radially over several solar radii (R-s), are released in the forming slow solar wind approximately 4-5 R-s above the solar surface. We related the signatures of this formation process to intermittent magnetic reconnection occurring continuously above helmet streamers. We now exploit the heliospheric imagery from the Solar Terrestrial Relation Observatory (STEREO) to map the sp... 
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KW  - methods: observational; solar wind; Sun: corona; Sun: general; Sun: heliosphere; Techniques: image processing; HELIOSPHERIC PLASMA SHEETS; DYNAMICS-OBSERVATORY SDO; HEAT-FLUX DROPOUTS; 1 AU; MAGNETOHYDRODYNAMIC MODELS; MAGNETIC-FIELDS; CORONAL INFLOWS; STREAMER BLOBS; RECONNECTION; SUN; 115 Astronomy, Space science 
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