{"record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.topic/1","content_sha256":"ae0a83119b651da6ea8a0aa0f78736a7ca247aa43a9d0d136c2aa862c930c69e","created":"2026-10-03T07:17:50Z","files":[],"origin":{"assisted_by":[],"kind":"seed"},"parents":[],"salt":"566d49785f6f25fd30877c625aa9fc302232db010907bf935a77f8523e3f7bf6","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"topic"},"content":{"external_id":"astro.solar-corona-wind","field":"astro","n":"1","review_cite":"J. A. Klimchuk, On solving the coronal heating problem, Solar Physics, 2006","review_link":"https://arxiv.org/abs/astro-ph/0511841","review_verified":"true","summary":"The Sun's outer atmosphere (corona) is over a million kelvin while its surface is about 6000 K, and it blows a continuous wind of charged particles into space. How the corona is heated and how the wind is launched are not fully explained.","title":"Solar corona heating and solar wind","topic_ref":null,"why":"The corona and wind drive the space weather that affects satellites and power grids, and are the nearest laboratory for magnetized plasma heating."},"attested":{"attestation":{"batch":null,"client_id":null,"id_token_sha256":null,"kind":"platform"},"record_hash":"065c0eeceaa7f840ee16fc5402d7cfeff05073c085c4558fd4ac6d41a8197c11","schema":"pubphys.attested/1"},"envelope":{"attested_hash":"bab8b053ad42f1ca29cfbe722c553b1bb924e45a3181b23db2ff5fa3bc988080","platform_signature":{"key_id":"c6afc19b31429869751f06879c75cd64ea92654423d15b44be775bf1310a60da","sig":"Gp1y4zKlXqE23fLhrOzl1zFBM2GB0GQaQ4lS5VBspH5jjEE1jr9jdGvEuLNXiy8DvvptYdB5AZbyepuUMs6rAQ"},"schema":"pubphys.envelope/1"},"record_hash":"065c0eeceaa7f840ee16fc5402d7cfeff05073c085c4558fd4ac6d41a8197c11","leaf_index":53}