{"id":1363,"date":"2024-07-11T11:06:22","date_gmt":"2024-07-11T09:06:22","guid":{"rendered":"http:\/\/brera.inaf.it\/?post_type=tesi&p=1363"},"modified":"2025-05-26T18:20:47","modified_gmt":"2025-05-26T16:20:47","slug":"exoplanets-high-resolution-spectroscopic-studies-of-the-atmospheres-of-solar-system-bodies-using-exoplanets-techniques","status":"publish","type":"tesi","link":"https:\/\/brera.inaf.it\/en\/tesi\/exoplanets-high-resolution-spectroscopic-studies-of-the-atmospheres-of-solar-system-bodies-using-exoplanets-techniques\/","title":{"rendered":"Exoplanets – PhD – MERATE (LC) – High-resolution spectroscopic studies of the atmospheres of Solar System bodies using exoplanets\u2019 techniques – Rainer, Borsa."},"content":{"rendered":"\n
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\"\"<\/figure>\n<\/div>\n\n\n\n
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Exoplanets<\/span><\/h5>\n\n\n\n
Phd Thesis<\/h5>\n\n\n\n
Site: Merate (LC)<\/h5>\n\n\n\n
Duration<\/h5>\n\n\n\n

3 years<\/p>\n\n\n\n

Tutors<\/h5>\n\n\n\n

 Monica Rainer, Francesco Borsa<\/p>\n\n\n\n

Contact<\/h5>\n\n\n\n

monica.rainer AT inaf.it
francesco.borsa AT inaf.it<\/p>\n\n\n\n

Description<\/h5>\n\n\n\n
\n

The aim of the thesis is to apply<\/strong> the techniques developed to study and characterize exoplanets\u2019 atmospheres to high-resolution spectra of Solar System bodies<\/strong> in order to study their atmospheric composition, variability, dynamics, and the possible relation of these observables to geological activities in the case of rocky planets\/satellites.
This work will help to characterize<\/strong> the Solar System bodies themselves and to better understand the results from the exoplanets\u2019 observations.
The data used will be partly retrieved from public archives and partly obtained with dedicated observations.<\/p>\n\n\n\n

[Crediti immagine: NASA]<\/em><\/p>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n

<\/p>\n","protected":false},"excerpt":{"rendered":"

Exoplanets Phd Thesis Site: Merate (LC) Duration 3 years Tutors  Monica Rainer, Francesco Borsa Contact monica.rainer AT inaf.itfrancesco.borsa AT inaf.it Description The aim of the thesis is to apply the techniques developed to study and characterize exoplanets\u2019 atmospheres to high-resolution spectra of Solar System bodies in order to study their atmospheric composition, variability, dynamics, and the possible relation of these […]<\/p>\n","protected":false},"author":1,"featured_media":1365,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"closed","template":"","format":"standard","meta":{"footnotes":""},"categories":[27,26],"tags":[117,118,119,120],"class_list":["post-1363","tesi","type-tesi","status-publish","format-standard","has-post-thumbnail","hentry","category-phd-thesis","category-thesis","tag-francesco-borsa-en","tag-high-resolution-spectra-en","tag-monica-rainer-en","tag-solar-system-bodies-en"],"blocksy_meta":[],"featured_image_urls":{"full":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer1.png",738,478,false],"thumbnail":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer1.png",150,97,false],"medium":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer1.png",300,194,false],"medium_large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer1.png",738,478,false],"large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer1.png",738,478,false],"1536x1536":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer1.png",738,478,false],"2048x2048":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer1.png",738,478,false]},"post_excerpt_stackable":"

Exoplanets Phd Thesis Site: Merate (LC) Duration 3 years Tutors  Monica Rainer, Francesco Borsa Contact monica.rainer AT inaf.itfrancesco.borsa AT inaf.it Description The aim of the thesis is to apply the techniques developed to study and characterize exoplanets\u2019 atmospheres to high-resolution spectra of Solar System bodies in order to study their atmospheric composition, variability, dynamics, and the possible relation of these observables to geological activities in the case of rocky planets\/satellites.This work will help to characterize the Solar System bodies themselves and to better understand the results from the exoplanets\u2019 observations.The data used will be partly retrieved from public archives and partly obtained with dedicated observations. [Crediti immagine:…<\/p>\n","category_list":"PhD thesis<\/a>, Thesis<\/a>","author_info":{"name":"Maria Rosa Panzera","url":"https:\/\/brera.inaf.it\/en\/author\/maria-rosa-panzera\/"},"comments_num":"0 comments","_links":{"self":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1363","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi"}],"about":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/types\/tesi"}],"author":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/comments?post=1363"}],"version-history":[{"count":7,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1363\/revisions"}],"predecessor-version":[{"id":6868,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1363\/revisions\/6868"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media\/1365"}],"wp:attachment":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=1363"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/categories?post=1363"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tags?post=1363"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}