{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:ZQBVXI5X2CXN3P6L7O3AFKIR3N","short_pith_number":"pith:ZQBVXI5X","schema_version":"1.0","canonical_sha256":"cc035ba3b7d0aeddbfcbfbb602a911db79ade9f8b8015243f72e5dffc3c19fc1","source":{"kind":"arxiv","id":"2411.16339","version":1},"attestation_state":"computed","paper":{"title":"Solaris: A Foundation Model of the Sun","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","cs.LG","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Francesco Tudisco, Harris Abdul Majid, Pietro Sittoni","submitted_at":"2024-11-25T12:36:15Z","abstract_excerpt":"Foundation models have demonstrated remarkable success across various scientific domains, motivating our exploration of their potential in solar physics. In this paper, we present Solaris, the first foundation model for forecasting the Sun's atmosphere. We leverage 13 years of full-disk, multi-wavelength solar imagery from the Solar Dynamics Observatory, spanning a complete solar cycle, to pre-train Solaris for 12-hour interval forecasting. Solaris is built on a large-scale 3D Swin Transformer architecture with 109 million parameters. We demonstrate Solaris' ability to generalize by fine-tunin"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2411.16339","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-11-25T12:36:15Z","cross_cats_sorted":["astro-ph.IM","cs.LG","physics.space-ph"],"title_canon_sha256":"75705c0641dd3bc2f0d7f989ded163c3b578d82f2ac69b8f5322acd0b54b601f","abstract_canon_sha256":"0ff0b9f38b53d5ed7d9901f8860b125d5e142d0ffbce92331534c7d384f92d1b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:40:07.881195Z","signature_b64":"14se+NFUN2eOyHNL7IuRHzyLA4iYUQpH7pQWHPuLGVjpnLdyYFev4mm6f9v0wxUII7kgBja7359I1dZJVQfKBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc035ba3b7d0aeddbfcbfbb602a911db79ade9f8b8015243f72e5dffc3c19fc1","last_reissued_at":"2026-07-05T09:40:07.880788Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:40:07.880788Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solaris: A Foundation Model of the Sun","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","cs.LG","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Francesco Tudisco, Harris Abdul Majid, Pietro Sittoni","submitted_at":"2024-11-25T12:36:15Z","abstract_excerpt":"Foundation models have demonstrated remarkable success across various scientific domains, motivating our exploration of their potential in solar physics. In this paper, we present Solaris, the first foundation model for forecasting the Sun's atmosphere. We leverage 13 years of full-disk, multi-wavelength solar imagery from the Solar Dynamics Observatory, spanning a complete solar cycle, to pre-train Solaris for 12-hour interval forecasting. Solaris is built on a large-scale 3D Swin Transformer architecture with 109 million parameters. We demonstrate Solaris' ability to generalize by fine-tunin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.16339","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.16339/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2411.16339","created_at":"2026-07-05T09:40:07.880846+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.16339v1","created_at":"2026-07-05T09:40:07.880846+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.16339","created_at":"2026-07-05T09:40:07.880846+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZQBVXI5X2CXN","created_at":"2026-07-05T09:40:07.880846+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZQBVXI5X2CXN3P6L","created_at":"2026-07-05T09:40:07.880846+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZQBVXI5X","created_at":"2026-07-05T09:40:07.880846+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2511.22958","citing_title":"Contrastive Heliophysical Image Pretraining for Solar Dynamics Observatory Records","ref_index":43,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N","json":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N.json","graph_json":"https://pith.science/api/pith-number/ZQBVXI5X2CXN3P6L7O3AFKIR3N/graph.json","events_json":"https://pith.science/api/pith-number/ZQBVXI5X2CXN3P6L7O3AFKIR3N/events.json","paper":"https://pith.science/paper/ZQBVXI5X"},"agent_actions":{"view_html":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N","download_json":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N.json","view_paper":"https://pith.science/paper/ZQBVXI5X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.16339&json=true","fetch_graph":"https://pith.science/api/pith-number/ZQBVXI5X2CXN3P6L7O3AFKIR3N/graph.json","fetch_events":"https://pith.science/api/pith-number/ZQBVXI5X2CXN3P6L7O3AFKIR3N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N/action/storage_attestation","attest_author":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N/action/author_attestation","sign_citation":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N/action/citation_signature","submit_replication":"https://pith.science/pith/ZQBVXI5X2CXN3P6L7O3AFKIR3N/action/replication_record"}},"created_at":"2026-07-05T09:40:07.880846+00:00","updated_at":"2026-07-05T09:40:07.880846+00:00"}