{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2023,4,13]],"date-time":"2023-04-13T08:28:01Z","timestamp":1681374481661},"reference-count":8,"publisher":"Cambridge University Press (CUP)","issue":"S325","license":[{"start":{"date-parts":[[2017,5,30]],"date-time":"2017-05-30T00:00:00Z","timestamp":1496102400000},"content-version":"unspecified","delay-in-days":241,"URL":"https:\/\/www.cambridge.org\/core\/terms"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Proc. IAU"],"published-print":{"date-parts":[[2016,10]]},"abstract":"<jats:title>Abstract<\/jats:title><jats:p>The structure of photospheric magnetic fields outside sunspots is investigated in three active regions using Hinode\/Solar Optical Telescope(SOT) observations. We analyze Zeeman effect in FeI 6301.5 and FeI 6302.5 lines and determine the observed magnetic field value <jats:italic>B<\/jats:italic><jats:sub>eff<\/jats:sub> for each of them. We find that the line ratio <jats:italic>B<\/jats:italic><jats:sub>eff<\/jats:sub>(6301)\/<jats:italic>B<\/jats:italic><jats:sub>eff<\/jats:sub>(6302) is close to 1.3 in the range <jats:italic>B<\/jats:italic><jats:sub>eff<\/jats:sub> &lt; 0.2 <jats:italic>kG<\/jats:italic>, and close to 1.0 for 0.8 <jats:italic>kG<\/jats:italic> &lt; <jats:italic>B<\/jats:italic><jats:sub>eff<\/jats:sub> &lt; 1.2 <jats:italic>kG<\/jats:italic>. We find that the observed magnetic field is formed by flux tubes with the magnetic field strengths 1.3 \u2212 2.3 <jats:italic>kG<\/jats:italic> even in places with weak observed magnetic field fluxes. We also estimate the diameters of smallest magnetic flux tubes to be 15 \u2212 20 <jats:italic>km<\/jats:italic>.<\/jats:p>","DOI":"10.1017\/s1743921316013016","type":"journal-article","created":{"date-parts":[[2017,5,30]],"date-time":"2017-05-30T07:04:51Z","timestamp":1496127891000},"page":"59-62","source":"Crossref","is-referenced-by-count":2,"title":["Investigation of Spatially Unresolved Magnetic Field Outside Sunspots Using Hinode\/SOT Observations"],"prefix":"10.1017","volume":"12","author":[{"given":"Olga","family":"Botygina","sequence":"first","affiliation":[]},{"given":"Mykola","family":"Gordovskyy","sequence":"additional","affiliation":[]},{"given":"Vsevolod","family":"Lozitsky","sequence":"additional","affiliation":[]}],"member":"56","published-online":{"date-parts":[[2017,5,30]]},"reference":[{"key":"S1743921316013016_ref008","doi-asserted-by":"publisher","DOI":"10.1007\/s00159-013-0066-3"},{"key":"S1743921316013016_ref004","first-page":"50","volume":"5","author":"Lozitsky","year":"1989","journal-title":"Kinematika i Fizika Neb. Tel"},{"key":"S1743921316013016_ref002","first-page":"741","volume":"407","author":"Cerdena","year":"2003","journal-title":"AandA"},{"key":"S1743921316013016_ref001","doi-asserted-by":"publisher","DOI":"10.17721\/2227-1481.6.20-23"},{"key":"S1743921316013016_ref007","doi-asserted-by":"publisher","DOI":"10.1051\/0004-6361\/201016275"},{"key":"S1743921316013016_ref005","doi-asserted-by":"publisher","DOI":"10.1002\/asna.201211725"},{"key":"S1743921316013016_ref006","first-page":"185","volume":"140","author":"Solanki","year":"1984","journal-title":"Astron. Astrophys."},{"key":"S1743921316013016_ref003","unstructured":"Lozitsky V. , Botygina O. , & Gordovskyy M. , 2016, Astron. Tsirkular No. 1631, 1"}],"container-title":["Proceedings of the International Astronomical Union"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.cambridge.org\/core\/services\/aop-cambridge-core\/content\/view\/S1743921316013016","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2019,4,18]],"date-time":"2019-04-18T19:38:20Z","timestamp":1555616300000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.cambridge.org\/core\/product\/identifier\/S1743921316013016\/type\/journal_article"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2016,10]]},"references-count":8,"journal-issue":{"issue":"S325","published-print":{"date-parts":[[2016,10]]}},"alternative-id":["S1743921316013016"],"URL":"https:\/\/doi.org\/10.1017\/s1743921316013016","relation":{},"ISSN":["1743-9213","1743-9221"],"issn-type":[{"value":"1743-9213","type":"print"},{"value":"1743-9221","type":"electronic"}],"subject":[],"published":{"date-parts":[[2016,10]]}}}