{"id":76,"date":"2018-05-22T12:03:19","date_gmt":"2018-05-22T12:03:19","guid":{"rendered":"http:\/\/capst.ncku.edu.tw\/PGS\/?page_id=76"},"modified":"2021-01-15T08:56:57","modified_gmt":"2021-01-15T08:56:57","slug":"laboratory-astrophysics-space-science","status":"publish","type":"page","link":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/laboratory-astrophysics-space-science\/","title":{"rendered":"Laboratory Astrophysics &#038; Space Science"},"content":{"rendered":"<div><span style=\"font-size: large;\"><b>1. Interactions between solar winds and planetary magnetic fields or unmagnetized planets will be studied<\/b><\/span><\/div>\n<div><a href=\"https:\/\/sites.google.com\/site\/ppgssncku\/research\/Laboratory-Astrophysics-and-Space-Science\/Solar_Magnetopause_Interaction.png?attredirects=0\"><img loading=\"lazy\" decoding=\"async\" class=\"\" src=\"https:\/\/sites.google.com\/site\/ppgssncku\/_\/rsrc\/1470811385413\/research\/Laboratory-Astrophysics-and-Space-Science\/Solar_Magnetopause_Interaction.png\" width=\"600\" height=\"305\" border=\"0\"><\/a><\/div>\n<div>&nbsp;<\/div>\n<ul>\n<li>Studies of the Martian bow shock location: The shock nose location is more sensitive to the solar EUV flux than solar wind dynamics pressure consisting with the spacecraft measurement results:<\/li>\n<\/ul>\n\n\n<figure class=\"wp-block-image size-large is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/03\/MartianBowShock-1024x636.png\" alt=\"\" class=\"wp-image-931\" width=\"656\" height=\"407\" srcset=\"https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/03\/MartianBowShock-1024x636.png 1024w, https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/03\/MartianBowShock-300x186.png 300w, https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/03\/MartianBowShock-768x477.png 768w, https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/03\/MartianBowShock-1536x954.png 1536w, https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/03\/MartianBowShock-2048x1272.png 2048w\" sizes=\"auto, (max-width: 656px) 100vw, 656px\" \/><\/figure>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"408\" height=\"560\" src=\"http:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/08\/DSC_4955_Cut_wScale.png\" alt=\"\" class=\"wp-image-1126\" srcset=\"https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/08\/DSC_4955_Cut_wScale.png 408w, https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/08\/DSC_4955_Cut_wScale-219x300.png 219w\" sizes=\"auto, (max-width: 408px) 100vw, 408px\" \/><\/figure>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"527\" height=\"357\" src=\"http:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/08\/DSC_5011_Bright_Cut_wScale.png\" alt=\"\" class=\"wp-image-1127\" srcset=\"https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/08\/DSC_5011_Bright_Cut_wScale.png 527w, https:\/\/capst.ncku.edu.tw\/PGS\/wp-content\/uploads\/2020\/08\/DSC_5011_Bright_Cut_wScale-300x203.png 300w\" sizes=\"auto, (max-width: 527px) 100vw, 527px\" \/><\/figure>\n\n\n\n<p><strong>2. Magnetic reconnections<\/strong><\/p>\n\n\n\n<figure class=\"wp-block-image\"><a href=\"https:\/\/sites.google.com\/site\/ppgssncku\/research\/Laboratory-Astrophysics-and-Space-Science\/Reconnection_Exp.png?attredirects=0\"><img decoding=\"async\" src=\"https:\/\/sites.google.com\/site\/ppgssncku\/_\/rsrc\/1470811473249\/research\/Laboratory-Astrophysics-and-Space-Science\/Reconnection_Exp.png?height=306&amp;width=400\" alt=\"\"\/><\/a><\/figure>\n\n\n\n<figure class=\"wp-block-image\"><a href=\"https:\/\/sites.google.com\/site\/ppgssncku\/research\/Laboratory-Astrophysics-and-Space-Science\/Reconnection_Exp_Control.png?attredirects=0\"><img decoding=\"async\" src=\"https:\/\/sites.google.com\/site\/ppgssncku\/_\/rsrc\/1470811507072\/research\/Laboratory-Astrophysics-and-Space-Science\/Reconnection_Exp_Control.png?height=254&amp;width=400\" alt=\"\"\/><\/a><\/figure>\n\n\n\n<p>\n&nbsp;\n&#8212;\nRef.\n\nLucy-Ann McFadden and Torrence Johnson and Paul Weissman, ed., Encyclopedia of the Solar System, 2nd Ed. (Academic Press, 2006).\n\n\n\n<\/p>\n","protected":false},"excerpt":{"rendered":"<p>1. Interactions between solar winds and planetary magnetic fields or unmagnetized planets will be studied &nbsp; Studies of the Martian bow shock location: The shock nose location is more sensitive to the solar EUV flux than solar wind dynamics pressure &hellip; <a href=\"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/laboratory-astrophysics-space-science\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"onecolumn-page.php","meta":{"ngg_post_thumbnail":0,"footnotes":""},"class_list":["post-76","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/wp-json\/wp\/v2\/pages\/76","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/wp-json\/wp\/v2\/comments?post=76"}],"version-history":[{"count":8,"href":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/wp-json\/wp\/v2\/pages\/76\/revisions"}],"predecessor-version":[{"id":1316,"href":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/wp-json\/wp\/v2\/pages\/76\/revisions\/1316"}],"wp:attachment":[{"href":"https:\/\/capst.ncku.edu.tw\/PGS\/index.php\/wp-json\/wp\/v2\/media?parent=76"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}