{"id":10,"date":"2019-09-11T10:04:21","date_gmt":"2019-09-11T08:04:21","guid":{"rendered":"http:\/\/195.96.236.139\/?page_id=10"},"modified":"2024-09-13T13:16:57","modified_gmt":"2024-09-13T11:16:57","slug":"soho-erne-proton-event-catalog","status":"publish","type":"page","link":"https:\/\/catalogs.astro.bas.bg\/index.php\/soho-erne-proton-event-catalog\/","title":{"rendered":"Proton events"},"content":{"rendered":"\r\n<p>The catalog lists the proton events from the <a href=\"https:\/\/srl.utu.fi\/projects\/erne\/\" target=\"_blank\" rel=\"noreferrer noopener\">SOHO\/ERNE<\/a> instrument presented separately in solar cycle (SC) 23 (1996-2008) and SC24 (2009-2017). In contrast to other catalogs available elsewhere, this catalog utilizes the highest temporal resolution as provided, namely 1 min.<\/p>\r\n<p>Results from the final SEP catalog are available here:<\/p>\r\n<p><a href=\"https:\/\/www.mdpi.com\/2073-4433\/15\/8\/1016\">Miteva et al. Atmosphere (2024)<\/a><\/p>\r\n<p>Preliminary results from the catalog are published here:<\/p>\r\n<p><a href=\"http:\/\/space.bas.bg\/SES\/archive\/SES%202023_DOKLADI\/PROCEEDINGS%20SES%202023.pdf\">Miteva et al. SES-Proceedings (2023)<\/a><\/p>\r\n<p><a href=\"https:\/\/www.astro.bas.bg\/AIJ\/issues\/n33\/RMiteva.pdf\">Miteva et al., Bulgarian Astronomical Journal, Vol. 33, pp. 99-108 (2020)<\/a><\/p>\r\n<p><a href=\"https:\/\/pubs.aip.org\/aip\/acp\/article-abstract\/2075\/1\/090014\/819724\/Spectral-analysis-of-SOHO-ERNE-protons-in-solar?redirectedFrom=fulltext\">Miteva &amp; Tsvetkov <em>AIP Conf. Proc.<\/em> 2075, 090014 (2019)<\/a><\/p>\r\n<p><a href=\"http:\/\/ws-sozopol.stil.bas.bg\/2018Primorsko\/Miteva_Danov_WS-10.pdf\">Miteva &amp; Danov WS-Proceedings (2019)<\/a><\/p>\r\n<p><a href=\"http:\/\/ws-sozopol.stil.bas.bg\/2017Sunny\/Miteva_SES2017.pdf\">Miteva SES-Proceedings (2017)<\/a><\/p>\r\n<p><strong>Funding:<\/strong> This research was supported by SCOSTEP\/PRESTO project \u2018On the relationship between major space weather phenomena in solar cycles 23 and 24\u2019; by the Bulgarian-Egyptian inter-academy project \u2018On space effects at near Earth environment\u2014from remote observations and in situ forecasting to impacts on satellites\u2019 (2022\u20132024), Bulgarian Academy of Sciences IC-EG\/08\/2022-2024 and Egyptian Academy of Scientific Research and Technology (ASRT)\/NRIAG (ASRT\/BAS\/2022-2023\/10116) and by the Bulgarian-Serbian inter-academy project \u2018Active Events on The Sun. Catalogs of Proton Events and Electron Signatures in X-Ray, UV and Radio Diapason. Influence of Collisions on Optical Properties of Dense Hydrogen Plasma\u2019 (2023\u20132025).<\/p>\r\n<p><strong>Acknowledgements:<\/strong> SOHO\/ERNE data was provided by Prof. Eino Valtonen (PI) and is also available via <span style=\"color: #993300;\"> <a style=\"color: #993300;\" href=\"http:\/\/server.sepserver.eu\/index.php?page=home\" target=\"_blank\" rel=\"noreferrer noopener\">SEPServer data server<\/a><\/span>. SOHO is a project of international collaboration between ESA and NASA.<\/p>\r\n<p><strong>Disclaimer:<\/strong> The data is a subject to instrumental saturation effects.\u00a0<\/p>\r\n<p><strong>Contact: <\/strong><span style=\"color: #993300;\"><a style=\"color: #993300;\" href=\"mailto:rmiteva@nao-rozhen.org\">rmiteva [at] nao-rozhen.org <\/a><\/span><\/p>\r\n<!--\r\n<p><strong>Explanatory notes:<\/strong><\/p>\r\n<p style=\"padding-left: 80px;\"><strong>Proton peak<\/strong>: identified at the maximum of the particle profile (local enhancements are not considered).<br \/><strong>Onset time<\/strong>: identified as the time of 3-sigma intensity value above pre-event level.<br \/><strong>Peak time<\/strong>: the time at the peak proton intensity.<br \/><strong><em>J<\/em><sub>p<\/sub><\/strong>: peak proton intensity after subtraction of the pre-event level in protons\/(cm<sup>2<\/sup> s sr MeV).<br \/><strong>class<\/strong>: GOES soft X-ray flare class <br \/><strong>speed<\/strong>: linear speed of the CME in km s<sup>-1<\/sup><br \/><strong>time<\/strong>: all time markers are in UT The reported here onset\/peak times and <em>J<\/em><sub>p<\/sub> are based on 5-min averaged data.<\/p>\r\n<!--\r\n\r\n<p>\r\n\r\n<\/p>\r\n\r\n\r\n\r\n\r\n","protected":false},"excerpt":{"rendered":"<p>The catalog lists the proton events from the SOHO\/ERNE instrument presented separately in solar cycle (SC) 23 (1996-2008) and SC24 (2009-2017). In contrast to other catalogs available elsewhere, this catalog utilizes the highest temporal resolution as provided, namely 1 min. Results from the final SEP catalog are available here: Miteva et al. Atmosphere (2024) Preliminary [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"full-width.php","meta":{"footnotes":""},"class_list":["post-10","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/catalogs.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages\/10"}],"collection":[{"href":"https:\/\/catalogs.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/catalogs.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/catalogs.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/catalogs.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/comments?post=10"}],"version-history":[{"count":34,"href":"https:\/\/catalogs.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages\/10\/revisions"}],"predecessor-version":[{"id":639,"href":"https:\/\/catalogs.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages\/10\/revisions\/639"}],"wp:attachment":[{"href":"https:\/\/catalogs.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/media?parent=10"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}