Monthly Notices of Royal Astronomical Society<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Vr\u00e1mci tejto spolupr\u00e1ce sme vyv\u00edjali met\u00f3dy charakteriz\u00e1cie aeros\u00f3lu z pozemnej r\u00e1diometrie a uk\u00e1zali sme, \u017ee kvalitat\u00edvne nov\u00e9 inform\u00e1cie mo\u017eno z\u00edska\u0165 len v synergii meran\u00ed oblohov\u00fdmi…<\/p>\n","protected":false},"author":4,"featured_media":0,"parent":6632,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":"","_links_to":"","_links_to_target":""},"class_list":["post-7403","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/pages\/7403","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/users\/4"}],"replies":[{"embeddable":true,"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/comments?post=7403"}],"version-history":[{"count":2,"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/pages\/7403\/revisions"}],"predecessor-version":[{"id":7904,"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/pages\/7403\/revisions\/7904"}],"up":[{"embeddable":true,"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/pages\/6632"}],"wp:attachment":[{"href":"https:\/\/ustarch.sav.sk\/sk\/wp-json\/wp\/v2\/media?parent=7403"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}
![\"\"](\"https:\/\/ustarch.sav.sk\/sk\/wp-content\/uploads\/sites\/2\/opt3-300x127.jpg\")
Vr\u00e1mci tejto spolupr\u00e1ce sme vyv\u00edjali met\u00f3dy charakteriz\u00e1cie aeros\u00f3lu z pozemnej r\u00e1diometrie a uk\u00e1zali sme, \u017ee kvalitat\u00edvne nov\u00e9 inform\u00e1cie mo\u017eno z\u00edska\u0165 len v synergii meran\u00ed oblohov\u00fdmi fotometrami a optick\u00fdm monitoringom spodnej troposf\u00e9ry. Navrhli sme komplement\u00e1rny experiment\u00e1lny setup pre kvantifik\u00e1ciu sveteln\u00e9ho po\u013ea v no\u010dnom prostred\u00ed (Obr. dole). Inverziou (I) r\u00e1diometrick\u00fdch d\u00e1t z\u00edskame vstupny do te\u00f3ri\u00ed (T) a n\u00e1sledne numerick\u00e9 predpovede jasu no\u010dnej oblohy (NSB) na miestach (T1…Tn), kde absentuj\u00fa priame merania (M). R\u00e1diometrick\u00e9 d\u00e1ta a stupe\u0148 polariz\u00e1cie P meran\u00e9 pozd\u013a\u017e vertik\u00e1ly od zenitu k horizontu sa uk\u00e1zali ako najobsiahlej\u0161\u00ed zdroj inform\u00e1ci\u00ed o emisnej funkcii zdroja svetla, zatia\u013e \u010do jeho spektr\u00e1lne zlo\u017eenie mo\u017eno extrahova\u0165 z dif\u00fazneho svetla oblohy. Akt\u00edvne optick\u00e9 sn\u00edmanie laserov\u00e9ho l\u00fa\u010da pozd\u013a\u017e jeho trajekt\u00f3rie spodn\u00fdmi vrstvami atmosf\u00e9ry je zdrojom inform\u00e1ci\u00ed o optick\u00fdch vlastnostiach atmosf\u00e9ry (ATM), napr. o f\u00e1zovej funkcii rozptylu p(\u03b8) v \u0161irokom rozsahu uhlov \u03b8.<\/p>\n