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Full-Sun observations for identifying the source of the slow solar wind
DOI: 10.1038/ncomms6947 Bibcode: 2015NatCo...6.5947B

Warren, Harry P.; Ugarte-Urra, Ignacio; Brooks, David H.

Fast (>700 km s-1) and slow (~400 km s-1) winds stream from the Sun, permeate the heliosphere and influence the near-Earth environment. While the fast wind is known to emanate primarily from polar coronal holes, the source of the slow wind remains unknown. Here we identify possible sites of origin using a slow solar wind s…

2015 Nature Communications
Hinode 149
Using the transit of Venus to probe the upper planetary atmosphere
DOI: 10.1038/ncomms8563 Bibcode: 2015NatCo...6.7563R

Piccioni, Giuseppe; Reale, Fabio; Widemann, Thomas +3 more

During a planetary transit, atoms with high atomic number absorb short-wavelength radiation in the upper atmosphere, and the planet should appear larger during a primary transit observed in high-energy bands than in the optical band. Here we measure the radius of Venus with subpixel accuracy during the transit in 2012 observed in the optical, ultr…

2015 Nature Communications
Hinode VenusExpress 5