{"id":119,"date":"2019-09-28T00:57:42","date_gmt":"2019-09-28T04:57:42","guid":{"rendered":"https:\/\/sites.bu.edu\/murdock-hart\/?page_id=119"},"modified":"2019-10-17T13:33:32","modified_gmt":"2019-10-17T17:33:32","slug":"temporal-variations","status":"publish","type":"page","link":"https:\/\/sites.bu.edu\/murdock-hart\/airglow\/temporal-variations\/","title":{"rendered":"Temporal Variations"},"content":{"rendered":"<p style=\"text-align: justify;\">The atmospheric airglow varies on time scales greater than 200 seconds, and on spatial scales greater than a few degrees. The Sloan Digital Sky Survey (SDSS) and Baryon-Acoustic Oscillation Spectroscopic Survey (BOSS) have observed sky spectra for over 15 years, and the OH emission intensity is significantly correlated to solar activity. The plot of sunspot number and F<sub>10.7cm<\/sub> are given below for comparison.<\/p>\n<p><img loading=\"lazy\" src=\"\/murdock-hart\/files\/2019\/09\/OH_emission_ray_vs_time-636x357.png\" alt=\"\" class=\"size-medium wp-image-128 aligncenter\" width=\"636\" height=\"357\" srcset=\"https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_ray_vs_time-636x357.png 636w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_ray_vs_time-768x431.png 768w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_ray_vs_time-1024x574.png 1024w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_ray_vs_time.png 1232w\" sizes=\"(max-width: 636px) 100vw, 636px\" \/><\/p>\n<p><img loading=\"lazy\" src=\"\/murdock-hart\/files\/2019\/09\/sunspot_number_and_F_10_7_vs_time-636x357.png\" alt=\"\" class=\"size-medium wp-image-130 aligncenter\" width=\"636\" height=\"357\" srcset=\"https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/sunspot_number_and_F_10_7_vs_time-636x357.png 636w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/sunspot_number_and_F_10_7_vs_time-768x431.png 768w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/sunspot_number_and_F_10_7_vs_time-1024x575.png 1024w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/sunspot_number_and_F_10_7_vs_time.png 1230w\" sizes=\"(max-width: 636px) 100vw, 636px\" \/><\/p>\n<p style=\"text-align: justify;\">The variations in OH intensity are the greatest on annual and over night time scales. The annual variations in OH intensity are due to global scale circulations.<\/p>\n<p><img loading=\"lazy\" src=\"\/murdock-hart\/files\/2019\/09\/OH_emission_annual_2_panels-636x357.png\" alt=\"\" class=\"size-medium wp-image-126 aligncenter\" width=\"636\" height=\"357\" srcset=\"https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_annual_2_panels-636x357.png 636w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_annual_2_panels-768x431.png 768w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_annual_2_panels-1024x575.png 1024w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_annual_2_panels.png 1230w\" sizes=\"(max-width: 636px) 100vw, 636px\" \/><\/p>\n<p style=\"text-align: justify;\">While the nightly variations are due to changes in emission layer thickness before local midnight, and an increase in chemistry after midnight.<\/p>\n<p><img loading=\"lazy\" src=\"\/murdock-hart\/files\/2019\/09\/OH_emission_nightly_2_panels-636x357.png\" alt=\"\" class=\"aligncenter wp-image-127 size-medium\" width=\"636\" height=\"357\" srcset=\"https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_nightly_2_panels-636x357.png 636w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_nightly_2_panels-768x431.png 768w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_nightly_2_panels-1024x575.png 1024w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/OH_emission_nightly_2_panels.png 1230w\" sizes=\"(max-width: 636px) 100vw, 636px\" \/><\/p>\n<p style=\"text-align: justify;\">\u00a0To further investigate the variations in OH emission intensity observed by ground based instruments satellite data was employed. The Sounding for Atmospheric Broadband Emission Radiometer (SABER) on board the Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED) satellite has conveniently been in operation since 2001. SABER samples volume emission rates in 17 channels to generate atmospheric profiles of temperature, concentrations, and emission intensity. The OH molecule is produced through the ozone hydration reaction, H + O<sub>3<\/sub><sub>\u00a0<\/sub>&#8211;&gt; OH + O<sub>2<\/sub>, and the OH emission intensity is proportional to O<sub>3<\/sub> concentration. Below is a plot of average nightly O and O<sub>3<\/sub> concentration profiles acquired near the SDSS telescope. The data has been binned into 2 hour intervals, with the solid line representing local midnight. The dotted lines represent the time bins before local midnight, and the dash-dotted lines represent the bins after local midnight. SABER showed a significant enhancement to the O and O<sub>3<\/sub> concentrations on the bottom side of the OH emission layer.\u00a0<img loading=\"lazy\" src=\"\/murdock-hart\/files\/2019\/09\/TIMED_nightly_median_O_and_O3_concentrations_O3_lower_enhancement-636x357.png\" alt=\"\" class=\"size-medium wp-image-132 aligncenter\" width=\"636\" height=\"357\" srcset=\"https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/TIMED_nightly_median_O_and_O3_concentrations_O3_lower_enhancement-636x357.png 636w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/TIMED_nightly_median_O_and_O3_concentrations_O3_lower_enhancement-768x431.png 768w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/TIMED_nightly_median_O_and_O3_concentrations_O3_lower_enhancement-1024x574.png 1024w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/TIMED_nightly_median_O_and_O3_concentrations_O3_lower_enhancement.png 1232w\" sizes=\"(max-width: 636px) 100vw, 636px\" \/><\/p>\n<p style=\"text-align: justify;\">The O<sub>3<\/sub> enhancement on the bottom side of the OH emission layer effectively increases the layer width, and since ground based instrument measure a column of emission this effectively increases the observed intensity. After local midnight the emission intensity increases at the altitude of peak emission.<\/p>\n<p><img loading=\"lazy\" src=\"\/murdock-hart\/files\/2019\/09\/TIMED_median_nightly_OH_VER_peaks_with_O3_lower_enhancement-636x357.png\" alt=\"\" class=\"size-medium wp-image-131 aligncenter\" width=\"636\" height=\"357\" srcset=\"https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/TIMED_median_nightly_OH_VER_peaks_with_O3_lower_enhancement-636x357.png 636w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/TIMED_median_nightly_OH_VER_peaks_with_O3_lower_enhancement-768x431.png 768w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/TIMED_median_nightly_OH_VER_peaks_with_O3_lower_enhancement-1024x574.png 1024w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/TIMED_median_nightly_OH_VER_peaks_with_O3_lower_enhancement.png 1232w\" sizes=\"(max-width: 636px) 100vw, 636px\" \/><\/p>\n<p style=\"text-align: justify;\">The plots below show the average nightly variations in temperature, O and O<sub>3<\/sub> concentrations, and OH 2.0 micron and OH 1.6 micron VER.<\/p>\n<p><img loading=\"lazy\" src=\"\/murdock-hart\/files\/2019\/09\/diurnal_median_temp_and_mixing_profiles_w_NO-636x357.png\" alt=\"\" class=\"size-medium wp-image-141 aligncenter\" width=\"636\" height=\"357\" srcset=\"https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/diurnal_median_temp_and_mixing_profiles_w_NO-636x357.png 636w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/diurnal_median_temp_and_mixing_profiles_w_NO-768x431.png 768w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/diurnal_median_temp_and_mixing_profiles_w_NO-1024x574.png 1024w, https:\/\/sites.bu.edu\/murdock-hart\/files\/2019\/09\/diurnal_median_temp_and_mixing_profiles_w_NO.png 1232w\" sizes=\"(max-width: 636px) 100vw, 636px\" \/><\/p>\n<p style=\"text-align: justify;\">For more detailed information about OH emission, and the temporal variations in intensity see my manuscript at this link \u00a0<a href=\"https:\/\/doi.org\/10.1088\/1538-3873\/aae972\">https:\/\/doi.org\/10.1088\/1538-3873\/aae972<\/a>.<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The atmospheric airglow varies on time scales greater than 200 seconds, and on spatial scales greater than a few degrees. The Sloan Digital Sky Survey (SDSS) and Baryon-Acoustic Oscillation Spectroscopic Survey (BOSS) have observed sky spectra for over 15 years, and the OH emission intensity is significantly correlated to solar activity. The plot of sunspot [&hellip;]<\/p>\n","protected":false},"author":16674,"featured_media":0,"parent":59,"menu_order":1,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"_links":{"self":[{"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/pages\/119"}],"collection":[{"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/users\/16674"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/comments?post=119"}],"version-history":[{"count":10,"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/pages\/119\/revisions"}],"predecessor-version":[{"id":205,"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/pages\/119\/revisions\/205"}],"up":[{"embeddable":true,"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/pages\/59"}],"wp:attachment":[{"href":"https:\/\/sites.bu.edu\/murdock-hart\/wp-json\/wp\/v2\/media?parent=119"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}