2025-02-21T08:28:39-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-119190%22&qt=morelikethis&rows=5
2025-02-21T08:28:39-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-119190%22&qt=morelikethis&rows=5
2025-02-21T08:28:39-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-21T08:28:39-05:00 DEBUG: Deserialized SOLR response
The energy sources of CME acceleration
We investigate the possibility that during the fast acceleration phase of a coronal mass ejection (CME), a freely propagating shock wave could be launched. We test this hypothesis by calculating the speeds of blast waves by using the Taylor-Sedov equation in changing density solar atmosphere, and co...
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Main Authors: | Allawi, H., Pohjolainen, S. |
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Format: | Article |
Language: | English |
Published: |
Головна астрономічна обсерваторія НАН України
2012
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Series: | Advances in Astronomy and Space Physics |
Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/119190 |
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2025-02-21T08:28:39-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query fl=%2A&rows=40&rows=5&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-119190%22&qt=morelikethis
2025-02-21T08:28:39-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&rows=40&rows=5&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-119190%22&qt=morelikethis
2025-02-21T08:28:39-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-21T08:28:39-05:00 DEBUG: Deserialized SOLR response
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