1769 / 2019-08-29 10:42:05
Sun glint thresholds for the remote detection of oil films on the ocean surface
摘要待审
It has been known that the presence of sun glint can enhance oil-water spatial contrast and thus facilitating oil slick detection in optical imagery. However, the strength of sun glint required to detect thin oil films has never been quantified objectively. Natural oil slicks in the western Gulf of Mexico are used to determine the sun glint threshold required for optical remote sensing of oil films. Thin oil films from the natural seeps are used here to minimize reflectance signal from oil optical properties (absorption and scattering). The threshold is determined using the same-day image pairs collected by Moderate Resolution Imaging Spectroradiometer (MODIS) Terra, MODIS Aqua, and Visible Infrared Imaging Radiometer Suite (VIIRS) (N = 2297 images) over the same oil slick locations where at least one of the sensors captures the oil slicks. For each sensor, statistics of sun glint strengths, represented by the normalized glint reflectance (LGN, sr-1), when oil slicks can and cannot be observed are generated. The LGN threshold for oil film detections is determined to be 10-5–10-6 sr-1 for MODIS Terra and MODIS Aqua, and 10-6–10-7 sr-1 for VIIRS. Below these thresholds, no oil films can be detected, while above these thresholds, oil films can always be detected except near the critical-angle zone where oil slicks reverse their contrast against the background water. The sun glint thresholds determined here will provide critical information on which images (or which portions of an image) can be used to search for oil, thus reducing false negative detection.
重要日期
  • 会议日期

    10月12日

    2019

    10月15日

    2019

  • 09月30日 2019

    初稿截稿日期

  • 10月15日 2019

    注册截止日期

  • 07月21日 2020

    报告提交截止日期

主办单位
青年地学论坛理事会
承办单位
中国科学院青海盐湖研究所
中国科学院西北高原生物研究所
青海师范大学
联系方式
历届会议
移动端
在手机上打开
小程序
打开微信小程序
客服
扫码或点此咨询