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In the cooler parts of the solar atmosphere as, e.g., the chromosphere, effects due to partial ionization may be relevant for wave dynamics and heating. Aims. We study resonant Alfven waves in partially ionized plasmas. Methods. We use the multifluid equations in the cold plasma approximation. We investigate propagating resonant MHD waves in partially ionized flux "},"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":"1111.4134","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-11-17T16:15:26Z","cross_cats_sorted":[],"title_canon_sha256":"34d82f6d4e3b9c6cc358deb59fc54b93c2bedefde842c725371f092f79ac5e9f","abstract_canon_sha256":"69113ec55ced212745ef07021bfe649dfe1b2c1cf291cc2530d32a65e358f46e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:31.645190Z","signature_b64":"5jzGNceDi2lfltbrCUm876wsO1Tuyta8TKtYqNvnbSrC/24q6vypyWL38/4DrNt6g2eUuilekSyfKt1x76LxDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"34b4ec5818dde00fcc3e2724e89bf74d544aeea83e7d8fe7b8d718924747ee5b","last_reissued_at":"2026-05-18T01:59:31.644607Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:31.644607Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resonant Alfven waves in partially ionized plasmas of the solar atmosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"J. Andries, M. Goossens, R. Soler","submitted_at":"2011-11-17T16:15:26Z","abstract_excerpt":"Context. Magnetohydrodynamic (MHD) waves are ubiquitous in the solar atmosphere. In magnetic waveguides resonant absorption due to plasma inhomogeneity naturally transfers wave energy from large-scale motions to small-scale motions. In the cooler parts of the solar atmosphere as, e.g., the chromosphere, effects due to partial ionization may be relevant for wave dynamics and heating. Aims. We study resonant Alfven waves in partially ionized plasmas. Methods. We use the multifluid equations in the cold plasma approximation. 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