Filament eruption deflection and associated CMEs
We present the observations of a quiescent filament eruption and its deflection from the radial direction. The event occurred in the southern solar hemisphere on 2021 May 9 and was observed by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO), by the STEREO A Obser...
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| creator | Koleva, K Chandra, R Duchlev, P Devi, P |
| description | We present the observations of a quiescent filament eruption and its
deflection from the radial direction. The event occurred in the southern solar
hemisphere on 2021 May 9 and was observed by the Atmospheric Imaging Assembly
(AIA) on board the Solar Dynamics Observatory (SDO), by the STEREO A
Observatory and GONG. Part of the filament erupted in the west direction, while
major part of the filament deviated towards east direction. LASCO observed a
very weak CME towards the west direction where it faded quickly. Moreover, the
eruption was associated with CME observed by STEREO A COR1 and COR2. Our
observations provide the evidence that the filament eruption was highly
non-radial in nature. |
| doi_str_mv | 10.48550/arxiv.2411.10110 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2411_10110</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2411_10110</sourcerecordid><originalsourceid>FETCH-arxiv_primary_2411_101103</originalsourceid><addsrcrecordid>eNpjYJA0NNAzsTA1NdBPLKrILNMzMjE01DM0MDQ04GQwcMvMScxNzStRSC0qLSjJzM9TSElNy0lNBjMT81IUEouL85MzE0tSUxScfV2LeRhY0xJzilN5oTQ3g7yba4izhy7Y7PiCoszcxKLKeJAd8WA7jAmrAABC2zCD</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Filament eruption deflection and associated CMEs</title><source>arXiv.org</source><creator>Koleva, K ; Chandra, R ; Duchlev, P ; Devi, P</creator><creatorcontrib>Koleva, K ; Chandra, R ; Duchlev, P ; Devi, P</creatorcontrib><description>We present the observations of a quiescent filament eruption and its
deflection from the radial direction. The event occurred in the southern solar
hemisphere on 2021 May 9 and was observed by the Atmospheric Imaging Assembly
(AIA) on board the Solar Dynamics Observatory (SDO), by the STEREO A
Observatory and GONG. Part of the filament erupted in the west direction, while
major part of the filament deviated towards east direction. LASCO observed a
very weak CME towards the west direction where it faded quickly. Moreover, the
eruption was associated with CME observed by STEREO A COR1 and COR2. Our
observations provide the evidence that the filament eruption was highly
non-radial in nature.</description><identifier>DOI: 10.48550/arxiv.2411.10110</identifier><language>eng</language><subject>Physics - Solar and Stellar Astrophysics</subject><creationdate>2024-11</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2411.10110$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2411.10110$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Koleva, K</creatorcontrib><creatorcontrib>Chandra, R</creatorcontrib><creatorcontrib>Duchlev, P</creatorcontrib><creatorcontrib>Devi, P</creatorcontrib><title>Filament eruption deflection and associated CMEs</title><description>We present the observations of a quiescent filament eruption and its
deflection from the radial direction. The event occurred in the southern solar
hemisphere on 2021 May 9 and was observed by the Atmospheric Imaging Assembly
(AIA) on board the Solar Dynamics Observatory (SDO), by the STEREO A
Observatory and GONG. Part of the filament erupted in the west direction, while
major part of the filament deviated towards east direction. LASCO observed a
very weak CME towards the west direction where it faded quickly. Moreover, the
eruption was associated with CME observed by STEREO A COR1 and COR2. Our
observations provide the evidence that the filament eruption was highly
non-radial in nature.</description><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJA0NNAzsTA1NdBPLKrILNMzMjE01DM0MDQ04GQwcMvMScxNzStRSC0qLSjJzM9TSElNy0lNBjMT81IUEouL85MzE0tSUxScfV2LeRhY0xJzilN5oTQ3g7yba4izhy7Y7PiCoszcxKLKeJAd8WA7jAmrAABC2zCD</recordid><startdate>20241115</startdate><enddate>20241115</enddate><creator>Koleva, K</creator><creator>Chandra, R</creator><creator>Duchlev, P</creator><creator>Devi, P</creator><scope>GOX</scope></search><sort><creationdate>20241115</creationdate><title>Filament eruption deflection and associated CMEs</title><author>Koleva, K ; Chandra, R ; Duchlev, P ; Devi, P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_2411_101103</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Koleva, K</creatorcontrib><creatorcontrib>Chandra, R</creatorcontrib><creatorcontrib>Duchlev, P</creatorcontrib><creatorcontrib>Devi, P</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Koleva, K</au><au>Chandra, R</au><au>Duchlev, P</au><au>Devi, P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Filament eruption deflection and associated CMEs</atitle><date>2024-11-15</date><risdate>2024</risdate><abstract>We present the observations of a quiescent filament eruption and its
deflection from the radial direction. The event occurred in the southern solar
hemisphere on 2021 May 9 and was observed by the Atmospheric Imaging Assembly
(AIA) on board the Solar Dynamics Observatory (SDO), by the STEREO A
Observatory and GONG. Part of the filament erupted in the west direction, while
major part of the filament deviated towards east direction. LASCO observed a
very weak CME towards the west direction where it faded quickly. Moreover, the
eruption was associated with CME observed by STEREO A COR1 and COR2. Our
observations provide the evidence that the filament eruption was highly
non-radial in nature.</abstract><doi>10.48550/arxiv.2411.10110</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Solar and Stellar Astrophysics |
| title | Filament eruption deflection and associated CMEs |
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