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- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 definition "An extended region in the solar corona where the density and temperature are lower than other places in the corona. The weak diverging and open magnetic field lines in coronal holes extend radially outward and do not immediately return to the sun. The high speed part of the solar wind comes from coronal holes. Reference: the Cambridge Encyclopedia of the Sun, The Cambridge University Press, Cambridge, CB2, 2RU, UK, 2001." @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 id "1661122" @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 path_id 1eb0ea0a-312c-4d74-8d42-6f1ad758f999 @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 path_id 2e83362e-d8f8-4bca-83fd-bae360ebe94b @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 path_id 57383ac5-614c-4b84-9202-e137b000422b @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 path_id e9f67a66-e9fc-435c-b720-ae32a2c3d8f5 @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 path_label "EARTH SCIENCE" @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 path_label "SOLAR ACTIVITY" @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 path_label "SUN-EARTH INTERACTIONS" @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 path_label "Science Keywords" @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 prefLabel "CORONA HOLES" @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 reference "From: NASA/MSFC Solar Physics: http://wwwssl.msfc.nasa.gov/ssl/pad/solar/feature3.htm" @default.
- 6a5a2ccf-3ba6-4519-bc9b-7617ef3b9087 tag "Science Keywords" @default.